Answer: R/3.
- A R/3
- B R/2
- C R
- D 2R
Correct answer: A. R/3
Explanation: Energy: (1/2)m(ve/2)<sup>2</sup> - GMm/R = -GMm/(R+h). (ve<sup>2</sup>/8) - GM/R = -GM/(R+h). ve<sup>2</sup> = 2gR = 2GM/R. GM/(4R) - GM/R = -GM/(R+h). -3GM/(4R) = -GM/(R+h). R+h = 4R/3. h = R/3.
g is maximum at Earth's surface; going up, it falls off as 1/r² (inverse-square); going down, it falls off linearly with depth (since only the mass enclosed within radius r contributes), reaching zero at the centre.
Concept context
Universal gravitation, orbital mechanics, gravitational potential, and escape velocity.