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 R/2, and the other mass, in a circular orbit of radius 3R/2. The difference between the final initial total energies is:
-GMm/2R
-GMm/6R
+GMm/6R
GMm/2R
Solution:
Initial energy = -GMm/R + 1/2 GMm/R = -GMm/2R Final energy = -GMm/(2(R/2)) - GMm/(2(3R/2)) ΔE = -GMm/6R