The gravitational potential \( V \) is related to the gravitational field \( E \) by: \[ E = -\frac{dV}{dx} \] We are given that \( E = \frac{K}{x^3} \), and we need to find \( V \).
Integrating \( E \) with respect to \( x \), we get: \[ V = -\int E \, dx = -\int \frac{K}{x^3} \, dx = \frac{K}{2x^2} \] Thus, the gravitational potential at distance \( x \) is \( \frac{K}{2x^2} \).
Final Answer: \( \frac{K}{2x^2} \)
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: 

Match the following physical quantities with their respective dimensional formulas.
