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Kepler's law (as we shall see can be generalised to p 2 =a 3 /M, for the period...
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Kepler's law (as we shall see can be generalised to p2 =a3/M, for the period in years and the semimajor axis in AU as before but now adding in the mass of the object being orbited in terms of the mass of the Sun (i.e. M=mass of object being orbited/MSun).
What is the orbital period of an object orbiting a star of mass 4 MSun at 4AU?
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