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I was under the impression that, if there were planets in a binary star system, the planets would orbit the whole binary as if it was a single star, rather than the second star being further out than the planets...
They can orbit either around both, or around one or the other. The Earth-Moon or Pluto-Charon systems are quite close in mass (at least, have mass ratios which wouldn't be beyond the bounds of a binary star system) and we could imagine something in orbit around Earth, or the Moon, or both (if the Sun weren't there to complicate things, that is).
I think it's more likely you'd have a habitable zone around either star of a binary (that is, where the stars are relatively separate, each could have a system of planets essentially like our Solar system) than that you'd have a habitable zone around the pair. I think to have a habitable zone around a pair they'd need to be close together and one or both stars would need to be very bright, so that the habitable zone would be a long way away and less subject to weird orbital perturbation effects.
Don't quote me, though. We spent most of our time looking at dust grains in the ISM, metrics and masers created by stars, all of which are very cool, and none of which I can remember either. |
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