Q.
A system of binary stars of masses M1 and M2 are moving in circular orbits of radii r1 and r2 respectively. If T1 and T2 are the time periods of revolution of masses M1 and M2 respectively and if r2r1=2, then find T2T1.
Centre fo mass of binary star lies at certre of their circular path. M1r1=M2r2
Then, G(r1+r2)2M1M2=M1ω12r1=M2ω22r2 ⇒ω1=ω2→T2T1=1.00
Same angular velocity and time period of revolution.