Imagine a light planet revolving around a very
massive star in a circular orbit of radius R with
time period of revolution T. If the gravitational force
of attraction between the planet and the star is
proportional to R^(-3/2), then
(1) T is proportional to R^(5/4)
(2) T is proportional to R^(7/4)
(3) T is proportional to R^(3/2)
(4) Tis proportional to R
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