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Question

Imagine a planet is revolving around a very massive star in a circular orbit of radius R with a period of revolution T. If the gravitational force of attraction between the planet and the star is proportional to R−52, then


A

T2 is proportional to R3

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B

T2 is proportional to R72

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C

T2 is proportional to R32

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D

T2 is proportional to R3.75

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Solution

The correct option is B

T2 is proportional to R72


If a planet of mass m is revolving with velocity v in an orbit of radius R, we have
mv2R=KR52 where K=GmM is a constant.
v=KmR32
Time period T=2πRv=2πmKR72
T2R72


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