Correct answer: 1: 1
Surface gravity is proportional to \(GM/R^2\), and mass can be written as \(\rho \cdot \frac{4}{3}\pi R^3\). So \(g \propto \rho R\); if the planet’s radius is doubled but \(g\) stays the same, its density must be halved? Wait—because the radius is doubled, the density must adjust so that \(\rho R\) remains unchanged, giving equal densities only if the radius comparison is handled correctly with the diameter relation. Since diameter doubles, radius doubles, and equal \(g\) requires \(\rho\) to be the same as Earth’s.