CLASSICAL MECHANICS & THERMODYNAMICS - Chapter 6, Exercise 2 Solution ========================================================== The Moon's Escape Velocity PROBLEM ------- The Moon has a surface gravity of about 1.62 m/s^2 and a radius of about 1.737 x 10^6 m. Using v = sqrt(2gr), calculate the Moon's escape velocity, and compare it to Earth's 11.2 km/s. SOLUTION -------- Using the surface-gravity form of the escape velocity formula: v = sqrt(2gr) g = 1.62 m/s^2 r = 1.737 x 10^6 m v = sqrt(2 x 1.62 x 1.737 x 10^6) v = sqrt(5.628 x 10^6) v = 2372 m/s (approximately) v = 2.37 km/s (approximately) ANSWER: The Moon's escape velocity is approximately 2.37 km/s - roughly one-fifth (about 21%) of Earth's 11.2 km/s. ---- WHY THIS WORKS AS AN ANSWER Escape velocity depends on both the strength of surface gravity (g) and the size (radius, r) of the body - a body needs a combination of strong enough gravity AND enough "distance to climb out of" for escape to be hard. The Moon has both a much weaker surface gravity than Earth (about 1/6th) and a smaller radius (roughly 27% of Earth's), and both factors combine inside the square root to make the Moon's escape velocity far lower than Earth's. This is exactly why the real Apollo lunar module needed only a comparatively small ascent engine to leave the Moon's surface and return to lunar orbit, while a rocket leaving Earth needs vastly more powerful engines to reach 11.2 km/s.