Step 1: Variation of gravity with height.
The acceleration due to gravity at a height \( h \) above the Earth's surface is given by: \[ g_h = g \left( \frac{R}{R + h} \right)^2, \] where \( g_h = g/4 \), \( R \) is the radius of Earth, and \( g \) is the acceleration due to gravity on the surface.
Step 2: Substituting \( g_h = g/4 \).
\[ \frac{g}{4} = g \left( \frac{R}{R + h} \right)^2. \] Cancel \( g \) from both sides: \[ \frac{1}{4} = \left( \frac{R}{R + h} \right)^2. \] Taking the square root: \[ \frac{1}{2} = \frac{R}{R + h}. \] Rearranging: \[ R + h = 2R \quad \Rightarrow \quad h = R. \] \[ \therefore \text{The height is: } R. \]
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 
