16.
Orbital radius of the planet to that of the moon is radius of the star to that of the moon. It is known that
the Moon has a lot to do with the conditions for life on Earth being good because its orbit holds the Earth
at its inclination to Sun its orbit preventing temperature extremes and allowing for the seasons. The
Schrödinger Wave Equation must be solved to determine the energies and orbitals of the electron in the
hydrogen atom. In spherical coordinates it is
17.
It has the solutions
18.
19.
I find the solutions are for the Earth orbiting the Sun are:
20.
21.
is the solar radius, that of the Moon. For Earth , third planet. For a star brighter than the Sun,
more massive, larger, it may be that in many cases the habitable zone, which is further out, still is the n=3
orbit for planets because the distribution of the planets might be stretched out putting the n=3 planet in the
habitable zone. The same may be true of stars that are dimmer, less massive and smaller, because the
planet distribution might be tighter. Since the n=3 habitable zone in such a scenario is closer in, n=3
might be in the habitable zone. While we don’t have complete data for brighter stars, like F stars, we do
for dimmer stars because it is easier to obtain and a good example of this is the M2V star TOI 700. We
have found four exoplanets around this star and TOI 700 e is an Earth-like planet in its habitable zone
which is also the third planet. With the equations so far we can solve planetary systems with a method that
is independent of orbit number, n. To solve the wave equation in the case of a protoplanetary disc you
would want the wave equation to be in cylindrical coordinates, to solve it looks like this, the time
independent Schrödinger equation is
22.