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: {Apply conservation of energy}
The total energy remains constant:
\[
{Increase in kinetic energy} = {Decrease in potential energy}
\]
Step 2: {Using gravitational potential energy}
\[
\frac{1}{2} mv^2 = mgR \left( \frac{1}{1 + \frac{h}{R}} \right)
\]
For \( h = R \):
\[
mv^2 = mgR
\]
\[
v = \sqrt{gR}
\]
Thus, the correct answer is \( \sqrt{gR} \).
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Approach Solution -2
Step 1: Given:
- Initial height from Earth’s surface = \( R \)
- Radius of Earth = \( R \)
- So, initial distance from Earth’s center = \( 2R \)
- Final distance from Earth’s center (on the surface) = \( R \)
- Initial velocity = 0 (body starts from rest)
Step 2: Use conservation of mechanical energy:
Initial total energy = Final total energy
\( \Rightarrow \frac{-GMm}{2R} + 0 = \frac{-GMm}{R} + \frac{1}{2}mv^2 \)
Step 3: Rearranging terms:
\( \frac{-GMm}{2R} = \frac{-GMm}{R} + \frac{1}{2}mv^2 \)
Bring all potential terms to one side:
\( \frac{-GMm}{2R} + \frac{GMm}{R} = \frac{1}{2}mv^2 \)
\( \frac{GMm}{2R} = \frac{1}{2}mv^2 \)
Step 4: Cancel \( m \) and simplify:
\( \frac{GM}{2R} = \frac{1}{2}v^2 \Rightarrow v^2 = \frac{GM}{R} \)
Step 5: Use \( g = \frac{GM}{R^2} \Rightarrow GM = gR^2 \)
Substitute into the equation:
\( v^2 = \frac{gR^2}{R} = gR \)
So, \( v = \sqrt{gR} \)