The formula is given by:
\[ g = \frac{GM}{r^2} \]
where:
- \( g \) is the acceleration due to gravity,
- \( G \) is the gravitational constant (\(6.67 \times 10^{-11} \, \text{m}^3 \, \text{kg}^{-1} \, \text{s}^{-2}\)),
- \( M \) is the mass of the planet (in
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