A body is released from a height equal to the radius (r) of the earth. The velocity of the body when it strikes the surface of the earth will be:
To solve this problem, we need to determine the velocity of a body when it strikes the surface of the Earth after being released from a height equal to the radius of the Earth, denoted as \( R \).
Start by considering the potential energy and kinetic energy concepts. At the height of release, the potential energy of the body is at a maximum, while the kinetic energy is zero since the body is at rest.
Initially, the gravitational potential energy \( U \) at height \( R \) above the Earth's surface is:
\(U_i = -\frac{G M m}{2R}\)
where:
At the surface of the Earth, the potential energy is:
\(U_f = -\frac{G M m}{R}\)
The change in potential energy as the body falls is:
\(\Delta U = U_f - U_i = -\frac{G M m}{R} + \frac{G M m}{2R} = -\frac{G M m}{2R}\)
When the body strikes the Earth, all potential energy change is converted into kinetic energy:
\(elta K = \frac{1}{2} m v^2\), where \( v \) is the velocity of the body at the surface of the Eart\)
Equating the change in potential energy to the change in kinetic energy, we have:
\(\frac{1}{2} m v^2 = -\Delta U = \frac{G M m}{2R}\)
Solving for \( v \), we find:
\(v^2 = \frac{G M}{R}\)
We know that the acceleration due to gravity \( g \) is given by:
\(g = \frac{G M}{R^2}\)
Thus, substituting \( G M = g R^2 \) into the equation for \( v^2 \), we get:
\(v^2 = g R\)
Therefore, the velocity \( v \) is:
\(v = \sqrt{gR}\)
This matches the option: \(\sqrt{gR}\), confirming it as the correct answer.