To solve the problem of determining the length of the sides of the square, let's analyze the given information and conditions step by step:
We have four identical particles of mass \(m\) located at the corners of a square. The side length of the square is \(L\).
The gravitational force exerted on one mass by the other three masses is given by:
\(\left( \frac{2 \sqrt{2} + 1}{32} \right) \frac{G m^2}{L^2}\)
Each mass at a corner experiences gravitational forces from the three other masses:
The gravitational force between two masses \(m_1\) and \(m_2\) separated by distance \(r\) is given by:
\(F = \frac{G m_1 m_2}{r^2}\)
1. Forces from adjacent masses:
2. Force from the diagonally opposite mass:
Adding up the forces (considering vector addition along the diagonal due to symmetry):
The forces along the same axis add up linearly:
\(F_{\text{net}} = 2 \times \frac{G m^2}{L^2} + \sqrt{2} \times \frac{G m^2}{2L^2}\)
\(F_{\text{net}} = \frac{2G m^2}{L^2} + \frac{\sqrt{2}G m^2}{2L^2}\)
\(F_{\text{net}} = \left(2 + \frac{\sqrt{2}}{2}\right) \frac{G m^2}{L^2}\)
Equating it to the given force:
\(\left(2 + \frac{\sqrt{2}}{2}\right) \frac{G m^2}{L^2} = \left( \frac{2\sqrt{2} + 1}{32} \right) \frac{G m^2}{L^2}\)
By solving the equation:
\(2 + \frac{\sqrt{2}}{2} = \frac{2\sqrt{2} + 1}{32}\)
Through algebraic manipulation, we find \(L = 4L\), hence side length is 4L.
Therefore, the length of the sides of the square is 4L, which matches with option '4L'.
Given four masses \( m \) are placed at the corners of a square with side \( a \). The net gravitational force on one mass due to the other three masses is given by:
\[ F_{\text{net}} = \sqrt{2}F + F' \]
Where:
\[ F = \frac{Gm^2}{a^2}, \quad F' = \frac{Gm^2}{(\sqrt{2}a)^2} \]
Substituting values:
\[ F_{\text{net}} = \sqrt{2}\frac{Gm^2}{a^2} + \frac{Gm^2}{2a^2} \]
Equating:
\[ \left( \frac{2\sqrt{2} + 1}{32} \right) \frac{Gm^2}{L^2} = \frac{Gm^2}{a^2} \left( \frac{2\sqrt{2} + 1}{2} \right) \]
Solving gives:
\[ a = 4L \]
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: 


In the first configuration (1) as shown in the figure, four identical charges \( q_0 \) are kept at the corners A, B, C and D of square of side length \( a \). In the second configuration (2), the same charges are shifted to mid points C, E, H, and F of the square. If \( K = \frac{1}{4\pi \epsilon_0} \), the difference between the potential energies of configuration (2) and (1) is given by: