 |
Wayne Throop wrote:
> ( I assume you mean "an earth-mass planet orbiting a planet of N^3
> lunar masses at N times lunar distance, the pair orbiting about 1au
> from the star". Unless I'm not understanding the discussion
upthread. )
I wasn't making any assumptions about N, though of course we know it
can be at least as high as 1 and give stable orbits. By orbiting I
meant around the center of mass. How large can N get and still give us
stability?
|
|
