This can be mathematically represented as:
\[ F = G \frac{{m_1 m_2}}{{r^2}} \]
where:
- \(F\) is the force between the masses,
- \(G\) is the gravitational constant,
- \(m_1\) and \(m_2\) are the two masses, and
- \(r\) is the distance between the centers of the
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