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Q. $R$ is the radius of the Earth and $\omega$ is its angular velocity and $g_{p}$ is the value of $g$ at poles. The effective value of ' $g$ ' at the latitude $\lambda=60^{\circ}$ will be equal to

Gravitation

Solution:

$ g=g_{p}-\omega^{2} R\, \cos ^{2}\, \lambda$
Here $\lambda=60^{\circ} $
$\Rightarrow g=g_{p}-\omega^{2} R \cos ^{2} 60^{\circ}=g_{p}-\frac{\omega^{2} R}{4}$