Question:

The escape velocity of a sphere of mass m is given by (G = Universal gravitational constant; M = Mass of the earth and R = Radius of the e earth)

Updated On: Oct 12, 2024
  • $\sqrt{\frac{ 2GM_e m }{ R_e}}$
  • $\sqrt{\frac{ 2GM_e }{ R_e}}$
  • $\sqrt{\frac{ GM_e m }{ R_e}}$
  • $\sqrt{\frac{ 2GM_e +R_e }{ R_e}}$
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The Correct Option is B

Solution and Explanation

The gravitational potential energy of a body of mass m placed on earth's surface is given by
$ U = - \frac{GM_e m }{ R_e}$
Threfore, in order to take a body from the earth's surface to infinity, the work required is $ \frac{ GM_e m }{ R_e} $.
Hence it is evident that if we throw a body of mass m with such a velocity that its kinetic energy is
$ \frac{ GM_e m }{ R_e} $, then it will move outside the gravitational field of earth.
Hence, $ \frac{ 1}{2} m {v_e}^2 = \frac{ GM_e m }{ R_e} $ or, $v_e = \sqrt { \frac{ 2GM_e m }{ R_e}}$.
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Concepts Used:

Gravitation

In mechanics, the universal force of attraction acting between all matter is known as Gravity, also called gravitation, . It is the weakest known force in nature.

Newton’s Law of Gravitation

According to Newton’s law of gravitation, “Every particle in the universe attracts every other particle with a force whose magnitude is,

  • F ∝ (M1M2) . . . . (1)
  • (F ∝ 1/r2) . . . . (2)

On combining equations (1) and (2) we get,

F ∝ M1M2/r2

F = G × [M1M2]/r2 . . . . (7)

Or, f(r) = GM1M2/r2

The dimension formula of G is [M-1L3T-2].