Question:

What is the ratio of escape velocity to orbital velocity?

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Escape velocity is \(\sqrt{2}\) times the orbital velocity for the same celestial body.
Updated On: Apr 22, 2026
  • \(1:1\)
  • \(2:1\)
  • \(\sqrt{2}:1\)
  • \(1:\sqrt{2}\)
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The Correct Option is C

Solution and Explanation

Concept: Escape velocity is the minimum velocity required for an object to escape the gravitational field of a planet without returning. \[ v_e = \sqrt{\frac{2GM}{R}} \] Orbital velocity is the velocity required for a satellite to remain in circular orbit around a planet. \[ v_o = \sqrt{\frac{GM}{R}} \] where \(G\) = gravitational constant, \(M\) = mass of the planet, \(R\) = radius of the planet.

Step 1:
Write the ratio of escape velocity to orbital velocity. \[ \frac{v_e}{v_o} = \frac{\sqrt{\frac{2GM}{R}}}{\sqrt{\frac{GM}{R}}} \]

Step 2:
Simplify the expression. \[ \frac{v_e}{v_o} = \sqrt{2} \] Thus the ratio is \[ \sqrt{2} : 1 \]
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