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.
a. T2 is proportional to R3
b. T2 is proportional to R7/2
c. T2 is proportional to R3/2
d. T2 is proportional to R3/73