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Orbits: Edexcel International A Level Physics questions

Edexcel International A Level Physics past-paper questions on 5.6.1.4 Orbits, 2019–2025, with mark schemes and examiner’s reports where available.

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2,865 questions

  1. Q13(b)

    June 2025 · Unit 5

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  2. Q14(a)

    January 2025 · Unit 5

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  3. Q18(a)

    October 2024 · Unit 5

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  5. Q18(a)

    June 2024 · Unit 5

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  6. Q18(b)(i)

    June 2024 · Unit 5

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  7. Q18(b)(ii)

    June 2024 · Unit 5

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  9. Q16(b)

    January 2024 · Unit 5

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  10. Q17(a)

    January 2024 · Unit 5

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  11. Q17(b)

    October 2023 · Unit 5

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  12. Q21(b)

    June 2023 · Unit 5

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  13. Q17(a)(ii)

    October 2022 · Unit 5

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  14. Q16(a)(i)

    June 2022 · Unit 5

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  15. Q16(a)(ii)

    June 2022 · Unit 5

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  16. Q16(a)(i)

    January 2022 · Unit 5

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  17. Q18(a)

    January 2022 · Unit 5

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  18. Q18(b)

    January 2022 · Unit 5

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  19. Q18(c)

    January 2022 · Unit 5

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  20. Q20(c)

    October 2021 · Unit 5

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All 25 questions on Orbits, as a list
  1. June 2025, Unit 5, Q13(b) (4 marks): The satellite is in orbit above the equator. Deduce whether the satellite would appear to be stationary above the surface of the Earth. period of rotation of Ea
  2. January 2025, Unit 5, Q14(a) (3 marks): Show that the mass of the Sun is about 2 × 10 30 kg. radius of Earth’s orbit about Sun = 1.49 × 10 11 m 1 year = 3.15 × 10 7 s (3)
  3. October 2024, Unit 5, Q18(a) (4 marks): Galileo made observations of the movement of these moons for 8 days. The largest moon is Ganymede. Deduce whether 8 days would have been enough time for Galileo
  4. June 2024, Unit 5, Q6 (1 mark): The dwarf planet Pluto orbits the Sun in an elliptical orbit. The gravitational force of the Sun on Pluto varies as Pluto orbits the Sun. Pluto moves away from
  5. June 2024, Unit 5, Q18(a) (3 marks): One law related the orbital time T of a planet to its average distance r from the Sun. Show that 2 r 3 4π T 2 GM where M is the solar mass. (3)
  6. June 2024, Unit 5, Q18(b)(i) (2 marks): A star in one of the outer arms of the galaxy is orbiting the centre of the galaxy. The star is 5.7 × 10 20 m from the centre of the galaxy. Show that the orbit
  7. June 2024, Unit 5, Q18(b)(ii) (4 marks): The orbital period of the star is actually 6.0 × 10 The two values for the orbital period of the star do not agree. Deduce what this tells us about our galaxy.
  8. January 2024, Unit 5, Q6 (1 mark): The planet Mercury orbits the Sun in an elliptical orbit. As a result, the speed of Mercury varies as it orbits the Sun. Which row of the table shows how the sp
  9. January 2024, Unit 5, Q16(b) (4 marks): Calculate the time, in years, that Pluto takes to make one complete orbit of the Sun. 7 s 1 year = 3.15 × 10 30 kg mass of Sun = 1.99 × 10 (4) Time for one orbi
  10. January 2024, Unit 5, Q17(a) (2 marks): Astronauts in orbit about the Earth are sometimes described as ‘weightless’, although they do experience a weight force. Explain why astronauts may be described
  11. October 2023, Unit 5, Q17(b) (6 marks): The average distance of Makemake from the Sun is similar to the average distance of the dwarf planet Pluto from the Sun. A website states: “The time taken by Ma
  12. June 2023, Unit 5, Q21(b) (3 marks): Scientists have observed an Earth-type planet in orbit around Ross-154. The radius of the orbit is 0.096 AU. Calculate the time for this planet to make one orbi
  13. October 2022, Unit 5, Q17(a)(ii) (4 marks): Determine the time T, in years, for Ceres to make one complete orbit about the Sun. 1 year = 3.15 × 107 s (4) T = years
  14. June 2022, Unit 5, Q16(a)(i) (3 marks): Show that T is related to r by the expression: T 2 µ r3 (3)
  15. June 2022, Unit 5, Q16(a)(ii) (5 marks): When planets align as they orbit the Sun they are said to be ‘in opposition’. The diagram shows the Earth and Jupiter in opposition. NOT TO SCALE Sun Earth Jupi
  16. January 2022, Unit 5, Q16(a)(i) (3 marks): The graph shows how astronomers expect v to vary with r. v r Explain how the expression gives the variation of v with r shown in the graph. (3)
  17. January 2022, Unit 5, Q18(a) (3 marks): The table shows data for Earth and Mars. Planet T / s R / m Earth 3.16 × 107 1.50 × 1011 Mars 5.93 × 107 2.28 × 1011 Show that, for Earth and for Mars, K has a
  18. January 2022, Unit 5, Q18(b) (3 marks): Kepler’s law of harmonies was derived later by Newton. Newton applied his law of gravitation to a planet moving in an approximately circular orbit around the Su
  19. January 2022, Unit 5, Q18(c) (2 marks): Jupiter is the most massive planet in the solar system and has many moons. Kepler’s law of harmonies applies to the orbiting moons. However, the value of K for
  20. October 2021, Unit 5, Q20(c) (3 marks): As the Sun continues its evolution, its mass will decrease. It is estimated that at its largest radius, the mass of the Sun will have decreased significantly. E
  21. October 2021, Unit 5, Q21(b) (5 marks): It is claimed that a satellite in orbit at a height of 8.50 × 105 m would make 15 orbits of the Earth every 24 hours. Assess the validity of this claim. (5)
  22. October 2021, Unit 5, Q21(c) (2 marks): It is suggested that the satellite could be placed in an equatorial orbit at a radius of 42 200 km. With this radius the satellite would have an orbital period
  23. June 2021, Unit 5, Q16(a) (3 marks): Calculate the orbital time of a Starlink satellite. (3) Orbital time of satellite =
  24. June 2021, Unit 5, Q16(b) (3 marks): Explain why satellites in low Earth orbits have a smaller orbital time than satellites in higher Earth orbits. (3)
  25. January 2021, Unit 5, Q17(a)(i) (4 marks): A textbook claims that for astronauts in Salyut 1, there would be a sunrise 16 times every day. Assess the validity of this claim. 1 day = 8.64 ´ 104 s (4)

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