S6 Physics Gravitation, Paper 3: inverse square and Kepler ratios
- 2026-11-02
S6 Physics Gravitation, Paper 3: inverse square and Kepler ratios
Ten graded items on weight on the Moon and other planets, g ratios, orbital radii from period ratios, plus escape and orbital speed.
Focus Surface g varies with mass and with the square of the radius, and Kepler ratios give radius as the two thirds power of the period.
01 Paper details (check answers afterwards)
| Item | Detail |
|---|---|
| Questions | 10 |
| Suggested time | 25 |
| Difficulty mix | Foundation 4 · Intermediate 3 · Challenge 2 · Error redo 1 |
| Chapter | Chapter: S6 Physics: Gravitation |
| Level | Four basic, three advanced, two challenge and one error-repair item |
02 Questions (10 items)
- FoundationThe Moon has surface g of 1.6 m/s^2. Find the weight of a 50 kg astronaut there.
- FoundationTwo 5 kg spheres are 1 m apart. Find the gravitational force between them.
- FoundationA planet has radius 5.0 x 10^6 m and surface g of 8.0 m/s^2. Find its mass.
- FoundationAt three Earth radii from the centre, what is g if the surface value is 9.8 m/s^2?
- IntermediateA satellite circles at 7.0 x 10^6 m from Earth centre. Find its period, with Earth mass 6.0 x 10^24 kg.
- IntermediateFind the escape speed of Earth, with mass 6.0 x 10^24 kg and radius 6.4 x 10^6 m.
- IntermediateA planet has twice the Earth mass and twice the radius. Find its surface g, taking the Earth value as 9.8 m/s^2.
- ChallengeTwo satellites orbit the same planet and the outer period is twice the inner one. Compare their orbital radii.
- ChallengeA planet has three times the Earth mass but the same radius. Find its surface g, taking the Earth value as 9.8 m/s^2.
- Error redoA student gets 7.9 km/s for the Earth escape speed using root gR. Find the mistake and the correct value.
03 Answers and one-line notes
| # | Answer | One-line note |
|---|---|---|
| 1 | 80 N | Weight is mass times surface gravity, so the astronaut weighs 80 newtons on the Moon. |
| 2 | About 1.67 x 10^-9 N | Five kilograms each at one metre apart gives about 1.67 times ten to the minus ninth newtons. |
| 3 | About 3.0 x 10^24 kg | Rearranging g equals GM over R squared gives a mass of about 3.0 times ten to the twenty-fourth kilograms. |
| 4 | About 1.09 m/s^2 | Distance triples, so g falls to one ninth of 9.8, about 1.09 metres per second squared. |
| 5 | About 5.8 x 10^3 s, roughly 97 minutes | The period works out near 5800 seconds, about 97 minutes, typical of a low Earth orbit. |
| 6 | About 11.2 km/s | The square root of twice GM over R gives about 11.2 kilometres per second, the well known Earth value. |
| 7 | Half, 4.9 m/s^2 | Doubling both mass and radius halves g, giving 4.9 metres per second squared. |
| 8 | About 1.59 times | Since the period scales as r to the three halves, doubling the period needs about 1.59 times the radius. |
| 9 | 29.4 m/s^2 | Mass triples at the same radius, so g triples to 29.4 metres per second squared. |
| 10 | Root gR is orbital speed; escape speed is root two times that, 11.2 km/s, about 1.41 times larger | Root gR is the circular orbital speed; escape speed needs the extra factor root two, giving 11.2 kilometres per second. |
04 What to do after marking
- After marking, redo only the wrong items and write down which step went wrong (formula, unit, or misread number).
- Repeat the same item two days later; move to the next paper only when both attempts are correct.
- Parents only need the answer and note columns; there is no need to explain every item.
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