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−52 then:
Mv2R∝R−52 ∴v∝R−34
Now, T=2πRv or T2∝(Rv)2 or T2∝(RR−34)2 or T2∝R72