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Gravitational field strength: AQA A‑Level Physics questions

AQA A-Level Physics past-paper questions on 3.7.2.2 Gravitational field strength, 2008–2025, with mark schemes and examiner’s reports where available.

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  2. Q06.1

    June 2025 · Paper 2

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  4. Q05.2

    June 2024 · Paper 2

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  5. Q03.1

    June 2023 · Paper 2

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  6. Q03.3

    June 2023 · Paper 2

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  7. Q03.4

    June 2023 · Paper 2

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  8. Q04.1

    June 2022 · Paper 2

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  9. Q04.2

    June 2022 · Paper 2

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  10. Q04.3

    June 2022 · Paper 2

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  11. Q04.4

    June 2022 · Paper 2

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  12. Q09

    June 2022 · Paper 2

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  13. Q12

    November 2021 · Paper 2

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  14. Q02.5

    November 2020 · Paper 2

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  15. Q12

    June 2019 · Paper 2

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  16. Q19

    June 2018 · Paper 2

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  17. Q06.1

    June 2017 · Paper 2

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  18. Q06.2

    June 2017 · Paper 2

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  20. Q07.3

    June 2017 · Paper 2

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All 50 questions on Gravitational field strength, as a list
  1. June 2025, Paper 2, Q04.2 (1 mark): A student suggests that, over the range of distances shown in Figure 2, the gravitational field strength due to the mass of Saturn alone is approximately consta
  2. June 2025, Paper 2, Q06.1 (3 marks): Student A suggests that the gravitational force acting on the ion due to Jupiter provides the centripetal acceleration of the ion. Deduce whether this suggestio
  3. June 2024, Paper 2, Q05.1 (3 marks): The resultant force on S1 is due to the gravitational forces from the Earth and the Moon. The magnitude of the Earth’s gravitational field strength at the orbit
  4. June 2024, Paper 2, Q05.2 (2 marks): Calculate the distance from S1 to the centre of the Moon. mass of the Moon = 7.35 × 1022 kg [2 marks] distance = m
  5. June 2023, Paper 2, Q03.1 (2 marks): Describe two properties of a radial gravitational field. [2 marks] 1 2
  6. June 2023, Paper 2, Q03.3 (2 marks): Calculate g g S E . distance from the Earth to the Sun = 1.50 × 1011 m [2 marks] g g S E =
  7. June 2023, Paper 2, Q03.4 (1 mark): Explain why gS is more important than gE in predicting the motion of the space probe as it escapes from the Solar System. [1 mark]
  8. June 2022, Paper 2, Q04.1 (2 marks): Compare, with reference to Figure 4, the masses of G and H. [2 marks]
  9. June 2022, Paper 2, Q04.2 (1 mark): X and Y are two points in the field. Annotate Figure 4 to show the field direction at X and the field direction at Y. [1 mark]
  10. June 2022, Paper 2, Q04.3 (1 mark): A spherical asteroid P has a mass of 2.0 × 1020 kg. The gravitational field strength at its surface is 0.40 N kg−1. Calculate the radius R of P. [1 mark] R = m
  11. June 2022, Paper 2, Q04.4 (1 mark): Sketch, on Figure 5, the variation of the gravitational field strength g with distance r. The distance r is measured from the centre of P. [1 mark] Figure 5
  12. June 2022, Paper 2, Q09 (1 mark): A planet of radius R and mass M has a gravitational field strength of g at its surface. Which row describes a planet with a gravitational field strength of 4g a
  13. November 2021, Paper 2, Q12 (1 mark): A planet has radius R and density ρ. The gravitational field strength at the surface is g. What is the gravitational field strength at the surface of a planet o
  14. November 2020, Paper 2, Q02.5 (3 marks): A spring mechanism can project an object vertically to a maximum height of 1.0 m from the surface of the Earth. Determine whether the same mechanism could proje
  15. June 2019, Paper 2, Q12 (1 mark): An object moves freely at 90° to the direction of a gravitational field. The acceleration of the object is [1 mark] A zero. B opposite to the direction of the g
  16. June 2018, Paper 2, Q19 (1 mark): The Earth can be assumed to be a uniform sphere of radius R. What is the mean density of the Earth? [1 mark] A 3g 4πRG B 3RG 4πg C 3G 4πRg D 3Rg 4πG
  17. June 2017, Paper 2, Q06.1 (1 mark): State what is represented by gravitational field lines. [1 mark]
  18. June 2017, Paper 2, Q06.2 (2 marks): Figure 6 shows the gravitational field above a small horizontal region on the surface of the Earth. Figure 6 Suggest why the field lines converge over a small a
  19. June 2017, Paper 2, Q06.3 (2 marks): A ball travelling at constant speed passes position J moving towards position K in Figure 6. Assume friction is negligible. Explain any change in the speed of t
  20. June 2017, Paper 2, Q07.3 (3 marks): A small mass released from rest just above the surface of Pluto has an acceleration of 0.617 m s−2. Assume Pluto has no atmosphere that could provide any resist
  21. June 2017, Paper 2, Q12 (1 mark): Charon is a moon of Pluto that has a mass equal to that of Pluto. The distance between the centre of Pluto and the centre of Charon is d. X is the point at whic
  22. Specimen, Paper 2, Q08 (1 mark): A planet has a radius half the Earth's radius and a mass a quarter of the Earth's mass. What is the approximate gravitational field strength on the surface of t
  23. Specimen, Paper 2, Q09 (1 mark): Two stars of mass M and 4M are at a distance d between their centres. The resultant gravitational field strength is zero along the line between their centres at
  24. June 2016, PHYA4 Section B (old spec), Q2(a)(i) (2 marks): Show that the gravitational field strength gs at the surface of a planet is related to the the density ρ and the radius R of the planet by the expression gs = –
  25. June 2016, PHYA4 Section B (old spec), Q2(a)(ii) (3 marks): Calculate the radius of Venus. Give your answer to an appropriate number of significant figures. [3 marks] radius = ___________________________ m
  26. June 2016, PHYA4 Section B (old spec), Q2(b) (3 marks): At a certain time, the positions of Earth and Venus are aligned so that the distance between them is a minimum. Sketch a graph on the axes below to show how the
  27. June 2015, PHYA4 Section A (old spec), Q10 (1 mark): The following data refer to two planets, P and Q. The gravitational field strength at the surface of P is 13.4 N kg–1. What is the gravitational field strength
  28. June 2015, PHYA4 Section A (old spec), Q11 (1 mark): The diagram shows an isolated binary star system. The two stars have equal masses, M, and the distance between their centres is r. The point P is half-way betwe
  29. June 2014, PHYA4 Section B (old spec), Q1(a)(i) (2 marks): Define gravitational field strength and state whether it is a scalar or vector quantity. [2 marks]
  30. June 2014, PHYA4 Section B (old spec), Q1(a)(ii) (2 marks): A mass m is at a height h above the surface of a planet of mass M and radius R. The gravitational field strength at height h is g. By considering the gravitatio
  31. June 2013, PHYA4 Section A (old spec), Q12 (1 mark): The gravitational field strengths at the surfaces of the Earth and the Moon are 9.8Nkg–1 and 1.7Nkg–1 respectively. If the mass of the Earth is 81 × the mass of
  32. June 2013, PHYA4 Section A (old spec), Q13 (1 mark): Two stars of mass M and 4M are at a distance d between their centres. The resultant gravitational field strength is zero along the line between their centres at
  33. January 2013, PHYA4 Section A (old spec), Q11 (1 mark): Which one of the following gives a correct unit for (––) ? A Nm–2 B Nkg–1 C Nm D N g2 G
  34. January 2013, PHYA4 Section A (old spec), Q12 (1 mark): The gravitational field strength at the surface of the Earth is 6 times its value at the surface of the Moon. The mean density of the Moon is 0.6 times the mean
  35. June 2012, PHYA4 Section A (old spec), Q11 (1 mark): Which one of the following statements about gravitational fields is incorrect? A Moving a mass in the direction of the field lines reduces its potential energy.
  36. June 2012, PHYA4 Section A (old spec), Q12 (1 mark): An object on the surface of a planet of radius R and mass M has weight W. What would be the weight of the same object when on the surface of a planet of radius
  37. June 2012, PHYA4 Section A (old spec), Q13 (1 mark): The gravitational field strength on the surface of a planet orbiting a star is 8.0Nkg–1. If the planet and star have a similar density but the diameter of the s
  38. June 2012, PHYA4 Section B (old spec), Q4(c) (6 marks): The amount of energy required to move a manned spacecraft from the Earth to the Moon is much greater than that required to return it to the Earth. By reference
  39. January 2012, PHYA4 Section A (old spec), Q11 (1 mark): A spherical planet of uniform density ρ has radius R. Which line, A to D, in the table gives correct expressions for the mass of the planet and the gravitationa
  40. June 2011, PHYA4 Section A (old spec), Q8 (1 mark): The time period of a pendulum on Earth is 1.0s. What would be the period of a pendulum of the same length on a planet with half the density but twice the radius
  41. June 2011, PHYA4 Section A (old spec), Q11 (1 mark): A planet has a radius half the Earth’s radius and a mass a quarter of the Earth’s mass. What is the approximate gravitational field strength on the surface of t
  42. June 2011, PHYA4 Section A (old spec), Q12 (1 mark): At the surface of the Earth the gravitational field strength is g, and the gravitational potential is V. The radius of the Earth is R. An object, whose weight o
  43. January 2011, PHYA4 Section A (old spec), Q9 (1 mark): The diagram shows two point masses each of mass m separated by a distance 2r. What is the value of the gravitational field strength at the mid-point, P, between
  44. January 2011, PHYA4 Section A (old spec), Q11 (1 mark): What would the period of rotation of the Earth need to be if objects at the equator were to appear weightless? radius of Earth = 6.4 × 106 m A 4.5 × 10–2 hours
  45. June 2010, PHYA4 Section A (old spec), Q9 (1 mark): A projectile moves in a gravitational field. Which one of the following is a correct statement about the gravitational force acting on the projectile? A The for
  46. January 2010, PHYA4 Section A (old spec), Q11 (1 mark): The radius of a certain planet is x times the radius of the Earth and its surface gravitational field strength is y times that of the Earth. mass of the planet
  47. January 2010, PHYA4 Section B (old spec), Q3(b)(iii) (2 marks): Calculate the centripetal acceleration of a satellite in orbit B. answer = ms–2 (2 marks)
  48. June 2008, PA04A (2008 spec), Q9 (2 marks): 9 Which one of the following has different units to the other three? A gravitational potential gradient B gravitational Þ eld strength C force per unit mass D g
  49. June 2008, PA10 (2008 spec), Q4(a) (4 marks): 4 (a) (i) Light takes 43 minutes to travel from the Sun to Jupiter. Calculate the distance from the Sun to Jupiter. 4 (a) (ii) The mass of the Sun is 1040 times
  50. January 2008, PA04A (2008 spec), Q10 (2 marks): 10 The diagram shows two objects of equal mass m separated by a distance r. Which line, A to D, in the table gives the correct values of the gravitational field

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