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Kepler-452b: Moons?


_Augustus_

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Upper mass constrain would likely comes from the total mass of the system (as it'll be pretty much like Moon - Earth, where the actual keplerian orbit of Earth - Moon system is the orbit of the barycenter and not Earth's center). Then you have hill sphere, constraining the distance from parent planet. From there, you can have a constraint where it won't be a binary planet (ha, pluto-charon "copy" at a distant star !) and density constraint (because we knew the planet radius already). Lastly you can work out whether tidal locking already happens or not, so we know whether somone can live nicely there.

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