physconst (4feb20)

git-svn-id: svn://tug.org/texlive/trunk@53674 c570f23f-e606-0410-a88d-b1316a301751

5 files changed, 8373 insertions, 188 deletions

diff --git a/Master/texmf-dist/doc/latex/physconst/CHANGELOG.md b/Master/texmf-dist/doc/latex/physconst/CHANGELOG.md
index 059256090c9..c765c612a02 100644
--- a/Master/texmf-dist/doc/latex/physconst/CHANGELOG.md
+++ b/Master/texmf-dist/doc/latex/physconst/CHANGELOG.md
@@ -13,7 +13,8 @@
 - added localuninstall and distuninstall targets to the makefile
 ### Changed
 - Modified the makefile to split up generation of the .sty, .dtx, and .pdf
-- Modified the .cpp so that every \DeclareRobustCommand starts a new line right away
+- Modified the .cpp so that every \DeclareRobustCommand starts a new line right 
+away
 - Added a newline in the middle of the title declaration (in .cpp)
 - Added a newline in the middle of the \DoNotIndex declaration (in .cpp)
 - Added dependency on imakeidx and changed the index to 2 column.
@@ -31,10 +32,30 @@
 - Add disribution specific readme
 - Add disribution specific makefile
 ### Changed
-- Update README to have clearer build, distribute, install, and uninstall instructions.
+- Update README to have clearer build, distribute, install, and uninstall 
+instructions.
 - Distribute with .dtx instead of .sty
 - Reordered build, install, distribute, and uninstall sections of the README
 - Pulled build up one level of headings in the README
 - fix some typos in README
-
-
+## [1.1.0] - 2020/02/03
+### Added
+- macro for Earth's mass
+- macro for Jupiter's mass
+- macro for Earth's radius
+- macro for Jupiter's radius
+- distribution specific change log
+- Numeric variant of each constant for use with e.g. tikz
+### Changes
+- Colomb constant in SI units had an incorrect magnitude; fixed to 10^9 instead 
+of 10^14
+- Vacuum permeability was incorrectly a duplicate of the permittivity.
+Premeability is now the correct value.
+- Mass of particles in eV was being computed incorrectly. Fixed values.
+- Order of magnitude of Newton's Gravity, Boltzmann, Planck, and 
+Stefan-Boltzmann constants were incorrect.
+- Acceleration due to gravity on Earth was accidentally a copy of G instead of g
+- Acceleration due to gravity on Earth had the wrong units
+- Corrected formatting of README file.
+- Fixed sections of macros - the individual macros were unintentionally
+subsections of the Naming Conversion
diff --git a/Master/texmf-dist/doc/latex/physconst/README.md b/Master/texmf-dist/doc/latex/physconst/README.md
index 8a43c78f495..8727bf5e438 100644
--- a/Master/texmf-dist/doc/latex/physconst/README.md
+++ b/Master/texmf-dist/doc/latex/physconst/README.md
@@ -16,7 +16,8 @@ and version 1.3c or later is part of all distributions of LaTeX
 version 2006/05/20 or later.
 
 # Dependencies
-- [`physunits` package](https://github.com/astrobit/physunits) also available at [CTAN](https://ctan.org)
+- [`physunits` package](https://github.com/astrobit/physunits) also available
+at [CTAN](https://ctan.org)
 
 # Build Dependencies
 - some LaTeX distribution.
@@ -27,7 +28,8 @@ version 2006/05/20 or later.
 
 # Files
 ```
-    makefile                GNU makefile to simplify building and installation on linux
+    makefile                GNU makefile to simplify building and installation
+                            on linux
     README.md               This file.
     CHANGELOG.md            List of changes
     physconst.ins           The installer file
@@ -40,28 +42,37 @@ version 2006/05/20 or later.
 1. `make`
 
 ## Otherwise
-1. Run `latex` on `physconst.ins` to create the `.sty` file. e.g. `latex physconst.ins`.
+1. Run `latex` on `physconst.ins` to create the `.sty` file. e.g. 
+`latex physconst.ins`.
 1. The following steps apply only if you want the documentation (recommended).
-  1. Run `latex` on `physconst.dtx` to create the `.pdf` file. e.g. `xelatex physconst.pdf`.
-  1. Run `makeindex` to create the index, e.g. `makeindex -s gind.ist -o physconst.ind physconst.idx`.
-  1. Run `makeindex` to create the change log, e.g. `makeindex -s gglo.ist -o physconst.gls physconst.glo`.
-  1. Run `latex` on `physconst.dtx` to create the `.pdf` file with index and change log. e.g. `xelatex physconst.pdf`.
-  1. Run `latex` on `physconst.dtx` to get the labels sorted out. e.g. `xelatex physconst.pdf`.
-
-Instructions that might help can be for windows can be found at [this post on StackExchange](https://tex.stackexchange.com/questions/369921/loading-packages-with-ins-and-dtx-files).
+  1. Run `latex` on `physconst.dtx` to create the `.pdf` file. e.g. 
+`xelatex physconst.pdf`.
+  1. Run `makeindex` to create the index, e.g. 
+`makeindex -s gind.ist -o physconst.ind physconst.idx`.
+  1. Run `makeindex` to create the change log, e.g. 
+`makeindex -s gglo.ist -o physconst.gls physconst.glo`.
+  1. Run `latex` on `physconst.dtx` to create the `.pdf` file with index and
+change log. e.g. `xelatex physconst.pdf`.
+  1. Run `latex` on `physconst.dtx` to get the labels sorted out. e.g.
+`xelatex physconst.pdf`.
+
+Instructions that might help can be for windows can be found at 
+[this post on StackExchange](https://tex.stackexchange.com/questions/369921/loading-packages-with-ins-and-dtx-files).
 
 # Installation
 First build the project as described above.
 
 ## For a single project
-1. Copy the `physconst.sty` into your project where your `.tex` files are located.
+1. Copy the `physconst.sty` into your project where your `.tex` files are
+located.
 
 ## for all users and projects
 ### Linux / Mac using make and xelatex
 1. `make localinstall`
 
 ### Otherwise
-Instructions that might help can be for windows can be found at [this post on StackExchange](https://tex.stackexchange.com/questions/369921/loading-packages-with-ins-and-dtx-files).
+Instructions that might help can be for windows can be found at 
+[this post on StackExchange](https://tex.stackexchange.com/questions/369921/loading-packages-with-ins-and-dtx-files).
 1. Figure out where your LaTeX local packages are installed.
 1. Create a directory named `physconst` in that location.
 1. Copy the `.sty` file into the directory you just created.
diff --git a/Master/texmf-dist/doc/latex/physconst/physconst.pdf b/Master/texmf-dist/doc/latex/physconst/physconst.pdf
index 67867850bce..ead2ea8bc7b 100644
--- a/Master/texmf-dist/doc/latex/physconst/physconst.pdf
+++ b/Master/texmf-dist/doc/latex/physconst/physconst.pdf
diff --git a/Master/texmf-dist/source/latex/physconst/physconst.dtx b/Master/texmf-dist/source/latex/physconst/physconst.dtx
index 691a5fd9018..7ade1893813 100644
--- a/Master/texmf-dist/source/latex/physconst/physconst.dtx
+++ b/Master/texmf-dist/source/latex/physconst/physconst.dtx
@@ -133,7 +133,7 @@
 % The normal macros are the ones that you will typically use, whose values are
 % determined by the choice of options when the package is invoked.
 %
-% \subsection{Naming Convention}
+% \subsubsection{Naming Convention}
 %
 % Each macro starts with a lower case `k' to indicate that it is a constant.
 % If the macro is of special units, e.g. eV, those units will be specified next.
@@ -147,41 +147,136 @@
 %\index{Mass|usage}
 %
 % \DescribeMacro{\kMassElectron}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % \index{Mass>Electron|usage}
 % |\kMassElectron| is the mass of an electron.
 %
 % \DescribeMacro{\keVMassElectron}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % \index{Mass>Electron>in eV|usage}
 % |\keVMassElectron| is the mass of an electron.
 %
+% \DescribeMacro{\kMassElectronNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% \index{Mass>Electron|usage}
+% |\kMassElectronNumeric| is the numeric value of
+%  the mass of an electron.
+%
+% \DescribeMacro{\keVMassElectronNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% \index{Mass>Electron>in eV|usage}
+% |\keVMassElectronNumeric| is the numeric value of
+%  the mass of an electron.
+%
 % \DescribeMacro{\kMassProton}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % \index{Mass>Proton|usage}
 % |\kMassProton| is the mass of a proton.
 %
 % \DescribeMacro{\keVMassProton}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % \index{Mass>Proton>in eV|usage}
 % |\keVMassProton| is the mass of a proton.
 %
+% \DescribeMacro{\kMassProtonNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% \index{Mass>Proton|usage}
+% |\kMassProtonNumeric| is the numeric value of
+%  the mass of a proton.
+%
+% \DescribeMacro{\keVMassProtonNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% \index{Mass>Proton>in eV|usage}
+% |\keVMassProtonNumeric| is the numeric value of
+%  the mass of a proton.
+%
 % \DescribeMacro{\kMassHydrogen}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % \index{Mass>Hydrogen atom|usage}
 % |\kMassHydrogen| is the mass of a neutral hydrogen atom.
 %
 % \DescribeMacro{\keVMassHydrogen}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % \index{Mass>Hydrogen atom>in eV|usage}
 % |\keVMassHydrogen| is the mass of a neutral hydrogen atom.
 %
+% \DescribeMacro{\kMassHydrogenNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% \index{Mass>Hydrogen atom|usage}
+% |\kMassHydrogenNumeric| is the numeric value of
+%  the mass of a neutral hydrogen atom.
+%
+% \DescribeMacro{\keVMassHydrogenNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% \index{Mass>Hydrogen atom>in eV|usage}
+% |\keVMassHydrogenNumeric| is the numeric value of
+%  the mass of a neutral hydrogen atom.
+%
 % \DescribeMacro{\kMassSun}
 % \index{Mass>Sun|usage}
 % |\kMassSun| is the mass of the Sun.
 %
+% \DescribeMacro{\kMassSunNumeric}
+% \index{Mass>Sun|usage}
+% |\kMassSunNumeric| is the numeric value of
+%  the mass of the Sun.
+%
+% \DescribeMacro{\kMassEarth}
+% \changes{v1.1.0}{2020/02/03}{Add mass of Earth}
+% |\kMassEarth| is the mass of the Earth.
+%
+% \DescribeMacro{\kMassEarthNumeric}
+% \changes{v1.1.0}{2020/02/03}{Add mass of Earth}
+% |\kMassEarthNumeric| is the numeric value of
+%  the mass of the Earth.
+%
+% \DescribeMacro{\kMassJupiter}
+% \changes{v1.1.0}{2020/02/03}{Add mass of Jupiter}
+% |\kMassJupiter| is the mass of Jupiter.
+%
+% \DescribeMacro{\kMassJupiterNumeric}
+% \changes{v1.1.0}{2020/02/03}{Add mass of Jupiter}
+% |\kMassJupiterNumeric| is the numeric value of
+%  the mass of Jupiter.
+%
 % \DescribeMacro{\kMassAMU}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % \index{Mass>amu|usage}
 % |\kMassAMU| is the mass of an atomic mass unit.
 %
 % \DescribeMacro{\keVMassAMU}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % \index{Mass>amu>in eV|usage}
 % |\keVMassAMU| is the mass of an atomic mass unit.
 %
+% \DescribeMacro{\kMassAMUNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% \index{Mass>amu|usage}
+% |\kMassAMUNumeric| is the numeric value of
+%  the mass of an atomic mass unit.
+%
+% \DescribeMacro{\keVMassAMUNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% \index{Mass>amu>in eV|usage}
+% |\keVMassAMUNumeric| is the numeric value of
+%  the mass of an atomic mass unit.
+%
 %
 %\subsubsection{Charge}
 %
@@ -192,14 +287,29 @@
 % \index{Charge>Elementary|usage}
 % |\kChargeFundamental| is the fundamental charge.
 %
+% \DescribeMacro{\kChargeFundamentalNumeric}
+% \index{Charge>Elementary|usage}
+% |\kChargeFundamentalNumeric| is the numeric value of
+%  the fundamental charge.
+%
 % \DescribeMacro{\kChargeElectron}
 % \index{Charge>Electron|usage}
 % |\kChargeElectron| is the charge of an electron.
 %
+% \DescribeMacro{\kChargeElectronNumeric}
+% \index{Charge>Electron|usage}
+% |\kChargeElectronNumeric| is the numeric value of
+%  the charge of an electron.
+%
 % \DescribeMacro{\kChargeProton}
 % \index{Charge>Proton|usage}
 % |\kChargeProton| is the charge of a proton.
 %
+% \DescribeMacro{\kChargeProtonNumeric}
+% \index{Charge>Proton|usage}
+% |\kChargeProtonNumeric| is the numeric value of
+%  the charge of a proton.
+%
 %
 %\subsubsection{Distances and Lengths}
 %
@@ -210,19 +320,58 @@
 % \index{Distances and Lengths>Bohr Radius|usage}
 % |\kRadiusBohr| is Bohr radius of an atom.
 %
+% \DescribeMacro{\kRadiusBohrNumeric}
+% \index{Distances and Lengths>Bohr Radius|usage}
+% |\kRadiusBohrNumeric| is the numeric value of
+%  Bohr radius of an atom.
+%
 % \DescribeMacro{\kAstronomicalUnit}
 % \index{Distances and Lengths>Astronomical Unit|usage}
 % |\kAstronomicalUnit| is the astronomical unit (the average distance between
 % the Earth and the Sun).
 %
+% \DescribeMacro{\kAstronomicalUnitNumeric}
+% \index{Distances and Lengths>Astronomical Unit|usage}
+% |\kAstronomicalUnitNumeric| is the numeric value of
+%  the astronomical unit (the average distance between the
+% Earth and the Sun).
+%
 % \DescribeMacro{\kParsec}
 % \index{Distances and Lengths>Parsec|usage}
 % |\kParsec| is the length of a parsec ($\frac{648000\au}{\pi}$).
 %
+% \DescribeMacro{\kParsecNumeric}
+% \index{Distances and Lengths>Parsec|usage}
+% |\kParsecNumeric| is the numeric value of
+%  the length of a parsec ($\frac{648000\au}{\pi}$).
+%
 % \DescribeMacro{\kRadiusSun}
 % \index{Distances and Lengths>Solar Radius|usage}
 % |\kRadiusSun| is the mean radius of the Sun.
 %
+% \DescribeMacro{\kRadiusSunNumeric}
+% \index{Distances and Lengths>Solar Radius|usage}
+% |\kRadiusSunNumeric| is the numeric value of
+%  the mean radius of the Sun.
+%
+% \DescribeMacro{\kRadiusEarth}
+% \changes{v1.1.0}{2020/02/03}{Add radius of Earth}
+% |\kRadiusEarth| is the mean radius of the Earth.
+%
+% \DescribeMacro{\kRadiusEarthNumeric}
+% \changes{v1.1.0}{2020/02/03}{Add radius of Earth}
+% |\kRadiusEarthNumeric| is the numeric value of
+%  the mean radius of the Earth.
+%
+% \DescribeMacro{\kRadiusJupiter}
+% \changes{v1.1.0}{2020/02/03}{Add radius of Jupiter}
+% |\kRadiusJupiter| is the mean radius of Jupiter.
+%
+% \DescribeMacro{\kRadiusJupiterNumeric}
+% \changes{v1.1.0}{2020/02/03}{Add radius of Jupiter}
+% |\kRadiusJupiterNumeric| is the numeric value of
+%  the mean radius of Jupiter.
+%
 %
 %\subsubsection{Energy, Power, and Luminosity}
 %
@@ -237,10 +386,25 @@
 % \index{Energy, Power, and Luminosity>Rydberg>in eV|usage}
 % |\keVRydberg| is the Rydberg energy (the binding energy of Hydrogen).
 %
+% \DescribeMacro{\kRydbergNumeric}
+% \index{Energy, Power, and Luminosity>Rydberg|usage}
+% |\kRydbergNumeric| is the numeric value of
+%  the Rydberg energy (the binding energy of Hydrogen).
+%
+% \DescribeMacro{\keVRydbergNumeric}
+% \index{Energy, Power, and Luminosity>Rydberg>in eV|usage}
+% |\keVRydbergNumeric| is the numeric value of
+%  the Rydberg energy (the binding energy of Hydrogen).
+%
 % \DescribeMacro{\kLuminositySun}
 % \index{Energy, Power, and Luminosity>Solar Luminosity|usage}
 % |\kLuminositySun| is the luminosity of the Sun.
 %
+% \DescribeMacro{\kLuminositySunNumeric}
+% \index{Energy, Power, and Luminosity>Solar Luminosity|usage}
+% |\kLuminositySunNumeric| is the numeric value of
+%  the luminosity of the Sun.
+%
 %
 %\subsubsection{Pressure}
 %
@@ -248,13 +412,27 @@
 %\index{Pressure|usage}
 %
 % \DescribeMacro{\kPressureAtmosphere}
+% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.}
 % \index{Pressure>Standard Atmosphere|usage}
 % |\kPressureAtmosphere| is the standard atmospheric pressure.
 %
+% \DescribeMacro{\kPressureAtmosphereNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.}
+% \index{Pressure>Standard Atmosphere|usage}
+% |\kPressureAtmosphereNumeric| is the numeric value of
+%  the standard atmospheric pressure.
+%
 % \DescribeMacro{\kPressureStandard}
+% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.}
 % \index{Pressure>Standard Pressure|usage}
 % |\kPressureStandard| is the standard atmospheric pressure.
 %
+% \DescribeMacro{\kPressureStandardNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.}
+% \index{Pressure>Standard Pressure|usage}
+% |\kPressureStandardNumeric| is the numeric value of
+%  the standard atmospheric pressure.
+%
 %
 %\subsubsection{Velocity, Speed and Acceleration}
 %
@@ -265,11 +443,25 @@
 % \index{Velocity, Speed and Acceleration>Speed of Light|usage}
 % |\kSpeedLight| is the speed of light.
 %
+% \DescribeMacro{\kSpeedLightNumeric}
+% \index{Velocity, Speed and Acceleration>Speed of Light|usage}
+% |\kSpeedLightNumeric| is the numeric value of
+%  the speed of light.
+%
 % \DescribeMacro{\kAccelGravity}
+% \changes{v1.1.0}{2020/02/03}{Correct value.}
+% \changes{v1.1.0}{2020/02/03}{Fix units.}
 % \index{Velocity, Speed and Acceleration>Acceleration due to Gravity|usage}
 % |\kAccelGravity| is the accelertion due to gravity at the surface of the
 % Earth.
 %
+% \DescribeMacro{\kAccelGravityNumeric}
+% \changes{v1.1.0}{2020/02/03}{Correct value.}
+% \changes{v1.1.0}{2020/02/03}{Fix units.}
+% \index{Velocity, Speed and Acceleration>Acceleration due to Gravity|usage}
+% |\kAccelGravityNumeric| is the numeric value of
+%  the accelertion due to gravity at the surface of the Earth.
+%
 %
 %\subsubsection{Other Constants}
 %
@@ -277,21 +469,45 @@
 %\index{Other Constants|usage}
 %
 % \DescribeMacro{\kCoulomb}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
 % \index{Other Constants>Coulomb Constant|usage}
 % |\kCoulomb| is the Coulomb constant ($\frac{1}{4\pi\epsilon_0}$).
 %
+% \DescribeMacro{\kCoulombNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \index{Other Constants>Coulomb Constant|usage}
+% |\kCoulombNumeric| is the numeric value of
+%  the Coulomb constant ($\frac{1}{4\pi\epsilon_0}$).
+%
 % \DescribeMacro{\kVacuumPermittivity}
 % \index{Other Constants>Vacuum Permittivity|usage}
 % |\kVacuumPermittivity| is the electric permittivity of the vacuum.
 %
+% \DescribeMacro{\kVacuumPermittivityNumeric}
+% \index{Other Constants>Vacuum Permittivity|usage}
+% |\kVacuumPermittivityNumeric| is the numeric value of
+%  the electric permittivity of the vacuum.
+%
 % \DescribeMacro{\kVacuumPermeability}
+% \changes{v1.1.0}{2020/02/03}{Fix value of constant.}
 % \index{Other Constants>Vacuum Permeability|usage}
 % |\kVacuumPermeability| is the magnetic permeability of the vacuum.
 %
+% \DescribeMacro{\kVacuumPermeabilityNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix value of constant.}
+% \index{Other Constants>Vacuum Permeability|usage}
+% |\kVacuumPermeabilityNumeric| is the numeric value of
+%  the magnetic permeability of the vacuum.
+%
 % \DescribeMacro{\kVacuumImpedance}
 % \index{Other Constants>Vacuum Impedance|usage}
 % |\kVacuumImpedance| is the characteristic impedance of the vacuum.
 %
+% \DescribeMacro{\kVacuumImpedanceNumeric}
+% \index{Other Constants>Vacuum Impedance|usage}
+% |\kVacuumImpedanceNumeric| is the numeric value of
+%  the characteristic impedance of the vacuum.
+%
 % \DescribeMacro{\kBoltzmann}
 % \index{Other Constants>Boltzmann|usage}
 % |\kBoltzmann| is the Boltzmann constant.
@@ -300,50 +516,124 @@
 % \index{Other Constants>Boltzmann>in eV|usage}
 % |\keVBoltzmann| is the Boltzmann constant.
 %
+% \DescribeMacro{\kBoltzmannNumeric}
+% \index{Other Constants>Boltzmann|usage}
+% |\kBoltzmannNumeric| is the numeric value of
+%  the Boltzmann constant.
+%
+% \DescribeMacro{\keVBoltzmannNumeric}
+% \index{Other Constants>Boltzmann>in eV|usage}
+% |\keVBoltzmannNumeric| is the numeric value of
+%  the Boltzmann constant.
+%
 % \DescribeMacro{\kPlanck}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
 % \index{Other Constants>Planck|usage}
 % |\kPlanck| is the Planck constant.
 %
 % \DescribeMacro{\keVPlanck}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
 % \index{Other Constants>Planck>in eV|usage}
 % |\keVPlanck| is the Planck constant.
 %
+% \DescribeMacro{\kPlanckNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \index{Other Constants>Planck|usage}
+% |\kPlanckNumeric| is the numeric value of
+%  the Planck constant.
+%
+% \DescribeMacro{\keVPlanckNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \index{Other Constants>Planck>in eV|usage}
+% |\keVPlanckNumeric| is the numeric value of
+%  the Planck constant.
+%
 % \DescribeMacro{\kPlanckReduced}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
 % \index{Other Constants>Reduced Planck|usage}
 % |\kPlanckReduced| is the Reduced Planck constant
 % $\left(\frac{h}{2\pi}\right)$.
 %
 % \DescribeMacro{\keVPlanckReduced}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
 % \index{Other Constants>Reduced Planck>in eV|usage}
 % |\keVPlanckReduced| is the Reduced Planck constant
 % $\left(\frac{h}{2\pi}\right)$.
 %
+% \DescribeMacro{\kPlanckReducedNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \index{Other Constants>Reduced Planck|usage}
+% |\kPlanckReducedNumeric| is the numeric value of
+%  the Reduced Planck constant $\left(\frac{h}{2\pi}\right)$.
+%
+% \DescribeMacro{\keVPlanckReducedNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \index{Other Constants>Reduced Planck>in eV|usage}
+% |\keVPlanckReducedNumeric| is the numeric value of
+%  the Reduced Planck constant $\left(\frac{h}{2\pi}\right)$.
+%
 % \DescribeMacro{\kGravity}
+% \changes{v1.1.0}{2020/02/03}{Fix value of constant.}
 % \index{Other Constants>Newton's Gravitational Constant|usage}
 % |\kGravity| is Newton's gravitational constant.
 %
+% \DescribeMacro{\kGravityNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix value of constant.}
+% \index{Other Constants>Newton's Gravitational Constant|usage}
+% |\kGravityNumeric| is the numeric value of
+%  Newton's gravitational constant.
+%
 % \DescribeMacro{\kStefanBoltzmann}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
 % \index{Other Constants>Stefan-Boltzmann|usage}
 % |\kStefanBoltzmann| is the Stefan-Boltzmann blackbody constant
 % $\left(\frac{2\pi^5k_\mathrm{B}}{15h^3c^2}\right)$.
 %
+% \DescribeMacro{\kStefanBoltzmannNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \index{Other Constants>Stefan-Boltzmann|usage}
+% |\kStefanBoltzmannNumeric| is the numeric value of
+%  the Stefan-Boltzmann blackbody constant
+% $\left(\frac{2\pi^5k_\mathrm{B}}{15h^3c^2}\right)$.
+%
 % \DescribeMacro{\kRadiation}
 % \index{Other Constants>Radiation|usage}
 % |\kRadiation| is the radiation constant, $a
 % \left(\frac{8\pi^5k_\mathrm{B}^4}{15c^3h^3}\right)$.
 %
+% \DescribeMacro{\kRadiationNumeric}
+% \index{Other Constants>Radiation|usage}
+% |\kRadiationNumeric| is the numeric value of
+%  the radiation constant, $a
+% \left(\frac{8\pi^5k_\mathrm{B}^4}{15c^3h^3}\right)$.
+%
 % \DescribeMacro{\kFineStructure}
 % \index{Other Constants>Fine Structure|usage}
 % |\kFineStructure| is the fine structure constant.
 %
+% \DescribeMacro{\kFineStructureNumeric}
+% \index{Other Constants>Fine Structure|usage}
+% |\kFineStructureNumeric| is the numeric value of
+%  the fine structure constant.
+%
 % \DescribeMacro{\kFineStructureReciprocal}
 % \index{Other Constants>Fine Structure>Reciprocal|usage}
 % |\kFineStructureReciprocal| is the reciprocal of the fine structure constant.
 %
+% \DescribeMacro{\kFineStructureReciprocalNumeric}
+% \index{Other Constants>Fine Structure>Reciprocal|usage}
+% |\kFineStructureReciprocalNumeric| is the numeric value of
+%  the reciprocal of the fine structure constant.
+%
 % \DescribeMacro{\kAvogadro}
 % \index{Other Constants>Avogadro's Number|usage}
 % |\kAvogadro| is Avogadro's Number (the number of particles in a mole).
 %
+% \DescribeMacro{\kAvogadroNumeric}
+% \index{Other Constants>Avogadro's Number|usage}
+% |\kAvogadroNumeric| is the numeric value of
+%  Avogadro's Number (the number of particles in a mole).
+%
 %
 %\subsection{Detailed Macros}
 %
@@ -353,7 +643,7 @@
 % by physconst to define the macros that are normally used (those described
 % above.
 %
-% \subsection{NamingConvention}
+% \subsubsection{NamingConvention}
 % The detailed macros are named like \k@units@precision@name. The units
 % specify which units the constant is in (SI, cgs, or eV). For constants that
 % are independent of the unit system (e.g. Avogadro's number and the fine
@@ -366,6 +656,8 @@
 %\subsubsection{Mass}
 %
 % \DescribeMacro{\k@SI@short@MassElectron}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % |\k@SI@short@MassElectron| is the mass of an electron in SI units with
 % reduced precision.
 % (CODATA~2018)
@@ -382,6 +674,8 @@
 % \makeatother
 %
 % \DescribeMacro{\k@SI@full@MassElectron}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % |\k@SI@full@MassElectron| is the mass of an electron in SI units with full
 % precision.
 % (CODATA~2018)
@@ -398,6 +692,8 @@
 % \makeatother
 %
 % \DescribeMacro{\k@cgs@short@MassElectron}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % |\k@cgs@short@MassElectron| is the mass of an electron in cgs units with
 % reduced precision.
 % (CODATA~2018)
@@ -414,6 +710,8 @@
 % \makeatother
 %
 % \DescribeMacro{\k@cgs@full@MassElectron}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % |\k@cgs@full@MassElectron| is the mass of an electron in cgs units with full
 % precision.
 % (CODATA~2018)
@@ -430,6 +728,8 @@
 % \makeatother
 %
 % \DescribeMacro{\k@eV@short@MassElectron}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % |\k@eV@short@MassElectron| is the mass of an electron in eV with reduced
 % precision.
 % (CODATA~2018)
@@ -446,6 +746,8 @@
 % \makeatother
 %
 % \DescribeMacro{\k@eV@full@MassElectron}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % |\k@eV@full@MassElectron| is the mass of an electron in eV with full
 % precision.
 % (CODATA~2018)
@@ -461,7 +763,121 @@
 % {The value is \k@eV@full@MassElectron}\end{mdframed}
 % \makeatother
 %
+% \DescribeMacro{\k@SI@short@MassElectronNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% |\k@SI@short@MassElectronNumeric| is a mathematical value of
+%  the mass of an electron in SI units with reduced
+% precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@SI@short@MassElectronNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@SI@short@MassElectronNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@SI@full@MassElectronNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% |\k@SI@full@MassElectronNumeric| is a mathematical value of
+%  the mass of an electron in SI units with full
+% precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@SI@full@MassElectronNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@SI@full@MassElectronNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@cgs@short@MassElectronNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% |\k@cgs@short@MassElectronNumeric| is a mathematical value of
+%  the mass of an electron in cgs units with reduced
+% precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@cgs@short@MassElectronNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@cgs@short@MassElectronNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@cgs@full@MassElectronNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% |\k@cgs@full@MassElectronNumeric| is a mathematical value of
+%  the mass of an electron in cgs units with full
+% precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@cgs@full@MassElectronNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@cgs@full@MassElectronNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@eV@short@MassElectronNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% |\k@eV@short@MassElectronNumeric| is a mathematical value of
+%  the mass of an electron in eV with reduced precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@eV@short@MassElectronNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@eV@short@MassElectronNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@eV@full@MassElectronNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% |\k@eV@full@MassElectronNumeric| is a mathematical value of
+%  the mass of an electron in eV with full precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@eV@full@MassElectronNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@eV@full@MassElectronNumeric}\end{mdframed}
+% \makeatother
+%
 % \DescribeMacro{\k@SI@short@MassProton}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % |\k@SI@short@MassProton| is the mass of a proton in SI units with reduced
 % precision.
 % (CODATA~2018)
@@ -478,6 +894,8 @@
 % \makeatother
 %
 % \DescribeMacro{\k@SI@full@MassProton}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % |\k@SI@full@MassProton| is the mass of a proton in SI units with full
 % precision.
 % (CODATA~2018)
@@ -494,6 +912,8 @@
 % \makeatother
 %
 % \DescribeMacro{\k@cgs@short@MassProton}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % |\k@cgs@short@MassProton| is the mass of a proton in cgs units with reduced
 % precision.
 % (CODATA~2018)
@@ -510,6 +930,8 @@
 % \makeatother
 %
 % \DescribeMacro{\k@cgs@full@MassProton}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % |\k@cgs@full@MassProton| is the mass of a proton in cgs units with full
 % precision.
 % (CODATA~2018)
@@ -526,6 +948,8 @@
 % \makeatother
 %
 % \DescribeMacro{\k@eV@short@MassProton}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % |\k@eV@short@MassProton| is the mass of a proton in eV with reduced precision.
 % (CODATA~2018)
 %
@@ -541,6 +965,8 @@
 % \makeatother
 %
 % \DescribeMacro{\k@eV@full@MassProton}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % |\k@eV@full@MassProton| is the mass of a proton in eV with full precision.
 % (CODATA~2018)
 %
@@ -555,7 +981,119 @@
 % {The value is \k@eV@full@MassProton}\end{mdframed}
 % \makeatother
 %
+% \DescribeMacro{\k@SI@short@MassProtonNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% |\k@SI@short@MassProtonNumeric| is a mathematical value of
+%  the mass of a proton in SI units with reduced
+% precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@SI@short@MassProtonNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@SI@short@MassProtonNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@SI@full@MassProtonNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% |\k@SI@full@MassProtonNumeric| is a mathematical value of
+%  the mass of a proton in SI units with full precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@SI@full@MassProtonNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@SI@full@MassProtonNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@cgs@short@MassProtonNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% |\k@cgs@short@MassProtonNumeric| is a mathematical value of
+%  the mass of a proton in cgs units with reduced
+% precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@cgs@short@MassProtonNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@cgs@short@MassProtonNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@cgs@full@MassProtonNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% |\k@cgs@full@MassProtonNumeric| is a mathematical value of
+%  the mass of a proton in cgs units with full precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@cgs@full@MassProtonNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@cgs@full@MassProtonNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@eV@short@MassProtonNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% |\k@eV@short@MassProtonNumeric| is a mathematical value of
+%  the mass of a proton in eV with reduced precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@eV@short@MassProtonNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@eV@short@MassProtonNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@eV@full@MassProtonNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% |\k@eV@full@MassProtonNumeric| is a mathematical value of
+%  the mass of a proton in eV with full precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@eV@full@MassProtonNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@eV@full@MassProtonNumeric}\end{mdframed}
+% \makeatother
+%
 % \DescribeMacro{\k@SI@short@MassHydrogen}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % |\k@SI@short@MassHydrogen| is the mass of a neutral hydrogen atom in SI units
 % with reduced precision.
 % (CODATA~2018)
@@ -572,6 +1110,8 @@
 % \makeatother
 %
 % \DescribeMacro{\k@SI@full@MassHydrogen}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % |\k@SI@full@MassHydrogen| is the mass of a neutral hydrogen atom in SI units
 % with full precision.
 % (CODATA~2018)
@@ -588,6 +1128,8 @@
 % \makeatother
 %
 % \DescribeMacro{\k@cgs@short@MassHydrogen}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % |\k@cgs@short@MassHydrogen| is the mass of a neutral hydrogen atom in cgs
 % units with reduced precision.
 % (CODATA~2018)
@@ -604,6 +1146,8 @@
 % \makeatother
 %
 % \DescribeMacro{\k@cgs@full@MassHydrogen}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % |\k@cgs@full@MassHydrogen| is the mass of a neutral hydrogen atom in cgs
 % units with full precision.
 % (CODATA~2018)
@@ -620,6 +1164,8 @@
 % \makeatother
 %
 % \DescribeMacro{\k@eV@short@MassHydrogen}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % |\k@eV@short@MassHydrogen| is the mass of a neutral hydrogen atom in eV with
 % reduced precision.
 % (CODATA~2018)
@@ -636,6 +1182,8 @@
 % \makeatother
 %
 % \DescribeMacro{\k@eV@full@MassHydrogen}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % |\k@eV@full@MassHydrogen| is the mass of a neutral hydrogen atom in eV with
 % full precision.
 % (CODATA~2018)
@@ -651,6 +1199,120 @@
 % {The value is \k@eV@full@MassHydrogen}\end{mdframed}
 % \makeatother
 %
+% \DescribeMacro{\k@SI@short@MassHydrogenNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% |\k@SI@short@MassHydrogenNumeric| is a mathematical value of
+%  the mass of a neutral hydrogen atom in SI units with
+% reduced precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@SI@short@MassHydrogenNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@SI@short@MassHydrogenNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@SI@full@MassHydrogenNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% |\k@SI@full@MassHydrogenNumeric| is a mathematical value of
+%  the mass of a neutral hydrogen atom in SI units with
+% full precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@SI@full@MassHydrogenNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@SI@full@MassHydrogenNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@cgs@short@MassHydrogenNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% |\k@cgs@short@MassHydrogenNumeric| is a mathematical value of
+%  the mass of a neutral hydrogen atom in cgs units
+% with reduced precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@cgs@short@MassHydrogenNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@cgs@short@MassHydrogenNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@cgs@full@MassHydrogenNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% |\k@cgs@full@MassHydrogenNumeric| is a mathematical value of
+%  the mass of a neutral hydrogen atom in cgs units
+% with full precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@cgs@full@MassHydrogenNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@cgs@full@MassHydrogenNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@eV@short@MassHydrogenNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% |\k@eV@short@MassHydrogenNumeric| is a mathematical value of
+%  the mass of a neutral hydrogen atom in eV with
+% reduced precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@eV@short@MassHydrogenNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@eV@short@MassHydrogenNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@eV@full@MassHydrogenNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% |\k@eV@full@MassHydrogenNumeric| is a mathematical value of
+%  the mass of a neutral hydrogen atom in eV with full
+% precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@eV@full@MassHydrogenNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@eV@full@MassHydrogenNumeric}\end{mdframed}
+% \makeatother
+%
 % \DescribeMacro{\k@SI@short@MassSun}
 % |\k@SI@short@MassSun| is the mass of the Sun in SI units with reduced
 % precision.
@@ -713,7 +1375,205 @@
 % {The value is \k@cgs@full@MassSun}\end{mdframed}
 % \makeatother
 %
+% \DescribeMacro{\k@SI@short@MassSunNumeric}
+% |\k@SI@short@MassSunNumeric| is a mathematical value of
+%  the mass of the Sun in SI units with reduced precision.
+% (IAU~Resolution~B3~2015)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@SI@short@MassSunNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@SI@short@MassSunNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@SI@full@MassSunNumeric}
+% |\k@SI@full@MassSunNumeric| is a mathematical value of
+%  the mass of the Sun in SI units with full precision.
+% (IAU~Resolution~B3~2015)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@SI@full@MassSunNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@SI@full@MassSunNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@cgs@short@MassSunNumeric}
+% |\k@cgs@short@MassSunNumeric| is a mathematical value of
+%  the mass of the Sun in cgs units with reduced precision.
+% (IAU~Resolution~B3~2015)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@cgs@short@MassSunNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@cgs@short@MassSunNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@cgs@full@MassSunNumeric}
+% |\k@cgs@full@MassSunNumeric| is a mathematical value of
+%  the mass of the Sun in cgs units with full precision.
+% (IAU~Resolution~B3~2015)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@cgs@full@MassSunNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@cgs@full@MassSunNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@short@MassEarth}
+% \changes{v1.1.0}{2020/02/03}{Add mass of Earth}
+% |\k@short@MassEarth| is the mass of the Earth with reduced precision.
+% (IAU~Resolution~B3~2015)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@short@MassEarth\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@short@MassEarth}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@full@MassEarth}
+% \changes{v1.1.0}{2020/02/03}{Add mass of Earth}
+% |\k@full@MassEarth| is the mass of the Earth with full precision.
+% (IAU~Resolution~B3~2015)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@full@MassEarth\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@full@MassEarth}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@short@MassEarthNumeric}
+% \changes{v1.1.0}{2020/02/03}{Add mass of Earth}
+% |\k@short@MassEarthNumeric| is a mathematical value of
+%  the mass of the Earth with reduced precision.
+% (IAU~Resolution~B3~2015)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@short@MassEarthNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@short@MassEarthNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@full@MassEarthNumeric}
+% \changes{v1.1.0}{2020/02/03}{Add mass of Earth}
+% |\k@full@MassEarthNumeric| is a mathematical value of
+%  the mass of the Earth with full precision.
+% (IAU~Resolution~B3~2015)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@full@MassEarthNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@full@MassEarthNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@short@MassJupiter}
+% \changes{v1.1.0}{2020/02/03}{Add mass of Jupiter}
+% |\k@short@MassJupiter| is the mass of Jupiter with reduced precision.
+% (IAU~Resolution~B3~2015)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@short@MassJupiter\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@short@MassJupiter}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@full@MassJupiter}
+% \changes{v1.1.0}{2020/02/03}{Add mass of Jupiter}
+% |\k@full@MassJupiter| is the mass of Jupiter with full precision.
+% (IAU~Resolution~B3~2015)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@full@MassJupiter\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@full@MassJupiter}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@short@MassJupiterNumeric}
+% \changes{v1.1.0}{2020/02/03}{Add mass of Jupiter}
+% |\k@short@MassJupiterNumeric| is a mathematical value of
+%  the mass of Jupiter with reduced precision.
+% (IAU~Resolution~B3~2015)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@short@MassJupiterNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@short@MassJupiterNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@full@MassJupiterNumeric}
+% \changes{v1.1.0}{2020/02/03}{Add mass of Jupiter}
+% |\k@full@MassJupiterNumeric| is a mathematical value of
+%  the mass of Jupiter with full precision.
+% (IAU~Resolution~B3~2015)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@full@MassJupiterNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@full@MassJupiterNumeric}\end{mdframed}
+% \makeatother
+%
 % \DescribeMacro{\k@SI@short@MassAMU}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % |\k@SI@short@MassAMU| is the mass of an atomic mass unit in SI units with
 % reduced precision.
 % (CODATA~2018)
@@ -730,6 +1590,8 @@
 % \makeatother
 %
 % \DescribeMacro{\k@SI@full@MassAMU}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % |\k@SI@full@MassAMU| is the mass of an atomic mass unit in SI units with full
 % precision.
 % (CODATA~2018)
@@ -746,6 +1608,8 @@
 % \makeatother
 %
 % \DescribeMacro{\k@cgs@short@MassAMU}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % |\k@cgs@short@MassAMU| is the mass of an atomic mass unit in cgs units with
 % reduced precision.
 % (CODATA~2018)
@@ -762,6 +1626,8 @@
 % \makeatother
 %
 % \DescribeMacro{\k@cgs@full@MassAMU}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % |\k@cgs@full@MassAMU| is the mass of an atomic mass unit in cgs units with
 % full precision.
 % (CODATA~2018)
@@ -778,6 +1644,8 @@
 % \makeatother
 %
 % \DescribeMacro{\k@eV@short@MassAMU}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % |\k@eV@short@MassAMU| is the mass of an atomic mass unit in eV with reduced
 % precision.
 % (CODATA~2018)
@@ -794,6 +1662,8 @@
 % \makeatother
 %
 % \DescribeMacro{\k@eV@full@MassAMU}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % |\k@eV@full@MassAMU| is the mass of an atomic mass unit in eV with full
 % precision.
 % (CODATA~2018)
@@ -809,6 +1679,119 @@
 % {The value is \k@eV@full@MassAMU}\end{mdframed}
 % \makeatother
 %
+% \DescribeMacro{\k@SI@short@MassAMUNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% |\k@SI@short@MassAMUNumeric| is a mathematical value of
+%  the mass of an atomic mass unit in SI units with reduced
+% precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@SI@short@MassAMUNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@SI@short@MassAMUNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@SI@full@MassAMUNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% |\k@SI@full@MassAMUNumeric| is a mathematical value of
+%  the mass of an atomic mass unit in SI units with full
+% precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@SI@full@MassAMUNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@SI@full@MassAMUNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@cgs@short@MassAMUNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% |\k@cgs@short@MassAMUNumeric| is a mathematical value of
+%  the mass of an atomic mass unit in cgs units with
+% reduced precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@cgs@short@MassAMUNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@cgs@short@MassAMUNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@cgs@full@MassAMUNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% |\k@cgs@full@MassAMUNumeric| is a mathematical value of
+%  the mass of an atomic mass unit in cgs units with full
+% precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@cgs@full@MassAMUNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@cgs@full@MassAMUNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@eV@short@MassAMUNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% |\k@eV@short@MassAMUNumeric| is a mathematical value of
+%  the mass of an atomic mass unit in eV with reduced
+% precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@eV@short@MassAMUNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@eV@short@MassAMUNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@eV@full@MassAMUNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% |\k@eV@full@MassAMUNumeric| is a mathematical value of
+%  the mass of an atomic mass unit in eV with full precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@eV@full@MassAMUNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@eV@full@MassAMUNumeric}\end{mdframed}
+% \makeatother
+%
 %
 %\subsubsection{Charge}
 %
@@ -876,6 +1859,74 @@
 % {The value is \k@cgs@full@ChargeFundamental}\end{mdframed}
 % \makeatother
 %
+% \DescribeMacro{\k@SI@short@ChargeFundamentalNumeric}
+% |\k@SI@short@ChargeFundamentalNumeric| is a mathematical value of
+%  the fundamental charge in SI units with reduced
+% precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@SI@short@ChargeFundamentalNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@SI@short@ChargeFundamentalNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@SI@full@ChargeFundamentalNumeric}
+% |\k@SI@full@ChargeFundamentalNumeric| is a mathematical value of
+%  the fundamental charge in SI units with full
+% precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@SI@full@ChargeFundamentalNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@SI@full@ChargeFundamentalNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@cgs@short@ChargeFundamentalNumeric}
+% |\k@cgs@short@ChargeFundamentalNumeric| is a mathematical value of
+%  the fundamental charge in cgs units with
+% reduced precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@cgs@short@ChargeFundamentalNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@cgs@short@ChargeFundamentalNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@cgs@full@ChargeFundamentalNumeric}
+% |\k@cgs@full@ChargeFundamentalNumeric| is a mathematical value of
+%  the fundamental charge in cgs units with full
+% precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@cgs@full@ChargeFundamentalNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@cgs@full@ChargeFundamentalNumeric}\end{mdframed}
+% \makeatother
+%
 % \DescribeMacro{\k@SI@short@ChargeElectron}
 % |\k@SI@short@ChargeElectron| is the charge of an electron in SI units with
 % reduced precision.
@@ -940,6 +1991,74 @@
 % {The value is \k@cgs@full@ChargeElectron}\end{mdframed}
 % \makeatother
 %
+% \DescribeMacro{\k@SI@short@ChargeElectronNumeric}
+% |\k@SI@short@ChargeElectronNumeric| is a mathematical value of
+%  the charge of an electron in SI units with reduced
+% precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@SI@short@ChargeElectronNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@SI@short@ChargeElectronNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@SI@full@ChargeElectronNumeric}
+% |\k@SI@full@ChargeElectronNumeric| is a mathematical value of
+%  the charge of an electron in SI units with full
+% precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@SI@full@ChargeElectronNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@SI@full@ChargeElectronNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@cgs@short@ChargeElectronNumeric}
+% |\k@cgs@short@ChargeElectronNumeric| is a mathematical value of
+%  the charge of an electron in cgs units with
+% reduced precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@cgs@short@ChargeElectronNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@cgs@short@ChargeElectronNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@cgs@full@ChargeElectronNumeric}
+% |\k@cgs@full@ChargeElectronNumeric| is a mathematical value of
+%  the charge of an electron in cgs units with full
+% precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@cgs@full@ChargeElectronNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@cgs@full@ChargeElectronNumeric}\end{mdframed}
+% \makeatother
+%
 % \DescribeMacro{\k@SI@short@ChargeProton}
 % |\k@SI@short@ChargeProton| is the charge of a proton in SI units with reduced
 % precision.
@@ -1004,6 +2123,74 @@
 % {The value is \k@cgs@full@ChargeProton}\end{mdframed}
 % \makeatother
 %
+% \DescribeMacro{\k@SI@short@ChargeProtonNumeric}
+% |\k@SI@short@ChargeProtonNumeric| is a mathematical value of
+%  the charge of a proton in SI units with reduced
+% precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@SI@short@ChargeProtonNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@SI@short@ChargeProtonNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@SI@full@ChargeProtonNumeric}
+% |\k@SI@full@ChargeProtonNumeric| is a mathematical value of
+%  the charge of a proton in SI units with full
+% precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@SI@full@ChargeProtonNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@SI@full@ChargeProtonNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@cgs@short@ChargeProtonNumeric}
+% |\k@cgs@short@ChargeProtonNumeric| is a mathematical value of
+%  the charge of a proton in cgs units with reduced
+% precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@cgs@short@ChargeProtonNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@cgs@short@ChargeProtonNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@cgs@full@ChargeProtonNumeric}
+% |\k@cgs@full@ChargeProtonNumeric| is a mathematical value of
+%  the charge of a proton in cgs units with full
+% precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@cgs@full@ChargeProtonNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@cgs@full@ChargeProtonNumeric}\end{mdframed}
+% \makeatother
+%
 %
 %\subsubsection{Distances and Lengths}
 %
@@ -1071,6 +2258,73 @@
 % {The value is \k@cgs@full@RadiusBohr}\end{mdframed}
 % \makeatother
 %
+% \DescribeMacro{\k@SI@short@RadiusBohrNumeric}
+% |\k@SI@short@RadiusBohrNumeric| is a mathematical value of
+%  Bohr radius of an atom in SI units with reduced
+% precision.
+% (Calculated)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@SI@short@RadiusBohrNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@SI@short@RadiusBohrNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@SI@full@RadiusBohrNumeric}
+% |\k@SI@full@RadiusBohrNumeric| is a mathematical value of
+%  Bohr radius of an atom in SI units with full precision.
+% (Calculated)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@SI@full@RadiusBohrNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@SI@full@RadiusBohrNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@cgs@short@RadiusBohrNumeric}
+% |\k@cgs@short@RadiusBohrNumeric| is a mathematical value of
+%  Bohr radius of an atom in cgs units with reduced
+% precision.
+% (Calculated)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@cgs@short@RadiusBohrNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@cgs@short@RadiusBohrNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@cgs@full@RadiusBohrNumeric}
+% |\k@cgs@full@RadiusBohrNumeric| is a mathematical value of
+%  Bohr radius of an atom in cgs units with full
+% precision.
+% (Calculated)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@cgs@full@RadiusBohrNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@cgs@full@RadiusBohrNumeric}\end{mdframed}
+% \makeatother
+%
 % \DescribeMacro{\k@SI@short@AstronomicalUnit}
 % |\k@SI@short@AstronomicalUnit| is the astronomical unit (the average distance
 % between the Earth and the Sun) in SI units with reduced precision.
@@ -1135,6 +2389,74 @@
 % {The value is \k@cgs@full@AstronomicalUnit}\end{mdframed}
 % \makeatother
 %
+% \DescribeMacro{\k@SI@short@AstronomicalUnitNumeric}
+% |\k@SI@short@AstronomicalUnitNumeric| is a mathematical value of
+%  the astronomical unit (the average distance
+% between the Earth and the Sun) in SI units with reduced precision.
+% (IAU~Resolution~B2~2012)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@SI@short@AstronomicalUnitNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@SI@short@AstronomicalUnitNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@SI@full@AstronomicalUnitNumeric}
+% |\k@SI@full@AstronomicalUnitNumeric| is a mathematical value of
+%  the astronomical unit (the average distance
+% between the Earth and the Sun) in SI units with full precision.
+% (IAU~Resolution~B2~2012)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@SI@full@AstronomicalUnitNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@SI@full@AstronomicalUnitNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@cgs@short@AstronomicalUnitNumeric}
+% |\k@cgs@short@AstronomicalUnitNumeric| is a mathematical value of
+%  the astronomical unit (the average distance
+% between the Earth and the Sun) in cgs units with reduced precision.
+% (IAU~Resolution~B2~2012)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@cgs@short@AstronomicalUnitNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@cgs@short@AstronomicalUnitNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@cgs@full@AstronomicalUnitNumeric}
+% |\k@cgs@full@AstronomicalUnitNumeric| is a mathematical value of
+%  the astronomical unit (the average distance
+% between the Earth and the Sun) in cgs units with full precision.
+% (IAU~Resolution~B2~2012)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@cgs@full@AstronomicalUnitNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@cgs@full@AstronomicalUnitNumeric}\end{mdframed}
+% \makeatother
+%
 % \DescribeMacro{\k@SI@short@Parsec}
 % |\k@SI@short@Parsec| is the length of a parsec ($\frac{648000\au}{\pi}$) in
 % SI units with reduced precision.
@@ -1199,6 +2521,74 @@
 % {The value is \k@cgs@full@Parsec}\end{mdframed}
 % \makeatother
 %
+% \DescribeMacro{\k@SI@short@ParsecNumeric}
+% |\k@SI@short@ParsecNumeric| is a mathematical value of
+%  the length of a parsec ($\frac{648000\au}{\pi}$) in SI
+% units with reduced precision.
+% (Calculated)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@SI@short@ParsecNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@SI@short@ParsecNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@SI@full@ParsecNumeric}
+% |\k@SI@full@ParsecNumeric| is a mathematical value of
+%  the length of a parsec ($\frac{648000\au}{\pi}$) in SI
+% units with full precision.
+% (Calculated)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@SI@full@ParsecNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@SI@full@ParsecNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@cgs@short@ParsecNumeric}
+% |\k@cgs@short@ParsecNumeric| is a mathematical value of
+%  the length of a parsec ($\frac{648000\au}{\pi}$) in cgs
+% units with reduced precision.
+% (Calculated)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@cgs@short@ParsecNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@cgs@short@ParsecNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@cgs@full@ParsecNumeric}
+% |\k@cgs@full@ParsecNumeric| is a mathematical value of
+%  the length of a parsec ($\frac{648000\au}{\pi}$) in cgs
+% units with full precision.
+% (Calculated)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@cgs@full@ParsecNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@cgs@full@ParsecNumeric}\end{mdframed}
+% \makeatother
+%
 % \DescribeMacro{\k@SI@short@RadiusSun}
 % |\k@SI@short@RadiusSun| is the mean radius of the Sun in SI units with
 % reduced precision.
@@ -1263,6 +2653,206 @@
 % {The value is \k@cgs@full@RadiusSun}\end{mdframed}
 % \makeatother
 %
+% \DescribeMacro{\k@SI@short@RadiusSunNumeric}
+% |\k@SI@short@RadiusSunNumeric| is a mathematical value of
+%  the mean radius of the Sun in SI units with reduced
+% precision.
+% (IAU~Resolution~B3~2015)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@SI@short@RadiusSunNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@SI@short@RadiusSunNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@SI@full@RadiusSunNumeric}
+% |\k@SI@full@RadiusSunNumeric| is a mathematical value of
+%  the mean radius of the Sun in SI units with full
+% precision.
+% (IAU~Resolution~B3~2015)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@SI@full@RadiusSunNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@SI@full@RadiusSunNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@cgs@short@RadiusSunNumeric}
+% |\k@cgs@short@RadiusSunNumeric| is a mathematical value of
+%  the mean radius of the Sun in cgs units with reduced
+% precision.
+% (IAU~Resolution~B3~2015)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@cgs@short@RadiusSunNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@cgs@short@RadiusSunNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@cgs@full@RadiusSunNumeric}
+% |\k@cgs@full@RadiusSunNumeric| is a mathematical value of
+%  the mean radius of the Sun in cgs units with full
+% precision.
+% (IAU~Resolution~B3~2015)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@cgs@full@RadiusSunNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@cgs@full@RadiusSunNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@short@RadiusEarth}
+% \changes{v1.1.0}{2020/02/03}{Add radius of Earth}
+% |\k@short@RadiusEarth| is the mean radius of the Earth with reduced precision.
+% (IAU~Resolution~B3~2015)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@short@RadiusEarth\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@short@RadiusEarth}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@full@RadiusEarth}
+% \changes{v1.1.0}{2020/02/03}{Add radius of Earth}
+% |\k@full@RadiusEarth| is the mean radius of the Earth with full precision.
+% (IAU~Resolution~B3~2015)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@full@RadiusEarth\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@full@RadiusEarth}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@short@RadiusEarthNumeric}
+% \changes{v1.1.0}{2020/02/03}{Add radius of Earth}
+% |\k@short@RadiusEarthNumeric| is a mathematical value of
+%  the mean radius of the Earth with reduced precision.
+% (IAU~Resolution~B3~2015)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@short@RadiusEarthNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@short@RadiusEarthNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@full@RadiusEarthNumeric}
+% \changes{v1.1.0}{2020/02/03}{Add radius of Earth}
+% |\k@full@RadiusEarthNumeric| is a mathematical value of
+%  the mean radius of the Earth with full precision.
+% (IAU~Resolution~B3~2015)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@full@RadiusEarthNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@full@RadiusEarthNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@short@RadiusJupiter}
+% \changes{v1.1.0}{2020/02/03}{Add radius of Jupiter}
+% |\k@short@RadiusJupiter| is the mean radius of Jupiter with reduced precision.
+% (IAU~Resolution~B3~2015)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@short@RadiusJupiter\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@short@RadiusJupiter}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@full@RadiusJupiter}
+% \changes{v1.1.0}{2020/02/03}{Add radius of Jupiter}
+% |\k@full@RadiusJupiter| is the mean radius of Jupiter with full precision.
+% (IAU~Resolution~B3~2015)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@full@RadiusJupiter\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@full@RadiusJupiter}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@short@RadiusJupiterNumeric}
+% \changes{v1.1.0}{2020/02/03}{Add radius of Jupiter}
+% |\k@short@RadiusJupiterNumeric| is a mathematical value of
+%  the mean radius of Jupiter with reduced precision.
+% (IAU~Resolution~B3~2015)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@short@RadiusJupiterNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@short@RadiusJupiterNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@full@RadiusJupiterNumeric}
+% \changes{v1.1.0}{2020/02/03}{Add radius of Jupiter}
+% |\k@full@RadiusJupiterNumeric| is a mathematical value of
+%  the mean radius of Jupiter with full precision.
+% (IAU~Resolution~B3~2015)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@full@RadiusJupiterNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@full@RadiusJupiterNumeric}\end{mdframed}
+% \makeatother
+%
 %
 %\subsubsection{Energy, Power, and Luminosity}
 %
@@ -1362,6 +2952,108 @@
 % {The value is \k@eV@full@Rydberg}\end{mdframed}
 % \makeatother
 %
+% \DescribeMacro{\k@SI@short@RydbergNumeric}
+% |\k@SI@short@RydbergNumeric| is a mathematical value of
+%  the Rydberg energy (the binding energy of Hydrogen) in SI
+% units with reduced precision.
+% (Calculated)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@SI@short@RydbergNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@SI@short@RydbergNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@SI@full@RydbergNumeric}
+% |\k@SI@full@RydbergNumeric| is a mathematical value of
+%  the Rydberg energy (the binding energy of Hydrogen) in SI
+% units with full precision.
+% (Calculated)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@SI@full@RydbergNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@SI@full@RydbergNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@cgs@short@RydbergNumeric}
+% |\k@cgs@short@RydbergNumeric| is a mathematical value of
+%  the Rydberg energy (the binding energy of Hydrogen) in
+% cgs units with reduced precision.
+% (Calculated)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@cgs@short@RydbergNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@cgs@short@RydbergNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@cgs@full@RydbergNumeric}
+% |\k@cgs@full@RydbergNumeric| is a mathematical value of
+%  the Rydberg energy (the binding energy of Hydrogen) in
+% cgs units with full precision.
+% (Calculated)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@cgs@full@RydbergNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@cgs@full@RydbergNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@eV@short@RydbergNumeric}
+% |\k@eV@short@RydbergNumeric| is a mathematical value of
+%  the Rydberg energy (the binding energy of Hydrogen) in eV
+% with reduced precision.
+% (Calculated)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@eV@short@RydbergNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@eV@short@RydbergNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@eV@full@RydbergNumeric}
+% |\k@eV@full@RydbergNumeric| is a mathematical value of
+%  the Rydberg energy (the binding energy of Hydrogen) in eV
+% with full precision.
+% (Calculated)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@eV@full@RydbergNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@eV@full@RydbergNumeric}\end{mdframed}
+% \makeatother
+%
 % \DescribeMacro{\k@SI@short@LuminositySun}
 % |\k@SI@short@LuminositySun| is the luminosity of the Sun in SI units with
 % reduced precision.
@@ -1426,10 +3118,79 @@
 % {The value is \k@cgs@full@LuminositySun}\end{mdframed}
 % \makeatother
 %
+% \DescribeMacro{\k@SI@short@LuminositySunNumeric}
+% |\k@SI@short@LuminositySunNumeric| is a mathematical value of
+%  the luminosity of the Sun in SI units with reduced
+% precision.
+% (IAU~Resolution~B3~2015)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@SI@short@LuminositySunNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@SI@short@LuminositySunNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@SI@full@LuminositySunNumeric}
+% |\k@SI@full@LuminositySunNumeric| is a mathematical value of
+%  the luminosity of the Sun in SI units with full
+% precision.
+% (IAU~Resolution~B3~2015)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@SI@full@LuminositySunNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@SI@full@LuminositySunNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@cgs@short@LuminositySunNumeric}
+% |\k@cgs@short@LuminositySunNumeric| is a mathematical value of
+%  the luminosity of the Sun in cgs units with
+% reduced precision.
+% (IAU~Resolution~B3~2015)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@cgs@short@LuminositySunNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@cgs@short@LuminositySunNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@cgs@full@LuminositySunNumeric}
+% |\k@cgs@full@LuminositySunNumeric| is a mathematical value of
+%  the luminosity of the Sun in cgs units with full
+% precision.
+% (IAU~Resolution~B3~2015)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@cgs@full@LuminositySunNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@cgs@full@LuminositySunNumeric}\end{mdframed}
+% \makeatother
+%
 %
 %\subsubsection{Pressure}
 %
 % \DescribeMacro{\k@SI@short@PressureAtmosphere}
+% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.}
 % |\k@SI@short@PressureAtmosphere| is the standard atmospheric pressure in SI
 % units with reduced precision.
 % (CODATA~2018)
@@ -1446,6 +3207,7 @@
 % \makeatother
 %
 % \DescribeMacro{\k@SI@full@PressureAtmosphere}
+% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.}
 % |\k@SI@full@PressureAtmosphere| is the standard atmospheric pressure in SI
 % units with full precision.
 % (CODATA~2018)
@@ -1462,6 +3224,7 @@
 % \makeatother
 %
 % \DescribeMacro{\k@cgs@short@PressureAtmosphere}
+% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.}
 % |\k@cgs@short@PressureAtmosphere| is the standard atmospheric pressure in cgs
 % units with reduced precision.
 % (CODATA~2018)
@@ -1478,6 +3241,7 @@
 % \makeatother
 %
 % \DescribeMacro{\k@cgs@full@PressureAtmosphere}
+% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.}
 % |\k@cgs@full@PressureAtmosphere| is the standard atmospheric pressure in cgs
 % units with full precision.
 % (CODATA~2018)
@@ -1493,7 +3257,80 @@
 % {The value is \k@cgs@full@PressureAtmosphere}\end{mdframed}
 % \makeatother
 %
+% \DescribeMacro{\k@SI@short@PressureAtmosphereNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.}
+% |\k@SI@short@PressureAtmosphereNumeric| is a mathematical value of
+%  the standard atmospheric pressure in SI units
+% with reduced precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@SI@short@PressureAtmosphereNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@SI@short@PressureAtmosphereNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@SI@full@PressureAtmosphereNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.}
+% |\k@SI@full@PressureAtmosphereNumeric| is a mathematical value of
+%  the standard atmospheric pressure in SI units
+% with full precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@SI@full@PressureAtmosphereNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@SI@full@PressureAtmosphereNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@cgs@short@PressureAtmosphereNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.}
+% |\k@cgs@short@PressureAtmosphereNumeric| is a mathematical value of
+%  the standard atmospheric pressure in cgs
+% units with reduced precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@cgs@short@PressureAtmosphereNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@cgs@short@PressureAtmosphereNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@cgs@full@PressureAtmosphereNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.}
+% |\k@cgs@full@PressureAtmosphereNumeric| is a mathematical value of
+%  the standard atmospheric pressure in cgs units
+% with full precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@cgs@full@PressureAtmosphereNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@cgs@full@PressureAtmosphereNumeric}\end{mdframed}
+% \makeatother
+%
 % \DescribeMacro{\k@SI@short@PressureStandard}
+% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.}
 % |\k@SI@short@PressureStandard| is the standard atmospheric pressure in SI
 % units with reduced precision.
 % (CODATA~2018)
@@ -1510,6 +3347,7 @@
 % \makeatother
 %
 % \DescribeMacro{\k@SI@full@PressureStandard}
+% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.}
 % |\k@SI@full@PressureStandard| is the standard atmospheric pressure in SI
 % units with full precision.
 % (CODATA~2018)
@@ -1526,6 +3364,7 @@
 % \makeatother
 %
 % \DescribeMacro{\k@cgs@short@PressureStandard}
+% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.}
 % |\k@cgs@short@PressureStandard| is the standard atmospheric pressure in cgs
 % units with reduced precision.
 % (CODATA~2018)
@@ -1542,6 +3381,7 @@
 % \makeatother
 %
 % \DescribeMacro{\k@cgs@full@PressureStandard}
+% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.}
 % |\k@cgs@full@PressureStandard| is the standard atmospheric pressure in cgs
 % units with full precision.
 % (CODATA~2018)
@@ -1557,6 +3397,78 @@
 % {The value is \k@cgs@full@PressureStandard}\end{mdframed}
 % \makeatother
 %
+% \DescribeMacro{\k@SI@short@PressureStandardNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.}
+% |\k@SI@short@PressureStandardNumeric| is a mathematical value of
+%  the standard atmospheric pressure in SI units
+% with reduced precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@SI@short@PressureStandardNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@SI@short@PressureStandardNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@SI@full@PressureStandardNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.}
+% |\k@SI@full@PressureStandardNumeric| is a mathematical value of
+%  the standard atmospheric pressure in SI units
+% with full precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@SI@full@PressureStandardNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@SI@full@PressureStandardNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@cgs@short@PressureStandardNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.}
+% |\k@cgs@short@PressureStandardNumeric| is a mathematical value of
+%  the standard atmospheric pressure in cgs units
+% with reduced precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@cgs@short@PressureStandardNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@cgs@short@PressureStandardNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@cgs@full@PressureStandardNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.}
+% |\k@cgs@full@PressureStandardNumeric| is a mathematical value of
+%  the standard atmospheric pressure in cgs units
+% with full precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@cgs@full@PressureStandardNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@cgs@full@PressureStandardNumeric}\end{mdframed}
+% \makeatother
+%
 %
 %\subsubsection{Velocity, Speed and Acceleration}
 %
@@ -1623,7 +3535,74 @@
 % {The value is \k@cgs@full@SpeedLight}\end{mdframed}
 % \makeatother
 %
+% \DescribeMacro{\k@SI@short@SpeedLightNumeric}
+% |\k@SI@short@SpeedLightNumeric| is a mathematical value of
+%  the speed of light in SI units with reduced precision.
+% (CODATA 2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@SI@short@SpeedLightNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@SI@short@SpeedLightNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@SI@full@SpeedLightNumeric}
+% |\k@SI@full@SpeedLightNumeric| is a mathematical value of
+%  the speed of light in SI units with full precision.
+% (CODATA 2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@SI@full@SpeedLightNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@SI@full@SpeedLightNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@cgs@short@SpeedLightNumeric}
+% |\k@cgs@short@SpeedLightNumeric| is a mathematical value of
+%  the speed of light in cgs units with reduced
+% precision.
+% (CODATA 2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@cgs@short@SpeedLightNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@cgs@short@SpeedLightNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@cgs@full@SpeedLightNumeric}
+% |\k@cgs@full@SpeedLightNumeric| is a mathematical value of
+%  the speed of light in cgs units with full precision.
+% (CODATA 2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@cgs@full@SpeedLightNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@cgs@full@SpeedLightNumeric}\end{mdframed}
+% \makeatother
+%
 % \DescribeMacro{\k@SI@short@AccelGravity}
+% \changes{v1.1.0}{2020/02/03}{Correct value.}
+% \changes{v1.1.0}{2020/02/03}{Fix units.}
 % |\k@SI@short@AccelGravity| is the accelertion due to gravity at the surface
 % of the Earth in SI units with reduced precision.
 % (CODATA 2018)
@@ -1640,6 +3619,8 @@
 % \makeatother
 %
 % \DescribeMacro{\k@SI@full@AccelGravity}
+% \changes{v1.1.0}{2020/02/03}{Correct value.}
+% \changes{v1.1.0}{2020/02/03}{Fix units.}
 % |\k@SI@full@AccelGravity| is the accelertion due to gravity at the surface of
 % the Earth in SI units with full precision.
 % (CODATA 2018)
@@ -1656,6 +3637,8 @@
 % \makeatother
 %
 % \DescribeMacro{\k@cgs@short@AccelGravity}
+% \changes{v1.1.0}{2020/02/03}{Correct value.}
+% \changes{v1.1.0}{2020/02/03}{Fix units.}
 % |\k@cgs@short@AccelGravity| is the accelertion due to gravity at the surface
 % of the Earth in cgs units with reduced precision.
 % (CODATA 2018)
@@ -1672,6 +3655,8 @@
 % \makeatother
 %
 % \DescribeMacro{\k@cgs@full@AccelGravity}
+% \changes{v1.1.0}{2020/02/03}{Correct value.}
+% \changes{v1.1.0}{2020/02/03}{Fix units.}
 % |\k@cgs@full@AccelGravity| is the accelertion due to gravity at the surface
 % of the Earth in cgs units with full precision.
 % (CODATA 2018)
@@ -1687,10 +3672,87 @@
 % {The value is \k@cgs@full@AccelGravity}\end{mdframed}
 % \makeatother
 %
+% \DescribeMacro{\k@SI@short@AccelGravityNumeric}
+% \changes{v1.1.0}{2020/02/03}{Correct value.}
+% \changes{v1.1.0}{2020/02/03}{Fix units.}
+% |\k@SI@short@AccelGravityNumeric| is a mathematical value of
+%  the accelertion due to gravity at the surface of the
+% Earth in SI units with reduced precision.
+% (CODATA 2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@SI@short@AccelGravityNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@SI@short@AccelGravityNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@SI@full@AccelGravityNumeric}
+% \changes{v1.1.0}{2020/02/03}{Correct value.}
+% \changes{v1.1.0}{2020/02/03}{Fix units.}
+% |\k@SI@full@AccelGravityNumeric| is a mathematical value of
+%  the accelertion due to gravity at the surface of the
+% Earth in SI units with full precision.
+% (CODATA 2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@SI@full@AccelGravityNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@SI@full@AccelGravityNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@cgs@short@AccelGravityNumeric}
+% \changes{v1.1.0}{2020/02/03}{Correct value.}
+% \changes{v1.1.0}{2020/02/03}{Fix units.}
+% |\k@cgs@short@AccelGravityNumeric| is a mathematical value of
+%  the accelertion due to gravity at the surface of
+% the Earth in cgs units with reduced precision.
+% (CODATA 2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@cgs@short@AccelGravityNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@cgs@short@AccelGravityNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@cgs@full@AccelGravityNumeric}
+% \changes{v1.1.0}{2020/02/03}{Correct value.}
+% \changes{v1.1.0}{2020/02/03}{Fix units.}
+% |\k@cgs@full@AccelGravityNumeric| is a mathematical value of
+%  the accelertion due to gravity at the surface of the
+% Earth in cgs units with full precision.
+% (CODATA 2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@cgs@full@AccelGravityNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@cgs@full@AccelGravityNumeric}\end{mdframed}
+% \makeatother
+%
 %
 %\subsubsection{Other Constants}
 %
 % \DescribeMacro{\k@SI@short@Coulomb}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
 % |\k@SI@short@Coulomb| is the Coulomb constant ($\frac{1}{4\pi\epsilon_0}$) in
 % SI units with reduced precision.
 % (Calculated)
@@ -1707,6 +3769,7 @@
 % \makeatother
 %
 % \DescribeMacro{\k@SI@full@Coulomb}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
 % |\k@SI@full@Coulomb| is the Coulomb constant ($\frac{1}{4\pi\epsilon_0}$) in
 % SI units with full precision.
 % (Calculated)
@@ -1723,6 +3786,7 @@
 % \makeatother
 %
 % \DescribeMacro{\k@cgs@short@Coulomb}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
 % |\k@cgs@short@Coulomb| is the Coulomb constant ($\frac{1}{4\pi\epsilon_0}$)
 % in cgs units with reduced precision.
 % (Calculated)
@@ -1739,6 +3803,7 @@
 % \makeatother
 %
 % \DescribeMacro{\k@cgs@full@Coulomb}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
 % |\k@cgs@full@Coulomb| is the Coulomb constant ($\frac{1}{4\pi\epsilon_0}$) in
 % cgs units with full precision.
 % (Calculated)
@@ -1754,6 +3819,78 @@
 % {The value is \k@cgs@full@Coulomb}\end{mdframed}
 % \makeatother
 %
+% \DescribeMacro{\k@SI@short@CoulombNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% |\k@SI@short@CoulombNumeric| is a mathematical value of
+%  the Coulomb constant ($\frac{1}{4\pi\epsilon_0}$) in SI
+% units with reduced precision.
+% (Calculated)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@SI@short@CoulombNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@SI@short@CoulombNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@SI@full@CoulombNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% |\k@SI@full@CoulombNumeric| is a mathematical value of
+%  the Coulomb constant ($\frac{1}{4\pi\epsilon_0}$) in SI
+% units with full precision.
+% (Calculated)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@SI@full@CoulombNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@SI@full@CoulombNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@cgs@short@CoulombNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% |\k@cgs@short@CoulombNumeric| is a mathematical value of
+%  the Coulomb constant ($\frac{1}{4\pi\epsilon_0}$) in cgs
+% units with reduced precision.
+% (Calculated)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@cgs@short@CoulombNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@cgs@short@CoulombNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@cgs@full@CoulombNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% |\k@cgs@full@CoulombNumeric| is a mathematical value of
+%  the Coulomb constant ($\frac{1}{4\pi\epsilon_0}$) in cgs
+% units with full precision.
+% (Calculated)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@cgs@full@CoulombNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@cgs@full@CoulombNumeric}\end{mdframed}
+% \makeatother
+%
 % \DescribeMacro{\k@SI@short@VacuumPermittivity}
 % |\k@SI@short@VacuumPermittivity| is the electric permittivity of the vacuum
 % in SI units with reduced precision.
@@ -1818,10 +3955,79 @@
 % {The value is \k@cgs@full@VacuumPermittivity}\end{mdframed}
 % \makeatother
 %
+% \DescribeMacro{\k@SI@short@VacuumPermittivityNumeric}
+% |\k@SI@short@VacuumPermittivityNumeric| is a mathematical value of
+%  the electric permittivity of the vacuum in SI
+% units with reduced precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@SI@short@VacuumPermittivityNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@SI@short@VacuumPermittivityNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@SI@full@VacuumPermittivityNumeric}
+% |\k@SI@full@VacuumPermittivityNumeric| is a mathematical value of
+%  the electric permittivity of the vacuum in SI
+% units with full precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@SI@full@VacuumPermittivityNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@SI@full@VacuumPermittivityNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@cgs@short@VacuumPermittivityNumeric}
+% |\k@cgs@short@VacuumPermittivityNumeric| is a mathematical value of
+%  the electric permittivity of the vacuum in
+% cgs units with reduced precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@cgs@short@VacuumPermittivityNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@cgs@short@VacuumPermittivityNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@cgs@full@VacuumPermittivityNumeric}
+% |\k@cgs@full@VacuumPermittivityNumeric| is a mathematical value of
+%  the electric permittivity of the vacuum in cgs
+% units with full precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@cgs@full@VacuumPermittivityNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@cgs@full@VacuumPermittivityNumeric}\end{mdframed}
+% \makeatother
+%
 % \DescribeMacro{\k@SI@short@VacuumPermeability}
+% \changes{v1.1.0}{2020/02/03}{Fix value of constant.}
 % |\k@SI@short@VacuumPermeability| is the magnetic permeability of the vacuum
 % in SI units with reduced precision.
-% (CODATA~2018)
+% (Calculated)
 %
 % The macro can be invoked by (e.g.)
 % \begin{mdframed}[backgroundcolor=orange!25]%
@@ -1835,9 +4041,10 @@
 % \makeatother
 %
 % \DescribeMacro{\k@SI@full@VacuumPermeability}
+% \changes{v1.1.0}{2020/02/03}{Fix value of constant.}
 % |\k@SI@full@VacuumPermeability| is the magnetic permeability of the vacuum in
 % SI units with full precision.
-% (CODATA~2018)
+% (Calculated)
 %
 % The macro can be invoked by (e.g.)
 % \begin{mdframed}[backgroundcolor=orange!25]%
@@ -1851,9 +4058,10 @@
 % \makeatother
 %
 % \DescribeMacro{\k@cgs@short@VacuumPermeability}
+% \changes{v1.1.0}{2020/02/03}{Fix value of constant.}
 % |\k@cgs@short@VacuumPermeability| is the magnetic permeability of the vacuum
 % in cgs units with reduced precision.
-% (CODATA~2018)
+% (Calculated)
 %
 % The macro can be invoked by (e.g.)
 % \begin{mdframed}[backgroundcolor=orange!25]%
@@ -1867,9 +4075,10 @@
 % \makeatother
 %
 % \DescribeMacro{\k@cgs@full@VacuumPermeability}
+% \changes{v1.1.0}{2020/02/03}{Fix value of constant.}
 % |\k@cgs@full@VacuumPermeability| is the magnetic permeability of the vacuum
 % in cgs units with full precision.
-% (CODATA~2018)
+% (Calculated)
 %
 % The macro can be invoked by (e.g.)
 % \begin{mdframed}[backgroundcolor=orange!25]%
@@ -1882,6 +4091,78 @@
 % {The value is \k@cgs@full@VacuumPermeability}\end{mdframed}
 % \makeatother
 %
+% \DescribeMacro{\k@SI@short@VacuumPermeabilityNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix value of constant.}
+% |\k@SI@short@VacuumPermeabilityNumeric| is a mathematical value of
+%  the magnetic permeability of the vacuum in SI
+% units with reduced precision.
+% (Calculated)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@SI@short@VacuumPermeabilityNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@SI@short@VacuumPermeabilityNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@SI@full@VacuumPermeabilityNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix value of constant.}
+% |\k@SI@full@VacuumPermeabilityNumeric| is a mathematical value of
+%  the magnetic permeability of the vacuum in SI
+% units with full precision.
+% (Calculated)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@SI@full@VacuumPermeabilityNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@SI@full@VacuumPermeabilityNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@cgs@short@VacuumPermeabilityNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix value of constant.}
+% |\k@cgs@short@VacuumPermeabilityNumeric| is a mathematical value of
+%  the magnetic permeability of the vacuum in
+% cgs units with reduced precision.
+% (Calculated)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@cgs@short@VacuumPermeabilityNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@cgs@short@VacuumPermeabilityNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@cgs@full@VacuumPermeabilityNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix value of constant.}
+% |\k@cgs@full@VacuumPermeabilityNumeric| is a mathematical value of
+%  the magnetic permeability of the vacuum in cgs
+% units with full precision.
+% (Calculated)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@cgs@full@VacuumPermeabilityNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@cgs@full@VacuumPermeabilityNumeric}\end{mdframed}
+% \makeatother
+%
 % \DescribeMacro{\k@short@VacuumImpedance}
 % |\k@short@VacuumImpedance| is the characteristic impedance of the vacuum with
 % reduced precision.
@@ -1914,6 +4195,40 @@
 % {The value is \k@full@VacuumImpedance}\end{mdframed}
 % \makeatother
 %
+% \DescribeMacro{\k@short@VacuumImpedanceNumeric}
+% |\k@short@VacuumImpedanceNumeric| is a mathematical value of
+%  the characteristic impedance of the vacuum with
+% reduced precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@short@VacuumImpedanceNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@short@VacuumImpedanceNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@full@VacuumImpedanceNumeric}
+% |\k@full@VacuumImpedanceNumeric| is a mathematical value of
+%  the characteristic impedance of the vacuum with full
+% precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@full@VacuumImpedanceNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@full@VacuumImpedanceNumeric}\end{mdframed}
+% \makeatother
+%
 % \DescribeMacro{\k@SI@short@Boltzmann}
 % |\k@SI@short@Boltzmann| is the Boltzmann constant in SI units with reduced
 % precision.
@@ -2009,7 +4324,106 @@
 % {The value is \k@eV@full@Boltzmann}\end{mdframed}
 % \makeatother
 %
+% \DescribeMacro{\k@SI@short@BoltzmannNumeric}
+% |\k@SI@short@BoltzmannNumeric| is a mathematical value of
+%  the Boltzmann constant in SI units with reduced
+% precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@SI@short@BoltzmannNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@SI@short@BoltzmannNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@SI@full@BoltzmannNumeric}
+% |\k@SI@full@BoltzmannNumeric| is a mathematical value of
+%  the Boltzmann constant in SI units with full precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@SI@full@BoltzmannNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@SI@full@BoltzmannNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@cgs@short@BoltzmannNumeric}
+% |\k@cgs@short@BoltzmannNumeric| is a mathematical value of
+%  the Boltzmann constant in cgs units with reduced
+% precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@cgs@short@BoltzmannNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@cgs@short@BoltzmannNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@cgs@full@BoltzmannNumeric}
+% |\k@cgs@full@BoltzmannNumeric| is a mathematical value of
+%  the Boltzmann constant in cgs units with full precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@cgs@full@BoltzmannNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@cgs@full@BoltzmannNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@eV@short@BoltzmannNumeric}
+% |\k@eV@short@BoltzmannNumeric| is a mathematical value of
+%  the Boltzmann constant in eV with reduced precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@eV@short@BoltzmannNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@eV@short@BoltzmannNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@eV@full@BoltzmannNumeric}
+% |\k@eV@full@BoltzmannNumeric| is a mathematical value of
+%  the Boltzmann constant in eV with full precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@eV@full@BoltzmannNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@eV@full@BoltzmannNumeric}\end{mdframed}
+% \makeatother
+%
 % \DescribeMacro{\k@SI@short@Planck}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
 % |\k@SI@short@Planck| is the Planck constant in SI units with reduced
 % precision.
 % (CODATA~2018)
@@ -2026,6 +4440,7 @@
 % \makeatother
 %
 % \DescribeMacro{\k@SI@full@Planck}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
 % |\k@SI@full@Planck| is the Planck constant in SI units with full precision.
 % (CODATA~2018)
 %
@@ -2041,6 +4456,7 @@
 % \makeatother
 %
 % \DescribeMacro{\k@cgs@short@Planck}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
 % |\k@cgs@short@Planck| is the Planck constant in cgs units with reduced
 % precision.
 % (CODATA~2018)
@@ -2057,6 +4473,7 @@
 % \makeatother
 %
 % \DescribeMacro{\k@cgs@full@Planck}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
 % |\k@cgs@full@Planck| is the Planck constant in cgs units with full precision.
 % (CODATA~2018)
 %
@@ -2072,6 +4489,7 @@
 % \makeatother
 %
 % \DescribeMacro{\k@eV@short@Planck}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
 % |\k@eV@short@Planck| is the Planck constant in eV with reduced precision.
 % (CODATA~2018)
 %
@@ -2087,6 +4505,7 @@
 % \makeatother
 %
 % \DescribeMacro{\k@eV@full@Planck}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
 % |\k@eV@full@Planck| is the Planck constant in eV with full precision.
 % (CODATA~2018)
 %
@@ -2101,7 +4520,110 @@
 % {The value is \k@eV@full@Planck}\end{mdframed}
 % \makeatother
 %
+% \DescribeMacro{\k@SI@short@PlanckNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% |\k@SI@short@PlanckNumeric| is a mathematical value of
+%  the Planck constant in SI units with reduced precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@SI@short@PlanckNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@SI@short@PlanckNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@SI@full@PlanckNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% |\k@SI@full@PlanckNumeric| is a mathematical value of
+%  the Planck constant in SI units with full precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@SI@full@PlanckNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@SI@full@PlanckNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@cgs@short@PlanckNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% |\k@cgs@short@PlanckNumeric| is a mathematical value of
+%  the Planck constant in cgs units with reduced precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@cgs@short@PlanckNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@cgs@short@PlanckNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@cgs@full@PlanckNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% |\k@cgs@full@PlanckNumeric| is a mathematical value of
+%  the Planck constant in cgs units with full precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@cgs@full@PlanckNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@cgs@full@PlanckNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@eV@short@PlanckNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% |\k@eV@short@PlanckNumeric| is a mathematical value of
+%  the Planck constant in eV with reduced precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@eV@short@PlanckNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@eV@short@PlanckNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@eV@full@PlanckNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% |\k@eV@full@PlanckNumeric| is a mathematical value of
+%  the Planck constant in eV with full precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@eV@full@PlanckNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@eV@full@PlanckNumeric}\end{mdframed}
+% \makeatother
+%
 % \DescribeMacro{\k@SI@short@PlanckReduced}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
 % |\k@SI@short@PlanckReduced| is the Reduced Planck constant
 % $\left(\frac{h}{2\pi}\right)$ in SI units with reduced precision.
 % (Calculated)
@@ -2118,6 +4640,7 @@
 % \makeatother
 %
 % \DescribeMacro{\k@SI@full@PlanckReduced}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
 % |\k@SI@full@PlanckReduced| is the Reduced Planck constant
 % $\left(\frac{h}{2\pi}\right)$ in SI units with full precision.
 % (Calculated)
@@ -2134,6 +4657,7 @@
 % \makeatother
 %
 % \DescribeMacro{\k@cgs@short@PlanckReduced}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
 % |\k@cgs@short@PlanckReduced| is the Reduced Planck constant
 % $\left(\frac{h}{2\pi}\right)$ in cgs units with reduced precision.
 % (Calculated)
@@ -2150,6 +4674,7 @@
 % \makeatother
 %
 % \DescribeMacro{\k@cgs@full@PlanckReduced}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
 % |\k@cgs@full@PlanckReduced| is the Reduced Planck constant
 % $\left(\frac{h}{2\pi}\right)$ in cgs units with full precision.
 % (Calculated)
@@ -2166,6 +4691,7 @@
 % \makeatother
 %
 % \DescribeMacro{\k@eV@short@PlanckReduced}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
 % |\k@eV@short@PlanckReduced| is the Reduced Planck constant
 % $\left(\frac{h}{2\pi}\right)$ in eV with reduced precision.
 % (Calculated)
@@ -2182,6 +4708,7 @@
 % \makeatother
 %
 % \DescribeMacro{\k@eV@full@PlanckReduced}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
 % |\k@eV@full@PlanckReduced| is the Reduced Planck constant
 % $\left(\frac{h}{2\pi}\right)$ in eV with full precision.
 % (Calculated)
@@ -2197,7 +4724,116 @@
 % {The value is \k@eV@full@PlanckReduced}\end{mdframed}
 % \makeatother
 %
+% \DescribeMacro{\k@SI@short@PlanckReducedNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% |\k@SI@short@PlanckReducedNumeric| is a mathematical value of
+%  the Reduced Planck constant
+% $\left(\frac{h}{2\pi}\right)$ in SI units with reduced precision.
+% (Calculated)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@SI@short@PlanckReducedNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@SI@short@PlanckReducedNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@SI@full@PlanckReducedNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% |\k@SI@full@PlanckReducedNumeric| is a mathematical value of
+%  the Reduced Planck constant
+% $\left(\frac{h}{2\pi}\right)$ in SI units with full precision.
+% (Calculated)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@SI@full@PlanckReducedNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@SI@full@PlanckReducedNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@cgs@short@PlanckReducedNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% |\k@cgs@short@PlanckReducedNumeric| is a mathematical value of
+%  the Reduced Planck constant
+% $\left(\frac{h}{2\pi}\right)$ in cgs units with reduced precision.
+% (Calculated)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@cgs@short@PlanckReducedNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@cgs@short@PlanckReducedNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@cgs@full@PlanckReducedNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% |\k@cgs@full@PlanckReducedNumeric| is a mathematical value of
+%  the Reduced Planck constant
+% $\left(\frac{h}{2\pi}\right)$ in cgs units with full precision.
+% (Calculated)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@cgs@full@PlanckReducedNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@cgs@full@PlanckReducedNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@eV@short@PlanckReducedNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% |\k@eV@short@PlanckReducedNumeric| is a mathematical value of
+%  the Reduced Planck constant
+% $\left(\frac{h}{2\pi}\right)$ in eV with reduced precision.
+% (Calculated)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@eV@short@PlanckReducedNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@eV@short@PlanckReducedNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@eV@full@PlanckReducedNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% |\k@eV@full@PlanckReducedNumeric| is a mathematical value of
+%  the Reduced Planck constant
+% $\left(\frac{h}{2\pi}\right)$ in eV with full precision.
+% (Calculated)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@eV@full@PlanckReducedNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@eV@full@PlanckReducedNumeric}\end{mdframed}
+% \makeatother
+%
 % \DescribeMacro{\k@SI@short@Gravity}
+% \changes{v1.1.0}{2020/02/03}{Fix value of constant.}
 % |\k@SI@short@Gravity| is Newton's gravitational constant in SI units with
 % reduced precision.
 % (CODATA~2018)
@@ -2214,6 +4850,7 @@
 % \makeatother
 %
 % \DescribeMacro{\k@SI@full@Gravity}
+% \changes{v1.1.0}{2020/02/03}{Fix value of constant.}
 % |\k@SI@full@Gravity| is Newton's gravitational constant in SI units with full
 % precision.
 % (CODATA~2018)
@@ -2230,6 +4867,7 @@
 % \makeatother
 %
 % \DescribeMacro{\k@cgs@short@Gravity}
+% \changes{v1.1.0}{2020/02/03}{Fix value of constant.}
 % |\k@cgs@short@Gravity| is Newton's gravitational constant in cgs units with
 % reduced precision.
 % (CODATA~2018)
@@ -2246,6 +4884,7 @@
 % \makeatother
 %
 % \DescribeMacro{\k@cgs@full@Gravity}
+% \changes{v1.1.0}{2020/02/03}{Fix value of constant.}
 % |\k@cgs@full@Gravity| is Newton's gravitational constant in cgs units with
 % full precision.
 % (CODATA~2018)
@@ -2261,7 +4900,80 @@
 % {The value is \k@cgs@full@Gravity}\end{mdframed}
 % \makeatother
 %
+% \DescribeMacro{\k@SI@short@GravityNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix value of constant.}
+% |\k@SI@short@GravityNumeric| is a mathematical value of
+%  Newton's gravitational constant in SI units with reduced
+% precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@SI@short@GravityNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@SI@short@GravityNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@SI@full@GravityNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix value of constant.}
+% |\k@SI@full@GravityNumeric| is a mathematical value of
+%  Newton's gravitational constant in SI units with full
+% precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@SI@full@GravityNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@SI@full@GravityNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@cgs@short@GravityNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix value of constant.}
+% |\k@cgs@short@GravityNumeric| is a mathematical value of
+%  Newton's gravitational constant in cgs units with
+% reduced precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@cgs@short@GravityNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@cgs@short@GravityNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@cgs@full@GravityNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix value of constant.}
+% |\k@cgs@full@GravityNumeric| is a mathematical value of
+%  Newton's gravitational constant in cgs units with full
+% precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@cgs@full@GravityNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@cgs@full@GravityNumeric}\end{mdframed}
+% \makeatother
+%
 % \DescribeMacro{\k@SI@short@StefanBoltzmann}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
 % |\k@SI@short@StefanBoltzmann| is the Stefan-Boltzmann blackbody constant
 % $\left(\frac{2\pi^5k_\mathrm{B}}{15h^3c^2}\right)$ in SI units with reduced
 % precision.
@@ -2279,6 +4991,7 @@
 % \makeatother
 %
 % \DescribeMacro{\k@SI@full@StefanBoltzmann}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
 % |\k@SI@full@StefanBoltzmann| is the Stefan-Boltzmann blackbody constant
 % $\left(\frac{2\pi^5k_\mathrm{B}}{15h^3c^2}\right)$ in SI units with full
 % precision.
@@ -2296,6 +5009,7 @@
 % \makeatother
 %
 % \DescribeMacro{\k@cgs@short@StefanBoltzmann}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
 % |\k@cgs@short@StefanBoltzmann| is the Stefan-Boltzmann blackbody constant
 % $\left(\frac{2\pi^5k_\mathrm{B}}{15h^3c^2}\right)$ in cgs units with reduced
 % precision.
@@ -2313,6 +5027,7 @@
 % \makeatother
 %
 % \DescribeMacro{\k@cgs@full@StefanBoltzmann}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
 % |\k@cgs@full@StefanBoltzmann| is the Stefan-Boltzmann blackbody constant
 % $\left(\frac{2\pi^5k_\mathrm{B}}{15h^3c^2}\right)$ in cgs units with full
 % precision.
@@ -2329,6 +5044,82 @@
 % {The value is \k@cgs@full@StefanBoltzmann}\end{mdframed}
 % \makeatother
 %
+% \DescribeMacro{\k@SI@short@StefanBoltzmannNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% |\k@SI@short@StefanBoltzmannNumeric| is a mathematical value of
+%  the Stefan-Boltzmann blackbody constant
+% $\left(\frac{2\pi^5k_\mathrm{B}}{15h^3c^2}\right)$ in SI units with reduced
+% precision.
+% (Calculated)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@SI@short@StefanBoltzmannNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@SI@short@StefanBoltzmannNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@SI@full@StefanBoltzmannNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% |\k@SI@full@StefanBoltzmannNumeric| is a mathematical value of
+%  the Stefan-Boltzmann blackbody constant
+% $\left(\frac{2\pi^5k_\mathrm{B}}{15h^3c^2}\right)$ in SI units with full
+% precision.
+% (Calculated)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@SI@full@StefanBoltzmannNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@SI@full@StefanBoltzmannNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@cgs@short@StefanBoltzmannNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% |\k@cgs@short@StefanBoltzmannNumeric| is a mathematical value of
+%  the Stefan-Boltzmann blackbody constant
+% $\left(\frac{2\pi^5k_\mathrm{B}}{15h^3c^2}\right)$ in cgs units with reduced
+% precision.
+% (Calculated)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@cgs@short@StefanBoltzmannNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@cgs@short@StefanBoltzmannNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@cgs@full@StefanBoltzmannNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% |\k@cgs@full@StefanBoltzmannNumeric| is a mathematical value of
+%  the Stefan-Boltzmann blackbody constant
+% $\left(\frac{2\pi^5k_\mathrm{B}}{15h^3c^2}\right)$ in cgs units with full
+% precision.
+% (Calculated)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@cgs@full@StefanBoltzmannNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@cgs@full@StefanBoltzmannNumeric}\end{mdframed}
+% \makeatother
+%
 % \DescribeMacro{\k@SI@short@Radiation}
 % |\k@SI@short@Radiation| is the radiation constant, $a
 % \left(\frac{8\pi^5k_\mathrm{B}^4}{15c^3h^3}\right)$ in SI units with reduced
@@ -2397,6 +5188,78 @@
 % {The value is \k@cgs@full@Radiation}\end{mdframed}
 % \makeatother
 %
+% \DescribeMacro{\k@SI@short@RadiationNumeric}
+% |\k@SI@short@RadiationNumeric| is a mathematical value of
+%  the radiation constant, $a
+% \left(\frac{8\pi^5k_\mathrm{B}^4}{15c^3h^3}\right)$ in SI units with reduced
+% precision.
+% (Calculated)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@SI@short@RadiationNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@SI@short@RadiationNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@SI@full@RadiationNumeric}
+% |\k@SI@full@RadiationNumeric| is a mathematical value of
+%  the radiation constant, $a
+% \left(\frac{8\pi^5k_\mathrm{B}^4}{15c^3h^3}\right)$ in SI units with full
+% precision.
+% (Calculated)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@SI@full@RadiationNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@SI@full@RadiationNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@cgs@short@RadiationNumeric}
+% |\k@cgs@short@RadiationNumeric| is a mathematical value of
+%  the radiation constant, $a
+% \left(\frac{8\pi^5k_\mathrm{B}^4}{15c^3h^3}\right)$ in cgs units with reduced
+% precision.
+% (Calculated)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@cgs@short@RadiationNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@cgs@short@RadiationNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@cgs@full@RadiationNumeric}
+% |\k@cgs@full@RadiationNumeric| is a mathematical value of
+%  the radiation constant, $a
+% \left(\frac{8\pi^5k_\mathrm{B}^4}{15c^3h^3}\right)$ in cgs units with full
+% precision.
+% (Calculated)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@cgs@full@RadiationNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@cgs@full@RadiationNumeric}\end{mdframed}
+% \makeatother
+%
 % \DescribeMacro{\k@short@FineStructure}
 % |\k@short@FineStructure| is the fine structure constant with reduced
 % precision.
@@ -2428,6 +5291,38 @@
 % {The value is \k@full@FineStructure}\end{mdframed}
 % \makeatother
 %
+% \DescribeMacro{\k@short@FineStructureNumeric}
+% |\k@short@FineStructureNumeric| is a mathematical value of
+%  the fine structure constant with reduced precision.
+% (Calculated)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@short@FineStructureNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@short@FineStructureNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@full@FineStructureNumeric}
+% |\k@full@FineStructureNumeric| is a mathematical value of
+%  the fine structure constant with full precision.
+% (Calculated)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@full@FineStructureNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@full@FineStructureNumeric}\end{mdframed}
+% \makeatother
+%
 % \DescribeMacro{\k@short@FineStructureReciprocal}
 % |\k@short@FineStructureReciprocal| is the reciprocal of the fine structure
 % constant with reduced precision.
@@ -2460,6 +5355,40 @@
 % {The value is \k@full@FineStructureReciprocal}\end{mdframed}
 % \makeatother
 %
+% \DescribeMacro{\k@short@FineStructureReciprocalNumeric}
+% |\k@short@FineStructureReciprocalNumeric| is a mathematical value of
+%  the reciprocal of the fine structure
+% constant with reduced precision.
+% (Calculated)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@short@FineStructureReciprocalNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@short@FineStructureReciprocalNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@full@FineStructureReciprocalNumeric}
+% |\k@full@FineStructureReciprocalNumeric| is a mathematical value of
+%  the reciprocal of the fine structure constant
+% with full precision.
+% (Calculated)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@full@FineStructureReciprocalNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@full@FineStructureReciprocalNumeric}\end{mdframed}
+% \makeatother
+%
 % \DescribeMacro{\k@short@Avogadro}
 % |\k@short@Avogadro| is Avogadro's Number (the number of particles in a mole)
 % with reduced precision.
@@ -2492,6 +5421,40 @@
 % {The value is \k@full@Avogadro}\end{mdframed}
 % \makeatother
 %
+% \DescribeMacro{\k@short@AvogadroNumeric}
+% |\k@short@AvogadroNumeric| is a mathematical value of
+%  Avogadro's Number (the number of particles in a mole) with
+% reduced precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@short@AvogadroNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@short@AvogadroNumeric}\end{mdframed}
+% \makeatother
+%
+% \DescribeMacro{\k@full@AvogadroNumeric}
+% |\k@full@AvogadroNumeric| is a mathematical value of
+%  Avogadro's Number (the number of particles in a mole) with
+% full precision.
+% (CODATA~2018)
+%
+% The macro can be invoked by (e.g.)
+% \begin{mdframed}[backgroundcolor=orange!25]%
+% {\small\texttt{\textbackslash makeatletter\\ The value is
+% \textbackslash k@full@AvogadroNumeric\\
+% \textbackslash makeatother}}\end{mdframed}
+% \makeatletter
+% Resulting in 
+% \begin{mdframed}[backgroundcolor=blue!25]%
+% {The value is \k@full@AvogadroNumeric}\end{mdframed}
+% \makeatother
+%
 \makeatletter
 % \StopEventually{}
 %
@@ -2527,6 +5490,8 @@
 %<*package>
 %\fi
 % \begin{macro}{\k@SI@short@MassElectron}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % |\k@SI@short@MassElectron| is the mass of an electron in SI units with
 % reduced precision.
 % Source: CODATA~2018
@@ -2535,7 +5500,7 @@
 \DeclareRobustCommand{\k@SI@short@MassElectron}{%
 \ensuremath{%
 9.11%
-\times 10^{-34}\kg}}
+\times 10^{-31}\kg}}
 %    \end{macrocode}
 % \end{macro}
 %
@@ -2546,6 +5511,8 @@
 %<*package>
 %\fi
 % \begin{macro}{\k@SI@full@MassElectron}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % |\k@SI@full@MassElectron| is the mass of an electron in SI units with full
 % precision.
 % Source: CODATA~2018
@@ -2557,7 +5524,7 @@
 980\expandafter\physconst@decimalsseparator%
 087\expandafter\physconst@decimalsseparator%
 382%
-\times 10^{-34}\kg}}
+\times 10^{-31}\kg}}
 %    \end{macrocode}
 % \end{macro}
 %
@@ -2568,6 +5535,8 @@
 %<*package>
 %\fi
 % \begin{macro}{\k@cgs@short@MassElectron}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % |\k@cgs@short@MassElectron| is the mass of an electron in cgs units with
 % reduced precision.
 % Source: CODATA~2018
@@ -2576,7 +5545,7 @@
 \DeclareRobustCommand{\k@cgs@short@MassElectron}{%
 \ensuremath{%
 9.11%
-\times 10^{-31}\gm}}
+\times 10^{-28}\gm}}
 %    \end{macrocode}
 % \end{macro}
 %
@@ -2587,6 +5556,8 @@
 %<*package>
 %\fi
 % \begin{macro}{\k@cgs@full@MassElectron}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % |\k@cgs@full@MassElectron| is the mass of an electron in cgs units with full
 % precision.
 % Source: CODATA~2018
@@ -2598,7 +5569,7 @@
 980\expandafter\physconst@decimalsseparator%
 087\expandafter\physconst@decimalsseparator%
 382%
-\times 10^{-31}\gm}}
+\times 10^{-28}\gm}}
 %    \end{macrocode}
 % \end{macro}
 %
@@ -2609,6 +5580,8 @@
 %<*package>
 %\fi
 % \begin{macro}{\k@eV@short@MassElectron}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % |\k@eV@short@MassElectron| is the mass of an electron in eV with reduced
 % precision.
 % Source: CODATA~2018
@@ -2616,8 +5589,8 @@
 %    \begin{macrocode}
 \DeclareRobustCommand{\k@eV@short@MassElectron}{%
 \ensuremath{%
-5.69%
-\times 10^{-19}\eV\,c^{-2}}}
+5.11%
+\times 10^{5}\eV\,c^{-2}}}
 %    \end{macrocode}
 % \end{macro}
 %
@@ -2628,6 +5601,8 @@
 %<*package>
 %\fi
 % \begin{macro}{\k@eV@full@MassElectron}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % |\k@eV@full@MassElectron| is the mass of an electron in eV with full
 % precision.
 % Source: CODATA~2018
@@ -2635,11 +5610,11 @@
 %    \begin{macrocode}
 \DeclareRobustCommand{\k@eV@full@MassElectron}{%
 \ensuremath{%
-5.685\expandafter\physconst@decimalsseparator%
-378\expandafter\physconst@decimalsseparator%
-187\expandafter\physconst@decimalsseparator%
-448%
-\times 10^{-19}\eV\,c^{-2}}}
+5.109\expandafter\physconst@decimalsseparator%
+763\expandafter\physconst@decimalsseparator%
+089\expandafter\physconst@decimalsseparator%
+046%
+\times 10^{5}\eV\,c^{-2}}}
 %    \end{macrocode}
 % \end{macro}
 %
@@ -2650,6 +5625,8 @@
 %<*package>
 %\fi
 % \begin{macro}{\kMassElectron}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % |\kMassElectron| is the mass of an electron.
 %
 %    \begin{macrocode}
@@ -2680,6 +5657,8 @@
 %<*package>
 %\fi
 % \begin{macro}{\keVMassElectron}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % |\keVMassElectron| is the mass of an electron.
 %
 %    \begin{macrocode}
@@ -2699,7 +5678,183 @@
 %\iffalse
 %<*package>
 %\fi
+% \begin{macro}{\k@SI@short@MassElectronNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% |\k@SI@short@MassElectronNumeric| is the mass of an electron in SI units with
+% reduced precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@SI@short@MassElectronNumeric}{%
+\ensuremath{%
+9.11e-31}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@SI@full@MassElectronNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% |\k@SI@full@MassElectronNumeric| is the mass of an electron in SI units with full
+% precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@SI@full@MassElectronNumeric}{%
+\ensuremath{%
+9.108980087382e-31}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@cgs@short@MassElectronNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% |\k@cgs@short@MassElectronNumeric| is the mass of an electron in cgs units with
+% reduced precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@cgs@short@MassElectronNumeric}{%
+\ensuremath{%
+9.11e-28}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@cgs@full@MassElectronNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% |\k@cgs@full@MassElectronNumeric| is the mass of an electron in cgs units with full
+% precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@cgs@full@MassElectronNumeric}{%
+\ensuremath{%
+9.108980087382e-28}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@eV@short@MassElectronNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% |\k@eV@short@MassElectronNumeric| is the mass of an electron in eV with reduced
+% precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@eV@short@MassElectronNumeric}{%
+\ensuremath{%
+5.11e+05}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@eV@full@MassElectronNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% |\k@eV@full@MassElectronNumeric| is the mass of an electron in eV with full
+% precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@eV@full@MassElectronNumeric}{%
+\ensuremath{%
+5.109763089046e+05}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\kMassElectronNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% |\kMassElectronNumeric| is the mass of an electron.
+%
+%    \begin{macrocode}
+\ifx\cgsunits\undefined
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kMassElectronNumeric}{%
+\k@SI@short@MassElectronNumeric}
+\else
+\DeclareRobustCommand {\kMassElectronNumeric}{%
+\k@SI@full@MassElectronNumeric}
+\fi
+\else
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kMassElectronNumeric}{%
+\k@cgs@short@MassElectronNumeric}
+\else
+\DeclareRobustCommand {\kMassElectronNumeric}{%
+\k@cgs@full@MassElectronNumeric}
+\fi
+\fi
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\keVMassElectronNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% |\keVMassElectronNumeric| is the mass of an electron.
+%
+%    \begin{macrocode}
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\keVMassElectronNumeric}{%
+\k@eV@short@MassElectronNumeric}
+\else
+\DeclareRobustCommand {\keVMassElectronNumeric}{%
+\k@eV@full@MassElectronNumeric}
+\fi
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
 % \begin{macro}{\k@SI@short@MassProton}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % |\k@SI@short@MassProton| is the mass of a proton in SI units with reduced
 % precision.
 % Source: CODATA~2018
@@ -2708,7 +5863,7 @@
 \DeclareRobustCommand{\k@SI@short@MassProton}{%
 \ensuremath{%
 1.67%
-\times 10^{-30}\kg}}
+\times 10^{-27}\kg}}
 %    \end{macrocode}
 % \end{macro}
 %
@@ -2719,6 +5874,8 @@
 %<*package>
 %\fi
 % \begin{macro}{\k@SI@full@MassProton}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % |\k@SI@full@MassProton| is the mass of a proton in SI units with full
 % precision.
 % Source: CODATA~2018
@@ -2730,7 +5887,7 @@
 547\expandafter\physconst@decimalsseparator%
 813\expandafter\physconst@decimalsseparator%
 969%
-\times 10^{-30}\kg}}
+\times 10^{-27}\kg}}
 %    \end{macrocode}
 % \end{macro}
 %
@@ -2741,6 +5898,8 @@
 %<*package>
 %\fi
 % \begin{macro}{\k@cgs@short@MassProton}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % |\k@cgs@short@MassProton| is the mass of a proton in cgs units with reduced
 % precision.
 % Source: CODATA~2018
@@ -2749,7 +5908,7 @@
 \DeclareRobustCommand{\k@cgs@short@MassProton}{%
 \ensuremath{%
 1.67%
-\times 10^{-27}\gm}}
+\times 10^{-24}\gm}}
 %    \end{macrocode}
 % \end{macro}
 %
@@ -2760,6 +5919,8 @@
 %<*package>
 %\fi
 % \begin{macro}{\k@cgs@full@MassProton}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % |\k@cgs@full@MassProton| is the mass of a proton in cgs units with full
 % precision.
 % Source: CODATA~2018
@@ -2771,7 +5932,7 @@
 547\expandafter\physconst@decimalsseparator%
 813\expandafter\physconst@decimalsseparator%
 969%
-\times 10^{-27}\gm}}
+\times 10^{-24}\gm}}
 %    \end{macrocode}
 % \end{macro}
 %
@@ -2782,14 +5943,16 @@
 %<*package>
 %\fi
 % \begin{macro}{\k@eV@short@MassProton}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % |\k@eV@short@MassProton| is the mass of a proton in eV with reduced precision.
 % Source: CODATA~2018
 %
 %    \begin{macrocode}
 \DeclareRobustCommand{\k@eV@short@MassProton}{%
 \ensuremath{%
-1.04%
-\times 10^{-15}\eV\,c^{-2}}}
+9.38%
+\times 10^{8}\eV\,c^{-2}}}
 %    \end{macrocode}
 % \end{macro}
 %
@@ -2800,17 +5963,19 @@
 %<*package>
 %\fi
 % \begin{macro}{\k@eV@full@MassProton}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % |\k@eV@full@MassProton| is the mass of a proton in eV with full precision.
 % Source: CODATA~2018
 %
 %    \begin{macrocode}
 \DeclareRobustCommand{\k@eV@full@MassProton}{%
 \ensuremath{%
-1.043\expandafter\physconst@decimalsseparator%
-922\expandafter\physconst@decimalsseparator%
-235\expandafter\physconst@decimalsseparator%
-836%
-\times 10^{-15}\eV\,c^{-2}}}
+9.382\expandafter\physconst@decimalsseparator%
+305\expandafter\physconst@decimalsseparator%
+156\expandafter\physconst@decimalsseparator%
+558%
+\times 10^{8}\eV\,c^{-2}}}
 %    \end{macrocode}
 % \end{macro}
 %
@@ -2821,6 +5986,8 @@
 %<*package>
 %\fi
 % \begin{macro}{\kMassProton}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % |\kMassProton| is the mass of a proton.
 %
 %    \begin{macrocode}
@@ -2851,6 +6018,8 @@
 %<*package>
 %\fi
 % \begin{macro}{\keVMassProton}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % |\keVMassProton| is the mass of a proton.
 %
 %    \begin{macrocode}
@@ -2870,7 +6039,181 @@
 %\iffalse
 %<*package>
 %\fi
+% \begin{macro}{\k@SI@short@MassProtonNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% |\k@SI@short@MassProtonNumeric| is the mass of a proton in SI units with reduced
+% precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@SI@short@MassProtonNumeric}{%
+\ensuremath{%
+1.67e-27}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@SI@full@MassProtonNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% |\k@SI@full@MassProtonNumeric| is the mass of a proton in SI units with full
+% precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@SI@full@MassProtonNumeric}{%
+\ensuremath{%
+1.672547813969e-27}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@cgs@short@MassProtonNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% |\k@cgs@short@MassProtonNumeric| is the mass of a proton in cgs units with reduced
+% precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@cgs@short@MassProtonNumeric}{%
+\ensuremath{%
+1.67e-24}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@cgs@full@MassProtonNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% |\k@cgs@full@MassProtonNumeric| is the mass of a proton in cgs units with full
+% precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@cgs@full@MassProtonNumeric}{%
+\ensuremath{%
+1.672547813969e-24}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@eV@short@MassProtonNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% |\k@eV@short@MassProtonNumeric| is the mass of a proton in eV with reduced precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@eV@short@MassProtonNumeric}{%
+\ensuremath{%
+9.38e+08}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@eV@full@MassProtonNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% |\k@eV@full@MassProtonNumeric| is the mass of a proton in eV with full precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@eV@full@MassProtonNumeric}{%
+\ensuremath{%
+9.382305156558e+08}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\kMassProtonNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% |\kMassProtonNumeric| is the mass of a proton.
+%
+%    \begin{macrocode}
+\ifx\cgsunits\undefined
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kMassProtonNumeric}{%
+\k@SI@short@MassProtonNumeric}
+\else
+\DeclareRobustCommand {\kMassProtonNumeric}{%
+\k@SI@full@MassProtonNumeric}
+\fi
+\else
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kMassProtonNumeric}{%
+\k@cgs@short@MassProtonNumeric}
+\else
+\DeclareRobustCommand {\kMassProtonNumeric}{%
+\k@cgs@full@MassProtonNumeric}
+\fi
+\fi
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\keVMassProtonNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% |\keVMassProtonNumeric| is the mass of a proton.
+%
+%    \begin{macrocode}
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\keVMassProtonNumeric}{%
+\k@eV@short@MassProtonNumeric}
+\else
+\DeclareRobustCommand {\keVMassProtonNumeric}{%
+\k@eV@full@MassProtonNumeric}
+\fi
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
 % \begin{macro}{\k@SI@short@MassHydrogen}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % |\k@SI@short@MassHydrogen| is the mass of a neutral hydrogen atom in SI units
 % with reduced precision.
 % Source: CODATA~2018
@@ -2879,7 +6222,7 @@
 \DeclareRobustCommand{\k@SI@short@MassHydrogen}{%
 \ensuremath{%
 1.67%
-\times 10^{-30}\kg}}
+\times 10^{-27}\kg}}
 %    \end{macrocode}
 % \end{macro}
 %
@@ -2890,6 +6233,8 @@
 %<*package>
 %\fi
 % \begin{macro}{\k@SI@full@MassHydrogen}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % |\k@SI@full@MassHydrogen| is the mass of a neutral hydrogen atom in SI units
 % with full precision.
 % Source: CODATA~2018
@@ -2901,7 +6246,7 @@
 458\expandafter\physconst@decimalsseparator%
 687\expandafter\physconst@decimalsseparator%
 724%
-\times 10^{-30}\kg}}
+\times 10^{-27}\kg}}
 %    \end{macrocode}
 % \end{macro}
 %
@@ -2912,6 +6257,8 @@
 %<*package>
 %\fi
 % \begin{macro}{\k@cgs@short@MassHydrogen}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % |\k@cgs@short@MassHydrogen| is the mass of a neutral hydrogen atom in cgs
 % units with reduced precision.
 % Source: CODATA~2018
@@ -2920,7 +6267,7 @@
 \DeclareRobustCommand{\k@cgs@short@MassHydrogen}{%
 \ensuremath{%
 1.67%
-\times 10^{-27}\gm}}
+\times 10^{-24}\gm}}
 %    \end{macrocode}
 % \end{macro}
 %
@@ -2931,6 +6278,8 @@
 %<*package>
 %\fi
 % \begin{macro}{\k@cgs@full@MassHydrogen}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % |\k@cgs@full@MassHydrogen| is the mass of a neutral hydrogen atom in cgs
 % units with full precision.
 % Source: CODATA~2018
@@ -2942,7 +6291,7 @@
 458\expandafter\physconst@decimalsseparator%
 687\expandafter\physconst@decimalsseparator%
 724%
-\times 10^{-27}\gm}}
+\times 10^{-24}\gm}}
 %    \end{macrocode}
 % \end{macro}
 %
@@ -2953,6 +6302,8 @@
 %<*package>
 %\fi
 % \begin{macro}{\k@eV@short@MassHydrogen}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % |\k@eV@short@MassHydrogen| is the mass of a neutral hydrogen atom in eV with
 % reduced precision.
 % Source: CODATA~2018
@@ -2960,8 +6311,8 @@
 %    \begin{macrocode}
 \DeclareRobustCommand{\k@eV@short@MassHydrogen}{%
 \ensuremath{%
-1.04%
-\times 10^{-15}\eV\,c^{-2}}}
+9.39%
+\times 10^{8}\eV\,c^{-2}}}
 %    \end{macrocode}
 % \end{macro}
 %
@@ -2972,6 +6323,8 @@
 %<*package>
 %\fi
 % \begin{macro}{\k@eV@full@MassHydrogen}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % |\k@eV@full@MassHydrogen| is the mass of a neutral hydrogen atom in eV with
 % full precision.
 % Source: CODATA~2018
@@ -2979,11 +6332,11 @@
 %    \begin{macrocode}
 \DeclareRobustCommand{\k@eV@full@MassHydrogen}{%
 \ensuremath{%
-1.044\expandafter\physconst@decimalsseparator%
-490\expandafter\physconst@decimalsseparator%
-758\expandafter\physconst@decimalsseparator%
-517%
-\times 10^{-15}\eV\,c^{-2}}}
+9.387\expandafter\physconst@decimalsseparator%
+414\expandafter\physconst@decimalsseparator%
+783\expandafter\physconst@decimalsseparator%
+596%
+\times 10^{8}\eV\,c^{-2}}}
 %    \end{macrocode}
 % \end{macro}
 %
@@ -2994,6 +6347,8 @@
 %<*package>
 %\fi
 % \begin{macro}{\kMassHydrogen}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % |\kMassHydrogen| is the mass of a neutral hydrogen atom.
 %
 %    \begin{macrocode}
@@ -3024,6 +6379,8 @@
 %<*package>
 %\fi
 % \begin{macro}{\keVMassHydrogen}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % |\keVMassHydrogen| is the mass of a neutral hydrogen atom.
 %
 %    \begin{macrocode}
@@ -3043,6 +6400,180 @@
 %\iffalse
 %<*package>
 %\fi
+% \begin{macro}{\k@SI@short@MassHydrogenNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% |\k@SI@short@MassHydrogenNumeric| is the mass of a neutral hydrogen atom in SI units
+% with reduced precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@SI@short@MassHydrogenNumeric}{%
+\ensuremath{%
+1.67e-27}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@SI@full@MassHydrogenNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% |\k@SI@full@MassHydrogenNumeric| is the mass of a neutral hydrogen atom in SI units
+% with full precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@SI@full@MassHydrogenNumeric}{%
+\ensuremath{%
+1.673458687724e-27}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@cgs@short@MassHydrogenNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% |\k@cgs@short@MassHydrogenNumeric| is the mass of a neutral hydrogen atom in cgs
+% units with reduced precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@cgs@short@MassHydrogenNumeric}{%
+\ensuremath{%
+1.67e-24}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@cgs@full@MassHydrogenNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% |\k@cgs@full@MassHydrogenNumeric| is the mass of a neutral hydrogen atom in cgs
+% units with full precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@cgs@full@MassHydrogenNumeric}{%
+\ensuremath{%
+1.673458687724e-24}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@eV@short@MassHydrogenNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% |\k@eV@short@MassHydrogenNumeric| is the mass of a neutral hydrogen atom in eV with
+% reduced precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@eV@short@MassHydrogenNumeric}{%
+\ensuremath{%
+9.39e+08}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@eV@full@MassHydrogenNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% |\k@eV@full@MassHydrogenNumeric| is the mass of a neutral hydrogen atom in eV with
+% full precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@eV@full@MassHydrogenNumeric}{%
+\ensuremath{%
+9.387414783596e+08}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\kMassHydrogenNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% |\kMassHydrogenNumeric| is the mass of a neutral hydrogen atom.
+%
+%    \begin{macrocode}
+\ifx\cgsunits\undefined
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kMassHydrogenNumeric}{%
+\k@SI@short@MassHydrogenNumeric}
+\else
+\DeclareRobustCommand {\kMassHydrogenNumeric}{%
+\k@SI@full@MassHydrogenNumeric}
+\fi
+\else
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kMassHydrogenNumeric}{%
+\k@cgs@short@MassHydrogenNumeric}
+\else
+\DeclareRobustCommand {\kMassHydrogenNumeric}{%
+\k@cgs@full@MassHydrogenNumeric}
+\fi
+\fi
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\keVMassHydrogenNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% |\keVMassHydrogenNumeric| is the mass of a neutral hydrogen atom.
+%
+%    \begin{macrocode}
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\keVMassHydrogenNumeric}{%
+\k@eV@short@MassHydrogenNumeric}
+\else
+\DeclareRobustCommand {\keVMassHydrogenNumeric}{%
+\k@eV@full@MassHydrogenNumeric}
+\fi
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
 % \begin{macro}{\k@SI@short@MassSun}
 % |\k@SI@short@MassSun| is the mass of the Sun in SI units with reduced
 % precision.
@@ -3151,7 +6682,344 @@
 %\iffalse
 %<*package>
 %\fi
+% \begin{macro}{\k@SI@short@MassSunNumeric}
+% |\k@SI@short@MassSunNumeric| is the mass of the Sun in SI units with reduced
+% precision.
+% Source: IAU~Resolution~B3~2015
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@SI@short@MassSunNumeric}{%
+\ensuremath{%
+1.99e+30}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@SI@full@MassSunNumeric}
+% |\k@SI@full@MassSunNumeric| is the mass of the Sun in SI units with full precision.
+% Source: IAU~Resolution~B3~2015
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@SI@full@MassSunNumeric}{%
+\ensuremath{%
+1.9884099e+30}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@cgs@short@MassSunNumeric}
+% |\k@cgs@short@MassSunNumeric| is the mass of the Sun in cgs units with reduced
+% precision.
+% Source: IAU~Resolution~B3~2015
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@cgs@short@MassSunNumeric}{%
+\ensuremath{%
+1.99e+33}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@cgs@full@MassSunNumeric}
+% |\k@cgs@full@MassSunNumeric| is the mass of the Sun in cgs units with full precision.
+% Source: IAU~Resolution~B3~2015
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@cgs@full@MassSunNumeric}{%
+\ensuremath{%
+1.9884099e+33}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\kMassSunNumeric}
+% |\kMassSunNumeric| is the mass of the Sun.
+%
+%    \begin{macrocode}
+\ifx\cgsunits\undefined
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kMassSunNumeric}{%
+\k@SI@short@MassSunNumeric}
+\else
+\DeclareRobustCommand {\kMassSunNumeric}{%
+\k@SI@full@MassSunNumeric}
+\fi
+\else
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kMassSunNumeric}{%
+\k@cgs@short@MassSunNumeric}
+\else
+\DeclareRobustCommand {\kMassSunNumeric}{%
+\k@cgs@full@MassSunNumeric}
+\fi
+\fi
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@short@MassEarth}
+% \changes{v1.1.0}{2020/02/03}{Add mass of Earth}
+% |\k@short@MassEarth| is the mass of the Earth with reduced precision.
+% Source: IAU~Resolution~B3~2015
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@short@MassEarth}{%
+\ensuremath{%
+5.97%
+\times 10^{24}\kg}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@full@MassEarth}
+% \changes{v1.1.0}{2020/02/03}{Add mass of Earth}
+% |\k@full@MassEarth| is the mass of the Earth with full precision.
+% Source: IAU~Resolution~B3~2015
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@full@MassEarth}{%
+\ensuremath{%
+5.972\expandafter\physconst@decimalsseparator%
+168%
+\times 10^{24}\kg}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\kMassEarth}
+% \changes{v1.1.0}{2020/02/03}{Add mass of Earth}
+% |\kMassEarth| is the mass of the Earth.
+%
+%    \begin{macrocode}
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kMassEarth}{%
+\k@short@MassEarth}
+\else
+\DeclareRobustCommand {\kMassEarth}{%
+\k@full@MassEarth}
+\fi
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@short@MassEarthNumeric}
+% \changes{v1.1.0}{2020/02/03}{Add mass of Earth}
+% |\k@short@MassEarthNumeric| is the mass of the Earth with reduced precision.
+% Source: IAU~Resolution~B3~2015
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@short@MassEarthNumeric}{%
+\ensuremath{%
+5.97e+24}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@full@MassEarthNumeric}
+% \changes{v1.1.0}{2020/02/03}{Add mass of Earth}
+% |\k@full@MassEarthNumeric| is the mass of the Earth with full precision.
+% Source: IAU~Resolution~B3~2015
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@full@MassEarthNumeric}{%
+\ensuremath{%
+5.972168e+24}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\kMassEarthNumeric}
+% \changes{v1.1.0}{2020/02/03}{Add mass of Earth}
+% |\kMassEarthNumeric| is the mass of the Earth.
+%
+%    \begin{macrocode}
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kMassEarthNumeric}{%
+\k@short@MassEarthNumeric}
+\else
+\DeclareRobustCommand {\kMassEarthNumeric}{%
+\k@full@MassEarthNumeric}
+\fi
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@short@MassJupiter}
+% \changes{v1.1.0}{2020/02/03}{Add mass of Jupiter}
+% |\k@short@MassJupiter| is the mass of Jupiter with reduced precision.
+% Source: IAU~Resolution~B3~2015
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@short@MassJupiter}{%
+\ensuremath{%
+1.90%
+\times 10^{27}\kg}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@full@MassJupiter}
+% \changes{v1.1.0}{2020/02/03}{Add mass of Jupiter}
+% |\k@full@MassJupiter| is the mass of Jupiter with full precision.
+% Source: IAU~Resolution~B3~2015
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@full@MassJupiter}{%
+\ensuremath{%
+1.898\expandafter\physconst@decimalsseparator%
+124\expandafter\physconst@decimalsseparator%
+6%
+\times 10^{27}\kg}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\kMassJupiter}
+% \changes{v1.1.0}{2020/02/03}{Add mass of Jupiter}
+% |\kMassJupiter| is the mass of Jupiter.
+%
+%    \begin{macrocode}
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kMassJupiter}{%
+\k@short@MassJupiter}
+\else
+\DeclareRobustCommand {\kMassJupiter}{%
+\k@full@MassJupiter}
+\fi
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@short@MassJupiterNumeric}
+% \changes{v1.1.0}{2020/02/03}{Add mass of Jupiter}
+% |\k@short@MassJupiterNumeric| is the mass of Jupiter with reduced precision.
+% Source: IAU~Resolution~B3~2015
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@short@MassJupiterNumeric}{%
+\ensuremath{%
+1.90e+27}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@full@MassJupiterNumeric}
+% \changes{v1.1.0}{2020/02/03}{Add mass of Jupiter}
+% |\k@full@MassJupiterNumeric| is the mass of Jupiter with full precision.
+% Source: IAU~Resolution~B3~2015
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@full@MassJupiterNumeric}{%
+\ensuremath{%
+1.8981246e+27}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\kMassJupiterNumeric}
+% \changes{v1.1.0}{2020/02/03}{Add mass of Jupiter}
+% |\kMassJupiterNumeric| is the mass of Jupiter.
+%
+%    \begin{macrocode}
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kMassJupiterNumeric}{%
+\k@short@MassJupiterNumeric}
+\else
+\DeclareRobustCommand {\kMassJupiterNumeric}{%
+\k@full@MassJupiterNumeric}
+\fi
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
 % \begin{macro}{\k@SI@short@MassAMU}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % |\k@SI@short@MassAMU| is the mass of an atomic mass unit in SI units with
 % reduced precision.
 % Source: CODATA~2018
@@ -3160,7 +7028,7 @@
 \DeclareRobustCommand{\k@SI@short@MassAMU}{%
 \ensuremath{%
 1.66%
-\times 10^{-30}\kg}}
+\times 10^{-27}\kg}}
 %    \end{macrocode}
 % \end{macro}
 %
@@ -3171,6 +7039,8 @@
 %<*package>
 %\fi
 % \begin{macro}{\k@SI@full@MassAMU}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % |\k@SI@full@MassAMU| is the mass of an atomic mass unit in SI units with full
 % precision.
 % Source: CODATA~2018
@@ -3182,7 +7052,7 @@
 465\expandafter\physconst@decimalsseparator%
 492\expandafter\physconst@decimalsseparator%
 239%
-\times 10^{-30}\kg}}
+\times 10^{-27}\kg}}
 %    \end{macrocode}
 % \end{macro}
 %
@@ -3193,6 +7063,8 @@
 %<*package>
 %\fi
 % \begin{macro}{\k@cgs@short@MassAMU}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % |\k@cgs@short@MassAMU| is the mass of an atomic mass unit in cgs units with
 % reduced precision.
 % Source: CODATA~2018
@@ -3201,7 +7073,7 @@
 \DeclareRobustCommand{\k@cgs@short@MassAMU}{%
 \ensuremath{%
 1.66%
-\times 10^{-27}\gm}}
+\times 10^{-24}\gm}}
 %    \end{macrocode}
 % \end{macro}
 %
@@ -3212,6 +7084,8 @@
 %<*package>
 %\fi
 % \begin{macro}{\k@cgs@full@MassAMU}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % |\k@cgs@full@MassAMU| is the mass of an atomic mass unit in cgs units with
 % full precision.
 % Source: CODATA~2018
@@ -3223,7 +7097,7 @@
 465\expandafter\physconst@decimalsseparator%
 492\expandafter\physconst@decimalsseparator%
 239%
-\times 10^{-27}\gm}}
+\times 10^{-24}\gm}}
 %    \end{macrocode}
 % \end{macro}
 %
@@ -3234,6 +7108,8 @@
 %<*package>
 %\fi
 % \begin{macro}{\k@eV@short@MassAMU}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % |\k@eV@short@MassAMU| is the mass of an atomic mass unit in eV with reduced
 % precision.
 % Source: CODATA~2018
@@ -3241,8 +7117,8 @@
 %    \begin{macrocode}
 \DeclareRobustCommand{\k@eV@short@MassAMU}{%
 \ensuremath{%
-1.04%
-\times 10^{-15}\eV\,c^{-2}}}
+9.31%
+\times 10^{8}\eV\,c^{-2}}}
 %    \end{macrocode}
 % \end{macro}
 %
@@ -3253,6 +7129,8 @@
 %<*package>
 %\fi
 % \begin{macro}{\k@eV@full@MassAMU}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % |\k@eV@full@MassAMU| is the mass of an atomic mass unit in eV with full
 % precision.
 % Source: CODATA~2018
@@ -3260,11 +7138,11 @@
 %    \begin{macrocode}
 \DeclareRobustCommand{\k@eV@full@MassAMU}{%
 \ensuremath{%
-1.036\expandafter\physconst@decimalsseparator%
-381\expandafter\physconst@decimalsseparator%
-043\expandafter\physconst@decimalsseparator%
-764%
-\times 10^{-15}\eV\,c^{-2}}}
+9.314\expandafter\physconst@decimalsseparator%
+528\expandafter\physconst@decimalsseparator%
+302\expandafter\physconst@decimalsseparator%
+276%
+\times 10^{8}\eV\,c^{-2}}}
 %    \end{macrocode}
 % \end{macro}
 %
@@ -3275,6 +7153,8 @@
 %<*package>
 %\fi
 % \begin{macro}{\kMassAMU}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % |\kMassAMU| is the mass of an atomic mass unit.
 %
 %    \begin{macrocode}
@@ -3305,6 +7185,8 @@
 %<*package>
 %\fi
 % \begin{macro}{\keVMassAMU}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
 % |\keVMassAMU| is the mass of an atomic mass unit.
 %
 %    \begin{macrocode}
@@ -3321,6 +7203,180 @@
 %\iffalse
 %</package>
 %\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@SI@short@MassAMUNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% |\k@SI@short@MassAMUNumeric| is the mass of an atomic mass unit in SI units with
+% reduced precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@SI@short@MassAMUNumeric}{%
+\ensuremath{%
+1.66e-27}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@SI@full@MassAMUNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% |\k@SI@full@MassAMUNumeric| is the mass of an atomic mass unit in SI units with full
+% precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@SI@full@MassAMUNumeric}{%
+\ensuremath{%
+1.660465492239e-27}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@cgs@short@MassAMUNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% |\k@cgs@short@MassAMUNumeric| is the mass of an atomic mass unit in cgs units with
+% reduced precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@cgs@short@MassAMUNumeric}{%
+\ensuremath{%
+1.66e-24}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@cgs@full@MassAMUNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% |\k@cgs@full@MassAMUNumeric| is the mass of an atomic mass unit in cgs units with
+% full precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@cgs@full@MassAMUNumeric}{%
+\ensuremath{%
+1.660465492239e-24}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@eV@short@MassAMUNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% |\k@eV@short@MassAMUNumeric| is the mass of an atomic mass unit in eV with reduced
+% precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@eV@short@MassAMUNumeric}{%
+\ensuremath{%
+9.31e+08}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@eV@full@MassAMUNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% |\k@eV@full@MassAMUNumeric| is the mass of an atomic mass unit in eV with full
+% precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@eV@full@MassAMUNumeric}{%
+\ensuremath{%
+9.314528302276e+08}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\kMassAMUNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% |\kMassAMUNumeric| is the mass of an atomic mass unit.
+%
+%    \begin{macrocode}
+\ifx\cgsunits\undefined
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kMassAMUNumeric}{%
+\k@SI@short@MassAMUNumeric}
+\else
+\DeclareRobustCommand {\kMassAMUNumeric}{%
+\k@SI@full@MassAMUNumeric}
+\fi
+\else
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kMassAMUNumeric}{%
+\k@cgs@short@MassAMUNumeric}
+\else
+\DeclareRobustCommand {\kMassAMUNumeric}{%
+\k@cgs@full@MassAMUNumeric}
+\fi
+\fi
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\keVMassAMUNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% \changes{v1.1.0}{2020/02/03}{Correct value in eV.}
+% |\keVMassAMUNumeric| is the mass of an atomic mass unit.
+%
+%    \begin{macrocode}
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\keVMassAMUNumeric}{%
+\k@eV@short@MassAMUNumeric}
+\else
+\DeclareRobustCommand {\keVMassAMUNumeric}{%
+\k@eV@full@MassAMUNumeric}
+\fi
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
 %
 %\subsection{Charge}
 %
@@ -3437,6 +7493,108 @@
 %\iffalse
 %<*package>
 %\fi
+% \begin{macro}{\k@SI@short@ChargeFundamentalNumeric}
+% |\k@SI@short@ChargeFundamentalNumeric| is the fundamental charge in SI units with
+% reduced precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@SI@short@ChargeFundamentalNumeric}{%
+\ensuremath{%
+1.60e-19}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@SI@full@ChargeFundamentalNumeric}
+% |\k@SI@full@ChargeFundamentalNumeric| is the fundamental charge in SI units with
+% full precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@SI@full@ChargeFundamentalNumeric}{%
+\ensuremath{%
+1.602176634e-19}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@cgs@short@ChargeFundamentalNumeric}
+% |\k@cgs@short@ChargeFundamentalNumeric| is the fundamental charge in cgs units with
+% reduced precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@cgs@short@ChargeFundamentalNumeric}{%
+\ensuremath{%
+4.80e-10}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@cgs@full@ChargeFundamentalNumeric}
+% |\k@cgs@full@ChargeFundamentalNumeric| is the fundamental charge in cgs units with
+% full precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@cgs@full@ChargeFundamentalNumeric}{%
+\ensuremath{%
+4.803204713e-10}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\kChargeFundamentalNumeric}
+% |\kChargeFundamentalNumeric| is the fundamental charge.
+%
+%    \begin{macrocode}
+\ifx\cgsunits\undefined
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kChargeFundamentalNumeric}{%
+\k@SI@short@ChargeFundamentalNumeric}
+\else
+\DeclareRobustCommand {\kChargeFundamentalNumeric}{%
+\k@SI@full@ChargeFundamentalNumeric}
+\fi
+\else
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kChargeFundamentalNumeric}{%
+\k@cgs@short@ChargeFundamentalNumeric}
+\else
+\DeclareRobustCommand {\kChargeFundamentalNumeric}{%
+\k@cgs@full@ChargeFundamentalNumeric}
+\fi
+\fi
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
 % \begin{macro}{\k@SI@short@ChargeElectron}
 % |\k@SI@short@ChargeElectron| is the charge of an electron in SI units with
 % reduced precision.
@@ -3547,6 +7705,108 @@
 %\iffalse
 %<*package>
 %\fi
+% \begin{macro}{\k@SI@short@ChargeElectronNumeric}
+% |\k@SI@short@ChargeElectronNumeric| is the charge of an electron in SI units with
+% reduced precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@SI@short@ChargeElectronNumeric}{%
+\ensuremath{%
+-1.60e-19}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@SI@full@ChargeElectronNumeric}
+% |\k@SI@full@ChargeElectronNumeric| is the charge of an electron in SI units with
+% full precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@SI@full@ChargeElectronNumeric}{%
+\ensuremath{%
+-1.602176634e-19}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@cgs@short@ChargeElectronNumeric}
+% |\k@cgs@short@ChargeElectronNumeric| is the charge of an electron in cgs units with
+% reduced precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@cgs@short@ChargeElectronNumeric}{%
+\ensuremath{%
+-4.80e-10}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@cgs@full@ChargeElectronNumeric}
+% |\k@cgs@full@ChargeElectronNumeric| is the charge of an electron in cgs units with
+% full precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@cgs@full@ChargeElectronNumeric}{%
+\ensuremath{%
+-4.803204713e-10}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\kChargeElectronNumeric}
+% |\kChargeElectronNumeric| is the charge of an electron.
+%
+%    \begin{macrocode}
+\ifx\cgsunits\undefined
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kChargeElectronNumeric}{%
+\k@SI@short@ChargeElectronNumeric}
+\else
+\DeclareRobustCommand {\kChargeElectronNumeric}{%
+\k@SI@full@ChargeElectronNumeric}
+\fi
+\else
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kChargeElectronNumeric}{%
+\k@cgs@short@ChargeElectronNumeric}
+\else
+\DeclareRobustCommand {\kChargeElectronNumeric}{%
+\k@cgs@full@ChargeElectronNumeric}
+\fi
+\fi
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
 % \begin{macro}{\k@SI@short@ChargeProton}
 % |\k@SI@short@ChargeProton| is the charge of a proton in SI units with reduced
 % precision.
@@ -3654,6 +7914,108 @@
 %\iffalse
 %</package>
 %\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@SI@short@ChargeProtonNumeric}
+% |\k@SI@short@ChargeProtonNumeric| is the charge of a proton in SI units with reduced
+% precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@SI@short@ChargeProtonNumeric}{%
+\ensuremath{%
+1.60e-19}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@SI@full@ChargeProtonNumeric}
+% |\k@SI@full@ChargeProtonNumeric| is the charge of a proton in SI units with full
+% precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@SI@full@ChargeProtonNumeric}{%
+\ensuremath{%
+1.602176634e-19}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@cgs@short@ChargeProtonNumeric}
+% |\k@cgs@short@ChargeProtonNumeric| is the charge of a proton in cgs units with
+% reduced precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@cgs@short@ChargeProtonNumeric}{%
+\ensuremath{%
+4.80e-10}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@cgs@full@ChargeProtonNumeric}
+% |\k@cgs@full@ChargeProtonNumeric| is the charge of a proton in cgs units with full
+% precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@cgs@full@ChargeProtonNumeric}{%
+\ensuremath{%
+4.803204713e-10}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\kChargeProtonNumeric}
+% |\kChargeProtonNumeric| is the charge of a proton.
+%
+%    \begin{macrocode}
+\ifx\cgsunits\undefined
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kChargeProtonNumeric}{%
+\k@SI@short@ChargeProtonNumeric}
+\else
+\DeclareRobustCommand {\kChargeProtonNumeric}{%
+\k@SI@full@ChargeProtonNumeric}
+\fi
+\else
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kChargeProtonNumeric}{%
+\k@cgs@short@ChargeProtonNumeric}
+\else
+\DeclareRobustCommand {\kChargeProtonNumeric}{%
+\k@cgs@full@ChargeProtonNumeric}
+\fi
+\fi
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
 %
 %\subsection{Distances and Lengths}
 %
@@ -3669,7 +8031,7 @@
 \DeclareRobustCommand{\k@SI@short@RadiusBohr}{%
 \ensuremath{%
 5.29%
-\times 10^{-8}\m}}
+\times 10^{-11}\m}}
 %    \end{macrocode}
 % \end{macro}
 %
@@ -3690,7 +8052,7 @@
 5.292\expandafter\physconst@decimalsseparator%
 006\expandafter\physconst@decimalsseparator%
 59%
-\times 10^{-8}\m}}
+\times 10^{-11}\m}}
 %    \end{macrocode}
 % \end{macro}
 %
@@ -3709,7 +8071,7 @@
 \DeclareRobustCommand{\k@cgs@short@RadiusBohr}{%
 \ensuremath{%
 5.29%
-\times 10^{-6}\cm}}
+\times 10^{-9}\cm}}
 %    \end{macrocode}
 % \end{macro}
 %
@@ -3730,7 +8092,7 @@
 5.292\expandafter\physconst@decimalsseparator%
 006\expandafter\physconst@decimalsseparator%
 59%
-\times 10^{-6}\cm}}
+\times 10^{-9}\cm}}
 %    \end{macrocode}
 % \end{macro}
 %
@@ -3770,6 +8132,108 @@
 %\iffalse
 %<*package>
 %\fi
+% \begin{macro}{\k@SI@short@RadiusBohrNumeric}
+% |\k@SI@short@RadiusBohrNumeric| is Bohr radius of an atom in SI units with reduced
+% precision.
+% Source: Calculated
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@SI@short@RadiusBohrNumeric}{%
+\ensuremath{%
+5.29e-11}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@SI@full@RadiusBohrNumeric}
+% |\k@SI@full@RadiusBohrNumeric| is Bohr radius of an atom in SI units with full
+% precision.
+% Source: Calculated
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@SI@full@RadiusBohrNumeric}{%
+\ensuremath{%
+5.29200659e-11}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@cgs@short@RadiusBohrNumeric}
+% |\k@cgs@short@RadiusBohrNumeric| is Bohr radius of an atom in cgs units with reduced
+% precision.
+% Source: Calculated
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@cgs@short@RadiusBohrNumeric}{%
+\ensuremath{%
+5.29e-09}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@cgs@full@RadiusBohrNumeric}
+% |\k@cgs@full@RadiusBohrNumeric| is Bohr radius of an atom in cgs units with full
+% precision.
+% Source: Calculated
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@cgs@full@RadiusBohrNumeric}{%
+\ensuremath{%
+5.29200659e-09}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\kRadiusBohrNumeric}
+% |\kRadiusBohrNumeric| is Bohr radius of an atom.
+%
+%    \begin{macrocode}
+\ifx\cgsunits\undefined
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kRadiusBohrNumeric}{%
+\k@SI@short@RadiusBohrNumeric}
+\else
+\DeclareRobustCommand {\kRadiusBohrNumeric}{%
+\k@SI@full@RadiusBohrNumeric}
+\fi
+\else
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kRadiusBohrNumeric}{%
+\k@cgs@short@RadiusBohrNumeric}
+\else
+\DeclareRobustCommand {\kRadiusBohrNumeric}{%
+\k@cgs@full@RadiusBohrNumeric}
+\fi
+\fi
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
 % \begin{macro}{\k@SI@short@AstronomicalUnit}
 % |\k@SI@short@AstronomicalUnit| is the astronomical unit (the average distance
 % between the Earth and the Sun) in SI units with reduced precision.
@@ -3881,6 +8345,109 @@
 %\iffalse
 %<*package>
 %\fi
+% \begin{macro}{\k@SI@short@AstronomicalUnitNumeric}
+% |\k@SI@short@AstronomicalUnitNumeric| is the astronomical unit (the average distance
+% between the Earth and the Sun) in SI units with reduced precision.
+% Source: IAU~Resolution~B2~2012
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@SI@short@AstronomicalUnitNumeric}{%
+\ensuremath{%
+1.50e+11}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@SI@full@AstronomicalUnitNumeric}
+% |\k@SI@full@AstronomicalUnitNumeric| is the astronomical unit (the average distance
+% between the Earth and the Sun) in SI units with full precision.
+% Source: IAU~Resolution~B2~2012
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@SI@full@AstronomicalUnitNumeric}{%
+\ensuremath{%
+1.495978707e+11}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@cgs@short@AstronomicalUnitNumeric}
+% |\k@cgs@short@AstronomicalUnitNumeric| is the astronomical unit (the average
+% distance between the Earth and the Sun) in cgs units with reduced precision.
+% Source: IAU~Resolution~B2~2012
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@cgs@short@AstronomicalUnitNumeric}{%
+\ensuremath{%
+1.50e+13}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@cgs@full@AstronomicalUnitNumeric}
+% |\k@cgs@full@AstronomicalUnitNumeric| is the astronomical unit (the average distance
+% between the Earth and the Sun) in cgs units with full precision.
+% Source: IAU~Resolution~B2~2012
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@cgs@full@AstronomicalUnitNumeric}{%
+\ensuremath{%
+1.495978707e+13}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\kAstronomicalUnitNumeric}
+% |\kAstronomicalUnitNumeric| is the astronomical unit (the average distance between
+% the Earth and the Sun).
+%
+%    \begin{macrocode}
+\ifx\cgsunits\undefined
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kAstronomicalUnitNumeric}{%
+\k@SI@short@AstronomicalUnitNumeric}
+\else
+\DeclareRobustCommand {\kAstronomicalUnitNumeric}{%
+\k@SI@full@AstronomicalUnitNumeric}
+\fi
+\else
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kAstronomicalUnitNumeric}{%
+\k@cgs@short@AstronomicalUnitNumeric}
+\else
+\DeclareRobustCommand {\kAstronomicalUnitNumeric}{%
+\k@cgs@full@AstronomicalUnitNumeric}
+\fi
+\fi
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
 % \begin{macro}{\k@SI@short@Parsec}
 % |\k@SI@short@Parsec| is the length of a parsec ($\frac{648000\au}{\pi}$) in
 % SI units with reduced precision.
@@ -3991,6 +8558,108 @@
 %\iffalse
 %<*package>
 %\fi
+% \begin{macro}{\k@SI@short@ParsecNumeric}
+% |\k@SI@short@ParsecNumeric| is the length of a parsec ($\frac{648000\au}{\pi}$) in
+% SI units with reduced precision.
+% Source: Calculated
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@SI@short@ParsecNumeric}{%
+\ensuremath{%
+3.09e+16}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@SI@full@ParsecNumeric}
+% |\k@SI@full@ParsecNumeric| is the length of a parsec ($\frac{648000\au}{\pi}$) in SI
+% units with full precision.
+% Source: Calculated
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@SI@full@ParsecNumeric}{%
+\ensuremath{%
+3.085677581e+16}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@cgs@short@ParsecNumeric}
+% |\k@cgs@short@ParsecNumeric| is the length of a parsec ($\frac{648000\au}{\pi}$) in
+% cgs units with reduced precision.
+% Source: Calculated
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@cgs@short@ParsecNumeric}{%
+\ensuremath{%
+3.09e+18}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@cgs@full@ParsecNumeric}
+% |\k@cgs@full@ParsecNumeric| is the length of a parsec ($\frac{648000\au}{\pi}$) in
+% cgs units with full precision.
+% Source: Calculated
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@cgs@full@ParsecNumeric}{%
+\ensuremath{%
+3.085677581e+18}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\kParsecNumeric}
+% |\kParsecNumeric| is the length of a parsec ($\frac{648000\au}{\pi}$).
+%
+%    \begin{macrocode}
+\ifx\cgsunits\undefined
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kParsecNumeric}{%
+\k@SI@short@ParsecNumeric}
+\else
+\DeclareRobustCommand {\kParsecNumeric}{%
+\k@SI@full@ParsecNumeric}
+\fi
+\else
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kParsecNumeric}{%
+\k@cgs@short@ParsecNumeric}
+\else
+\DeclareRobustCommand {\kParsecNumeric}{%
+\k@cgs@full@ParsecNumeric}
+\fi
+\fi
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
 % \begin{macro}{\k@SI@short@RadiusSun}
 % |\k@SI@short@RadiusSun| is the mean radius of the Sun in SI units with
 % reduced precision.
@@ -4094,6 +8763,342 @@
 %\iffalse
 %</package>
 %\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@SI@short@RadiusSunNumeric}
+% |\k@SI@short@RadiusSunNumeric| is the mean radius of the Sun in SI units with
+% reduced precision.
+% Source: IAU~Resolution~B3~2015
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@SI@short@RadiusSunNumeric}{%
+\ensuremath{%
+6.96e+08}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@SI@full@RadiusSunNumeric}
+% |\k@SI@full@RadiusSunNumeric| is the mean radius of the Sun in SI units with full
+% precision.
+% Source: IAU~Resolution~B3~2015
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@SI@full@RadiusSunNumeric}{%
+\ensuremath{%
+6.957e+08}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@cgs@short@RadiusSunNumeric}
+% |\k@cgs@short@RadiusSunNumeric| is the mean radius of the Sun in cgs units with
+% reduced precision.
+% Source: IAU~Resolution~B3~2015
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@cgs@short@RadiusSunNumeric}{%
+\ensuremath{%
+6.96e+10}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@cgs@full@RadiusSunNumeric}
+% |\k@cgs@full@RadiusSunNumeric| is the mean radius of the Sun in cgs units with full
+% precision.
+% Source: IAU~Resolution~B3~2015
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@cgs@full@RadiusSunNumeric}{%
+\ensuremath{%
+6.957e+10}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\kRadiusSunNumeric}
+% |\kRadiusSunNumeric| is the mean radius of the Sun.
+%
+%    \begin{macrocode}
+\ifx\cgsunits\undefined
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kRadiusSunNumeric}{%
+\k@SI@short@RadiusSunNumeric}
+\else
+\DeclareRobustCommand {\kRadiusSunNumeric}{%
+\k@SI@full@RadiusSunNumeric}
+\fi
+\else
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kRadiusSunNumeric}{%
+\k@cgs@short@RadiusSunNumeric}
+\else
+\DeclareRobustCommand {\kRadiusSunNumeric}{%
+\k@cgs@full@RadiusSunNumeric}
+\fi
+\fi
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@short@RadiusEarth}
+% \changes{v1.1.0}{2020/02/03}{Add radius of Earth}
+% |\k@short@RadiusEarth| is the mean radius of the Earth with reduced precision.
+% Source: IAU~Resolution~B3~2015
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@short@RadiusEarth}{%
+\ensuremath{%
+6.37%
+\times 10^{6}\m}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@full@RadiusEarth}
+% \changes{v1.1.0}{2020/02/03}{Add radius of Earth}
+% |\k@full@RadiusEarth| is the mean radius of the Earth with full precision.
+% Source: IAU~Resolution~B3~2015
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@full@RadiusEarth}{%
+\ensuremath{%
+6.371\expandafter\physconst@decimalsseparator%
+0%
+\times 10^{6}\m}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\kRadiusEarth}
+% \changes{v1.1.0}{2020/02/03}{Add radius of Earth}
+% |\kRadiusEarth| is the mean radius of the Earth.
+%
+%    \begin{macrocode}
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kRadiusEarth}{%
+\k@short@RadiusEarth}
+\else
+\DeclareRobustCommand {\kRadiusEarth}{%
+\k@full@RadiusEarth}
+\fi
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@short@RadiusEarthNumeric}
+% \changes{v1.1.0}{2020/02/03}{Add radius of Earth}
+% |\k@short@RadiusEarthNumeric| is the mean radius of the Earth with reduced precision.
+% Source: IAU~Resolution~B3~2015
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@short@RadiusEarthNumeric}{%
+\ensuremath{%
+6.37e+06}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@full@RadiusEarthNumeric}
+% \changes{v1.1.0}{2020/02/03}{Add radius of Earth}
+% |\k@full@RadiusEarthNumeric| is the mean radius of the Earth with full precision.
+% Source: IAU~Resolution~B3~2015
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@full@RadiusEarthNumeric}{%
+\ensuremath{%
+6.3710e+06}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\kRadiusEarthNumeric}
+% \changes{v1.1.0}{2020/02/03}{Add radius of Earth}
+% |\kRadiusEarthNumeric| is the mean radius of the Earth.
+%
+%    \begin{macrocode}
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kRadiusEarthNumeric}{%
+\k@short@RadiusEarthNumeric}
+\else
+\DeclareRobustCommand {\kRadiusEarthNumeric}{%
+\k@full@RadiusEarthNumeric}
+\fi
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@short@RadiusJupiter}
+% \changes{v1.1.0}{2020/02/03}{Add radius of Jupiter}
+% |\k@short@RadiusJupiter| is the mean radius of Jupiter with reduced precision.
+% Source: IAU~Resolution~B3~2015
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@short@RadiusJupiter}{%
+\ensuremath{%
+6.99%
+\times 10^{7}\m}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@full@RadiusJupiter}
+% \changes{v1.1.0}{2020/02/03}{Add radius of Jupiter}
+% |\k@full@RadiusJupiter| is the mean radius of Jupiter with full precision.
+% Source: IAU~Resolution~B3~2015
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@full@RadiusJupiter}{%
+\ensuremath{%
+6.991\expandafter\physconst@decimalsseparator%
+1%
+\times 10^{7}\m}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\kRadiusJupiter}
+% \changes{v1.1.0}{2020/02/03}{Add radius of Jupiter}
+% |\kRadiusJupiter| is the mean radius of Jupiter.
+%
+%    \begin{macrocode}
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kRadiusJupiter}{%
+\k@short@RadiusJupiter}
+\else
+\DeclareRobustCommand {\kRadiusJupiter}{%
+\k@full@RadiusJupiter}
+\fi
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@short@RadiusJupiterNumeric}
+% \changes{v1.1.0}{2020/02/03}{Add radius of Jupiter}
+% |\k@short@RadiusJupiterNumeric| is the mean radius of Jupiter with reduced precision.
+% Source: IAU~Resolution~B3~2015
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@short@RadiusJupiterNumeric}{%
+\ensuremath{%
+6.99e+07}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@full@RadiusJupiterNumeric}
+% \changes{v1.1.0}{2020/02/03}{Add radius of Jupiter}
+% |\k@full@RadiusJupiterNumeric| is the mean radius of Jupiter with full precision.
+% Source: IAU~Resolution~B3~2015
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@full@RadiusJupiterNumeric}{%
+\ensuremath{%
+6.9911e+07}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\kRadiusJupiterNumeric}
+% \changes{v1.1.0}{2020/02/03}{Add radius of Jupiter}
+% |\kRadiusJupiterNumeric| is the mean radius of Jupiter.
+%
+%    \begin{macrocode}
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kRadiusJupiterNumeric}{%
+\k@short@RadiusJupiterNumeric}
+\else
+\DeclareRobustCommand {\kRadiusJupiterNumeric}{%
+\k@full@RadiusJupiterNumeric}
+\fi
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
 %
 %\subsection{Energy, Power, and Luminosity}
 %
@@ -4109,7 +9114,7 @@
 \DeclareRobustCommand{\k@SI@short@Rydberg}{%
 \ensuremath{%
 2.18%
-\times 10^{-21}\Joule}}
+\times 10^{-18}\Joule}}
 %    \end{macrocode}
 % \end{macro}
 %
@@ -4130,7 +9135,7 @@
 2.179\expandafter\physconst@decimalsseparator%
 775\expandafter\physconst@decimalsseparator%
 77%
-\times 10^{-21}\Joule}}
+\times 10^{-18}\Joule}}
 %    \end{macrocode}
 % \end{macro}
 %
@@ -4149,7 +9154,7 @@
 \DeclareRobustCommand{\k@cgs@short@Rydberg}{%
 \ensuremath{%
 2.18%
-\times 10^{-14}\erg}}
+\times 10^{-11}\erg}}
 %    \end{macrocode}
 % \end{macro}
 %
@@ -4170,7 +9175,7 @@
 2.179\expandafter\physconst@decimalsseparator%
 775\expandafter\physconst@decimalsseparator%
 77%
-\times 10^{-14}\erg}}
+\times 10^{-11}\erg}}
 %    \end{macrocode}
 % \end{macro}
 %
@@ -4189,7 +9194,7 @@
 \DeclareRobustCommand{\k@eV@short@Rydberg}{%
 \ensuremath{%
 1.36%
-\times 10^{-2}\eV}}
+\times 10^{1}\eV}}
 %    \end{macrocode}
 % \end{macro}
 %
@@ -4210,7 +9215,7 @@
 1.360\expandafter\physconst@decimalsseparator%
 509\expandafter\physconst@decimalsseparator%
 03%
-\times 10^{-2}\eV}}
+\times 10^{1}\eV}}
 %    \end{macrocode}
 % \end{macro}
 %
@@ -4270,6 +9275,164 @@
 %\iffalse
 %<*package>
 %\fi
+% \begin{macro}{\k@SI@short@RydbergNumeric}
+% |\k@SI@short@RydbergNumeric| is the Rydberg energy (the binding energy of Hydrogen)
+% in SI units with reduced precision.
+% Source: Calculated
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@SI@short@RydbergNumeric}{%
+\ensuremath{%
+2.18e-18}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@SI@full@RydbergNumeric}
+% |\k@SI@full@RydbergNumeric| is the Rydberg energy (the binding energy of Hydrogen)
+% in SI units with full precision.
+% Source: Calculated
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@SI@full@RydbergNumeric}{%
+\ensuremath{%
+2.17977577e-18}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@cgs@short@RydbergNumeric}
+% |\k@cgs@short@RydbergNumeric| is the Rydberg energy (the binding energy of Hydrogen)
+% in cgs units with reduced precision.
+% Source: Calculated
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@cgs@short@RydbergNumeric}{%
+\ensuremath{%
+2.18e-11}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@cgs@full@RydbergNumeric}
+% |\k@cgs@full@RydbergNumeric| is the Rydberg energy (the binding energy of Hydrogen)
+% in cgs units with full precision.
+% Source: Calculated
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@cgs@full@RydbergNumeric}{%
+\ensuremath{%
+2.17977577e-11}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@eV@short@RydbergNumeric}
+% |\k@eV@short@RydbergNumeric| is the Rydberg energy (the binding energy of Hydrogen)
+% in eV with reduced precision.
+% Source: Calculated
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@eV@short@RydbergNumeric}{%
+\ensuremath{%
+1.36e+01}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@eV@full@RydbergNumeric}
+% |\k@eV@full@RydbergNumeric| is the Rydberg energy (the binding energy of Hydrogen)
+% in eV with full precision.
+% Source: Calculated
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@eV@full@RydbergNumeric}{%
+\ensuremath{%
+1.36050903e+01}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\kRydbergNumeric}
+% |\kRydbergNumeric| is the Rydberg energy (the binding energy of Hydrogen).
+%
+%    \begin{macrocode}
+\ifx\cgsunits\undefined
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kRydbergNumeric}{%
+\k@SI@short@RydbergNumeric}
+\else
+\DeclareRobustCommand {\kRydbergNumeric}{%
+\k@SI@full@RydbergNumeric}
+\fi
+\else
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kRydbergNumeric}{%
+\k@cgs@short@RydbergNumeric}
+\else
+\DeclareRobustCommand {\kRydbergNumeric}{%
+\k@cgs@full@RydbergNumeric}
+\fi
+\fi
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\keVRydbergNumeric}
+% |\keVRydbergNumeric| is the Rydberg energy (the binding energy of Hydrogen).
+%
+%    \begin{macrocode}
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\keVRydbergNumeric}{%
+\k@eV@short@RydbergNumeric}
+\else
+\DeclareRobustCommand {\keVRydbergNumeric}{%
+\k@eV@full@RydbergNumeric}
+\fi
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
 % \begin{macro}{\k@SI@short@LuminositySun}
 % |\k@SI@short@LuminositySun| is the luminosity of the Sun in SI units with
 % reduced precision.
@@ -4373,6 +9536,108 @@
 %\iffalse
 %</package>
 %\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@SI@short@LuminositySunNumeric}
+% |\k@SI@short@LuminositySunNumeric| is the luminosity of the Sun in SI units with
+% reduced precision.
+% Source: IAU~Resolution~B3~2015
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@SI@short@LuminositySunNumeric}{%
+\ensuremath{%
+3.83e+26}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@SI@full@LuminositySunNumeric}
+% |\k@SI@full@LuminositySunNumeric| is the luminosity of the Sun in SI units with full
+% precision.
+% Source: IAU~Resolution~B3~2015
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@SI@full@LuminositySunNumeric}{%
+\ensuremath{%
+3.828e+26}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@cgs@short@LuminositySunNumeric}
+% |\k@cgs@short@LuminositySunNumeric| is the luminosity of the Sun in cgs units with
+% reduced precision.
+% Source: IAU~Resolution~B3~2015
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@cgs@short@LuminositySunNumeric}{%
+\ensuremath{%
+3.83e+33}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@cgs@full@LuminositySunNumeric}
+% |\k@cgs@full@LuminositySunNumeric| is the luminosity of the Sun in cgs units with
+% full precision.
+% Source: IAU~Resolution~B3~2015
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@cgs@full@LuminositySunNumeric}{%
+\ensuremath{%
+3.828e+33}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\kLuminositySunNumeric}
+% |\kLuminositySunNumeric| is the luminosity of the Sun.
+%
+%    \begin{macrocode}
+\ifx\cgsunits\undefined
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kLuminositySunNumeric}{%
+\k@SI@short@LuminositySunNumeric}
+\else
+\DeclareRobustCommand {\kLuminositySunNumeric}{%
+\k@SI@full@LuminositySunNumeric}
+\fi
+\else
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kLuminositySunNumeric}{%
+\k@cgs@short@LuminositySunNumeric}
+\else
+\DeclareRobustCommand {\kLuminositySunNumeric}{%
+\k@cgs@full@LuminositySunNumeric}
+\fi
+\fi
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
 %
 %\subsection{Pressure}
 %
@@ -4380,6 +9645,7 @@
 %<*package>
 %\fi
 % \begin{macro}{\k@SI@short@PressureAtmosphere}
+% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.}
 % |\k@SI@short@PressureAtmosphere| is the standard atmospheric pressure in SI
 % units with reduced precision.
 % Source: CODATA~2018
@@ -4399,6 +9665,7 @@
 %<*package>
 %\fi
 % \begin{macro}{\k@SI@full@PressureAtmosphere}
+% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.}
 % |\k@SI@full@PressureAtmosphere| is the standard atmospheric pressure in SI
 % units with full precision.
 % Source: CODATA~2018
@@ -4419,6 +9686,7 @@
 %<*package>
 %\fi
 % \begin{macro}{\k@cgs@short@PressureAtmosphere}
+% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.}
 % |\k@cgs@short@PressureAtmosphere| is the standard atmospheric pressure in cgs
 % units with reduced precision.
 % Source: CODATA~2018
@@ -4426,7 +9694,7 @@
 %    \begin{macrocode}
 \DeclareRobustCommand{\k@cgs@short@PressureAtmosphere}{%
 \ensuremath{%
-1.01\barP[m]}}
+1.01\barP}}
 %    \end{macrocode}
 % \end{macro}
 %
@@ -4437,6 +9705,7 @@
 %<*package>
 %\fi
 % \begin{macro}{\k@cgs@full@PressureAtmosphere}
+% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.}
 % |\k@cgs@full@PressureAtmosphere| is the standard atmospheric pressure in cgs
 % units with full precision.
 % Source: CODATA~2018
@@ -4445,7 +9714,7 @@
 \DeclareRobustCommand{\k@cgs@full@PressureAtmosphere}{%
 \ensuremath{%
 1.013\expandafter\physconst@decimalsseparator%
-25\barP[m]}}
+25\barP}}
 %    \end{macrocode}
 % \end{macro}
 %
@@ -4456,6 +9725,7 @@
 %<*package>
 %\fi
 % \begin{macro}{\kPressureAtmosphere}
+% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.}
 % |\kPressureAtmosphere| is the standard atmospheric pressure.
 %
 %    \begin{macrocode}
@@ -4485,7 +9755,115 @@
 %\iffalse
 %<*package>
 %\fi
+% \begin{macro}{\k@SI@short@PressureAtmosphereNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.}
+% |\k@SI@short@PressureAtmosphereNumeric| is the standard atmospheric pressure in SI
+% units with reduced precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@SI@short@PressureAtmosphereNumeric}{%
+\ensuremath{%
+1.01e+05}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@SI@full@PressureAtmosphereNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.}
+% |\k@SI@full@PressureAtmosphereNumeric| is the standard atmospheric pressure in SI
+% units with full precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@SI@full@PressureAtmosphereNumeric}{%
+\ensuremath{%
+1.01325e+05}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@cgs@short@PressureAtmosphereNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.}
+% |\k@cgs@short@PressureAtmosphereNumeric| is the standard atmospheric pressure in cgs
+% units with reduced precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@cgs@short@PressureAtmosphereNumeric}{%
+\ensuremath{%
+1.01e+00}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@cgs@full@PressureAtmosphereNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.}
+% |\k@cgs@full@PressureAtmosphereNumeric| is the standard atmospheric pressure in cgs
+% units with full precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@cgs@full@PressureAtmosphereNumeric}{%
+\ensuremath{%
+1.01325e+00}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\kPressureAtmosphereNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.}
+% |\kPressureAtmosphereNumeric| is the standard atmospheric pressure.
+%
+%    \begin{macrocode}
+\ifx\cgsunits\undefined
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kPressureAtmosphereNumeric}{%
+\k@SI@short@PressureAtmosphereNumeric}
+\else
+\DeclareRobustCommand {\kPressureAtmosphereNumeric}{%
+\k@SI@full@PressureAtmosphereNumeric}
+\fi
+\else
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kPressureAtmosphereNumeric}{%
+\k@cgs@short@PressureAtmosphereNumeric}
+\else
+\DeclareRobustCommand {\kPressureAtmosphereNumeric}{%
+\k@cgs@full@PressureAtmosphereNumeric}
+\fi
+\fi
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
 % \begin{macro}{\k@SI@short@PressureStandard}
+% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.}
 % |\k@SI@short@PressureStandard| is the standard atmospheric pressure in SI
 % units with reduced precision.
 % Source: CODATA~2018
@@ -4505,6 +9883,7 @@
 %<*package>
 %\fi
 % \begin{macro}{\k@SI@full@PressureStandard}
+% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.}
 % |\k@SI@full@PressureStandard| is the standard atmospheric pressure in SI
 % units with full precision.
 % Source: CODATA~2018
@@ -4525,6 +9904,7 @@
 %<*package>
 %\fi
 % \begin{macro}{\k@cgs@short@PressureStandard}
+% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.}
 % |\k@cgs@short@PressureStandard| is the standard atmospheric pressure in cgs
 % units with reduced precision.
 % Source: CODATA~2018
@@ -4532,7 +9912,7 @@
 %    \begin{macrocode}
 \DeclareRobustCommand{\k@cgs@short@PressureStandard}{%
 \ensuremath{%
-1.00\barP[m]}}
+1.00\barP}}
 %    \end{macrocode}
 % \end{macro}
 %
@@ -4543,6 +9923,7 @@
 %<*package>
 %\fi
 % \begin{macro}{\k@cgs@full@PressureStandard}
+% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.}
 % |\k@cgs@full@PressureStandard| is the standard atmospheric pressure in cgs
 % units with full precision.
 % Source: CODATA~2018
@@ -4551,7 +9932,7 @@
 \DeclareRobustCommand{\k@cgs@full@PressureStandard}{%
 \ensuremath{%
 1.000\expandafter\physconst@decimalsseparator%
-00\barP[m]}}
+00\barP}}
 %    \end{macrocode}
 % \end{macro}
 %
@@ -4562,6 +9943,7 @@
 %<*package>
 %\fi
 % \begin{macro}{\kPressureStandard}
+% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.}
 % |\kPressureStandard| is the standard atmospheric pressure.
 %
 %    \begin{macrocode}
@@ -4588,6 +9970,113 @@
 %\iffalse
 %</package>
 %\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@SI@short@PressureStandardNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.}
+% |\k@SI@short@PressureStandardNumeric| is the standard atmospheric pressure in SI
+% units with reduced precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@SI@short@PressureStandardNumeric}{%
+\ensuremath{%
+1.00e+05}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@SI@full@PressureStandardNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.}
+% |\k@SI@full@PressureStandardNumeric| is the standard atmospheric pressure in SI
+% units with full precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@SI@full@PressureStandardNumeric}{%
+\ensuremath{%
+1.00000e+05}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@cgs@short@PressureStandardNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.}
+% |\k@cgs@short@PressureStandardNumeric| is the standard atmospheric pressure in cgs
+% units with reduced precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@cgs@short@PressureStandardNumeric}{%
+\ensuremath{%
+1.00e+00}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@cgs@full@PressureStandardNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.}
+% |\k@cgs@full@PressureStandardNumeric| is the standard atmospheric pressure in cgs
+% units with full precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@cgs@full@PressureStandardNumeric}{%
+\ensuremath{%
+1.00000e+00}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\kPressureStandardNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.}
+% |\kPressureStandardNumeric| is the standard atmospheric pressure.
+%
+%    \begin{macrocode}
+\ifx\cgsunits\undefined
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kPressureStandardNumeric}{%
+\k@SI@short@PressureStandardNumeric}
+\else
+\DeclareRobustCommand {\kPressureStandardNumeric}{%
+\k@SI@full@PressureStandardNumeric}
+\fi
+\else
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kPressureStandardNumeric}{%
+\k@cgs@short@PressureStandardNumeric}
+\else
+\DeclareRobustCommand {\kPressureStandardNumeric}{%
+\k@cgs@full@PressureStandardNumeric}
+\fi
+\fi
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
 %
 %\subsection{Velocity, Speed and Acceleration}
 %
@@ -4703,7 +10192,110 @@
 %\iffalse
 %<*package>
 %\fi
+% \begin{macro}{\k@SI@short@SpeedLightNumeric}
+% |\k@SI@short@SpeedLightNumeric| is the speed of light in SI units with reduced
+% precision.
+% Source: CODATA 2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@SI@short@SpeedLightNumeric}{%
+\ensuremath{%
+3.00e+08}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@SI@full@SpeedLightNumeric}
+% |\k@SI@full@SpeedLightNumeric| is the speed of light in SI units with full precision.
+% Source: CODATA 2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@SI@full@SpeedLightNumeric}{%
+\ensuremath{%
+2.99792458e+08}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@cgs@short@SpeedLightNumeric}
+% |\k@cgs@short@SpeedLightNumeric| is the speed of light in cgs units with reduced
+% precision.
+% Source: CODATA 2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@cgs@short@SpeedLightNumeric}{%
+\ensuremath{%
+3.00e+10}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@cgs@full@SpeedLightNumeric}
+% |\k@cgs@full@SpeedLightNumeric| is the speed of light in cgs units with full
+% precision.
+% Source: CODATA 2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@cgs@full@SpeedLightNumeric}{%
+\ensuremath{%
+2.99792458e+10}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\kSpeedLightNumeric}
+% |\kSpeedLightNumeric| is the speed of light.
+%
+%    \begin{macrocode}
+\ifx\cgsunits\undefined
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kSpeedLightNumeric}{%
+\k@SI@short@SpeedLightNumeric}
+\else
+\DeclareRobustCommand {\kSpeedLightNumeric}{%
+\k@SI@full@SpeedLightNumeric}
+\fi
+\else
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kSpeedLightNumeric}{%
+\k@cgs@short@SpeedLightNumeric}
+\else
+\DeclareRobustCommand {\kSpeedLightNumeric}{%
+\k@cgs@full@SpeedLightNumeric}
+\fi
+\fi
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
 % \begin{macro}{\k@SI@short@AccelGravity}
+% \changes{v1.1.0}{2020/02/03}{Correct value.}
+% \changes{v1.1.0}{2020/02/03}{Fix units.}
 % |\k@SI@short@AccelGravity| is the accelertion due to gravity at the surface
 % of the Earth in SI units with reduced precision.
 % Source: CODATA 2018
@@ -4711,8 +10303,7 @@
 %    \begin{macrocode}
 \DeclareRobustCommand{\k@SI@short@AccelGravity}{%
 \ensuremath{%
-6.67%
-\times 10^{-11}\N\kg^{-2}\m^2}}
+9.81\m\Sec^{-2}}}
 %    \end{macrocode}
 % \end{macro}
 %
@@ -4723,6 +10314,8 @@
 %<*package>
 %\fi
 % \begin{macro}{\k@SI@full@AccelGravity}
+% \changes{v1.1.0}{2020/02/03}{Correct value.}
+% \changes{v1.1.0}{2020/02/03}{Fix units.}
 % |\k@SI@full@AccelGravity| is the accelertion due to gravity at the surface of
 % the Earth in SI units with full precision.
 % Source: CODATA 2018
@@ -4730,9 +10323,8 @@
 %    \begin{macrocode}
 \DeclareRobustCommand{\k@SI@full@AccelGravity}{%
 \ensuremath{%
-6.674\expandafter\physconst@decimalsseparator%
-30%
-\times 10^{-11}\N\kg^{-2}\m^2}}
+9.806\expandafter\physconst@decimalsseparator%
+65\m\Sec^{-2}}}
 %    \end{macrocode}
 % \end{macro}
 %
@@ -4743,6 +10335,8 @@
 %<*package>
 %\fi
 % \begin{macro}{\k@cgs@short@AccelGravity}
+% \changes{v1.1.0}{2020/02/03}{Correct value.}
+% \changes{v1.1.0}{2020/02/03}{Fix units.}
 % |\k@cgs@short@AccelGravity| is the accelertion due to gravity at the surface
 % of the Earth in cgs units with reduced precision.
 % Source: CODATA 2018
@@ -4750,8 +10344,8 @@
 %    \begin{macrocode}
 \DeclareRobustCommand{\k@cgs@short@AccelGravity}{%
 \ensuremath{%
-6.67%
-\times 10^{-8}\dyne\gm^{-2}\cm^2}}
+9.81%
+\times 10^{2}\cm\Sec^{-2}}}
 %    \end{macrocode}
 % \end{macro}
 %
@@ -4762,6 +10356,8 @@
 %<*package>
 %\fi
 % \begin{macro}{\k@cgs@full@AccelGravity}
+% \changes{v1.1.0}{2020/02/03}{Correct value.}
+% \changes{v1.1.0}{2020/02/03}{Fix units.}
 % |\k@cgs@full@AccelGravity| is the accelertion due to gravity at the surface
 % of the Earth in cgs units with full precision.
 % Source: CODATA 2018
@@ -4769,9 +10365,9 @@
 %    \begin{macrocode}
 \DeclareRobustCommand{\k@cgs@full@AccelGravity}{%
 \ensuremath{%
-6.674\expandafter\physconst@decimalsseparator%
-30%
-\times 10^{-8}\dyne\gm^{-2}\cm^2}}
+9.806\expandafter\physconst@decimalsseparator%
+65%
+\times 10^{2}\cm\Sec^{-2}}}
 %    \end{macrocode}
 % \end{macro}
 %
@@ -4782,6 +10378,8 @@
 %<*package>
 %\fi
 % \begin{macro}{\kAccelGravity}
+% \changes{v1.1.0}{2020/02/03}{Correct value.}
+% \changes{v1.1.0}{2020/02/03}{Fix units.}
 % |\kAccelGravity| is the accelertion due to gravity at the surface of the
 % Earth.
 %
@@ -4809,6 +10407,119 @@
 %\iffalse
 %</package>
 %\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@SI@short@AccelGravityNumeric}
+% \changes{v1.1.0}{2020/02/03}{Correct value.}
+% \changes{v1.1.0}{2020/02/03}{Fix units.}
+% |\k@SI@short@AccelGravityNumeric| is the accelertion due to gravity at the surface
+% of the Earth in SI units with reduced precision.
+% Source: CODATA 2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@SI@short@AccelGravityNumeric}{%
+\ensuremath{%
+9.81e+00}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@SI@full@AccelGravityNumeric}
+% \changes{v1.1.0}{2020/02/03}{Correct value.}
+% \changes{v1.1.0}{2020/02/03}{Fix units.}
+% |\k@SI@full@AccelGravityNumeric| is the accelertion due to gravity at the surface of
+% the Earth in SI units with full precision.
+% Source: CODATA 2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@SI@full@AccelGravityNumeric}{%
+\ensuremath{%
+9.80665e+00}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@cgs@short@AccelGravityNumeric}
+% \changes{v1.1.0}{2020/02/03}{Correct value.}
+% \changes{v1.1.0}{2020/02/03}{Fix units.}
+% |\k@cgs@short@AccelGravityNumeric| is the accelertion due to gravity at the surface
+% of the Earth in cgs units with reduced precision.
+% Source: CODATA 2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@cgs@short@AccelGravityNumeric}{%
+\ensuremath{%
+9.81e+02}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@cgs@full@AccelGravityNumeric}
+% \changes{v1.1.0}{2020/02/03}{Correct value.}
+% \changes{v1.1.0}{2020/02/03}{Fix units.}
+% |\k@cgs@full@AccelGravityNumeric| is the accelertion due to gravity at the surface
+% of the Earth in cgs units with full precision.
+% Source: CODATA 2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@cgs@full@AccelGravityNumeric}{%
+\ensuremath{%
+9.80665e+02}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\kAccelGravityNumeric}
+% \changes{v1.1.0}{2020/02/03}{Correct value.}
+% \changes{v1.1.0}{2020/02/03}{Fix units.}
+% |\kAccelGravityNumeric| is the accelertion due to gravity at the surface of the
+% Earth.
+%
+%    \begin{macrocode}
+\ifx\cgsunits\undefined
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kAccelGravityNumeric}{%
+\k@SI@short@AccelGravityNumeric}
+\else
+\DeclareRobustCommand {\kAccelGravityNumeric}{%
+\k@SI@full@AccelGravityNumeric}
+\fi
+\else
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kAccelGravityNumeric}{%
+\k@cgs@short@AccelGravityNumeric}
+\else
+\DeclareRobustCommand {\kAccelGravityNumeric}{%
+\k@cgs@full@AccelGravityNumeric}
+\fi
+\fi
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
 %
 %\subsection{Other Constants}
 %
@@ -4816,6 +10527,7 @@
 %<*package>
 %\fi
 % \begin{macro}{\k@SI@short@Coulomb}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
 % |\k@SI@short@Coulomb| is the Coulomb constant ($\frac{1}{4\pi\epsilon_0}$) in
 % SI units with reduced precision.
 % Source: Calculated
@@ -4824,7 +10536,7 @@
 \DeclareRobustCommand{\k@SI@short@Coulomb}{%
 \ensuremath{%
 8.99%
-\times 10^{13}\N\m^2\Coulomb^{-2}}}
+\times 10^{9}\N\m^2\Coulomb^{-2}}}
 %    \end{macrocode}
 % \end{macro}
 %
@@ -4835,6 +10547,7 @@
 %<*package>
 %\fi
 % \begin{macro}{\k@SI@full@Coulomb}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
 % |\k@SI@full@Coulomb| is the Coulomb constant ($\frac{1}{4\pi\epsilon_0}$) in
 % SI units with full precision.
 % Source: Calculated
@@ -4845,7 +10558,7 @@
 8.987\expandafter\physconst@decimalsseparator%
 551\expandafter\physconst@decimalsseparator%
 79%
-\times 10^{13}\N\m^2\Coulomb^{-2}}}
+\times 10^{9}\N\m^2\Coulomb^{-2}}}
 %    \end{macrocode}
 % \end{macro}
 %
@@ -4856,6 +10569,7 @@
 %<*package>
 %\fi
 % \begin{macro}{\k@cgs@short@Coulomb}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
 % |\k@cgs@short@Coulomb| is the Coulomb constant ($\frac{1}{4\pi\epsilon_0}$)
 % in cgs units with reduced precision.
 % Source: Calculated
@@ -4874,6 +10588,7 @@
 %<*package>
 %\fi
 % \begin{macro}{\k@cgs@full@Coulomb}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
 % |\k@cgs@full@Coulomb| is the Coulomb constant ($\frac{1}{4\pi\epsilon_0}$) in
 % cgs units with full precision.
 % Source: Calculated
@@ -4894,6 +10609,7 @@
 %<*package>
 %\fi
 % \begin{macro}{\kCoulomb}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
 % |\kCoulomb| is the Coulomb constant ($\frac{1}{4\pi\epsilon_0}$).
 %
 %    \begin{macrocode}
@@ -4923,6 +10639,113 @@
 %\iffalse
 %<*package>
 %\fi
+% \begin{macro}{\k@SI@short@CoulombNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% |\k@SI@short@CoulombNumeric| is the Coulomb constant ($\frac{1}{4\pi\epsilon_0}$) in
+% SI units with reduced precision.
+% Source: Calculated
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@SI@short@CoulombNumeric}{%
+\ensuremath{%
+8.99e+09}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@SI@full@CoulombNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% |\k@SI@full@CoulombNumeric| is the Coulomb constant ($\frac{1}{4\pi\epsilon_0}$) in
+% SI units with full precision.
+% Source: Calculated
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@SI@full@CoulombNumeric}{%
+\ensuremath{%
+8.98755179e+09}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@cgs@short@CoulombNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% |\k@cgs@short@CoulombNumeric| is the Coulomb constant ($\frac{1}{4\pi\epsilon_0}$)
+% in cgs units with reduced precision.
+% Source: Calculated
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@cgs@short@CoulombNumeric}{%
+\ensuremath{%
+1.00e+00}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@cgs@full@CoulombNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% |\k@cgs@full@CoulombNumeric| is the Coulomb constant ($\frac{1}{4\pi\epsilon_0}$) in
+% cgs units with full precision.
+% Source: Calculated
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@cgs@full@CoulombNumeric}{%
+\ensuremath{%
+1.00000000e+00}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\kCoulombNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% |\kCoulombNumeric| is the Coulomb constant ($\frac{1}{4\pi\epsilon_0}$).
+%
+%    \begin{macrocode}
+\ifx\cgsunits\undefined
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kCoulombNumeric}{%
+\k@SI@short@CoulombNumeric}
+\else
+\DeclareRobustCommand {\kCoulombNumeric}{%
+\k@SI@full@CoulombNumeric}
+\fi
+\else
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kCoulombNumeric}{%
+\k@cgs@short@CoulombNumeric}
+\else
+\DeclareRobustCommand {\kCoulombNumeric}{%
+\k@cgs@full@CoulombNumeric}
+\fi
+\fi
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
 % \begin{macro}{\k@SI@short@VacuumPermittivity}
 % |\k@SI@short@VacuumPermittivity| is the electric permittivity of the vacuum
 % in SI units with reduced precision.
@@ -5035,16 +10858,119 @@
 %\iffalse
 %<*package>
 %\fi
+% \begin{macro}{\k@SI@short@VacuumPermittivityNumeric}
+% |\k@SI@short@VacuumPermittivityNumeric| is the electric permittivity of the vacuum
+% in SI units with reduced precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@SI@short@VacuumPermittivityNumeric}{%
+\ensuremath{%
+8.85e-12}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@SI@full@VacuumPermittivityNumeric}
+% |\k@SI@full@VacuumPermittivityNumeric| is the electric permittivity of the vacuum in
+% SI units with full precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@SI@full@VacuumPermittivityNumeric}{%
+\ensuremath{%
+8.8541878128e-12}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@cgs@short@VacuumPermittivityNumeric}
+% |\k@cgs@short@VacuumPermittivityNumeric| is the electric permittivity of the vacuum
+% in cgs units with reduced precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@cgs@short@VacuumPermittivityNumeric}{%
+\ensuremath{%
+7.96e-02}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@cgs@full@VacuumPermittivityNumeric}
+% |\k@cgs@full@VacuumPermittivityNumeric| is the electric permittivity of the vacuum
+% in cgs units with full precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@cgs@full@VacuumPermittivityNumeric}{%
+\ensuremath{%
+7.9577471546e-02}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\kVacuumPermittivityNumeric}
+% |\kVacuumPermittivityNumeric| is the electric permittivity of the vacuum.
+%
+%    \begin{macrocode}
+\ifx\cgsunits\undefined
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kVacuumPermittivityNumeric}{%
+\k@SI@short@VacuumPermittivityNumeric}
+\else
+\DeclareRobustCommand {\kVacuumPermittivityNumeric}{%
+\k@SI@full@VacuumPermittivityNumeric}
+\fi
+\else
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kVacuumPermittivityNumeric}{%
+\k@cgs@short@VacuumPermittivityNumeric}
+\else
+\DeclareRobustCommand {\kVacuumPermittivityNumeric}{%
+\k@cgs@full@VacuumPermittivityNumeric}
+\fi
+\fi
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
 % \begin{macro}{\k@SI@short@VacuumPermeability}
+% \changes{v1.1.0}{2020/02/03}{Fix value of constant.}
 % |\k@SI@short@VacuumPermeability| is the magnetic permeability of the vacuum
 % in SI units with reduced precision.
-% Source: CODATA~2018
+% Source: Calculated
 %
 %    \begin{macrocode}
 \DeclareRobustCommand{\k@SI@short@VacuumPermeability}{%
 \ensuremath{%
-8.85%
-\times 10^{-12}\N\Amp^{-2}}}
+1.26%
+\times 10^{-6}\N\Amp^{-2}}}
 %    \end{macrocode}
 % \end{macro}
 %
@@ -5055,18 +10981,19 @@
 %<*package>
 %\fi
 % \begin{macro}{\k@SI@full@VacuumPermeability}
+% \changes{v1.1.0}{2020/02/03}{Fix value of constant.}
 % |\k@SI@full@VacuumPermeability| is the magnetic permeability of the vacuum in
 % SI units with full precision.
-% Source: CODATA~2018
+% Source: Calculated
 %
 %    \begin{macrocode}
 \DeclareRobustCommand{\k@SI@full@VacuumPermeability}{%
 \ensuremath{%
-8.854\expandafter\physconst@decimalsseparator%
-187\expandafter\physconst@decimalsseparator%
-812\expandafter\physconst@decimalsseparator%
-8%
-\times 10^{-12}\N\Amp^{-2}}}
+1.256\expandafter\physconst@decimalsseparator%
+637\expandafter\physconst@decimalsseparator%
+062\expandafter\physconst@decimalsseparator%
+1%
+\times 10^{-6}\N\Amp^{-2}}}
 %    \end{macrocode}
 % \end{macro}
 %
@@ -5077,9 +11004,10 @@
 %<*package>
 %\fi
 % \begin{macro}{\k@cgs@short@VacuumPermeability}
+% \changes{v1.1.0}{2020/02/03}{Fix value of constant.}
 % |\k@cgs@short@VacuumPermeability| is the magnetic permeability of the vacuum
 % in cgs units with reduced precision.
-% Source: CODATA~2018
+% Source: Calculated
 %
 %    \begin{macrocode}
 \DeclareRobustCommand{\k@cgs@short@VacuumPermeability}{%
@@ -5096,9 +11024,10 @@
 %<*package>
 %\fi
 % \begin{macro}{\k@cgs@full@VacuumPermeability}
+% \changes{v1.1.0}{2020/02/03}{Fix value of constant.}
 % |\k@cgs@full@VacuumPermeability| is the magnetic permeability of the vacuum
 % in cgs units with full precision.
-% Source: CODATA~2018
+% Source: Calculated
 %
 %    \begin{macrocode}
 \DeclareRobustCommand{\k@cgs@full@VacuumPermeability}{%
@@ -5118,6 +11047,7 @@
 %<*package>
 %\fi
 % \begin{macro}{\kVacuumPermeability}
+% \changes{v1.1.0}{2020/02/03}{Fix value of constant.}
 % |\kVacuumPermeability| is the magnetic permeability of the vacuum.
 %
 %    \begin{macrocode}
@@ -5147,6 +11077,113 @@
 %\iffalse
 %<*package>
 %\fi
+% \begin{macro}{\k@SI@short@VacuumPermeabilityNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix value of constant.}
+% |\k@SI@short@VacuumPermeabilityNumeric| is the magnetic permeability of the vacuum
+% in SI units with reduced precision.
+% Source: Calculated
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@SI@short@VacuumPermeabilityNumeric}{%
+\ensuremath{%
+1.26e-06}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@SI@full@VacuumPermeabilityNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix value of constant.}
+% |\k@SI@full@VacuumPermeabilityNumeric| is the magnetic permeability of the vacuum in
+% SI units with full precision.
+% Source: Calculated
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@SI@full@VacuumPermeabilityNumeric}{%
+\ensuremath{%
+1.2566370621e-06}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@cgs@short@VacuumPermeabilityNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix value of constant.}
+% |\k@cgs@short@VacuumPermeabilityNumeric| is the magnetic permeability of the vacuum
+% in cgs units with reduced precision.
+% Source: Calculated
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@cgs@short@VacuumPermeabilityNumeric}{%
+\ensuremath{%
+1.26e+01}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@cgs@full@VacuumPermeabilityNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix value of constant.}
+% |\k@cgs@full@VacuumPermeabilityNumeric| is the magnetic permeability of the vacuum
+% in cgs units with full precision.
+% Source: Calculated
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@cgs@full@VacuumPermeabilityNumeric}{%
+\ensuremath{%
+1.2566370614e+01}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\kVacuumPermeabilityNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix value of constant.}
+% |\kVacuumPermeabilityNumeric| is the magnetic permeability of the vacuum.
+%
+%    \begin{macrocode}
+\ifx\cgsunits\undefined
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kVacuumPermeabilityNumeric}{%
+\k@SI@short@VacuumPermeabilityNumeric}
+\else
+\DeclareRobustCommand {\kVacuumPermeabilityNumeric}{%
+\k@SI@full@VacuumPermeabilityNumeric}
+\fi
+\else
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kVacuumPermeabilityNumeric}{%
+\k@cgs@short@VacuumPermeabilityNumeric}
+\else
+\DeclareRobustCommand {\kVacuumPermeabilityNumeric}{%
+\k@cgs@full@VacuumPermeabilityNumeric}
+\fi
+\fi
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
 % \begin{macro}{\k@short@VacuumImpedance}
 % |\k@short@VacuumImpedance| is the characteristic impedance of the vacuum with
 % reduced precision.
@@ -5208,6 +11245,62 @@
 %\iffalse
 %<*package>
 %\fi
+% \begin{macro}{\k@short@VacuumImpedanceNumeric}
+% |\k@short@VacuumImpedanceNumeric| is the characteristic impedance of the vacuum with
+% reduced precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@short@VacuumImpedanceNumeric}{%
+\ensuremath{%
+3.77e+02}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@full@VacuumImpedanceNumeric}
+% |\k@full@VacuumImpedanceNumeric| is the characteristic impedance of the vacuum with
+% full precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@full@VacuumImpedanceNumeric}{%
+\ensuremath{%
+3.76730313668e+02}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\kVacuumImpedanceNumeric}
+% |\kVacuumImpedanceNumeric| is the characteristic impedance of the vacuum.
+%
+%    \begin{macrocode}
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kVacuumImpedanceNumeric}{%
+\k@short@VacuumImpedanceNumeric}
+\else
+\DeclareRobustCommand {\kVacuumImpedanceNumeric}{%
+\k@full@VacuumImpedanceNumeric}
+\fi
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
 % \begin{macro}{\k@SI@short@Boltzmann}
 % |\k@SI@short@Boltzmann| is the Boltzmann constant in SI units with reduced
 % precision.
@@ -5374,7 +11467,165 @@
 %\iffalse
 %<*package>
 %\fi
+% \begin{macro}{\k@SI@short@BoltzmannNumeric}
+% |\k@SI@short@BoltzmannNumeric| is the Boltzmann constant in SI units with reduced
+% precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@SI@short@BoltzmannNumeric}{%
+\ensuremath{%
+1.38e-23}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@SI@full@BoltzmannNumeric}
+% |\k@SI@full@BoltzmannNumeric| is the Boltzmann constant in SI units with full
+% precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@SI@full@BoltzmannNumeric}{%
+\ensuremath{%
+1.380649e-23}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@cgs@short@BoltzmannNumeric}
+% |\k@cgs@short@BoltzmannNumeric| is the Boltzmann constant in cgs units with reduced
+% precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@cgs@short@BoltzmannNumeric}{%
+\ensuremath{%
+1.38e-16}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@cgs@full@BoltzmannNumeric}
+% |\k@cgs@full@BoltzmannNumeric| is the Boltzmann constant in cgs units with full
+% precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@cgs@full@BoltzmannNumeric}{%
+\ensuremath{%
+1.380649e-16}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@eV@short@BoltzmannNumeric}
+% |\k@eV@short@BoltzmannNumeric| is the Boltzmann constant in eV with reduced
+% precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@eV@short@BoltzmannNumeric}{%
+\ensuremath{%
+8.62e-05}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@eV@full@BoltzmannNumeric}
+% |\k@eV@full@BoltzmannNumeric| is the Boltzmann constant in eV with full precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@eV@full@BoltzmannNumeric}{%
+\ensuremath{%
+8.617333e-05}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\kBoltzmannNumeric}
+% |\kBoltzmannNumeric| is the Boltzmann constant.
+%
+%    \begin{macrocode}
+\ifx\cgsunits\undefined
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kBoltzmannNumeric}{%
+\k@SI@short@BoltzmannNumeric}
+\else
+\DeclareRobustCommand {\kBoltzmannNumeric}{%
+\k@SI@full@BoltzmannNumeric}
+\fi
+\else
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kBoltzmannNumeric}{%
+\k@cgs@short@BoltzmannNumeric}
+\else
+\DeclareRobustCommand {\kBoltzmannNumeric}{%
+\k@cgs@full@BoltzmannNumeric}
+\fi
+\fi
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\keVBoltzmannNumeric}
+% |\keVBoltzmannNumeric| is the Boltzmann constant.
+%
+%    \begin{macrocode}
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\keVBoltzmannNumeric}{%
+\k@eV@short@BoltzmannNumeric}
+\else
+\DeclareRobustCommand {\keVBoltzmannNumeric}{%
+\k@eV@full@BoltzmannNumeric}
+\fi
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
 % \begin{macro}{\k@SI@short@Planck}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
 % |\k@SI@short@Planck| is the Planck constant in SI units with reduced
 % precision.
 % Source: CODATA~2018
@@ -5394,6 +11645,7 @@
 %<*package>
 %\fi
 % \begin{macro}{\k@SI@full@Planck}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
 % |\k@SI@full@Planck| is the Planck constant in SI units with full precision.
 % Source: CODATA~2018
 %
@@ -5414,6 +11666,7 @@
 %<*package>
 %\fi
 % \begin{macro}{\k@cgs@short@Planck}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
 % |\k@cgs@short@Planck| is the Planck constant in cgs units with reduced
 % precision.
 % Source: CODATA~2018
@@ -5433,6 +11686,7 @@
 %<*package>
 %\fi
 % \begin{macro}{\k@cgs@full@Planck}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
 % |\k@cgs@full@Planck| is the Planck constant in cgs units with full precision.
 % Source: CODATA~2018
 %
@@ -5453,6 +11707,7 @@
 %<*package>
 %\fi
 % \begin{macro}{\k@eV@short@Planck}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
 % |\k@eV@short@Planck| is the Planck constant in eV with reduced precision.
 % Source: CODATA~2018
 %
@@ -5471,6 +11726,7 @@
 %<*package>
 %\fi
 % \begin{macro}{\k@eV@full@Planck}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
 % |\k@eV@full@Planck| is the Planck constant in eV with full precision.
 % Source: CODATA~2018
 %
@@ -5491,6 +11747,7 @@
 %<*package>
 %\fi
 % \begin{macro}{\kPlanck}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
 % |\kPlanck| is the Planck constant.
 %
 %    \begin{macrocode}
@@ -5521,6 +11778,7 @@
 %<*package>
 %\fi
 % \begin{macro}{\keVPlanck}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
 % |\keVPlanck| is the Planck constant.
 %
 %    \begin{macrocode}
@@ -5540,7 +11798,170 @@
 %\iffalse
 %<*package>
 %\fi
+% \begin{macro}{\k@SI@short@PlanckNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% |\k@SI@short@PlanckNumeric| is the Planck constant in SI units with reduced
+% precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@SI@short@PlanckNumeric}{%
+\ensuremath{%
+6.63e-34}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@SI@full@PlanckNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% |\k@SI@full@PlanckNumeric| is the Planck constant in SI units with full precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@SI@full@PlanckNumeric}{%
+\ensuremath{%
+6.62607015e-34}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@cgs@short@PlanckNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% |\k@cgs@short@PlanckNumeric| is the Planck constant in cgs units with reduced
+% precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@cgs@short@PlanckNumeric}{%
+\ensuremath{%
+6.63e-27}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@cgs@full@PlanckNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% |\k@cgs@full@PlanckNumeric| is the Planck constant in cgs units with full precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@cgs@full@PlanckNumeric}{%
+\ensuremath{%
+6.62607015e-27}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@eV@short@PlanckNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% |\k@eV@short@PlanckNumeric| is the Planck constant in eV with reduced precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@eV@short@PlanckNumeric}{%
+\ensuremath{%
+4.14e-15}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@eV@full@PlanckNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% |\k@eV@full@PlanckNumeric| is the Planck constant in eV with full precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@eV@full@PlanckNumeric}{%
+\ensuremath{%
+4.13566770e-15}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\kPlanckNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% |\kPlanckNumeric| is the Planck constant.
+%
+%    \begin{macrocode}
+\ifx\cgsunits\undefined
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kPlanckNumeric}{%
+\k@SI@short@PlanckNumeric}
+\else
+\DeclareRobustCommand {\kPlanckNumeric}{%
+\k@SI@full@PlanckNumeric}
+\fi
+\else
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kPlanckNumeric}{%
+\k@cgs@short@PlanckNumeric}
+\else
+\DeclareRobustCommand {\kPlanckNumeric}{%
+\k@cgs@full@PlanckNumeric}
+\fi
+\fi
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\keVPlanckNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% |\keVPlanckNumeric| is the Planck constant.
+%
+%    \begin{macrocode}
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\keVPlanckNumeric}{%
+\k@eV@short@PlanckNumeric}
+\else
+\DeclareRobustCommand {\keVPlanckNumeric}{%
+\k@eV@full@PlanckNumeric}
+\fi
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
 % \begin{macro}{\k@SI@short@PlanckReduced}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
 % |\k@SI@short@PlanckReduced| is the Reduced Planck constant
 % $\left(\frac{h}{2\pi}\right)$ in SI units with reduced precision.
 % Source: Calculated
@@ -5560,6 +11981,7 @@
 %<*package>
 %\fi
 % \begin{macro}{\k@SI@full@PlanckReduced}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
 % |\k@SI@full@PlanckReduced| is the Reduced Planck constant
 % $\left(\frac{h}{2\pi}\right)$ in SI units with full precision.
 % Source: Calculated
@@ -5581,6 +12003,7 @@
 %<*package>
 %\fi
 % \begin{macro}{\k@cgs@short@PlanckReduced}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
 % |\k@cgs@short@PlanckReduced| is the Reduced Planck constant
 % $\left(\frac{h}{2\pi}\right)$ in cgs units with reduced precision.
 % Source: Calculated
@@ -5600,6 +12023,7 @@
 %<*package>
 %\fi
 % \begin{macro}{\k@cgs@full@PlanckReduced}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
 % |\k@cgs@full@PlanckReduced| is the Reduced Planck constant
 % $\left(\frac{h}{2\pi}\right)$ in cgs units with full precision.
 % Source: Calculated
@@ -5621,6 +12045,7 @@
 %<*package>
 %\fi
 % \begin{macro}{\k@eV@short@PlanckReduced}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
 % |\k@eV@short@PlanckReduced| is the Reduced Planck constant
 % $\left(\frac{h}{2\pi}\right)$ in eV with reduced precision.
 % Source: Calculated
@@ -5640,6 +12065,7 @@
 %<*package>
 %\fi
 % \begin{macro}{\k@eV@full@PlanckReduced}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
 % |\k@eV@full@PlanckReduced| is the Reduced Planck constant
 % $\left(\frac{h}{2\pi}\right)$ in eV with full precision.
 % Source: Calculated
@@ -5661,6 +12087,7 @@
 %<*package>
 %\fi
 % \begin{macro}{\kPlanckReduced}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
 % |\kPlanckReduced| is the Reduced Planck constant
 % $\left(\frac{h}{2\pi}\right)$.
 %
@@ -5692,6 +12119,7 @@
 %<*package>
 %\fi
 % \begin{macro}{\keVPlanckReduced}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
 % |\keVPlanckReduced| is the Reduced Planck constant
 % $\left(\frac{h}{2\pi}\right)$.
 %
@@ -5712,7 +12140,176 @@
 %\iffalse
 %<*package>
 %\fi
+% \begin{macro}{\k@SI@short@PlanckReducedNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% |\k@SI@short@PlanckReducedNumeric| is the Reduced Planck constant
+% $\left(\frac{h}{2\pi}\right)$ in SI units with reduced precision.
+% Source: Calculated
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@SI@short@PlanckReducedNumeric}{%
+\ensuremath{%
+1.05e-34}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@SI@full@PlanckReducedNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% |\k@SI@full@PlanckReducedNumeric| is the Reduced Planck constant
+% $\left(\frac{h}{2\pi}\right)$ in SI units with full precision.
+% Source: Calculated
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@SI@full@PlanckReducedNumeric}{%
+\ensuremath{%
+1.05457182e-34}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@cgs@short@PlanckReducedNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% |\k@cgs@short@PlanckReducedNumeric| is the Reduced Planck constant
+% $\left(\frac{h}{2\pi}\right)$ in cgs units with reduced precision.
+% Source: Calculated
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@cgs@short@PlanckReducedNumeric}{%
+\ensuremath{%
+1.05e-27}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@cgs@full@PlanckReducedNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% |\k@cgs@full@PlanckReducedNumeric| is the Reduced Planck constant
+% $\left(\frac{h}{2\pi}\right)$ in cgs units with full precision.
+% Source: Calculated
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@cgs@full@PlanckReducedNumeric}{%
+\ensuremath{%
+1.05457182e-27}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@eV@short@PlanckReducedNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% |\k@eV@short@PlanckReducedNumeric| is the Reduced Planck constant
+% $\left(\frac{h}{2\pi}\right)$ in eV with reduced precision.
+% Source: Calculated
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@eV@short@PlanckReducedNumeric}{%
+\ensuremath{%
+6.58e-16}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@eV@full@PlanckReducedNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% |\k@eV@full@PlanckReducedNumeric| is the Reduced Planck constant
+% $\left(\frac{h}{2\pi}\right)$ in eV with full precision.
+% Source: Calculated
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@eV@full@PlanckReducedNumeric}{%
+\ensuremath{%
+6.58211957e-16}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\kPlanckReducedNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% |\kPlanckReducedNumeric| is the Reduced Planck constant
+% $\left(\frac{h}{2\pi}\right)$.
+%
+%    \begin{macrocode}
+\ifx\cgsunits\undefined
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kPlanckReducedNumeric}{%
+\k@SI@short@PlanckReducedNumeric}
+\else
+\DeclareRobustCommand {\kPlanckReducedNumeric}{%
+\k@SI@full@PlanckReducedNumeric}
+\fi
+\else
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kPlanckReducedNumeric}{%
+\k@cgs@short@PlanckReducedNumeric}
+\else
+\DeclareRobustCommand {\kPlanckReducedNumeric}{%
+\k@cgs@full@PlanckReducedNumeric}
+\fi
+\fi
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\keVPlanckReducedNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% |\keVPlanckReducedNumeric| is the Reduced Planck constant
+% $\left(\frac{h}{2\pi}\right)$.
+%
+%    \begin{macrocode}
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\keVPlanckReducedNumeric}{%
+\k@eV@short@PlanckReducedNumeric}
+\else
+\DeclareRobustCommand {\keVPlanckReducedNumeric}{%
+\k@eV@full@PlanckReducedNumeric}
+\fi
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
 % \begin{macro}{\k@SI@short@Gravity}
+% \changes{v1.1.0}{2020/02/03}{Fix value of constant.}
 % |\k@SI@short@Gravity| is Newton's gravitational constant in SI units with
 % reduced precision.
 % Source: CODATA~2018
@@ -5721,7 +12318,7 @@
 \DeclareRobustCommand{\k@SI@short@Gravity}{%
 \ensuremath{%
 6.67%
-\times 10^{-15}\N\kg^{-2}\m^2}}
+\times 10^{-11}\N\kg^{-2}\m^2}}
 %    \end{macrocode}
 % \end{macro}
 %
@@ -5732,6 +12329,7 @@
 %<*package>
 %\fi
 % \begin{macro}{\k@SI@full@Gravity}
+% \changes{v1.1.0}{2020/02/03}{Fix value of constant.}
 % |\k@SI@full@Gravity| is Newton's gravitational constant in SI units with full
 % precision.
 % Source: CODATA~2018
@@ -5741,7 +12339,7 @@
 \ensuremath{%
 6.674\expandafter\physconst@decimalsseparator%
 30%
-\times 10^{-15}\N\kg^{-2}\m^2}}
+\times 10^{-11}\N\kg^{-2}\m^2}}
 %    \end{macrocode}
 % \end{macro}
 %
@@ -5752,6 +12350,7 @@
 %<*package>
 %\fi
 % \begin{macro}{\k@cgs@short@Gravity}
+% \changes{v1.1.0}{2020/02/03}{Fix value of constant.}
 % |\k@cgs@short@Gravity| is Newton's gravitational constant in cgs units with
 % reduced precision.
 % Source: CODATA~2018
@@ -5771,6 +12370,7 @@
 %<*package>
 %\fi
 % \begin{macro}{\k@cgs@full@Gravity}
+% \changes{v1.1.0}{2020/02/03}{Fix value of constant.}
 % |\k@cgs@full@Gravity| is Newton's gravitational constant in cgs units with
 % full precision.
 % Source: CODATA~2018
@@ -5791,6 +12391,7 @@
 %<*package>
 %\fi
 % \begin{macro}{\kGravity}
+% \changes{v1.1.0}{2020/02/03}{Fix value of constant.}
 % |\kGravity| is Newton's gravitational constant.
 %
 %    \begin{macrocode}
@@ -5820,7 +12421,115 @@
 %\iffalse
 %<*package>
 %\fi
+% \begin{macro}{\k@SI@short@GravityNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix value of constant.}
+% |\k@SI@short@GravityNumeric| is Newton's gravitational constant in SI units with
+% reduced precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@SI@short@GravityNumeric}{%
+\ensuremath{%
+6.67e-11}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@SI@full@GravityNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix value of constant.}
+% |\k@SI@full@GravityNumeric| is Newton's gravitational constant in SI units with full
+% precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@SI@full@GravityNumeric}{%
+\ensuremath{%
+6.67430e-11}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@cgs@short@GravityNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix value of constant.}
+% |\k@cgs@short@GravityNumeric| is Newton's gravitational constant in cgs units with
+% reduced precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@cgs@short@GravityNumeric}{%
+\ensuremath{%
+6.67e-08}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@cgs@full@GravityNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix value of constant.}
+% |\k@cgs@full@GravityNumeric| is Newton's gravitational constant in cgs units with
+% full precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@cgs@full@GravityNumeric}{%
+\ensuremath{%
+6.67430e-08}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\kGravityNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix value of constant.}
+% |\kGravityNumeric| is Newton's gravitational constant.
+%
+%    \begin{macrocode}
+\ifx\cgsunits\undefined
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kGravityNumeric}{%
+\k@SI@short@GravityNumeric}
+\else
+\DeclareRobustCommand {\kGravityNumeric}{%
+\k@SI@full@GravityNumeric}
+\fi
+\else
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kGravityNumeric}{%
+\k@cgs@short@GravityNumeric}
+\else
+\DeclareRobustCommand {\kGravityNumeric}{%
+\k@cgs@full@GravityNumeric}
+\fi
+\fi
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
 % \begin{macro}{\k@SI@short@StefanBoltzmann}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
 % |\k@SI@short@StefanBoltzmann| is the Stefan-Boltzmann blackbody constant
 % $\left(\frac{2\pi^5k_\mathrm{B}}{15h^3c^2}\right)$ in SI units with reduced
 % precision.
@@ -5830,7 +12539,7 @@
 \DeclareRobustCommand{\k@SI@short@StefanBoltzmann}{%
 \ensuremath{%
 5.67%
-\times 10^{-6}\J\Kelvin^{-4}\m^{-2}\Sec^{-1}}}
+\times 10^{-8}\J\Kelvin^{-4}\m^{-2}\Sec^{-1}}}
 %    \end{macrocode}
 % \end{macro}
 %
@@ -5841,6 +12550,7 @@
 %<*package>
 %\fi
 % \begin{macro}{\k@SI@full@StefanBoltzmann}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
 % |\k@SI@full@StefanBoltzmann| is the Stefan-Boltzmann blackbody constant
 % $\left(\frac{2\pi^5k_\mathrm{B}}{15h^3c^2}\right)$ in SI units with full
 % precision.
@@ -5851,7 +12561,7 @@
 \ensuremath{%
 5.670\expandafter\physconst@decimalsseparator%
 374%
-\times 10^{-6}\J\Kelvin^{-4}\m^{-2}\Sec^{-1}}}
+\times 10^{-8}\J\Kelvin^{-4}\m^{-2}\Sec^{-1}}}
 %    \end{macrocode}
 % \end{macro}
 %
@@ -5862,6 +12572,7 @@
 %<*package>
 %\fi
 % \begin{macro}{\k@cgs@short@StefanBoltzmann}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
 % |\k@cgs@short@StefanBoltzmann| is the Stefan-Boltzmann blackbody constant
 % $\left(\frac{2\pi^5k_\mathrm{B}}{15h^3c^2}\right)$ in cgs units with reduced
 % precision.
@@ -5882,6 +12593,7 @@
 %<*package>
 %\fi
 % \begin{macro}{\k@cgs@full@StefanBoltzmann}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
 % |\k@cgs@full@StefanBoltzmann| is the Stefan-Boltzmann blackbody constant
 % $\left(\frac{2\pi^5k_\mathrm{B}}{15h^3c^2}\right)$ in cgs units with full
 % precision.
@@ -5903,6 +12615,7 @@
 %<*package>
 %\fi
 % \begin{macro}{\kStefanBoltzmann}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
 % |\kStefanBoltzmann| is the Stefan-Boltzmann blackbody constant
 % $\left(\frac{2\pi^5k_\mathrm{B}}{15h^3c^2}\right)$.
 %
@@ -5933,6 +12646,118 @@
 %\iffalse
 %<*package>
 %\fi
+% \begin{macro}{\k@SI@short@StefanBoltzmannNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% |\k@SI@short@StefanBoltzmannNumeric| is the Stefan-Boltzmann blackbody constant
+% $\left(\frac{2\pi^5k_\mathrm{B}}{15h^3c^2}\right)$ in SI units with reduced
+% precision.
+% Source: Calculated
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@SI@short@StefanBoltzmannNumeric}{%
+\ensuremath{%
+5.67e-08}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@SI@full@StefanBoltzmannNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% |\k@SI@full@StefanBoltzmannNumeric| is the Stefan-Boltzmann blackbody constant
+% $\left(\frac{2\pi^5k_\mathrm{B}}{15h^3c^2}\right)$ in SI units with full
+% precision.
+% Source: Calculated
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@SI@full@StefanBoltzmannNumeric}{%
+\ensuremath{%
+5.670374e-08}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@cgs@short@StefanBoltzmannNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% |\k@cgs@short@StefanBoltzmannNumeric| is the Stefan-Boltzmann blackbody constant
+% $\left(\frac{2\pi^5k_\mathrm{B}}{15h^3c^2}\right)$ in cgs units with reduced
+% precision.
+% Source: Calculated
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@cgs@short@StefanBoltzmannNumeric}{%
+\ensuremath{%
+5.67e-05}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@cgs@full@StefanBoltzmannNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% |\k@cgs@full@StefanBoltzmannNumeric| is the Stefan-Boltzmann blackbody constant
+% $\left(\frac{2\pi^5k_\mathrm{B}}{15h^3c^2}\right)$ in cgs units with full
+% precision.
+% Source: Calculated
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@cgs@full@StefanBoltzmannNumeric}{%
+\ensuremath{%
+5.670374e-05}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\kStefanBoltzmannNumeric}
+% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.}
+% |\kStefanBoltzmannNumeric| is the Stefan-Boltzmann blackbody constant
+% $\left(\frac{2\pi^5k_\mathrm{B}}{15h^3c^2}\right)$.
+%
+%    \begin{macrocode}
+\ifx\cgsunits\undefined
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kStefanBoltzmannNumeric}{%
+\k@SI@short@StefanBoltzmannNumeric}
+\else
+\DeclareRobustCommand {\kStefanBoltzmannNumeric}{%
+\k@SI@full@StefanBoltzmannNumeric}
+\fi
+\else
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kStefanBoltzmannNumeric}{%
+\k@cgs@short@StefanBoltzmannNumeric}
+\else
+\DeclareRobustCommand {\kStefanBoltzmannNumeric}{%
+\k@cgs@full@StefanBoltzmannNumeric}
+\fi
+\fi
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
 % \begin{macro}{\k@SI@short@Radiation}
 % |\k@SI@short@Radiation| is the radiation constant, $a
 % \left(\frac{8\pi^5k_\mathrm{B}^4}{15c^3h^3}\right)$ in SI units with reduced
@@ -6046,6 +12871,113 @@
 %\iffalse
 %<*package>
 %\fi
+% \begin{macro}{\k@SI@short@RadiationNumeric}
+% |\k@SI@short@RadiationNumeric| is the radiation constant, $a
+% \left(\frac{8\pi^5k_\mathrm{B}^4}{15c^3h^3}\right)$ in SI units with reduced
+% precision.
+% Source: Calculated
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@SI@short@RadiationNumeric}{%
+\ensuremath{%
+7.57e-16}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@SI@full@RadiationNumeric}
+% |\k@SI@full@RadiationNumeric| is the radiation constant, $a
+% \left(\frac{8\pi^5k_\mathrm{B}^4}{15c^3h^3}\right)$ in SI units with full
+% precision.
+% Source: Calculated
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@SI@full@RadiationNumeric}{%
+\ensuremath{%
+7.565733e-16}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@cgs@short@RadiationNumeric}
+% |\k@cgs@short@RadiationNumeric| is the radiation constant, $a
+% \left(\frac{8\pi^5k_\mathrm{B}^4}{15c^3h^3}\right)$ in cgs units with reduced
+% precision.
+% Source: Calculated
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@cgs@short@RadiationNumeric}{%
+\ensuremath{%
+7.57e-15}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@cgs@full@RadiationNumeric}
+% |\k@cgs@full@RadiationNumeric| is the radiation constant, $a
+% \left(\frac{8\pi^5k_\mathrm{B}^4}{15c^3h^3}\right)$ in cgs units with full
+% precision.
+% Source: Calculated
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@cgs@full@RadiationNumeric}{%
+\ensuremath{%
+7.565733e-15}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\kRadiationNumeric}
+% |\kRadiationNumeric| is the radiation constant, $a
+% \left(\frac{8\pi^5k_\mathrm{B}^4}{15c^3h^3}\right)$.
+%
+%    \begin{macrocode}
+\ifx\cgsunits\undefined
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kRadiationNumeric}{%
+\k@SI@short@RadiationNumeric}
+\else
+\DeclareRobustCommand {\kRadiationNumeric}{%
+\k@SI@full@RadiationNumeric}
+\fi
+\else
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kRadiationNumeric}{%
+\k@cgs@short@RadiationNumeric}
+\else
+\DeclareRobustCommand {\kRadiationNumeric}{%
+\k@cgs@full@RadiationNumeric}
+\fi
+\fi
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
 % \begin{macro}{\k@short@FineStructure}
 % |\k@short@FineStructure| is the fine structure constant with reduced
 % precision.
@@ -6105,6 +13037,61 @@
 %\iffalse
 %<*package>
 %\fi
+% \begin{macro}{\k@short@FineStructureNumeric}
+% |\k@short@FineStructureNumeric| is the fine structure constant with reduced
+% precision.
+% Source: Calculated
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@short@FineStructureNumeric}{%
+\ensuremath{%
+7.30e-03}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@full@FineStructureNumeric}
+% |\k@full@FineStructureNumeric| is the fine structure constant with full precision.
+% Source: Calculated
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@full@FineStructureNumeric}{%
+\ensuremath{%
+7.29735257e-03}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\kFineStructureNumeric}
+% |\kFineStructureNumeric| is the fine structure constant.
+%
+%    \begin{macrocode}
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kFineStructureNumeric}{%
+\k@short@FineStructureNumeric}
+\else
+\DeclareRobustCommand {\kFineStructureNumeric}{%
+\k@full@FineStructureNumeric}
+\fi
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
 % \begin{macro}{\k@short@FineStructureReciprocal}
 % |\k@short@FineStructureReciprocal| is the reciprocal of the fine structure
 % constant with reduced precision.
@@ -6165,6 +13152,62 @@
 %\iffalse
 %<*package>
 %\fi
+% \begin{macro}{\k@short@FineStructureReciprocalNumeric}
+% |\k@short@FineStructureReciprocalNumeric| is the reciprocal of the fine structure
+% constant with reduced precision.
+% Source: Calculated
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@short@FineStructureReciprocalNumeric}{%
+\ensuremath{%
+1.37e+02}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@full@FineStructureReciprocalNumeric}
+% |\k@full@FineStructureReciprocalNumeric| is the reciprocal of the fine structure
+% constant with full precision.
+% Source: Calculated
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@full@FineStructureReciprocalNumeric}{%
+\ensuremath{%
+1.37035999e+02}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\kFineStructureReciprocalNumeric}
+% |\kFineStructureReciprocalNumeric| is the reciprocal of the fine structure constant.
+%
+%    \begin{macrocode}
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kFineStructureReciprocalNumeric}{%
+\k@short@FineStructureReciprocalNumeric}
+\else
+\DeclareRobustCommand {\kFineStructureReciprocalNumeric}{%
+\k@full@FineStructureReciprocalNumeric}
+\fi
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
 % \begin{macro}{\k@short@Avogadro}
 % |\k@short@Avogadro| is Avogadro's Number (the number of particles in a mole)
 % with reduced precision.
@@ -6222,6 +13265,62 @@
 %\iffalse
 %</package>
 %\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@short@AvogadroNumeric}
+% |\k@short@AvogadroNumeric| is Avogadro's Number (the number of particles in a mole)
+% with reduced precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@short@AvogadroNumeric}{%
+\ensuremath{%
+6.02e+23}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\k@full@AvogadroNumeric}
+% |\k@full@AvogadroNumeric| is Avogadro's Number (the number of particles in a mole)
+% with full precision.
+% Source: CODATA~2018
+%
+%    \begin{macrocode}
+\DeclareRobustCommand{\k@full@AvogadroNumeric}{%
+\ensuremath{%
+6.02240760e+23}}
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
+%\iffalse
+%<*package>
+%\fi
+% \begin{macro}{\kAvogadroNumeric}
+% |\kAvogadroNumeric| is Avogadro's Number (the number of particles in a mole).
+%
+%    \begin{macrocode}
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kAvogadroNumeric}{%
+\k@short@AvogadroNumeric}
+\else
+\DeclareRobustCommand {\kAvogadroNumeric}{%
+\k@full@AvogadroNumeric}
+\fi
+%    \end{macrocode}
+% \end{macro}
+%
+%\iffalse
+%</package>
+%\fi
 % \CheckSum{0}
 % \Finale
 \makeatother
diff --git a/Master/texmf-dist/tex/latex/physconst/physconst.sty b/Master/texmf-dist/tex/latex/physconst/physconst.sty
index 2c3befffb73..c1231f2e241 100644
--- a/Master/texmf-dist/tex/latex/physconst/physconst.sty
+++ b/Master/texmf-dist/tex/latex/physconst/physconst.sty
@@ -41,36 +41,36 @@
 \DeclareRobustCommand{\k@SI@short@MassElectron}{%
 \ensuremath{%
 9.11%
-\times 10^{-34}\kg}}
+\times 10^{-31}\kg}}
 \DeclareRobustCommand{\k@SI@full@MassElectron}{%
 \ensuremath{%
 9.108\expandafter\physconst@decimalsseparator%
 980\expandafter\physconst@decimalsseparator%
 087\expandafter\physconst@decimalsseparator%
 382%
-\times 10^{-34}\kg}}
+\times 10^{-31}\kg}}
 \DeclareRobustCommand{\k@cgs@short@MassElectron}{%
 \ensuremath{%
 9.11%
-\times 10^{-31}\gm}}
+\times 10^{-28}\gm}}
 \DeclareRobustCommand{\k@cgs@full@MassElectron}{%
 \ensuremath{%
 9.108\expandafter\physconst@decimalsseparator%
 980\expandafter\physconst@decimalsseparator%
 087\expandafter\physconst@decimalsseparator%
 382%
-\times 10^{-31}\gm}}
+\times 10^{-28}\gm}}
 \DeclareRobustCommand{\k@eV@short@MassElectron}{%
 \ensuremath{%
-5.69%
-\times 10^{-19}\eV\,c^{-2}}}
+5.11%
+\times 10^{5}\eV\,c^{-2}}}
 \DeclareRobustCommand{\k@eV@full@MassElectron}{%
 \ensuremath{%
-5.685\expandafter\physconst@decimalsseparator%
-378\expandafter\physconst@decimalsseparator%
-187\expandafter\physconst@decimalsseparator%
-448%
-\times 10^{-19}\eV\,c^{-2}}}
+5.109\expandafter\physconst@decimalsseparator%
+763\expandafter\physconst@decimalsseparator%
+089\expandafter\physconst@decimalsseparator%
+046%
+\times 10^{5}\eV\,c^{-2}}}
 \ifx\cgsunits\undefined
 \ifx\shortconst\undefined
 \DeclareRobustCommand {\kMassElectron}{%
@@ -95,39 +95,81 @@
 \DeclareRobustCommand {\keVMassElectron}{%
 \k@eV@full@MassElectron}
 \fi
+\DeclareRobustCommand{\k@SI@short@MassElectronNumeric}{%
+\ensuremath{%
+9.11e-31}}
+\DeclareRobustCommand{\k@SI@full@MassElectronNumeric}{%
+\ensuremath{%
+9.108980087382e-31}}
+\DeclareRobustCommand{\k@cgs@short@MassElectronNumeric}{%
+\ensuremath{%
+9.11e-28}}
+\DeclareRobustCommand{\k@cgs@full@MassElectronNumeric}{%
+\ensuremath{%
+9.108980087382e-28}}
+\DeclareRobustCommand{\k@eV@short@MassElectronNumeric}{%
+\ensuremath{%
+5.11e+05}}
+\DeclareRobustCommand{\k@eV@full@MassElectronNumeric}{%
+\ensuremath{%
+5.109763089046e+05}}
+\ifx\cgsunits\undefined
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kMassElectronNumeric}{%
+\k@SI@short@MassElectronNumeric}
+\else
+\DeclareRobustCommand {\kMassElectronNumeric}{%
+\k@SI@full@MassElectronNumeric}
+\fi
+\else
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kMassElectronNumeric}{%
+\k@cgs@short@MassElectronNumeric}
+\else
+\DeclareRobustCommand {\kMassElectronNumeric}{%
+\k@cgs@full@MassElectronNumeric}
+\fi
+\fi
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\keVMassElectronNumeric}{%
+\k@eV@short@MassElectronNumeric}
+\else
+\DeclareRobustCommand {\keVMassElectronNumeric}{%
+\k@eV@full@MassElectronNumeric}
+\fi
 \DeclareRobustCommand{\k@SI@short@MassProton}{%
 \ensuremath{%
 1.67%
-\times 10^{-30}\kg}}
+\times 10^{-27}\kg}}
 \DeclareRobustCommand{\k@SI@full@MassProton}{%
 \ensuremath{%
 1.672\expandafter\physconst@decimalsseparator%
 547\expandafter\physconst@decimalsseparator%
 813\expandafter\physconst@decimalsseparator%
 969%
-\times 10^{-30}\kg}}
+\times 10^{-27}\kg}}
 \DeclareRobustCommand{\k@cgs@short@MassProton}{%
 \ensuremath{%
 1.67%
-\times 10^{-27}\gm}}
+\times 10^{-24}\gm}}
 \DeclareRobustCommand{\k@cgs@full@MassProton}{%
 \ensuremath{%
 1.672\expandafter\physconst@decimalsseparator%
 547\expandafter\physconst@decimalsseparator%
 813\expandafter\physconst@decimalsseparator%
 969%
-\times 10^{-27}\gm}}
+\times 10^{-24}\gm}}
 \DeclareRobustCommand{\k@eV@short@MassProton}{%
 \ensuremath{%
-1.04%
-\times 10^{-15}\eV\,c^{-2}}}
+9.38%
+\times 10^{8}\eV\,c^{-2}}}
 \DeclareRobustCommand{\k@eV@full@MassProton}{%
 \ensuremath{%
-1.043\expandafter\physconst@decimalsseparator%
-922\expandafter\physconst@decimalsseparator%
-235\expandafter\physconst@decimalsseparator%
-836%
-\times 10^{-15}\eV\,c^{-2}}}
+9.382\expandafter\physconst@decimalsseparator%
+305\expandafter\physconst@decimalsseparator%
+156\expandafter\physconst@decimalsseparator%
+558%
+\times 10^{8}\eV\,c^{-2}}}
 \ifx\cgsunits\undefined
 \ifx\shortconst\undefined
 \DeclareRobustCommand {\kMassProton}{%
@@ -152,39 +194,81 @@
 \DeclareRobustCommand {\keVMassProton}{%
 \k@eV@full@MassProton}
 \fi
+\DeclareRobustCommand{\k@SI@short@MassProtonNumeric}{%
+\ensuremath{%
+1.67e-27}}
+\DeclareRobustCommand{\k@SI@full@MassProtonNumeric}{%
+\ensuremath{%
+1.672547813969e-27}}
+\DeclareRobustCommand{\k@cgs@short@MassProtonNumeric}{%
+\ensuremath{%
+1.67e-24}}
+\DeclareRobustCommand{\k@cgs@full@MassProtonNumeric}{%
+\ensuremath{%
+1.672547813969e-24}}
+\DeclareRobustCommand{\k@eV@short@MassProtonNumeric}{%
+\ensuremath{%
+9.38e+08}}
+\DeclareRobustCommand{\k@eV@full@MassProtonNumeric}{%
+\ensuremath{%
+9.382305156558e+08}}
+\ifx\cgsunits\undefined
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kMassProtonNumeric}{%
+\k@SI@short@MassProtonNumeric}
+\else
+\DeclareRobustCommand {\kMassProtonNumeric}{%
+\k@SI@full@MassProtonNumeric}
+\fi
+\else
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kMassProtonNumeric}{%
+\k@cgs@short@MassProtonNumeric}
+\else
+\DeclareRobustCommand {\kMassProtonNumeric}{%
+\k@cgs@full@MassProtonNumeric}
+\fi
+\fi
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\keVMassProtonNumeric}{%
+\k@eV@short@MassProtonNumeric}
+\else
+\DeclareRobustCommand {\keVMassProtonNumeric}{%
+\k@eV@full@MassProtonNumeric}
+\fi
 \DeclareRobustCommand{\k@SI@short@MassHydrogen}{%
 \ensuremath{%
 1.67%
-\times 10^{-30}\kg}}
+\times 10^{-27}\kg}}
 \DeclareRobustCommand{\k@SI@full@MassHydrogen}{%
 \ensuremath{%
 1.673\expandafter\physconst@decimalsseparator%
 458\expandafter\physconst@decimalsseparator%
 687\expandafter\physconst@decimalsseparator%
 724%
-\times 10^{-30}\kg}}
+\times 10^{-27}\kg}}
 \DeclareRobustCommand{\k@cgs@short@MassHydrogen}{%
 \ensuremath{%
 1.67%
-\times 10^{-27}\gm}}
+\times 10^{-24}\gm}}
 \DeclareRobustCommand{\k@cgs@full@MassHydrogen}{%
 \ensuremath{%
 1.673\expandafter\physconst@decimalsseparator%
 458\expandafter\physconst@decimalsseparator%
 687\expandafter\physconst@decimalsseparator%
 724%
-\times 10^{-27}\gm}}
+\times 10^{-24}\gm}}
 \DeclareRobustCommand{\k@eV@short@MassHydrogen}{%
 \ensuremath{%
-1.04%
-\times 10^{-15}\eV\,c^{-2}}}
+9.39%
+\times 10^{8}\eV\,c^{-2}}}
 \DeclareRobustCommand{\k@eV@full@MassHydrogen}{%
 \ensuremath{%
-1.044\expandafter\physconst@decimalsseparator%
-490\expandafter\physconst@decimalsseparator%
-758\expandafter\physconst@decimalsseparator%
-517%
-\times 10^{-15}\eV\,c^{-2}}}
+9.387\expandafter\physconst@decimalsseparator%
+414\expandafter\physconst@decimalsseparator%
+783\expandafter\physconst@decimalsseparator%
+596%
+\times 10^{8}\eV\,c^{-2}}}
 \ifx\cgsunits\undefined
 \ifx\shortconst\undefined
 \DeclareRobustCommand {\kMassHydrogen}{%
@@ -209,6 +293,48 @@
 \DeclareRobustCommand {\keVMassHydrogen}{%
 \k@eV@full@MassHydrogen}
 \fi
+\DeclareRobustCommand{\k@SI@short@MassHydrogenNumeric}{%
+\ensuremath{%
+1.67e-27}}
+\DeclareRobustCommand{\k@SI@full@MassHydrogenNumeric}{%
+\ensuremath{%
+1.673458687724e-27}}
+\DeclareRobustCommand{\k@cgs@short@MassHydrogenNumeric}{%
+\ensuremath{%
+1.67e-24}}
+\DeclareRobustCommand{\k@cgs@full@MassHydrogenNumeric}{%
+\ensuremath{%
+1.673458687724e-24}}
+\DeclareRobustCommand{\k@eV@short@MassHydrogenNumeric}{%
+\ensuremath{%
+9.39e+08}}
+\DeclareRobustCommand{\k@eV@full@MassHydrogenNumeric}{%
+\ensuremath{%
+9.387414783596e+08}}
+\ifx\cgsunits\undefined
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kMassHydrogenNumeric}{%
+\k@SI@short@MassHydrogenNumeric}
+\else
+\DeclareRobustCommand {\kMassHydrogenNumeric}{%
+\k@SI@full@MassHydrogenNumeric}
+\fi
+\else
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kMassHydrogenNumeric}{%
+\k@cgs@short@MassHydrogenNumeric}
+\else
+\DeclareRobustCommand {\kMassHydrogenNumeric}{%
+\k@cgs@full@MassHydrogenNumeric}
+\fi
+\fi
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\keVMassHydrogenNumeric}{%
+\k@eV@short@MassHydrogenNumeric}
+\else
+\DeclareRobustCommand {\keVMassHydrogenNumeric}{%
+\k@eV@full@MassHydrogenNumeric}
+\fi
 \DeclareRobustCommand{\k@SI@short@MassSun}{%
 \ensuremath{%
 1.99%
@@ -246,39 +372,127 @@
 \k@cgs@full@MassSun}
 \fi
 \fi
+\DeclareRobustCommand{\k@SI@short@MassSunNumeric}{%
+\ensuremath{%
+1.99e+30}}
+\DeclareRobustCommand{\k@SI@full@MassSunNumeric}{%
+\ensuremath{%
+1.9884099e+30}}
+\DeclareRobustCommand{\k@cgs@short@MassSunNumeric}{%
+\ensuremath{%
+1.99e+33}}
+\DeclareRobustCommand{\k@cgs@full@MassSunNumeric}{%
+\ensuremath{%
+1.9884099e+33}}
+\ifx\cgsunits\undefined
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kMassSunNumeric}{%
+\k@SI@short@MassSunNumeric}
+\else
+\DeclareRobustCommand {\kMassSunNumeric}{%
+\k@SI@full@MassSunNumeric}
+\fi
+\else
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kMassSunNumeric}{%
+\k@cgs@short@MassSunNumeric}
+\else
+\DeclareRobustCommand {\kMassSunNumeric}{%
+\k@cgs@full@MassSunNumeric}
+\fi
+\fi
+\DeclareRobustCommand{\k@short@MassEarth}{%
+\ensuremath{%
+5.97%
+\times 10^{24}\kg}}
+\DeclareRobustCommand{\k@full@MassEarth}{%
+\ensuremath{%
+5.972\expandafter\physconst@decimalsseparator%
+168%
+\times 10^{24}\kg}}
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kMassEarth}{%
+\k@short@MassEarth}
+\else
+\DeclareRobustCommand {\kMassEarth}{%
+\k@full@MassEarth}
+\fi
+\DeclareRobustCommand{\k@short@MassEarthNumeric}{%
+\ensuremath{%
+5.97e+24}}
+\DeclareRobustCommand{\k@full@MassEarthNumeric}{%
+\ensuremath{%
+5.972168e+24}}
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kMassEarthNumeric}{%
+\k@short@MassEarthNumeric}
+\else
+\DeclareRobustCommand {\kMassEarthNumeric}{%
+\k@full@MassEarthNumeric}
+\fi
+\DeclareRobustCommand{\k@short@MassJupiter}{%
+\ensuremath{%
+1.90%
+\times 10^{27}\kg}}
+\DeclareRobustCommand{\k@full@MassJupiter}{%
+\ensuremath{%
+1.898\expandafter\physconst@decimalsseparator%
+124\expandafter\physconst@decimalsseparator%
+6%
+\times 10^{27}\kg}}
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kMassJupiter}{%
+\k@short@MassJupiter}
+\else
+\DeclareRobustCommand {\kMassJupiter}{%
+\k@full@MassJupiter}
+\fi
+\DeclareRobustCommand{\k@short@MassJupiterNumeric}{%
+\ensuremath{%
+1.90e+27}}
+\DeclareRobustCommand{\k@full@MassJupiterNumeric}{%
+\ensuremath{%
+1.8981246e+27}}
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kMassJupiterNumeric}{%
+\k@short@MassJupiterNumeric}
+\else
+\DeclareRobustCommand {\kMassJupiterNumeric}{%
+\k@full@MassJupiterNumeric}
+\fi
 \DeclareRobustCommand{\k@SI@short@MassAMU}{%
 \ensuremath{%
 1.66%
-\times 10^{-30}\kg}}
+\times 10^{-27}\kg}}
 \DeclareRobustCommand{\k@SI@full@MassAMU}{%
 \ensuremath{%
 1.660\expandafter\physconst@decimalsseparator%
 465\expandafter\physconst@decimalsseparator%
 492\expandafter\physconst@decimalsseparator%
 239%
-\times 10^{-30}\kg}}
+\times 10^{-27}\kg}}
 \DeclareRobustCommand{\k@cgs@short@MassAMU}{%
 \ensuremath{%
 1.66%
-\times 10^{-27}\gm}}
+\times 10^{-24}\gm}}
 \DeclareRobustCommand{\k@cgs@full@MassAMU}{%
 \ensuremath{%
 1.660\expandafter\physconst@decimalsseparator%
 465\expandafter\physconst@decimalsseparator%
 492\expandafter\physconst@decimalsseparator%
 239%
-\times 10^{-27}\gm}}
+\times 10^{-24}\gm}}
 \DeclareRobustCommand{\k@eV@short@MassAMU}{%
 \ensuremath{%
-1.04%
-\times 10^{-15}\eV\,c^{-2}}}
+9.31%
+\times 10^{8}\eV\,c^{-2}}}
 \DeclareRobustCommand{\k@eV@full@MassAMU}{%
 \ensuremath{%
-1.036\expandafter\physconst@decimalsseparator%
-381\expandafter\physconst@decimalsseparator%
-043\expandafter\physconst@decimalsseparator%
-764%
-\times 10^{-15}\eV\,c^{-2}}}
+9.314\expandafter\physconst@decimalsseparator%
+528\expandafter\physconst@decimalsseparator%
+302\expandafter\physconst@decimalsseparator%
+276%
+\times 10^{8}\eV\,c^{-2}}}
 \ifx\cgsunits\undefined
 \ifx\shortconst\undefined
 \DeclareRobustCommand {\kMassAMU}{%
@@ -303,6 +517,48 @@
 \DeclareRobustCommand {\keVMassAMU}{%
 \k@eV@full@MassAMU}
 \fi
+\DeclareRobustCommand{\k@SI@short@MassAMUNumeric}{%
+\ensuremath{%
+1.66e-27}}
+\DeclareRobustCommand{\k@SI@full@MassAMUNumeric}{%
+\ensuremath{%
+1.660465492239e-27}}
+\DeclareRobustCommand{\k@cgs@short@MassAMUNumeric}{%
+\ensuremath{%
+1.66e-24}}
+\DeclareRobustCommand{\k@cgs@full@MassAMUNumeric}{%
+\ensuremath{%
+1.660465492239e-24}}
+\DeclareRobustCommand{\k@eV@short@MassAMUNumeric}{%
+\ensuremath{%
+9.31e+08}}
+\DeclareRobustCommand{\k@eV@full@MassAMUNumeric}{%
+\ensuremath{%
+9.314528302276e+08}}
+\ifx\cgsunits\undefined
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kMassAMUNumeric}{%
+\k@SI@short@MassAMUNumeric}
+\else
+\DeclareRobustCommand {\kMassAMUNumeric}{%
+\k@SI@full@MassAMUNumeric}
+\fi
+\else
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kMassAMUNumeric}{%
+\k@cgs@short@MassAMUNumeric}
+\else
+\DeclareRobustCommand {\kMassAMUNumeric}{%
+\k@cgs@full@MassAMUNumeric}
+\fi
+\fi
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\keVMassAMUNumeric}{%
+\k@eV@short@MassAMUNumeric}
+\else
+\DeclareRobustCommand {\keVMassAMUNumeric}{%
+\k@eV@full@MassAMUNumeric}
+\fi
 \DeclareRobustCommand{\k@SI@short@ChargeFundamental}{%
 \ensuremath{%
 1.60%
@@ -340,6 +596,35 @@
 \k@cgs@full@ChargeFundamental}
 \fi
 \fi
+\DeclareRobustCommand{\k@SI@short@ChargeFundamentalNumeric}{%
+\ensuremath{%
+1.60e-19}}
+\DeclareRobustCommand{\k@SI@full@ChargeFundamentalNumeric}{%
+\ensuremath{%
+1.602176634e-19}}
+\DeclareRobustCommand{\k@cgs@short@ChargeFundamentalNumeric}{%
+\ensuremath{%
+4.80e-10}}
+\DeclareRobustCommand{\k@cgs@full@ChargeFundamentalNumeric}{%
+\ensuremath{%
+4.803204713e-10}}
+\ifx\cgsunits\undefined
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kChargeFundamentalNumeric}{%
+\k@SI@short@ChargeFundamentalNumeric}
+\else
+\DeclareRobustCommand {\kChargeFundamentalNumeric}{%
+\k@SI@full@ChargeFundamentalNumeric}
+\fi
+\else
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kChargeFundamentalNumeric}{%
+\k@cgs@short@ChargeFundamentalNumeric}
+\else
+\DeclareRobustCommand {\kChargeFundamentalNumeric}{%
+\k@cgs@full@ChargeFundamentalNumeric}
+\fi
+\fi
 \DeclareRobustCommand{\k@SI@short@ChargeElectron}{%
 \ensuremath{%
 -1.60%
@@ -377,6 +662,35 @@
 \k@cgs@full@ChargeElectron}
 \fi
 \fi
+\DeclareRobustCommand{\k@SI@short@ChargeElectronNumeric}{%
+\ensuremath{%
+-1.60e-19}}
+\DeclareRobustCommand{\k@SI@full@ChargeElectronNumeric}{%
+\ensuremath{%
+-1.602176634e-19}}
+\DeclareRobustCommand{\k@cgs@short@ChargeElectronNumeric}{%
+\ensuremath{%
+-4.80e-10}}
+\DeclareRobustCommand{\k@cgs@full@ChargeElectronNumeric}{%
+\ensuremath{%
+-4.803204713e-10}}
+\ifx\cgsunits\undefined
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kChargeElectronNumeric}{%
+\k@SI@short@ChargeElectronNumeric}
+\else
+\DeclareRobustCommand {\kChargeElectronNumeric}{%
+\k@SI@full@ChargeElectronNumeric}
+\fi
+\else
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kChargeElectronNumeric}{%
+\k@cgs@short@ChargeElectronNumeric}
+\else
+\DeclareRobustCommand {\kChargeElectronNumeric}{%
+\k@cgs@full@ChargeElectronNumeric}
+\fi
+\fi
 \DeclareRobustCommand{\k@SI@short@ChargeProton}{%
 \ensuremath{%
 1.60%
@@ -414,26 +728,55 @@
 \k@cgs@full@ChargeProton}
 \fi
 \fi
+\DeclareRobustCommand{\k@SI@short@ChargeProtonNumeric}{%
+\ensuremath{%
+1.60e-19}}
+\DeclareRobustCommand{\k@SI@full@ChargeProtonNumeric}{%
+\ensuremath{%
+1.602176634e-19}}
+\DeclareRobustCommand{\k@cgs@short@ChargeProtonNumeric}{%
+\ensuremath{%
+4.80e-10}}
+\DeclareRobustCommand{\k@cgs@full@ChargeProtonNumeric}{%
+\ensuremath{%
+4.803204713e-10}}
+\ifx\cgsunits\undefined
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kChargeProtonNumeric}{%
+\k@SI@short@ChargeProtonNumeric}
+\else
+\DeclareRobustCommand {\kChargeProtonNumeric}{%
+\k@SI@full@ChargeProtonNumeric}
+\fi
+\else
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kChargeProtonNumeric}{%
+\k@cgs@short@ChargeProtonNumeric}
+\else
+\DeclareRobustCommand {\kChargeProtonNumeric}{%
+\k@cgs@full@ChargeProtonNumeric}
+\fi
+\fi
 \DeclareRobustCommand{\k@SI@short@RadiusBohr}{%
 \ensuremath{%
 5.29%
-\times 10^{-8}\m}}
+\times 10^{-11}\m}}
 \DeclareRobustCommand{\k@SI@full@RadiusBohr}{%
 \ensuremath{%
 5.292\expandafter\physconst@decimalsseparator%
 006\expandafter\physconst@decimalsseparator%
 59%
-\times 10^{-8}\m}}
+\times 10^{-11}\m}}
 \DeclareRobustCommand{\k@cgs@short@RadiusBohr}{%
 \ensuremath{%
 5.29%
-\times 10^{-6}\cm}}
+\times 10^{-9}\cm}}
 \DeclareRobustCommand{\k@cgs@full@RadiusBohr}{%
 \ensuremath{%
 5.292\expandafter\physconst@decimalsseparator%
 006\expandafter\physconst@decimalsseparator%
 59%
-\times 10^{-6}\cm}}
+\times 10^{-9}\cm}}
 \ifx\cgsunits\undefined
 \ifx\shortconst\undefined
 \DeclareRobustCommand {\kRadiusBohr}{%
@@ -451,6 +794,35 @@
 \k@cgs@full@RadiusBohr}
 \fi
 \fi
+\DeclareRobustCommand{\k@SI@short@RadiusBohrNumeric}{%
+\ensuremath{%
+5.29e-11}}
+\DeclareRobustCommand{\k@SI@full@RadiusBohrNumeric}{%
+\ensuremath{%
+5.29200659e-11}}
+\DeclareRobustCommand{\k@cgs@short@RadiusBohrNumeric}{%
+\ensuremath{%
+5.29e-09}}
+\DeclareRobustCommand{\k@cgs@full@RadiusBohrNumeric}{%
+\ensuremath{%
+5.29200659e-09}}
+\ifx\cgsunits\undefined
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kRadiusBohrNumeric}{%
+\k@SI@short@RadiusBohrNumeric}
+\else
+\DeclareRobustCommand {\kRadiusBohrNumeric}{%
+\k@SI@full@RadiusBohrNumeric}
+\fi
+\else
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kRadiusBohrNumeric}{%
+\k@cgs@short@RadiusBohrNumeric}
+\else
+\DeclareRobustCommand {\kRadiusBohrNumeric}{%
+\k@cgs@full@RadiusBohrNumeric}
+\fi
+\fi
 \DeclareRobustCommand{\k@SI@short@AstronomicalUnit}{%
 \ensuremath{%
 1.50%
@@ -488,6 +860,35 @@
 \k@cgs@full@AstronomicalUnit}
 \fi
 \fi
+\DeclareRobustCommand{\k@SI@short@AstronomicalUnitNumeric}{%
+\ensuremath{%
+1.50e+11}}
+\DeclareRobustCommand{\k@SI@full@AstronomicalUnitNumeric}{%
+\ensuremath{%
+1.495978707e+11}}
+\DeclareRobustCommand{\k@cgs@short@AstronomicalUnitNumeric}{%
+\ensuremath{%
+1.50e+13}}
+\DeclareRobustCommand{\k@cgs@full@AstronomicalUnitNumeric}{%
+\ensuremath{%
+1.495978707e+13}}
+\ifx\cgsunits\undefined
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kAstronomicalUnitNumeric}{%
+\k@SI@short@AstronomicalUnitNumeric}
+\else
+\DeclareRobustCommand {\kAstronomicalUnitNumeric}{%
+\k@SI@full@AstronomicalUnitNumeric}
+\fi
+\else
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kAstronomicalUnitNumeric}{%
+\k@cgs@short@AstronomicalUnitNumeric}
+\else
+\DeclareRobustCommand {\kAstronomicalUnitNumeric}{%
+\k@cgs@full@AstronomicalUnitNumeric}
+\fi
+\fi
 \DeclareRobustCommand{\k@SI@short@Parsec}{%
 \ensuremath{%
 3.09%
@@ -525,6 +926,35 @@
 \k@cgs@full@Parsec}
 \fi
 \fi
+\DeclareRobustCommand{\k@SI@short@ParsecNumeric}{%
+\ensuremath{%
+3.09e+16}}
+\DeclareRobustCommand{\k@SI@full@ParsecNumeric}{%
+\ensuremath{%
+3.085677581e+16}}
+\DeclareRobustCommand{\k@cgs@short@ParsecNumeric}{%
+\ensuremath{%
+3.09e+18}}
+\DeclareRobustCommand{\k@cgs@full@ParsecNumeric}{%
+\ensuremath{%
+3.085677581e+18}}
+\ifx\cgsunits\undefined
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kParsecNumeric}{%
+\k@SI@short@ParsecNumeric}
+\else
+\DeclareRobustCommand {\kParsecNumeric}{%
+\k@SI@full@ParsecNumeric}
+\fi
+\else
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kParsecNumeric}{%
+\k@cgs@short@ParsecNumeric}
+\else
+\DeclareRobustCommand {\kParsecNumeric}{%
+\k@cgs@full@ParsecNumeric}
+\fi
+\fi
 \DeclareRobustCommand{\k@SI@short@RadiusSun}{%
 \ensuremath{%
 6.96%
@@ -558,36 +988,123 @@
 \k@cgs@full@RadiusSun}
 \fi
 \fi
+\DeclareRobustCommand{\k@SI@short@RadiusSunNumeric}{%
+\ensuremath{%
+6.96e+08}}
+\DeclareRobustCommand{\k@SI@full@RadiusSunNumeric}{%
+\ensuremath{%
+6.957e+08}}
+\DeclareRobustCommand{\k@cgs@short@RadiusSunNumeric}{%
+\ensuremath{%
+6.96e+10}}
+\DeclareRobustCommand{\k@cgs@full@RadiusSunNumeric}{%
+\ensuremath{%
+6.957e+10}}
+\ifx\cgsunits\undefined
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kRadiusSunNumeric}{%
+\k@SI@short@RadiusSunNumeric}
+\else
+\DeclareRobustCommand {\kRadiusSunNumeric}{%
+\k@SI@full@RadiusSunNumeric}
+\fi
+\else
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kRadiusSunNumeric}{%
+\k@cgs@short@RadiusSunNumeric}
+\else
+\DeclareRobustCommand {\kRadiusSunNumeric}{%
+\k@cgs@full@RadiusSunNumeric}
+\fi
+\fi
+\DeclareRobustCommand{\k@short@RadiusEarth}{%
+\ensuremath{%
+6.37%
+\times 10^{6}\m}}
+\DeclareRobustCommand{\k@full@RadiusEarth}{%
+\ensuremath{%
+6.371\expandafter\physconst@decimalsseparator%
+0%
+\times 10^{6}\m}}
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kRadiusEarth}{%
+\k@short@RadiusEarth}
+\else
+\DeclareRobustCommand {\kRadiusEarth}{%
+\k@full@RadiusEarth}
+\fi
+\DeclareRobustCommand{\k@short@RadiusEarthNumeric}{%
+\ensuremath{%
+6.37e+06}}
+\DeclareRobustCommand{\k@full@RadiusEarthNumeric}{%
+\ensuremath{%
+6.3710e+06}}
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kRadiusEarthNumeric}{%
+\k@short@RadiusEarthNumeric}
+\else
+\DeclareRobustCommand {\kRadiusEarthNumeric}{%
+\k@full@RadiusEarthNumeric}
+\fi
+\DeclareRobustCommand{\k@short@RadiusJupiter}{%
+\ensuremath{%
+6.99%
+\times 10^{7}\m}}
+\DeclareRobustCommand{\k@full@RadiusJupiter}{%
+\ensuremath{%
+6.991\expandafter\physconst@decimalsseparator%
+1%
+\times 10^{7}\m}}
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kRadiusJupiter}{%
+\k@short@RadiusJupiter}
+\else
+\DeclareRobustCommand {\kRadiusJupiter}{%
+\k@full@RadiusJupiter}
+\fi
+\DeclareRobustCommand{\k@short@RadiusJupiterNumeric}{%
+\ensuremath{%
+6.99e+07}}
+\DeclareRobustCommand{\k@full@RadiusJupiterNumeric}{%
+\ensuremath{%
+6.9911e+07}}
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kRadiusJupiterNumeric}{%
+\k@short@RadiusJupiterNumeric}
+\else
+\DeclareRobustCommand {\kRadiusJupiterNumeric}{%
+\k@full@RadiusJupiterNumeric}
+\fi
 \DeclareRobustCommand{\k@SI@short@Rydberg}{%
 \ensuremath{%
 2.18%
-\times 10^{-21}\Joule}}
+\times 10^{-18}\Joule}}
 \DeclareRobustCommand{\k@SI@full@Rydberg}{%
 \ensuremath{%
 2.179\expandafter\physconst@decimalsseparator%
 775\expandafter\physconst@decimalsseparator%
 77%
-\times 10^{-21}\Joule}}
+\times 10^{-18}\Joule}}
 \DeclareRobustCommand{\k@cgs@short@Rydberg}{%
 \ensuremath{%
 2.18%
-\times 10^{-14}\erg}}
+\times 10^{-11}\erg}}
 \DeclareRobustCommand{\k@cgs@full@Rydberg}{%
 \ensuremath{%
 2.179\expandafter\physconst@decimalsseparator%
 775\expandafter\physconst@decimalsseparator%
 77%
-\times 10^{-14}\erg}}
+\times 10^{-11}\erg}}
 \DeclareRobustCommand{\k@eV@short@Rydberg}{%
 \ensuremath{%
 1.36%
-\times 10^{-2}\eV}}
+\times 10^{1}\eV}}
 \DeclareRobustCommand{\k@eV@full@Rydberg}{%
 \ensuremath{%
 1.360\expandafter\physconst@decimalsseparator%
 509\expandafter\physconst@decimalsseparator%
 03%
-\times 10^{-2}\eV}}
+\times 10^{1}\eV}}
 \ifx\cgsunits\undefined
 \ifx\shortconst\undefined
 \DeclareRobustCommand {\kRydberg}{%
@@ -612,6 +1129,48 @@
 \DeclareRobustCommand {\keVRydberg}{%
 \k@eV@full@Rydberg}
 \fi
+\DeclareRobustCommand{\k@SI@short@RydbergNumeric}{%
+\ensuremath{%
+2.18e-18}}
+\DeclareRobustCommand{\k@SI@full@RydbergNumeric}{%
+\ensuremath{%
+2.17977577e-18}}
+\DeclareRobustCommand{\k@cgs@short@RydbergNumeric}{%
+\ensuremath{%
+2.18e-11}}
+\DeclareRobustCommand{\k@cgs@full@RydbergNumeric}{%
+\ensuremath{%
+2.17977577e-11}}
+\DeclareRobustCommand{\k@eV@short@RydbergNumeric}{%
+\ensuremath{%
+1.36e+01}}
+\DeclareRobustCommand{\k@eV@full@RydbergNumeric}{%
+\ensuremath{%
+1.36050903e+01}}
+\ifx\cgsunits\undefined
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kRydbergNumeric}{%
+\k@SI@short@RydbergNumeric}
+\else
+\DeclareRobustCommand {\kRydbergNumeric}{%
+\k@SI@full@RydbergNumeric}
+\fi
+\else
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kRydbergNumeric}{%
+\k@cgs@short@RydbergNumeric}
+\else
+\DeclareRobustCommand {\kRydbergNumeric}{%
+\k@cgs@full@RydbergNumeric}
+\fi
+\fi
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\keVRydbergNumeric}{%
+\k@eV@short@RydbergNumeric}
+\else
+\DeclareRobustCommand {\keVRydbergNumeric}{%
+\k@eV@full@RydbergNumeric}
+\fi
 \DeclareRobustCommand{\k@SI@short@LuminositySun}{%
 \ensuremath{%
 3.83%
@@ -645,6 +1204,35 @@
 \k@cgs@full@LuminositySun}
 \fi
 \fi
+\DeclareRobustCommand{\k@SI@short@LuminositySunNumeric}{%
+\ensuremath{%
+3.83e+26}}
+\DeclareRobustCommand{\k@SI@full@LuminositySunNumeric}{%
+\ensuremath{%
+3.828e+26}}
+\DeclareRobustCommand{\k@cgs@short@LuminositySunNumeric}{%
+\ensuremath{%
+3.83e+33}}
+\DeclareRobustCommand{\k@cgs@full@LuminositySunNumeric}{%
+\ensuremath{%
+3.828e+33}}
+\ifx\cgsunits\undefined
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kLuminositySunNumeric}{%
+\k@SI@short@LuminositySunNumeric}
+\else
+\DeclareRobustCommand {\kLuminositySunNumeric}{%
+\k@SI@full@LuminositySunNumeric}
+\fi
+\else
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kLuminositySunNumeric}{%
+\k@cgs@short@LuminositySunNumeric}
+\else
+\DeclareRobustCommand {\kLuminositySunNumeric}{%
+\k@cgs@full@LuminositySunNumeric}
+\fi
+\fi
 \DeclareRobustCommand{\k@SI@short@PressureAtmosphere}{%
 \ensuremath{%
 1.01%
@@ -656,11 +1244,11 @@
 \times 10^{5}\Pa}}
 \DeclareRobustCommand{\k@cgs@short@PressureAtmosphere}{%
 \ensuremath{%
-1.01\barP[m]}}
+1.01\barP}}
 \DeclareRobustCommand{\k@cgs@full@PressureAtmosphere}{%
 \ensuremath{%
 1.013\expandafter\physconst@decimalsseparator%
-25\barP[m]}}
+25\barP}}
 \ifx\cgsunits\undefined
 \ifx\shortconst\undefined
 \DeclareRobustCommand {\kPressureAtmosphere}{%
@@ -678,6 +1266,35 @@
 \k@cgs@full@PressureAtmosphere}
 \fi
 \fi
+\DeclareRobustCommand{\k@SI@short@PressureAtmosphereNumeric}{%
+\ensuremath{%
+1.01e+05}}
+\DeclareRobustCommand{\k@SI@full@PressureAtmosphereNumeric}{%
+\ensuremath{%
+1.01325e+05}}
+\DeclareRobustCommand{\k@cgs@short@PressureAtmosphereNumeric}{%
+\ensuremath{%
+1.01e+00}}
+\DeclareRobustCommand{\k@cgs@full@PressureAtmosphereNumeric}{%
+\ensuremath{%
+1.01325e+00}}
+\ifx\cgsunits\undefined
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kPressureAtmosphereNumeric}{%
+\k@SI@short@PressureAtmosphereNumeric}
+\else
+\DeclareRobustCommand {\kPressureAtmosphereNumeric}{%
+\k@SI@full@PressureAtmosphereNumeric}
+\fi
+\else
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kPressureAtmosphereNumeric}{%
+\k@cgs@short@PressureAtmosphereNumeric}
+\else
+\DeclareRobustCommand {\kPressureAtmosphereNumeric}{%
+\k@cgs@full@PressureAtmosphereNumeric}
+\fi
+\fi
 \DeclareRobustCommand{\k@SI@short@PressureStandard}{%
 \ensuremath{%
 1.00%
@@ -689,11 +1306,11 @@
 \times 10^{5}\Pa}}
 \DeclareRobustCommand{\k@cgs@short@PressureStandard}{%
 \ensuremath{%
-1.00\barP[m]}}
+1.00\barP}}
 \DeclareRobustCommand{\k@cgs@full@PressureStandard}{%
 \ensuremath{%
 1.000\expandafter\physconst@decimalsseparator%
-00\barP[m]}}
+00\barP}}
 \ifx\cgsunits\undefined
 \ifx\shortconst\undefined
 \DeclareRobustCommand {\kPressureStandard}{%
@@ -711,6 +1328,35 @@
 \k@cgs@full@PressureStandard}
 \fi
 \fi
+\DeclareRobustCommand{\k@SI@short@PressureStandardNumeric}{%
+\ensuremath{%
+1.00e+05}}
+\DeclareRobustCommand{\k@SI@full@PressureStandardNumeric}{%
+\ensuremath{%
+1.00000e+05}}
+\DeclareRobustCommand{\k@cgs@short@PressureStandardNumeric}{%
+\ensuremath{%
+1.00e+00}}
+\DeclareRobustCommand{\k@cgs@full@PressureStandardNumeric}{%
+\ensuremath{%
+1.00000e+00}}
+\ifx\cgsunits\undefined
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kPressureStandardNumeric}{%
+\k@SI@short@PressureStandardNumeric}
+\else
+\DeclareRobustCommand {\kPressureStandardNumeric}{%
+\k@SI@full@PressureStandardNumeric}
+\fi
+\else
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kPressureStandardNumeric}{%
+\k@cgs@short@PressureStandardNumeric}
+\else
+\DeclareRobustCommand {\kPressureStandardNumeric}{%
+\k@cgs@full@PressureStandardNumeric}
+\fi
+\fi
 \DeclareRobustCommand{\k@SI@short@SpeedLight}{%
 \ensuremath{%
 3.00%
@@ -748,24 +1394,51 @@
 \k@cgs@full@SpeedLight}
 \fi
 \fi
+\DeclareRobustCommand{\k@SI@short@SpeedLightNumeric}{%
+\ensuremath{%
+3.00e+08}}
+\DeclareRobustCommand{\k@SI@full@SpeedLightNumeric}{%
+\ensuremath{%
+2.99792458e+08}}
+\DeclareRobustCommand{\k@cgs@short@SpeedLightNumeric}{%
+\ensuremath{%
+3.00e+10}}
+\DeclareRobustCommand{\k@cgs@full@SpeedLightNumeric}{%
+\ensuremath{%
+2.99792458e+10}}
+\ifx\cgsunits\undefined
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kSpeedLightNumeric}{%
+\k@SI@short@SpeedLightNumeric}
+\else
+\DeclareRobustCommand {\kSpeedLightNumeric}{%
+\k@SI@full@SpeedLightNumeric}
+\fi
+\else
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kSpeedLightNumeric}{%
+\k@cgs@short@SpeedLightNumeric}
+\else
+\DeclareRobustCommand {\kSpeedLightNumeric}{%
+\k@cgs@full@SpeedLightNumeric}
+\fi
+\fi
 \DeclareRobustCommand{\k@SI@short@AccelGravity}{%
 \ensuremath{%
-6.67%
-\times 10^{-11}\N\kg^{-2}\m^2}}
+9.81\m\Sec^{-2}}}
 \DeclareRobustCommand{\k@SI@full@AccelGravity}{%
 \ensuremath{%
-6.674\expandafter\physconst@decimalsseparator%
-30%
-\times 10^{-11}\N\kg^{-2}\m^2}}
+9.806\expandafter\physconst@decimalsseparator%
+65\m\Sec^{-2}}}
 \DeclareRobustCommand{\k@cgs@short@AccelGravity}{%
 \ensuremath{%
-6.67%
-\times 10^{-8}\dyne\gm^{-2}\cm^2}}
+9.81%
+\times 10^{2}\cm\Sec^{-2}}}
 \DeclareRobustCommand{\k@cgs@full@AccelGravity}{%
 \ensuremath{%
-6.674\expandafter\physconst@decimalsseparator%
-30%
-\times 10^{-8}\dyne\gm^{-2}\cm^2}}
+9.806\expandafter\physconst@decimalsseparator%
+65%
+\times 10^{2}\cm\Sec^{-2}}}
 \ifx\cgsunits\undefined
 \ifx\shortconst\undefined
 \DeclareRobustCommand {\kAccelGravity}{%
@@ -783,16 +1456,45 @@
 \k@cgs@full@AccelGravity}
 \fi
 \fi
+\DeclareRobustCommand{\k@SI@short@AccelGravityNumeric}{%
+\ensuremath{%
+9.81e+00}}
+\DeclareRobustCommand{\k@SI@full@AccelGravityNumeric}{%
+\ensuremath{%
+9.80665e+00}}
+\DeclareRobustCommand{\k@cgs@short@AccelGravityNumeric}{%
+\ensuremath{%
+9.81e+02}}
+\DeclareRobustCommand{\k@cgs@full@AccelGravityNumeric}{%
+\ensuremath{%
+9.80665e+02}}
+\ifx\cgsunits\undefined
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kAccelGravityNumeric}{%
+\k@SI@short@AccelGravityNumeric}
+\else
+\DeclareRobustCommand {\kAccelGravityNumeric}{%
+\k@SI@full@AccelGravityNumeric}
+\fi
+\else
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kAccelGravityNumeric}{%
+\k@cgs@short@AccelGravityNumeric}
+\else
+\DeclareRobustCommand {\kAccelGravityNumeric}{%
+\k@cgs@full@AccelGravityNumeric}
+\fi
+\fi
 \DeclareRobustCommand{\k@SI@short@Coulomb}{%
 \ensuremath{%
 8.99%
-\times 10^{13}\N\m^2\Coulomb^{-2}}}
+\times 10^{9}\N\m^2\Coulomb^{-2}}}
 \DeclareRobustCommand{\k@SI@full@Coulomb}{%
 \ensuremath{%
 8.987\expandafter\physconst@decimalsseparator%
 551\expandafter\physconst@decimalsseparator%
 79%
-\times 10^{13}\N\m^2\Coulomb^{-2}}}
+\times 10^{9}\N\m^2\Coulomb^{-2}}}
 \DeclareRobustCommand{\k@cgs@short@Coulomb}{%
 \ensuremath{%
 1.00}}
@@ -818,6 +1520,35 @@
 \k@cgs@full@Coulomb}
 \fi
 \fi
+\DeclareRobustCommand{\k@SI@short@CoulombNumeric}{%
+\ensuremath{%
+8.99e+09}}
+\DeclareRobustCommand{\k@SI@full@CoulombNumeric}{%
+\ensuremath{%
+8.98755179e+09}}
+\DeclareRobustCommand{\k@cgs@short@CoulombNumeric}{%
+\ensuremath{%
+1.00e+00}}
+\DeclareRobustCommand{\k@cgs@full@CoulombNumeric}{%
+\ensuremath{%
+1.00000000e+00}}
+\ifx\cgsunits\undefined
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kCoulombNumeric}{%
+\k@SI@short@CoulombNumeric}
+\else
+\DeclareRobustCommand {\kCoulombNumeric}{%
+\k@SI@full@CoulombNumeric}
+\fi
+\else
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kCoulombNumeric}{%
+\k@cgs@short@CoulombNumeric}
+\else
+\DeclareRobustCommand {\kCoulombNumeric}{%
+\k@cgs@full@CoulombNumeric}
+\fi
+\fi
 \DeclareRobustCommand{\k@SI@short@VacuumPermittivity}{%
 \ensuremath{%
 8.85%
@@ -857,17 +1588,46 @@
 \k@cgs@full@VacuumPermittivity}
 \fi
 \fi
+\DeclareRobustCommand{\k@SI@short@VacuumPermittivityNumeric}{%
+\ensuremath{%
+8.85e-12}}
+\DeclareRobustCommand{\k@SI@full@VacuumPermittivityNumeric}{%
+\ensuremath{%
+8.8541878128e-12}}
+\DeclareRobustCommand{\k@cgs@short@VacuumPermittivityNumeric}{%
+\ensuremath{%
+7.96e-02}}
+\DeclareRobustCommand{\k@cgs@full@VacuumPermittivityNumeric}{%
+\ensuremath{%
+7.9577471546e-02}}
+\ifx\cgsunits\undefined
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kVacuumPermittivityNumeric}{%
+\k@SI@short@VacuumPermittivityNumeric}
+\else
+\DeclareRobustCommand {\kVacuumPermittivityNumeric}{%
+\k@SI@full@VacuumPermittivityNumeric}
+\fi
+\else
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kVacuumPermittivityNumeric}{%
+\k@cgs@short@VacuumPermittivityNumeric}
+\else
+\DeclareRobustCommand {\kVacuumPermittivityNumeric}{%
+\k@cgs@full@VacuumPermittivityNumeric}
+\fi
+\fi
 \DeclareRobustCommand{\k@SI@short@VacuumPermeability}{%
 \ensuremath{%
-8.85%
-\times 10^{-12}\N\Amp^{-2}}}
+1.26%
+\times 10^{-6}\N\Amp^{-2}}}
 \DeclareRobustCommand{\k@SI@full@VacuumPermeability}{%
 \ensuremath{%
-8.854\expandafter\physconst@decimalsseparator%
-187\expandafter\physconst@decimalsseparator%
-812\expandafter\physconst@decimalsseparator%
-8%
-\times 10^{-12}\N\Amp^{-2}}}
+1.256\expandafter\physconst@decimalsseparator%
+637\expandafter\physconst@decimalsseparator%
+062\expandafter\physconst@decimalsseparator%
+1%
+\times 10^{-6}\N\Amp^{-2}}}
 \DeclareRobustCommand{\k@cgs@short@VacuumPermeability}{%
 \ensuremath{%
 1.26%
@@ -896,6 +1656,35 @@
 \k@cgs@full@VacuumPermeability}
 \fi
 \fi
+\DeclareRobustCommand{\k@SI@short@VacuumPermeabilityNumeric}{%
+\ensuremath{%
+1.26e-06}}
+\DeclareRobustCommand{\k@SI@full@VacuumPermeabilityNumeric}{%
+\ensuremath{%
+1.2566370621e-06}}
+\DeclareRobustCommand{\k@cgs@short@VacuumPermeabilityNumeric}{%
+\ensuremath{%
+1.26e+01}}
+\DeclareRobustCommand{\k@cgs@full@VacuumPermeabilityNumeric}{%
+\ensuremath{%
+1.2566370614e+01}}
+\ifx\cgsunits\undefined
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kVacuumPermeabilityNumeric}{%
+\k@SI@short@VacuumPermeabilityNumeric}
+\else
+\DeclareRobustCommand {\kVacuumPermeabilityNumeric}{%
+\k@SI@full@VacuumPermeabilityNumeric}
+\fi
+\else
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kVacuumPermeabilityNumeric}{%
+\k@cgs@short@VacuumPermeabilityNumeric}
+\else
+\DeclareRobustCommand {\kVacuumPermeabilityNumeric}{%
+\k@cgs@full@VacuumPermeabilityNumeric}
+\fi
+\fi
 \DeclareRobustCommand{\k@short@VacuumImpedance}{%
 \ensuremath{%
 3.77%
@@ -914,6 +1703,19 @@
 \DeclareRobustCommand {\kVacuumImpedance}{%
 \k@full@VacuumImpedance}
 \fi
+\DeclareRobustCommand{\k@short@VacuumImpedanceNumeric}{%
+\ensuremath{%
+3.77e+02}}
+\DeclareRobustCommand{\k@full@VacuumImpedanceNumeric}{%
+\ensuremath{%
+3.76730313668e+02}}
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kVacuumImpedanceNumeric}{%
+\k@short@VacuumImpedanceNumeric}
+\else
+\DeclareRobustCommand {\kVacuumImpedanceNumeric}{%
+\k@full@VacuumImpedanceNumeric}
+\fi
 \DeclareRobustCommand{\k@SI@short@Boltzmann}{%
 \ensuremath{%
 1.38%
@@ -965,6 +1767,48 @@
 \DeclareRobustCommand {\keVBoltzmann}{%
 \k@eV@full@Boltzmann}
 \fi
+\DeclareRobustCommand{\k@SI@short@BoltzmannNumeric}{%
+\ensuremath{%
+1.38e-23}}
+\DeclareRobustCommand{\k@SI@full@BoltzmannNumeric}{%
+\ensuremath{%
+1.380649e-23}}
+\DeclareRobustCommand{\k@cgs@short@BoltzmannNumeric}{%
+\ensuremath{%
+1.38e-16}}
+\DeclareRobustCommand{\k@cgs@full@BoltzmannNumeric}{%
+\ensuremath{%
+1.380649e-16}}
+\DeclareRobustCommand{\k@eV@short@BoltzmannNumeric}{%
+\ensuremath{%
+8.62e-05}}
+\DeclareRobustCommand{\k@eV@full@BoltzmannNumeric}{%
+\ensuremath{%
+8.617333e-05}}
+\ifx\cgsunits\undefined
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kBoltzmannNumeric}{%
+\k@SI@short@BoltzmannNumeric}
+\else
+\DeclareRobustCommand {\kBoltzmannNumeric}{%
+\k@SI@full@BoltzmannNumeric}
+\fi
+\else
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kBoltzmannNumeric}{%
+\k@cgs@short@BoltzmannNumeric}
+\else
+\DeclareRobustCommand {\kBoltzmannNumeric}{%
+\k@cgs@full@BoltzmannNumeric}
+\fi
+\fi
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\keVBoltzmannNumeric}{%
+\k@eV@short@BoltzmannNumeric}
+\else
+\DeclareRobustCommand {\keVBoltzmannNumeric}{%
+\k@eV@full@BoltzmannNumeric}
+\fi
 \DeclareRobustCommand{\k@SI@short@Planck}{%
 \ensuremath{%
 6.63%
@@ -1019,6 +1863,48 @@
 \DeclareRobustCommand {\keVPlanck}{%
 \k@eV@full@Planck}
 \fi
+\DeclareRobustCommand{\k@SI@short@PlanckNumeric}{%
+\ensuremath{%
+6.63e-34}}
+\DeclareRobustCommand{\k@SI@full@PlanckNumeric}{%
+\ensuremath{%
+6.62607015e-34}}
+\DeclareRobustCommand{\k@cgs@short@PlanckNumeric}{%
+\ensuremath{%
+6.63e-27}}
+\DeclareRobustCommand{\k@cgs@full@PlanckNumeric}{%
+\ensuremath{%
+6.62607015e-27}}
+\DeclareRobustCommand{\k@eV@short@PlanckNumeric}{%
+\ensuremath{%
+4.14e-15}}
+\DeclareRobustCommand{\k@eV@full@PlanckNumeric}{%
+\ensuremath{%
+4.13566770e-15}}
+\ifx\cgsunits\undefined
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kPlanckNumeric}{%
+\k@SI@short@PlanckNumeric}
+\else
+\DeclareRobustCommand {\kPlanckNumeric}{%
+\k@SI@full@PlanckNumeric}
+\fi
+\else
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kPlanckNumeric}{%
+\k@cgs@short@PlanckNumeric}
+\else
+\DeclareRobustCommand {\kPlanckNumeric}{%
+\k@cgs@full@PlanckNumeric}
+\fi
+\fi
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\keVPlanckNumeric}{%
+\k@eV@short@PlanckNumeric}
+\else
+\DeclareRobustCommand {\keVPlanckNumeric}{%
+\k@eV@full@PlanckNumeric}
+\fi
 \DeclareRobustCommand{\k@SI@short@PlanckReduced}{%
 \ensuremath{%
 1.05%
@@ -1073,15 +1959,57 @@
 \DeclareRobustCommand {\keVPlanckReduced}{%
 \k@eV@full@PlanckReduced}
 \fi
+\DeclareRobustCommand{\k@SI@short@PlanckReducedNumeric}{%
+\ensuremath{%
+1.05e-34}}
+\DeclareRobustCommand{\k@SI@full@PlanckReducedNumeric}{%
+\ensuremath{%
+1.05457182e-34}}
+\DeclareRobustCommand{\k@cgs@short@PlanckReducedNumeric}{%
+\ensuremath{%
+1.05e-27}}
+\DeclareRobustCommand{\k@cgs@full@PlanckReducedNumeric}{%
+\ensuremath{%
+1.05457182e-27}}
+\DeclareRobustCommand{\k@eV@short@PlanckReducedNumeric}{%
+\ensuremath{%
+6.58e-16}}
+\DeclareRobustCommand{\k@eV@full@PlanckReducedNumeric}{%
+\ensuremath{%
+6.58211957e-16}}
+\ifx\cgsunits\undefined
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kPlanckReducedNumeric}{%
+\k@SI@short@PlanckReducedNumeric}
+\else
+\DeclareRobustCommand {\kPlanckReducedNumeric}{%
+\k@SI@full@PlanckReducedNumeric}
+\fi
+\else
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kPlanckReducedNumeric}{%
+\k@cgs@short@PlanckReducedNumeric}
+\else
+\DeclareRobustCommand {\kPlanckReducedNumeric}{%
+\k@cgs@full@PlanckReducedNumeric}
+\fi
+\fi
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\keVPlanckReducedNumeric}{%
+\k@eV@short@PlanckReducedNumeric}
+\else
+\DeclareRobustCommand {\keVPlanckReducedNumeric}{%
+\k@eV@full@PlanckReducedNumeric}
+\fi
 \DeclareRobustCommand{\k@SI@short@Gravity}{%
 \ensuremath{%
 6.67%
-\times 10^{-15}\N\kg^{-2}\m^2}}
+\times 10^{-11}\N\kg^{-2}\m^2}}
 \DeclareRobustCommand{\k@SI@full@Gravity}{%
 \ensuremath{%
 6.674\expandafter\physconst@decimalsseparator%
 30%
-\times 10^{-15}\N\kg^{-2}\m^2}}
+\times 10^{-11}\N\kg^{-2}\m^2}}
 \DeclareRobustCommand{\k@cgs@short@Gravity}{%
 \ensuremath{%
 6.67%
@@ -1108,15 +2036,44 @@
 \k@cgs@full@Gravity}
 \fi
 \fi
+\DeclareRobustCommand{\k@SI@short@GravityNumeric}{%
+\ensuremath{%
+6.67e-11}}
+\DeclareRobustCommand{\k@SI@full@GravityNumeric}{%
+\ensuremath{%
+6.67430e-11}}
+\DeclareRobustCommand{\k@cgs@short@GravityNumeric}{%
+\ensuremath{%
+6.67e-08}}
+\DeclareRobustCommand{\k@cgs@full@GravityNumeric}{%
+\ensuremath{%
+6.67430e-08}}
+\ifx\cgsunits\undefined
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kGravityNumeric}{%
+\k@SI@short@GravityNumeric}
+\else
+\DeclareRobustCommand {\kGravityNumeric}{%
+\k@SI@full@GravityNumeric}
+\fi
+\else
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kGravityNumeric}{%
+\k@cgs@short@GravityNumeric}
+\else
+\DeclareRobustCommand {\kGravityNumeric}{%
+\k@cgs@full@GravityNumeric}
+\fi
+\fi
 \DeclareRobustCommand{\k@SI@short@StefanBoltzmann}{%
 \ensuremath{%
 5.67%
-\times 10^{-6}\J\Kelvin^{-4}\m^{-2}\Sec^{-1}}}
+\times 10^{-8}\J\Kelvin^{-4}\m^{-2}\Sec^{-1}}}
 \DeclareRobustCommand{\k@SI@full@StefanBoltzmann}{%
 \ensuremath{%
 5.670\expandafter\physconst@decimalsseparator%
 374%
-\times 10^{-6}\J\Kelvin^{-4}\m^{-2}\Sec^{-1}}}
+\times 10^{-8}\J\Kelvin^{-4}\m^{-2}\Sec^{-1}}}
 \DeclareRobustCommand{\k@cgs@short@StefanBoltzmann}{%
 \ensuremath{%
 5.67%
@@ -1143,6 +2100,35 @@
 \k@cgs@full@StefanBoltzmann}
 \fi
 \fi
+\DeclareRobustCommand{\k@SI@short@StefanBoltzmannNumeric}{%
+\ensuremath{%
+5.67e-08}}
+\DeclareRobustCommand{\k@SI@full@StefanBoltzmannNumeric}{%
+\ensuremath{%
+5.670374e-08}}
+\DeclareRobustCommand{\k@cgs@short@StefanBoltzmannNumeric}{%
+\ensuremath{%
+5.67e-05}}
+\DeclareRobustCommand{\k@cgs@full@StefanBoltzmannNumeric}{%
+\ensuremath{%
+5.670374e-05}}
+\ifx\cgsunits\undefined
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kStefanBoltzmannNumeric}{%
+\k@SI@short@StefanBoltzmannNumeric}
+\else
+\DeclareRobustCommand {\kStefanBoltzmannNumeric}{%
+\k@SI@full@StefanBoltzmannNumeric}
+\fi
+\else
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kStefanBoltzmannNumeric}{%
+\k@cgs@short@StefanBoltzmannNumeric}
+\else
+\DeclareRobustCommand {\kStefanBoltzmannNumeric}{%
+\k@cgs@full@StefanBoltzmannNumeric}
+\fi
+\fi
 \DeclareRobustCommand{\k@SI@short@Radiation}{%
 \ensuremath{%
 7.57%
@@ -1178,6 +2164,35 @@
 \k@cgs@full@Radiation}
 \fi
 \fi
+\DeclareRobustCommand{\k@SI@short@RadiationNumeric}{%
+\ensuremath{%
+7.57e-16}}
+\DeclareRobustCommand{\k@SI@full@RadiationNumeric}{%
+\ensuremath{%
+7.565733e-16}}
+\DeclareRobustCommand{\k@cgs@short@RadiationNumeric}{%
+\ensuremath{%
+7.57e-15}}
+\DeclareRobustCommand{\k@cgs@full@RadiationNumeric}{%
+\ensuremath{%
+7.565733e-15}}
+\ifx\cgsunits\undefined
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kRadiationNumeric}{%
+\k@SI@short@RadiationNumeric}
+\else
+\DeclareRobustCommand {\kRadiationNumeric}{%
+\k@SI@full@RadiationNumeric}
+\fi
+\else
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kRadiationNumeric}{%
+\k@cgs@short@RadiationNumeric}
+\else
+\DeclareRobustCommand {\kRadiationNumeric}{%
+\k@cgs@full@RadiationNumeric}
+\fi
+\fi
 \DeclareRobustCommand{\k@short@FineStructure}{%
 \ensuremath{%
 7.30%
@@ -1195,6 +2210,19 @@
 \DeclareRobustCommand {\kFineStructure}{%
 \k@full@FineStructure}
 \fi
+\DeclareRobustCommand{\k@short@FineStructureNumeric}{%
+\ensuremath{%
+7.30e-03}}
+\DeclareRobustCommand{\k@full@FineStructureNumeric}{%
+\ensuremath{%
+7.29735257e-03}}
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kFineStructureNumeric}{%
+\k@short@FineStructureNumeric}
+\else
+\DeclareRobustCommand {\kFineStructureNumeric}{%
+\k@full@FineStructureNumeric}
+\fi
 \DeclareRobustCommand{\k@short@FineStructureReciprocal}{%
 \ensuremath{%
 1.37%
@@ -1212,6 +2240,19 @@
 \DeclareRobustCommand {\kFineStructureReciprocal}{%
 \k@full@FineStructureReciprocal}
 \fi
+\DeclareRobustCommand{\k@short@FineStructureReciprocalNumeric}{%
+\ensuremath{%
+1.37e+02}}
+\DeclareRobustCommand{\k@full@FineStructureReciprocalNumeric}{%
+\ensuremath{%
+1.37035999e+02}}
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kFineStructureReciprocalNumeric}{%
+\k@short@FineStructureReciprocalNumeric}
+\else
+\DeclareRobustCommand {\kFineStructureReciprocalNumeric}{%
+\k@full@FineStructureReciprocalNumeric}
+\fi
 \DeclareRobustCommand{\k@short@Avogadro}{%
 \ensuremath{%
 6.02%
@@ -1229,6 +2270,19 @@
 \DeclareRobustCommand {\kAvogadro}{%
 \k@full@Avogadro}
 \fi
+\DeclareRobustCommand{\k@short@AvogadroNumeric}{%
+\ensuremath{%
+6.02e+23}}
+\DeclareRobustCommand{\k@full@AvogadroNumeric}{%
+\ensuremath{%
+6.02240760e+23}}
+\ifx\shortconst\undefined
+\DeclareRobustCommand {\kAvogadroNumeric}{%
+\k@short@AvogadroNumeric}
+\else
+\DeclareRobustCommand {\kAvogadroNumeric}{%
+\k@full@AvogadroNumeric}
+\fi
 \makeatother
 \endinput
 %%