Step 1:
\[ [\Delta x] = \text{m}, \quad [\Delta v] = \text{m s}^{-1} \]
Step 2:
\[ [\Delta x \cdot \Delta v] = \text{m}^2 \text{s}^{-1} \]
Step 3:
\[ \text{Rewrite: } \text{m}^2 \text{s}^{-1} = \frac{1}{\text{m}^{-2} \text{s}} \]
Step 4:
\[ \text{Closest form: } \text{m}^{-2}\text{s}^{-1} \]
Final Answer:
\[ Option (D) \]
Kepler's second law (law of areas) of planetary motion leads to law of conservation of