Question:

The ratio of escape velocity at earth $v_e$ to the escape velocity at a planet $v_p$ whose radius and mean density are twice as that of earth is :

Updated On: Apr 20, 2025
  • $1 : 2 \sqrt{2}$
  • $1 : 4$
  • $1 : \sqrt{2}$
  • $ 1 : 2 $
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The Correct Option is A

Solution and Explanation

Escape Velocity and Density Relation 

The escape velocity \( V_e \) from a spherical body is given by the formula:

\(V_e = \sqrt{\frac{2GM}{R}}\)

Where:

  • \( G \) is the gravitational constant,
  • \( M \) is the mass of the body,
  • \( R \) is the radius of the body.

 

Substituting the expression for mass \( M \) in terms of density \( \rho \) (where \( M = \frac{4}{3} \pi R^3 \rho \)), we get:

\(V_e = \sqrt{\frac{2G}{R} \left(\frac{4}{3} \pi R^3 \rho \right)}\)

This simplifies to:

\(V_e \propto R \sqrt{\rho}\)

Conclusion:

Therefore, the ratio of escape velocities for two bodies with different radii and densities is:

\(1 : 2 \sqrt{2}\)

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Concepts Used:

Escape Speed

Escape speed is the minimum speed, which is required by the object to escape from the gravitational influence of a plannet. Escape speed for Earth’s surface is 11,186 m/sec. 

The formula for escape speed is given below:

ve = (2GM / r)1/2 

where ,

ve = Escape Velocity 

G = Universal Gravitational Constant 

M = Mass of the body to be escaped from 

r = Distance from the centre of the mass