1.

A system consists of two stars of equal masses that revolve in a circular orbit about a centre of mass midway between them. Orbital speed of each star is v and period is T. Find the mass M of each star (G is gravitational constant)                     

A. \[\frac{2G{{v}^{3}}}{\pi T}\]
B. \[\frac{{{v}^{3}}T}{\pi G}\]
C. \[\frac{{{v}^{3}}T}{2\pi G}\]
D. \[\frac{2T{{v}^{3}}}{\pi G}\]
Answer» E.


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