Farrooh F. answered 12/09/23
Physics & Math Expert — AP, SAT, Olympiads, Advanced Courses
Recall that orbital velocities/speeds depend on the mass of the host star only:
v = √(GM/r)
where G is the gravitational constant, M is the mass, and r is the orbital radius.
(a) Solve this for radius, substitute their speeds respectively, and take the ratio of the two radii for each planet.
(b) Do the same using the orbital period formula: T = 2πr/v