\(\frac{Rk^2}{1-k^2}\)
\(R(\frac{k}{1-k})^2\)
\(R(\frac{k}{1+k})^2\)
\(\frac{R^2k}{1+k}\)
To solve this problem, we need to determine the maximum height reached by a particle projected upwards from the Earth's surface with an initial velocity defined in terms of escape velocity. Let's break down the solution step-by-step:
The given data includes:
The escape velocity from the Earth's surface is given by:
\(V_e = \sqrt{\frac{2GM}{R}}\)
where:
The initial kinetic energy of the particle is:
\(\frac{1}{2}mv^2 = \frac{1}{2}m(kV_e)^2 = \frac{1}{2}mk^2V_e^2\)
The initial gravitational potential energy at the Earth's surface is:
\(-\frac{GMm}{R}\)
At the maximum height \( h \) above the Earth's surface, the particle will momentarily stop, and all initial kinetic energy is converted into gravitational potential energy.
Equating the initial total energy to the total energy at the maximum height, we have:
\(\frac{1}{2}mk^2V_e^2 - \frac{GMm}{R} = -\frac{GMm}{R + h}\)
From the expression of escape velocity, substitute \( V_e^2 = \frac{2GM}{R} \) to get:
\(\frac{1}{2}mk^2 \cdot \frac{2GM}{R} - \frac{GMm}{R} = - \frac{GMm}{R + h}\)
Simplifying this equation:
\(mk^2 \frac{GM}{R} - \frac{GMm}{R} = -\frac{GMm}{R + h}\)
Further simplification gives:
\(GMm \left(\frac{k^2}{R} - \frac{1}{R}\right) = -\frac{GMm}{R + h}\)
This can be simplified to:
\(GMm \left(\frac{k^2 - 1}{R}\right) = -\frac{GMm}{R + h}\)
Cancelling GMm from both sides and solving for \( h \), we get:
\(R + h = \frac{R}{1-k^2}\)
Hence, the maximum height \( h \) above the Earth's surface is:
\(h = \frac{R}{1-k^2} - R = \frac{Rk^2}{1-k^2}\)
Therefore, the correct answer is: \(\frac{Rk^2}{1-k^2}\)
Match the LIST-I with LIST-II
\[ \begin{array}{|l|l|} \hline \text{LIST-I} & \text{LIST-II} \\ \hline \text{A. Gravitational constant} & \text{I. } [LT^{-2}] \\ \hline \text{B. Gravitational potential energy} & \text{II. } [L^2T^{-2}] \\ \hline \text{C. Gravitational potential} & \text{III. } [ML^2T^{-2}] \\ \hline \text{D. Acceleration due to gravity} & \text{IV. } [M^{-1}L^3T^{-2}] \\ \hline \end{array} \]
Choose the correct answer from the options given below:
A small point of mass \(m\) is placed at a distance \(2R\) from the center \(O\) of a big uniform solid sphere of mass \(M\) and radius \(R\). The gravitational force on \(m\) due to \(M\) is \(F_1\). A spherical part of radius \(R/3\) is removed from the big sphere as shown in the figure, and the gravitational force on \(m\) due to the remaining part of \(M\) is found to be \(F_2\). The value of the ratio \( F_1 : F_2 \) is: 
Escape speed is the minimum speed, which is required by the object to escape from the gravitational influence of a plannet. Escape speed for Earth’s surface is 11,186 m/sec.
The formula for escape speed is given below:
ve = (2GM / r)1/2
where ,
ve = Escape Velocity
G = Universal Gravitational Constant
M = Mass of the body to be escaped from
r = Distance from the centre of the mass