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Imagine a light planet revolving around ...

Imagine a light planet revolving around a very massive star in 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 `T^2` is proportional to

A

`R^3`

B

`R^(7/2)`

C

`R^(3/2)`

D

`R^(15/4)`

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