Imagine a light planet revolving around a very massive star in a circular orbit of radius R with a speed 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 R3.75
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