Step 1:
We start by writing down the Newton's law of universal gravitation:
\[F = G \frac{m_1 m_2}{r^2}\]
where \(F\) is the gravitational force, \(G\) is the gravitational constant, \(m_1\) and \(m_2\) are the masses of the two objects, and \(r\) is the distance
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