The gravitational force provides the centripetal force for circular motion, meaning \(F_{\text{gravity}} = F_{\text{centripetal}}\). The gravitational force between two particles is given by \(F = \frac{G M_1 M_2}{d^2}\), where \( G \) is the gravitational constant, \( M_1 = M_2 = m \), and \( d = 2a \) is the distance between them. Substituting these values yields \(F = \frac{G m^2}{(2a)^2} = \frac{G m^2}{4a^2}\). For circular motion, the centripetal force is \(F = m \omega^2 r\), with \( r = a \). Equating the two expressions for force, we get \(\frac{G m^2}{4a^2} = m \omega^2 a\). Simplifying this equation leads to \(\omega^2 = \frac{G m}{4a^3}\). Taking the square root gives the angular velocity: \(\omega = \sqrt{\frac{G m}{4a^3}}\). Final Answer: \[\boxed{\sqrt{\frac{G m}{4a^3}}}\]