Imagine a light planet 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 planet and star is proportional to R−52, then T2 is proportional to
A
R3
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B
R7/2
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C
R5/2
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D
R3/2
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Solution
The correct option is BR7/2 For revolution of planet centripetal force is provided by gravitational force of attraction mω2R∝R−5/2