
To find the total gravitational potential energy of the system, we need to consider the potential energy between each pair of masses. The system consists of four spheres of mass \( m \) at the corners of a square of side \( d \), and a fifth sphere of mass \( M \) at the center.
The correct option corresponds to: \(-\frac{Gm}{d}\bigg[\bigg(4+\sqrt2\bigg)m+4\sqrt2M\bigg]\).