A body which is initially at rest at a height \( R \) above the surface of the Earth of radius \( R \), falls freely towards the Earth. The velocity on reaching the surface of the Earth is:
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For free fall from height \( h \), the velocity on reaching the surface can be found using energy conservation:
\[
v = \sqrt{2 g h}
\]
or using gravitational potential.
Step 1: {Conserve total energy} Total energy is constant:\[{Kinetic energy gain} = {Potential energy loss}\]Step 2: {Apply gravitational potential energy formula} \[\frac{1}{2} mv^2 = mgR \left( \frac{1}{1 + \frac{h}{R}} \right)\]When \( h = R \):\[mv^2 = mgR\]\[v = \sqrt{gR}\]Therefore, the correct result is \( \sqrt{gR} \).