isaac newton the laws of motion and relativity a
ormula: \[ F = G \frac{m_1 m_2}{r^2} \] Where: \( F \) is the gravitational force between two objects. \( G \) is the gravitational constant. \( m_1 \) and \( m_2 \) are the masses. \( r \) is the distance between the centers of the two masses. Significance: Explained the ellipt