A body of mass m is moving in a circular orbit of radius R about a planet of mass M. At some instant, it splits into two equal masses. The first mass moves in a circular orbit of radius 2R , and the other mass, in a circular orbit of radius 23R . The difference between the final and initial total energies is:
(1) −2RGMm
(2) +6RGMm
(3) −6RGMm
(4) 2RGMm