The acceleration due to gravity at a height \( h \) above the Earth's surface is defined by the equation: \[ g_h = \frac{g}{\left( 1 + \frac{h}{R} \right)^2} \]. Here, \( g \) represents the acceleration due to gravity at the Earth's surface, \( g_h \) denotes the acceleration due to gravity at height \( h \), and \( R \) is the Earth's radius. Given that the acceleration due to gravity at height \( h \) equals \( \frac{g}{\sqrt{3}} \), we can write: \[ \frac{g}{\sqrt{3}} = \frac{g}{\left( 1 + \frac{h}{R} \right)^2} \]. By canceling \( g \) from both sides: \[ \frac{1}{\sqrt{3}} = \frac{1}{\left( 1 + \frac{h}{R} \right)^2} \]. Taking the square root of both sides yields: \[ \frac{1}{\sqrt{3}} = \frac{1}{1 + \frac{h}{R}} \]. Solving for \( h \): \[ 1 + \frac{h}{R} = \sqrt{3} \] \[ \frac{h}{R} = \sqrt{3} - 1 \] \[ h = R(\sqrt{3} - 1) \] Consequently, the height \( h \) is \( R \). The correct selection is option (a).
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 
