The escape speed \( v_e \) for any celestial body is given by the formula: \[ v_e = \sqrt{\frac{2GM}{R}}, \] where \( G \) is the gravitational constant, \( M \) is the mass of the body, and \( R \) is its radius.
The escape speed depends on both the mass of the body and its radius. Let's compare the escape speeds of the Earth and the Moon.
Let \( v_e^{{Earth}} \) and \( v_e^{{Moon}} \) represent the escape speeds of the Earth and the Moon, respectively.
The ratio of the escape speeds is: \[ \frac{v_e^{{Moon}}}{v_e^{{Earth}}} = \sqrt{\frac{2GM_{{Moon}}/R_{{Moon}}}{2GM_{{Earth}}/R_{{Earth}}}} = \sqrt{\frac{M_{{Moon}} R_{{Earth}}}{M_{{Earth}} R_{{Moon}}}}. \] Given that:
- \( M_{{Moon}} \approx 0.012 \, M_{{Earth}} \),
- \( R_{{Moon}} \approx 0.27 \, R_{{Earth}} \), the ratio becomes: \[ \frac{v_e^{{Moon}}}{v_e^{{Earth}}} = \sqrt{\frac{0.012 \, M_{{Earth}} \times R_{{Earth}}}{M_{{Earth}} \times 0.27 \, R_{{Earth}}}} = \sqrt{\frac{0.012}{0.27}} \approx \sqrt{\frac{1}{22.5}} \approx \frac{1}{5}. \] Thus, the escape speed of the Moon is approximately 5 times smaller than that of the Earth.
Thus, the correct answer is option (D), 5 times smaller.
Kepler's second law (law of areas) of planetary motion leads to law of conservation of
Kepler's second law (law of areas) of planetary motion leads to law of conservation of