The formula is given by \(F = G \frac{m_1 m_2}{r^2}\), where \(F\) is the gravitational force between the two masses, \(G\) is the gravitational constant (\(6.674 \times 10^{-11} \, \text{Nm}^2/\text{kg}^2\)), \(m_1\) and \(m_2\) are the masses of the two objects,
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