Three uniform spheres, each having mass m and radius R are kept in such a way that each touches other two. Then, the magnitude of gravitational force on any sphere due to other two is
(a) \(\frac{3\,Gm}{2\,R^2}\)
(b) \(\frac{3\,Gm}{R^2}\)
(c) \(\frac{Gm}{2\,R^2}\)
(d) \(\frac {\sqrt3}{4} \) \(\frac{Gm^2}{R^2}\)