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Binary stars of comparable masses m1 and m2 rotate under the influence of each other gravity with a time period T. If they are stopped suddenly in their motions. find their relative velocity when they collide with each other . The radii of the stars are R1 and R2 respectively. G is the universal constant of gravitation.

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Both the stars rotate about their centre of mass(COM)

For the position of COM

Applying conservation of mechanical energy we have

vr = relative velocity between the two stars.

Substitution the value of r from Eq. (i), we get

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