The formula is given by:
\[ g = 2 \pi G \rho h \]
where:
- \(g\) is the gravity anomaly,
- \(G\) is the gravitational constant (\(6.674 \times 10^{-11} \, \text{m}^3\text{kg}^{-1}\text{s}^{-2}\)),
- \(\rho\) is the density contrast (difference in density between
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