Concept: Newton's Law of Universal Gravitation states that the gravitational force (\(F\)) between two objects of masses \(m_1\) and \(m_2\), separated by a distance \(r\) between their centers, is given by:
\[ F = G \frac{m_1 m_2}{r^2} \]
where \(G\) is the gravitational constant.
This formula shows that the force of gravitation is inversely proportional to the square of the distance between the objects (\(F \propto \frac{1}{r^2}\)).
Step 1: Write the initial force
Let the initial distance between the two objects be \(r_1\).
The initial gravitational force \(F_1\) is:
\[ F_1 = G \frac{m_1 m_2}{r_1^2} \]
Step 2: Define the new distance
The distance between them is reduced to half. Let the new distance be \(r_2\).
So, \(r_2 = \frac{r_1}{2}\).
Step 3: Calculate the new force (\(F_2\)) with the new distance
The new gravitational force \(F_2\) with distance \(r_2\) is:
\[ F_2 = G \frac{m_1 m_2}{r_2^2} \]
Substitute \(r_2 = \frac{r_1}{2}\):
\[ F_2 = G \frac{m_1 m_2}{\left(\frac{r_1}{2}\right)^2} \]
\[ F_2 = G \frac{m_1 m_2}{\frac{r_1^2}{4}} \]
To simplify the fraction in the denominator, multiply the numerator by the reciprocal of \(\frac{r_1^2}{4}\), which is \(\frac{4}{r_1^2}\):
\[ F_2 = G \frac{m_1 m_2}{1} \times \frac{4}{r_1^2} \]
\[ F_2 = 4 \left( G \frac{m_1 m_2}{r_1^2} \right) \]
Step 4: Relate the new force (\(F_2\)) to the initial force (\(F_1\))
We know from Step 1 that \(F_1 = G \frac{m_1 m_2}{r_1^2}\).
Substituting this into the expression for \(F_2\):
\[ F_2 = 4 F_1 \]
This means the new force \(F_2\) is 4 times the initial force \(F_1\).
So, when the distance is reduced to half, the force of gravitation becomes 4 times stronger. This matches option (2).