Imagine a planet is 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−52, then
T2 is proportional to R72
If a planet of mass m is revolving with velocity v in an orbit of radius R, we have
mv2R=KR52 where K=GmM is a constant.
⇒v=√KmR32
Time period T=2πRv=2π√mKR72
⇒T2∝R72