To determine the acceleration due to gravity on the surface of a planet, we use the formula \( g = \frac{G \cdot M}{R^2} \), where \( G \) is the gravitational constant, \( M \) is the mass of the planet, and \( R \) is its radius. For Earth, the gravity \( g_{\text{Earth}} \) is given as 10 m/s². Let \( M_{\text{Earth}} \) and \( R_{\text{Earth}} \) be the mass and radius of Earth, respectively. On the new planet:
We substitute these into the formula for gravity: \( g = \frac{G \cdot (M_{\text{Earth}}/80)}{(\frac{R_{\text{Earth}}}{4})^2} = \frac{G \cdot M_{\text{Earth}}}{80 \cdot \frac{R_{\text{Earth}}^2}{16}} = \frac{16 \cdot G \cdot M_{\text{Earth}}}{80 \cdot R_{\text{Earth}}^2} = \frac{1}{5} \cdot \frac{G \cdot M_{\text{Earth}}}{R_{\text{Earth}}^2} = \frac{1}{5} \cdot g_{\text{Earth}} \). Since \( g_{\text{Earth}} = 10 \, \text{m/s}^2 \), it follows that \( g = \frac{1}{5} \times 10 = 2 \, \text{m/s}^2 \).