\(\mathbf{22.4 \text{ km/s}}\)
Step 1: Understanding the escape velocity formula The escape velocity is given by the formula: \[ v_e = \sqrt{\frac{2 G M}{R}} \] where: - \( v_e \) is the escape velocity, - \( G \) is the universal gravitational constant, - \( M \) is the mass of the planet, - \( R \) is the radius of the planet.
Step 2: Expressing in terms of density Since density \( \rho \) is given by: \[ \rho = \frac{M}{\frac{4}{3} \pi R^3} \] we can express the mass in terms of density and radius: \[ M = \rho \times \frac{4}{3} \pi R^3 \] Substituting in the escape velocity formula: \[ v_e = \sqrt{\frac{2 G \rho \times \frac{4}{3} \pi R^3}{R}} \] Since \( \rho \) is constant for both Earth and the given planet, the escape velocity depends on: \[ v_e \propto \sqrt{\frac{M}{R}} \] Step 3: Finding the relation between escape velocities For Earth: \[ v_{e,E} = \sqrt{\frac{2 G M_E}{R_E}} \] For the given planet (with mass \( M_P = 8 M_E \) and same density): \[ \frac{M_P}{M_E} = 8 \] Since density is the same: \[ \frac{M_P}{M_E} = \frac{R_P^3}{R_E^3} \] Taking cube root: \[ \frac{R_P}{R_E} = \sqrt[3]{8} = 2 \] Now, the escape velocity ratio is: \[ \frac{v_{e,P}}{v_{e,E}} = \sqrt{\frac{M_P}{R_P}} \] \[ = \sqrt{\frac{8 M_E}{2 R_E}} = \sqrt{4} = 2 \] Thus, \[ v_{e,P} = 2 v_{e,E} \]
Step 4: Calculating the final value Given that: \[ v_{e,E} = 11.2 \text{ km/s} \] \[ v_{e,P} = 2 \times 11.2 = 22.4 \text{ km/s} \]
Step 5: Verifying the correct option Comparing with given options, the correct answer is: \[ \mathbf{22.4 \text{ km/s}} \]
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 
