Gravitational potential energy E=−rGMm where M= mass of earth m= mass of body r= radius of earth Energy required to move a body of mass m from an orbit of radius 2R to 3R=( Potential energy of the Earth-mass system when mass is at distance 3R)− (Potential energy of the Earth-mass system when mass is at distance 2R ) =3R−GMm−(2R−GMm)=3R−GMm+2RGMm=6R−2GMm+3GMm=6RGMm