$r^{-2}$
Step 1: The gravitational force between two masses is given by Newton's Law of Gravitation: \[ F = \frac{G m_1 m_2}{d^2} \] where $m_1$ and $m_2$ are the masses and $d$ is the separation.
Step 2: The masses of spheres are proportional to their volumes: \[ m_1 \propto r^3, \quad m_2 \propto \left(\frac{r}{2}\right)^3 = \frac{r^3}{8} \] Step 3: Since they are in contact, the separation $d$ is approximately the sum of their radii: \[ d \approx r + \frac{r}{2} = \frac{3r}{2} \]
Step 4: Substituting in the gravitational force formula: \[ F \propto \frac{(r^3) \times (r^3 / 8)}{(3r/2)^2} \]
Step 5: Simplifying: \[ F \propto \frac{r^6}{8 \times (9r^2 / 4)} \] \[ F \propto \frac{r^6}{18r^2} \] \[ F \propto r^{6 - 2} = r^4 \]
Step 6: Since force is inversely proportional to $r^2$, we get: \[ F \propto r^{-2} \]
Step 7: Therefore, the correct answer is (E). \bigskip
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: 