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.
(1) T2 is proportional to R3
(2) T2 is proportional to R7/2
(3) T2 is proportional to R3/2
(4) T2 is proportional to R3/73