Question: Consider two binary systems, one consisting of a 1.0M star and an Earth-mass (1.0M) planet, the other consisting of two 1.0M stars. Both have an
Consider two binary systems, one consisting of a 1.0M star and an Earth-mass (1.0M⊕) planet, the other consisting of two 1.0M stars. Both have an orbital separation of 50 AU and roughly circular orbits. How, if at all, do the orbital periods differ between these systems?
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