Step 1: Gravitational variation with altitude. The acceleration due to gravity at an altitude \( h \) from Earth's surface is defined by: \[ g_h = g \left( \frac{R}{R + h} \right)^2, \] where \( g_h = g/4 \), \( R \) represents Earth's radius, and \( g \) is the surface acceleration due to gravity.
Step 2: Substitution of \( g_h = g/4 \).
\[ \frac{g}{4} = g \left( \frac{R}{R + h} \right)^2. \] Divide both sides by \( g \): \[ \frac{1}{4} = \left( \frac{R}{R + h} \right)^2. \] Apply the square root: \[ \frac{1}{2} = \frac{R}{R + h}. \] Rearrange the equation: \[ R + h = 2R \quad \Rightarrow \quad h = R. \] \[ \therefore \text{The altitude is: } R. \]
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 
