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Two point masses of mass $$m_1 = fM$$ and $$m_2 = (1-f)M\ (f<1)$$ are in outer space (far from gravitational influence of other objects) at a distance $$R$$ from each other. They move in circular orbits about their centre of mass with angular velocities $$\omega_1$$ for $$m_1$$ and $$\omega_2$$ for $$m_2$$. In that case
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