Question:

The acceleration due to gravity at the poles and the equator is $g_p$ and $g_e$ respectively. If the earth is a sphere of radius $R_E$ and rotating about its axis with angular speed 0), then $g_p - g_e$ is given by

Updated On: Jul 7, 2022
  • $\frac{\omega^{2}}{R_{E}}$
  • $\frac{\omega^{2}}{R^2_{E}}$
  • $\omega^{2}R_{E}^2$
  • $\omega^{2}R_{E}$
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The Correct Option is D

Solution and Explanation

Acceleration due to gravity at a place of latitude $\lambda$ due to the rotation of earth is $g'= g - R_{E}\omega^{2}cos^{2}\lambda$ At equator, $\lambda = 0^{\circ}, cos0^{\circ} = 1$ $\therefore g'= g_{ e}=g - R_{E}\omega^{2}$ At poles, $\lambda = 90^{\circ}, cos90^{\circ} = 0$ $\therefore g'=g_{p}=g$ $\therefore g_{p}-g_{e} = g - \left( g - R_{E}\omega^{2}\right) = R_{E}\omega^{2}$
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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