$r^{-2}$
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
Kepler's second law (law of areas) of planetary motion leads to law of conservation of
Kepler's second law (law of areas) of planetary motion leads to law of conservation of