A small planet is revolving with a speed v around a very massive star in a circular orbit of radius r with a revolution period T. If the gravitational force between the planet and the star were inversely proportional to r, then,
v is independent of r
T increases if r is increased.
F = kr, k is constant.
mv2r=kr⇒v=√km, which is independent of r.
T=2πrv=2π√mkr⇒T∝r