A double star is a system of two stars moving around the centre of inertia of the system due to gravitation. Find the distance between the components of the double star, if its total mass equals M and the period of revolution T.
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Solution
The double star can be replaced by a single star of mass m1m2m1+m2 moving about the centre of mass subjected to the force γm1m2r2. Then T=2πr32
⎷γm1m2m1m2m1+m2=2πr32√γM So, r32=T2π√γM or, r=(T2π)23(γM)13=3√γM(T2π)2