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Aug 26, 2016 at 3:53 comment added Joanna Marietti Unfortunately, it's not a stable orbital configuration... any perturbation from the center, and the planet, no longer in equilibrium with its surroundings, falls straight into the nearest sun. Artificial intervention (in the form of a massive, powerful, steerable moon) would be required to keep it centered, and it's hard to imagine how it ever got to be there in the first place...
Jan 30, 2016 at 22:26 comment added JRaymond @sh1 sort of, the intent was that the planet be in the barycenter of the system, which I guess in the case of relatively equal masses would also be L1 (can you tell I'm not an astronomer? :) ) along those lines, it does seem that you could have objects at L4/L5, which would be at about halfway along the orbital path between the two bodies. As to the black hole, sure, why not? it's just a mass
Jan 30, 2016 at 19:48 comment added sh1 I think that's L1 you've used for your planet, right? Does this imply that you can have objects at L4 and L5 that subjectively appear to also be orbiting the planet, or do those disappear when both major bodies are the same size? And can we replace one star with a black hole of the same mass?
Jan 30, 2016 at 17:48 review First posts
Jan 30, 2016 at 17:54
Jan 30, 2016 at 17:44 history answered JRaymond CC BY-SA 3.0