Suppose a light planet is revolving in circular orbit of radius R about a heavy star and its time period is T. Gravitational force between the planet and the star is directly proportional to R-5/2, then:
(a) T2 ∝ R3
(b) T2 ∝ R7/2
(c) T2 ∝ R3/2
(d) T2 ∝ r3.75