To solve the problem, we need to determine the velocity with which a particle should be projected from the surface of the Earth so that it reaches a height equal to the radius of the Earth.
Let the radius of the Earth be R and the gravitational constant be G. The mass of the Earth is M.
When a particle is projected with an initial velocity v from the Earth's surface and reaches a height equal to R, its potential energy and kinetic energy at the maximum height can be used to derive this velocity.
At the surface of the Earth:
At the height R:
By conservation of energy, the total initial energy is equal to the total energy at the maximum height:
\frac{1}{2}mv^2 - \frac{GMm}{R} = -\frac{GMm}{2R}
Simplifying this equation:
From this, we can simplify to find the initial velocity v:
v^2 = \frac{GM}{R}
Thus, the required initial velocity v is:
v = \bigg( \frac{GM}{R} \bigg)^{1/2}
This corresponds to the correct option: \bigg( \frac{GM}{R} \bigg)^{1/2}.
The height from Earth's surface at which acceleration due to gravity becomes \(\frac{g}{4}\) is \(\_\_\)? (Where \(g\) is the acceleration due to gravity on the surface of the Earth and \(R\) is the radius of the Earth.)