Three identical point masses each of mass m are located at the vertices of an equilateral triangle of side a. They revolve in a circular orbit circumscribing the triangle, maintaining their relative positions, under the influence of their gravitational force. The speed of each is
(1) \(\sqrt{\frac{GM}{a}}\)
(2) \(\sqrt{\frac{2GM}{a}}\)
(3) \(\sqrt{\frac{3GM}{a}}\)
(4) \(\frac{2Gm}{3a}\)