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The escape velocities of two planets A a...

The escape velocities of two planets `A `and` B` are in the ratio` 1 : 2`. If the ratio of their radii respectively is `1 : 3,` then the ratio of acceleration due to gravity of planet` A` to the acceleration of gravity of planet `B` will be :

A

`3/2`

B

`2/3`

C

`3/4`

D

`4/3`

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To solve the problem, we need to find the ratio of the acceleration due to gravity of planet A (g_A) to that of planet B (g_B) given the ratios of their escape velocities and radii. ### Step-by-Step Solution: 1. **Understanding Escape Velocity**: The escape velocity (v_e) from the surface of a planet is given by the formula: \[ v_e = \sqrt{2gR} \] where \( g \) is the acceleration due to gravity and \( R \) is the radius of the planet. 2. **Setting Up the Ratios**: We are given that the escape velocities of planets A and B are in the ratio: \[ \frac{v_{eA}}{v_{eB}} = \frac{1}{2} \] This implies: \[ v_{eA} = \frac{1}{2} v_{eB} \] 3. **Expressing Escape Velocities**: Using the escape velocity formula, we can express the escape velocities in terms of g and R: \[ v_{eA} = \sqrt{2g_A R_A} \] \[ v_{eB} = \sqrt{2g_B R_B} \] 4. **Substituting into the Ratio**: Substituting these expressions into the ratio of escape velocities: \[ \frac{\sqrt{2g_A R_A}}{\sqrt{2g_B R_B}} = \frac{1}{2} \] This simplifies to: \[ \frac{\sqrt{g_A R_A}}{\sqrt{g_B R_B}} = \frac{1}{2} \] 5. **Squaring Both Sides**: Squaring both sides gives: \[ \frac{g_A R_A}{g_B R_B} = \frac{1}{4} \] 6. **Using the Radius Ratio**: We are given that the ratio of the radii is: \[ \frac{R_A}{R_B} = \frac{1}{3} \] Therefore, we can express \( R_A \) in terms of \( R_B \): \[ R_A = \frac{1}{3} R_B \] 7. **Substituting Radius Ratio**: Substituting \( R_A \) into the equation: \[ \frac{g_A \left(\frac{1}{3} R_B\right)}{g_B R_B} = \frac{1}{4} \] Simplifying this gives: \[ \frac{g_A}{g_B} \cdot \frac{1}{3} = \frac{1}{4} \] 8. **Solving for the Gravity Ratio**: Multiplying both sides by 3: \[ \frac{g_A}{g_B} = \frac{3}{4} \] ### Final Result: Thus, the ratio of the acceleration due to gravity of planet A to that of planet B is: \[ \frac{g_A}{g_B} = \frac{3}{4} \]
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