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The radius of a planet is 1/4th of R(c )...

The radius of a planet is 1/4th of `R_(c )` and its acc accleration due to gravity is 2 g. What would be the value of escape velocity on the planet, if escape velocity on earth is V.

A

`(V)/(sqrt(2))`

B

`Vsqrt(2)`

C

`2 V `

D

`V//2`

Text Solution

AI Generated Solution

The correct Answer is:
To solve the problem, we need to find the escape velocity on the planet given its radius and acceleration due to gravity. Let's break it down step by step. ### Step 1: Understand the relationship between escape velocity, gravitational acceleration, and radius. The escape velocity \( V \) from the surface of a planet is given by the formula: \[ V = \sqrt{2gR} \] where \( g \) is the acceleration due to gravity at the surface of the planet, and \( R \) is the radius of the planet. ### Step 2: Substitute the values for the planet. According to the problem: - The radius of the planet \( R_p = \frac{1}{4} R_e \) (where \( R_e \) is the radius of the Earth). - The acceleration due to gravity on the planet \( g_p = 2g_e \) (where \( g_e \) is the acceleration due to gravity on Earth). ### Step 3: Substitute \( g_p \) and \( R_p \) into the escape velocity formula. Now we can substitute these values into the escape velocity formula: \[ V_p = \sqrt{2g_p R_p} \] Substituting the values we have: \[ V_p = \sqrt{2(2g_e)\left(\frac{1}{4}R_e\right)} \] ### Step 4: Simplify the expression. Now simplify the expression: \[ V_p = \sqrt{2 \cdot 2g_e \cdot \frac{1}{4}R_e} = \sqrt{\frac{4g_e R_e}{4}} = \sqrt{g_e R_e} \] ### Step 5: Relate this to the escape velocity on Earth. We know that the escape velocity on Earth \( V_e \) is: \[ V_e = \sqrt{2g_e R_e} \] Now, we can express \( V_p \) in terms of \( V_e \): \[ V_p = \sqrt{g_e R_e} = \sqrt{\frac{1}{2} \cdot 2g_e R_e} = \frac{V_e}{\sqrt{2}} \] ### Step 6: Final expression for escape velocity on the planet. Thus, the escape velocity on the planet \( V_p \) can be expressed as: \[ V_p = \frac{V}{\sqrt{2}} \] ### Conclusion The value of escape velocity on the planet is \( \frac{V}{\sqrt{2}} \).
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