GravitationHard

Question

If the gravitational force were to vary inversely-as mth power of the distance, then the time period of a planet in circular orbit of radius r around the Sun will be proportional to

Options

A.r-3m/2
B.r3m/2
C.rm+1/2
D.r(m+1)/2

Solution

F ∝ ; F =
This force will provide the required centripetal force
Therefore
2 r = ; ω2 =
T = ⇒ T ∝ r(m+1)/2

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