Given:
Step 1: Understand escape speed
The escape speed \( v_e \) is the minimum speed needed to break free from Earth's gravitational pull without additional propulsion. At escape speed, the total energy at infinity is zero.
Step 2: Apply energy conservation
At Earth's surface:
\[ \text{Total Energy} = \text{Kinetic Energy} + \text{Potential Energy} \] \[ E_{\text{total}} = \frac{1}{2}mv_0^2 - \frac{GMm}{R} \]
Where:
At infinity (far from Earth):
\[ E_{\text{total}} = \frac{1}{2}mv_{\infty}^2 \]
Step 3: Relate to escape speed
We know that escape speed relates to potential energy:
\[ \frac{1}{2}mv_e^2 = \frac{GMm}{R} \]
Substituting into the energy equation:
\[ \frac{1}{2}mv_0^2 - \frac{1}{2}mv_e^2 = \frac{1}{2}mv_{\infty}^2 \]
Step 4: Solve for final speed
\[ v_{\infty}^2 = v_0^2 - v_e^2 \] \[ v_{\infty} = \sqrt{(3v_e)^2 - v_e^2} \] \[ v_{\infty} = \sqrt{9v_e^2 - v_e^2} \] \[ v_{\infty} = \sqrt{8v_e^2} \] \[ v_{\infty} = v_e\sqrt{8} \] \[ v_{\infty} = 11.2 \times 2.828 \] \[ v_{\infty} \approx 31.7 \, \text{km/s} \]
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 
