What is the orbital radius of the planet in AU? 0.1340
What is the orbital period of the planet in EarthDays? 27.80978
The orbital velocity of the planet is: 52420.957031 m/s
What is the mass of the planet in EarthMasses? 0.818
The kinetic energy of the planet is 6.712016E33 J
The Planck Constant for the system is 6.936936E33 Js
What is the radius of the star in Solar Radii? 0.420
What is the molar mass of element 1? 5
What is the molar mass of element 2? 9
The Moon's orbital radius is 1.624000E8 m
What is the orbital number n? 3
The mass the this planet's moon is 3.051824E23 kg
The radius of this planet's moon is 2.368144E6 m
The density of the moon of this planet is: 5.485880 g/cm3
Program ended with exit code: 0
As we can see the program works well. Let us guess that a G2V star like our sun uses Au/Ag, the
more sophisticated metals, and that a more crude star like a red dwarf, M star, uses more crude
metals. It is my guess that because a more luminous star like the Sun has higher radiation
pressure, that in the formation of the its planetary system, the elements have to be heavier to
stay close in. In a red dwarf M star, this shouldn’t be so much the case. Let us run it for 2/3…
What is the orbital radius of the planet in AU? 0.1340
What is the orbital period of the planet in EarthDays? 27.80978
The orbital velocity of the planet is: 52420.957031 m/s
What is the mass of the planet in EarthMasses? 0.818
The kinetic energy of the planet is 6.712016E33 J
The Planck Constant for the system is 6.936936E33 Js
What is the radius of the star in Solar Radii? 0.420
What is the molar mass of element 1? 2
What is the molar mass of element 2? 3
The Moon's orbital radius is 1.948800E8 m
What is the orbital number n? 3
The mass the this planet's moon is 3.243046E23 kg
The radius of this planet's moon is 2.841773E6 m
The density of the moon of this planet is: 3.373621 g/cm3
Program ended with exit code: 0
We find that in fact it uses metals that are closer together, but this is interesting. We get the
density of the Moon in the ratio of 2/3 for the elements associated with it, the base ratio in the
fibonacci sequence whose ratios of successive terms converge on the golden ratio. This is good
because red dwarf M stars are the coolest stars on the main sequence, so they are the basis stars
in HR diagrams. And this is perfectly iron (Fe) over krypton (Kr) which is
(Fe/Kr)=55.85/83.80=0.67 in that 2/3=0.67.
An interesting thing that is happening here is the Moon of the Earth is mostly silicates
(composed of silicon) and the moon of TOI 700 e is using the gold to silver of the Earth equation
produces the density of germanium, the next element down below silicon in the periodic table,
and the orbital period of the habitable planet of TOI 700 e about its star that is about the same
size as the Earth, has almost exactly the orbital period of the Moon around the Earth. It seems to
suggest that the yellow spectral class G stars are connected to the red spectral class M stars in
some kind of an inversion. Indeed, one could suggest there might be a uniformity of life among
the red dwarf stars that is related to the uniformity of life in the yellow stars. The possibility begs
for data on the K stars, F stars, B stars, A stars, and O stars concerning habitable planets for