I suspect that the exact locations of stable orbits requires complex simulation and stuff, but are there some "quick-and-dirty" formulae for the outermost stable orbit around one component of a binary star system and the innermost stable orbit around both, given the masses of the two components, separation, eccentricity and stuff like that?
Thanks,
Chaos.
Stable orbits around binary stars
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The original reference for this stuff is Szebehely's Stability of Planetary Orbits in Binary Systems.
You might also want to look at Holman and Wiegert's Long-term Stability of Planets in Binary Systems. Of course, the existence of stable orbits doesn't imply that planets can actually form in those positions: so Whitmire et al's Habitable Planet Formation in Binary Systems is of interest.
Grant
You might also want to look at Holman and Wiegert's Long-term Stability of Planets in Binary Systems. Of course, the existence of stable orbits doesn't imply that planets can actually form in those positions: so Whitmire et al's Habitable Planet Formation in Binary Systems is of interest.
Grant
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