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Doppler effect, redshift and Hubble’s law: Edexcel International A Level Physics questions

Edexcel International A Level Physics past-paper questions on 5.6.4.1 Doppler effect, redshift and Hubble’s law, 2019–2025, with mark schemes and examiner’s reports where available.

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  2. Q18(b)

    January 2025 · Unit 5

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  3. Q17(a)(i)

    October 2024 · Unit 5

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  4. Q17(a)(ii)

    October 2024 · Unit 5

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  5. Q17(b)

    October 2024 · Unit 5

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  6. Q16(b)

    June 2024 · Unit 5

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  7. Q13

    January 2024 · Unit 5

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  8. The start of question 18

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  9. Q5

    October 2023 · Unit 5

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  10. Q14(a)

    October 2023 · Unit 5

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  11. Q14(b)

    October 2023 · Unit 5

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  12. Q21(b)

    October 2023 · Unit 5

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  13. Q2

    June 2023 · Unit 5

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  14. Q5

    June 2023 · Unit 5

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  15. Q5

    January 2023 · Unit 5

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  16. Q13

    January 2023 · Unit 5

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  17. Q6

    October 2022 · Unit 5

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  18. Q15(a)

    October 2022 · Unit 5

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  19. Q15(b)

    October 2022 · Unit 5

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  20. Q15(c)

    October 2022 · Unit 5

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All 35 questions on Doppler effect, redshift and Hubble’s law, as a list
  1. June 2025, Unit 5, Q5 (1 mark): On Earth, hydrogen is observed to emit a spectral line with a wavelength of 410 nm. The same spectral line is observed in the radiation received from a galaxy t
  2. January 2025, Unit 5, Q18(b) (5 marks): The Sun rotates on its axis. The diagram shows the Sun rotating at its ‘equator’. Sun equator of Sun (Source: © NASA / SDO / SCIENCE PHOTO LIBRARY) One of the d
  3. October 2024, Unit 5, Q17(a)(i) (2 marks): Explain why the spectrum of radiation received from Arcturus is shifted as shown. (2)
  4. October 2024, Unit 5, Q17(a)(ii) (3 marks): Determine the speed of Arcturus relative to the Sun. (3) Speed of Arcturus =
  5. October 2024, Unit 5, Q17(b) (3 marks): When light from galaxies is analysed, a shift towards greater wavelengths in the spectra of radiation is observed. Describe how astronomers use a knowledge of t
  6. June 2024, Unit 5, Q16(b) (3 marks): ε-Eridani is moving away from the Earth with a velocity of 1.55 × 10 A scientist observed the light received from ε-Eridani using a spectrometer. Deduce whether
  7. January 2024, Unit 5, Q13 (3 marks): A particular line in the spectrum of light from a source in the laboratory has a frequency of 6.173 × 10 14 Hz. The same line in the spectrum of light from a di
  8. January 2024, Unit 5, Q18(c) (4 marks): NGC 1357 is a spiral galaxy moving away from the Milky Way at a speed of 2.02 × 10 6 m s –1. The spiral galaxy is 8.70 × 10 23 m from the Earth. Calculate a val
  9. October 2023, Unit 5, Q5 (1 mark): A star is moving away from the Earth. The wavelengths of spectral lines in the light received from the star are measured. These wavelengths are not the same as
  10. October 2023, Unit 5, Q14(a) (1 mark): State how astronomers knew that galaxies were moving away from the Earth. (1)
  11. October 2023, Unit 5, Q14(b) (3 marks): Hubble suggested that the recessional velocity v of a galaxy was related to the distance d of the galaxy from the Earth by the expression v = H0 d where H0 is a
  12. October 2023, Unit 5, Q21(b) (6 marks): The final stage of evolution for a massive star may be a rotating neutron star. One neutron star rotates with a period of 33.5 ms. As this star rotates, one sid
  13. June 2023, Unit 5, Q2 (1 mark): A hydrogen source on Earth emits a spectral line with a wavelength of 410 nm. An observer determines the wavelength of the same line in the spectrum of a star.
  14. June 2023, Unit 5, Q5 (1 mark): Measurements related to a distant galaxy may be used to determine the value of the Hubble constant. Which two measurements related to a distant galaxy must be u
  15. January 2023, Unit 5, Q5 (1 mark): Absorption lines in the spectrum of light from a star are shifted to higher frequencies than the same lines viewed from a source on Earth. Which of the followin
  16. January 2023, Unit 5, Q13 (5 marks): The following statement appears on a website: Messier 87 (M87) is 55 million light‑years from Earth. The spectrum of light from M87 includes an absorption line
  17. October 2022, Unit 5, Q6 (1 mark): A graph of red shift against distance in metres was plotted for a range of nearby galaxies. The value of the gradient of the graph was 5.4 × 10–27 Which of the
  18. October 2022, Unit 5, Q15(a) (2 marks): Radiation with a wavelength of 134 nm was emitted from GN-z11. Calculate the wavelength λo of this radiation when it is detected at the HST. (2) λo =
  19. October 2022, Unit 5, Q15(b) (3 marks): The graph shows how z, for light emitted from a galaxy, varies with the distance the light has travelled in reaching the Earth. A light year (ly) is the distanc
  20. October 2022, Unit 5, Q15(c) (2 marks): The recently launched James Webb Space Telescope is designed to operate in the infrared region of the spectrum. Explain why this will be helpful for studying ve
  21. June 2022, Unit 5, Q3 (1 mark): Which of the following does not have the base unit s–1? A angular velocity B frequency C redshift D rate of decay
  22. June 2022, Unit 5, Q12(a)(i) (2 marks): Show that 72 km s–1 Mpc–1 is equivalent to a Hubble constant of about 2.3 × 10–18 s–1. 1 Mpc = 3.09 × 1022 m (2)
  23. June 2022, Unit 5, Q19(b) (4 marks): One line in the spectrum of light from Chi Lupi has a wavelength of 576.933 nm. The equivalent line in a mercury spectrum produced on Earth is 576.959 nm. A stu
  24. January 2022, Unit 5, Q6 (1 mark): Current theory suggests that the universe is expanding. Which of the following is evidence to support this theory? A All galaxies appear to be rotating in space
  25. January 2022, Unit 5, Q9 (1 mark): The spectrum of electromagnetic radiation from a galaxy is observed to have a redshift. Which of the following is a correct statement about lines in this spectr
  26. October 2021, Unit 5, Q16(a) (1 mark): Complete the table with the letters A, B and C to indicate the point corresponding to each wavelength. (1) λα / nm Point 656.2837 656.2797 656.2757
  27. October 2021, Unit 5, Q16(b) (2 marks): Explain why there is a variation in the wavelength of the light from different points on the Sun. (2)
  28. October 2021, Unit 5, Q16(c) (4 marks): In the laboratory, the wavelength of the alpha line in the hydrogen spectrum is 656.2797 nm. Assess whether this is consistent with the Sun having a period of r
  29. October 2021, Unit 5, Q17(b) (4 marks): Explain how a knowledge of the distances to distant galaxies has enabled astronomers to determine a value for the age of the universe. (4)
  30. June 2021, Unit 5, Q15(b) (5 marks): Radiation from the star is analysed. The radiation from the star has spectral lines at different wavelengths from the same spectral lines produced by a source i
  31. January 2021, Unit 5, Q16(a)(i) (2 marks): Explain what is meant by redshift. (2)
  32. January 2021, Unit 5, Q16(a)(ii) (3 marks): Calculate the distance of NGC 6052 from Earth. H0 = 1.62 ´ 10−18 s−1 (3) Distance of NGC 6052 from Earth =
  33. January 2021, Unit 5, Q20(b)(i) (4 marks): The graph shows part of the spectrum of radiation received from Andromeda. Relative intensity 390 395 400 Wavelength / nm (Source: © Nasa) The two intensity min
  34. October 2020, Unit 5, Q12(a) (3 marks): Explain how a massive planet orbiting a star can cause a change in the wavelength of light received from the star. (3)
  35. October 2020, Unit 5, Q12(b) (2 marks): The maximum shift in a spectral line of wavelength 4.35 × 10−7 m in the light received from Gliese 876 is 3.19 × 10−13 m. Calculate the maximum velocity of Glie

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