The relationship between distance and gravitational force is a key concept in this exercise.
- If the Moon were twice as close to Earth as it is now, we need to apply the inverse square law to understand the change in gravitational force.
Since the distance \( r \) is halved (making it \( \frac{1}{2} \) of the original distance), we substitute \( r \rightarrow \frac{r}{2} \) into the inverse square formula:
\[ \frac{1}{\left(\frac{r}{2}\right)^2} = \frac{1}{\frac{r^2}{4}} = 4 \]
This calculation shows that the gravitational force would be \textbf{4 times stronger} if the Moon were twice as close to Earth. It highlights how the inverse square law can be practically applied to predict changes in gravitational force based on changes in distance.