Q.
An artificial satellite revolves around a planet for which gravitational force (F) varies with distance r from its centre as F∝r2. If v0 its orbital speed, then
Gravitational force (F) provides the necessary centripetal force to keep the satellite in orbit, ⇒rmv02∝F rmv02∝r2 v0→ Orbital speed r→ Radius of orbit ⇒v0∝r3/2