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Doppler effect: AQA A‑Level Physics questions

AQA A-Level Physics past-paper questions on 3.9.3.1 Doppler effect, 2008–2025, with mark schemes and examiner’s reports where available.

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4,856 questions

  1. Q04.4

    June 2025 · Paper 3 Astrophysics

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  2. Q04.5

    June 2025 · Paper 3 Astrophysics

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  3. Q04.1

    June 2024 · Paper 3 Astrophysics

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  4. Q03.3

    June 2023 · Paper 3 Astrophysics

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  5. Q02.1

    June 2022 · Paper 3 Astrophysics

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  6. Q02.2

    June 2022 · Paper 3 Astrophysics

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  7. Q02.3

    June 2022 · Paper 3 Astrophysics

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  8. Q02.4

    June 2022 · Paper 3 Astrophysics

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  9. Q04.2

    November 2021 · Paper 3 Astrophysics

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  10. Q03.3

    November 2020 · Paper 3 Astrophysics

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  11. Q04.1

    June 2019 · Paper 3 Astrophysics

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  12. Q2(a)

    June 2015 · PHYA5 Astrophysics (old spec)

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  13. Q4(b)(i)

    June 2013 · PHYA5 Astrophysics (old spec)

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  14. Q4(a)

    June 2012 · PHYA5 Astrophysics (old spec)

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  15. Q3(a)(i)

    June 2011 · PHYA5 Astrophysics (old spec)

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  16. Q4(b)(i)

    June 2010 · PHYA5 Astrophysics (old spec)

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  17. Q5(b)

    June 2008 · PHA5W (2008 spec)

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All 17 questions on Doppler effect, as a list
  1. June 2025, Paper 3 Astrophysics, Q04.4 (3 marks): Explain the variation in apparent magnitude shown in Figure 2. In your answer you should explain: • the changes in observed brightness at P and Q, as shown in F
  2. June 2025, Paper 3 Astrophysics, Q04.5 (2 marks): Determine the angular velocity of the binary system. [2 marks] angular velocity = rad s−1
  3. June 2024, Paper 3 Astrophysics, Q04.1 (2 marks): The Andromeda Galaxy approaches the Milky Way at a speed of 110 km s−1. The distance between the galaxies is 770 kpc. Discuss whether these data can be used to
  4. June 2023, Paper 3 Astrophysics, Q03.3 (3 marks): A star is orbiting the black hole in M87. The star is observed in the plane of its orbit. The wavelength of a spectral line observed in the light emitted from t
  5. June 2022, Paper 3 Astrophysics, Q02.1 (2 marks): Explain the shape of the graph in Figure 1. [2 marks]
  6. June 2022, Paper 3 Astrophysics, Q02.2 (1 mark): State why the average of the values in Table 1 is different from the laboratory value. [1 mark]
  7. June 2022, Paper 3 Astrophysics, Q02.3 (3 marks): Show that the orbital speed of the primary star is about 250 km s−1. [3 marks]
  8. June 2022, Paper 3 Astrophysics, Q02.4 (2 marks): Calculate the orbital radius of the primary star. [2 marks] orbital radius = m
  9. November 2021, Paper 3 Astrophysics, Q04.2 (4 marks): IC2497 has a red shift of 0.0516 Determine the distance from the Earth to IC2497. Give an appropriate unit for your answer. [4 marks] distance = unit =
  10. November 2020, Paper 3 Astrophysics, Q03.3 (6 marks): Measurements of type 1a supernovae are used to find a value for the Hubble constant. The distance from Earth is known for many type 1a supernovae. Describe how
  11. June 2019, Paper 3 Astrophysics, Q04.1 (3 marks): Table 3 contains information about two galaxies. Table 3 Galaxy Red shift, z Distance from Earth / ly NGC 936 4.8 × 10–3 6.8 × 107 NGC 3379 3.0 × 10–3 3.2 × 107
  12. June 2015, PHYA5 Astrophysics (old spec), Q2(a) (6 marks): Describe the physical processes that give rise to the shape of each graph. Go on to show how the information in the graphs can be used to determine properties,
  13. June 2013, PHYA5 Astrophysics (old spec), Q4(b)(i) (3 marks): Use these data to calculate a value for the Hubble constant. value kms–1 Mpc–1 (3 marks)
  14. June 2012, PHYA5 Astrophysics (old spec), Q4(a) (4 marks): Cygnus A has a redshift, z, of 0.057. Calculate the distance to Cygnus A. State an appropriate unit. answer = unit = (4 marks)
  15. June 2011, PHYA5 Astrophysics (old spec), Q3(a)(i) (1 mark): Explain what is meant by red shift. (1 mark)
  16. June 2010, PHYA5 Astrophysics (old spec), Q4(b)(i) (1 mark): Calculate the value of the red shift, z, for this galaxy. z = (1 mark)
  17. June 2008, PHA5W (2008 spec), Q5(b) (4 marks): 5 (b) Analysis of radio waves from the galaxy IZW 1, suggest it is 800 million light years from Earth. 5 (b) (i) Calculate the recessional speed of the galaxy.

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