Steve
Penultimate Amazing
It may be a good answer to something. But it has no connection whatsoever to the post by JesseCuster that you quoted. Your "brain" works in very strange ways.A good answer here:
"A more careful calculation, including the effects of the Sun is slightly more optimistic and provides a Hill radius of r=58,050km. In either case though, hopefully you can see that the radius for a selenostationary orbit is much farther than the Hill radius, meaning that no stable orbit can be achieved as it would be too much perturbed by the Earth and/or the Sun.
One final, semi-related point. It turns out almost no orbits around the Moon are stable, even if they're inside the Hill radius. This is primarily to do with mass concentrations (or mascons) in the Moon's crust and mantle which make the gravitational field non-uniform and act to degrade orbits. There are only a handful of "stable" orbits and these are only achieved by orbiting in such a way as to miss passing over these mascons."
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