Standard difficulty · 20 questions · 40 marks
Show your working for Sections B and C. Answers are on the last page — try every question first!
Gravitation · AW-11P-GRV-2026-V1 · For parents — fold back or tear off before handing the sheet to your child.
| Q | Answer | Working |
|---|---|---|
| 1 | (d) 544 N | F ∝ 1/r2 |
| 2 | (a) 50 m/s2 | g = GM/R2, so g′ = g × m/r2 |
| 3 | (d) 3 | vₑ = √(2GM/R) ∝ √(M/R) |
| 4 | (c) 27 | T2 ∝ r3, so T ∝ r^(3/2) |
| 5 | (d) 6.67 × 10−11 N m2 kg−2 | — |
| 6 | (a) 9.5 m/s2 | 10 × (1 − 320/6400) |
| 7 | (d) 6.25 m/s2 | g′ = g(1 − d/R) |
| 8 | (c) A is true, but R is false. | A is true: g′ = g/4, so the weight is 84 ÷ 4 = 21 N. R is false. |
| 9 | Mass 46 kg; weight 230 N; on the earth 460 N | mass does not change; weight = mg |
| 10 | 19,200 km (= 3R) | R2/(R + h)2 = 1/16, so R + h = 4R |
| 11 | 4,800 km | g′ = g(1 − d/R); d/R = 75/100 |
| 12 | v = √(gR) = 10000 m/s; T = 2πR/v = 3,142.86 s; KE = 9.50 × 1010 J | mg = mv2/R |
| 13 | 64 years | T2 ∝ r3: T = 16^(3/2) years |
| 14 | 2.02 × 10−7 N | F = Gm1m2/r2 = 6.67 × 10−11 × 91 × 48 ÷ 1.44 |
| 15 | 1.28 × 1010 J | ΔU = GMm[1/R − 1/(R + h)] = mgR × 2/3 |
| 16 | 22.4 km/s | vₑ ∝ √(M/R): 11.2 × √4 |
| 17 | (a) 0.016 m/s2; (b) 1,600 m/s; (c) 6.29 × 105 s; (d) 2.43 × 109 J | v = √(gR2/(R + h)) = 8000/√25; T = 2π(R + h)/v |
| 18 | (a) 88.89 N; (b) 400 N; (c) 0 N, because g is zero at the centre: the earth's mass pulls equally in all directions | g′ = gR2/(R + h)2; g′ = g(1 − d/R) |
| 19 | 256 hours; Kepler's third law (T2 ∝ r3) | T2 = T1 × (16)^(3/2) |
| 20 | 360,000 km from the 81M body (40,000 km from M) | GM/x2 = G(81M)/(d − x)2, so (d − x)/x = 9 |