Answer: r aph : r per.
- A r<sub>aph</sub> : r<sub>per</sub>
- B r<sub>per</sub> : r<sub>aph</sub>
- C r<sub>aph</sub><sup>2</sup> : r<sub>per</sub><sup>2</sup>
- D r<sub>per</sub><sup>2</sup> : r<sub>aph</sub><sup>2</sup>
Correct answer: A. r<sub>aph</sub> : r<sub>per</sub>
Explanation: By conservation of angular momentum: m x v<sub>per</sub> x r<sub>per</sub> = m x v<sub>aph</sub> x r<sub>aph</sub>. So v<sub>per</sub>/v<sub>aph</sub> = r<sub>aph</sub>/r<sub>per</sub>.
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.