A moon of mass M and radius R orbits a planet of mass 3M and radius 2R. At a particular time, the distance between their centres is D, as shown in Fig. 2.1. Point P is a point along the line between the centres of the planet and the moon, at a variable distance x from the centre of the planet. The variation with x of the gravitational potential φ at point P, for points between the planet and the moon, is shown in Fig. 2.2. [Figure 2.1] [Figure 2.2] [Figure 2.3]
- (a)State the relationship between gravitational potential and gravitational field strength.[2]
- (b)(i)Explain why φ is negative throughout the entire range x = 2R to x = D – R.[3]
- (b)(ii)One of the features of Fig. 2.2 is that φ is negative throughout. Describe two other features of Fig. 2.2.[2]
- (b)(iii)On Fig. 2.3, sketch the variation with x of the gravitational field strength g at point P between x = 2R and x = D – R.[3]
This question uses a diagram from the original paper, which isn't shown here. Open the full paper from the past papers archive to see it.
Mark scheme
Marking points from the official mark scheme (Oct/Nov 2021). The mark or mark type is shown in brackets.
- (gravitational) field strength equals (gravitational) potential gradient
- reference to minus sign
- potential is zero at infinity
- (gravitational) force is attractive
- (test) mass getting closer (from infinity) loses potential energy
- potential at (surface of) planet is smaller than at (surface of) moon
- potential gradient at (surface of) planet is smaller than at (surface of) moon
- magnitude of potential varies inversely with distance from centre near the spheres
- (point of) maximum potential is nearer to moon than planet
- sketch: one curve, starting with gradient of decreasing magnitude at 2R and finishing with gradient of increasing magnitude at D – R
- field strength shown as zero (only) near the point of maximum potential
- negative field strength near one sphere and positive field strength near the other
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