$r^{-2}$
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
The height from Earth's surface at which acceleration due to gravity becomes \(\frac{g}{4}\) is \(\_\_\)? (Where \(g\) is the acceleration due to gravity on the surface of the Earth and \(R\) is the radius of the Earth.)