Mass of each star, M = 2 x 1030 kg
Initial distance between two stars = r
= 109 km = 1012 m
Initial P.E. of the system = -GMM/r
Total K.E. of the stars = 1/2Mv2 + 1/2Mv2 = Mv2
where v is the speed of collision of stars. Just before they are colliding, the distance between their centres = 2R
Hence, final P.E. of the system = -GMM/2R
Gain in K.E. is at the cost of loss in P.E.
We have,
