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 the planet and the star is proportional to R−5/2 then,
A
T2 is proportional to R2
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B
T2 is proportional to R7/2
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C
T2 is proportional to R3/2
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D
T2 is proportional to R5/2
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Solution
The correct option is AT2 is proportional to R7/2 Given, mv2R∝R−5/2 V∝R−3/4 Now, T=2πRv T2∝(Rv)2 ⇒T2∝(Rv)2⇒T2∝R72