The gravitational force between two objects is described by Newton's Law of Universal Gravitation, which is given by the formula:
\[ F = \frac{G \cdot m_1 \cdot m_2}{r^2} \]
where:
- \( F \) is the gravitational force,
- \( G \) is the gravitational constant,
- \( m_1 \) and \( m_2 \) are the masses of the two objects,
- \( r \) is the distance between the centers of the two masses.
If the mass of one object decreases by one-half (\( m_1 \) becomes \( \frac{m_1}{2} \)), while the mass of the second object (\( m_2 \)) remains the same, the new gravitational force (\( F' \)) becomes:
\[ F' = \frac{G \cdot \frac{m_1}{2} \cdot m_2}{r^2} \]
This can be simplified to:
\[ F' = \frac{1}{2} \cdot \left( \frac{G \cdot m_1 \cdot m_2}{r^2} \right) = \frac{1}{2} F \]
Therefore, the gravitational force decreases by one-half.
Thus, the correct response is:
The gravitational force decreases by one-half.