This problem is solved by analyzing the gravitational interactions among spheres and the impact of mass and distance variations on collision duration. The initial setup involves three spheres, each with mass \( m \), positioned at the vertices of an equilateral triangle with side length \( a \). These spheres collide after \( T = 4 \) seconds. The computations required are as follows:
Therefore, in the modified configuration, the spheres will collide in approximately 8 seconds. This result is confirmed as it falls within the expected range of 8,8.
Net gravitational force at the center of a square is found to be \( F_1 \) when four particles having masses \( M, 2M, 3M \) and \( 4M \) are placed at the four corners of the square as shown in figure, and it is \( F_2 \) when the positions of \( 3M \) and \( 4M \) are interchanged. The ratio \( \dfrac{F_1}{F_2} = \dfrac{\alpha}{\sqrt{5}} \). The value of \( \alpha \) is 
