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: \( \frac{K}{2x^2} \)
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:
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