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Parallax and standard candles: Edexcel International A Level Physics questions

Edexcel International A Level Physics past-paper questions on 5.6.3.1 Parallax and standard candles, 2019–2025, with mark schemes and examiner’s reports where available.

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2,865 questions

  1. Q14(a)

    June 2025 · Unit 5

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  2. Q14(b)(i)

    June 2025 · Unit 5

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  3. Q14(b)(ii)

    June 2025 · Unit 5

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  4. Q5

    January 2025 · Unit 5

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  5. Q16(a)

    January 2025 · Unit 5

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  6. Q16(b)(i)

    January 2025 · Unit 5

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  7. Q16(b)(ii)

    January 2025 · Unit 5

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  8. Q2

    June 2024 · Unit 5

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  9. Q2

    January 2024 · Unit 5

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  10. Q18(b)

    January 2024 · Unit 5

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  11. Q2

    October 2023 · Unit 5

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  12. Q3

    June 2023 · Unit 5

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  13. Q20(c)

    June 2023 · Unit 5

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  14. Q18(a)(i)

    January 2023 · Unit 5

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  15. Q18(a)(ii)

    January 2023 · Unit 5

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  16. Q18(b)(i)

    January 2023 · Unit 5

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  17. Q18(b)(ii)

    January 2023 · Unit 5

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  18. Q13

    October 2022 · Unit 5

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  20. Q18(a)(i)

    June 2022 · Unit 5

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All 27 questions on Parallax and standard candles, as a list
  1. June 2025, Unit 5, Q14(a) (2 marks): Explain why trigonometric parallax can only be used to determine the distance to objects that are relatively close to the Earth. (2)
  2. June 2025, Unit 5, Q14(b)(i) (1 mark): State what is meant by a standard candle. (1)
  3. June 2025, Unit 5, Q14(b)(ii) (3 marks): Describe how the method of standard candles is used to determine the distance to a distant star cluster. (3)
  4. January 2025, Unit 5, Q5 (1 mark): Astronomers use trigonometric parallax to determine the distances to stars. Which of the following must the astronomers know? A The distance between the Sun and
  5. January 2025, Unit 5, Q16(a) (1 mark): State what is meant by a standard candle. (1)
  6. January 2025, Unit 5, Q16(b)(i) (4 marks): The variation in luminosity L of this Cepheid variable star with time t is shown below. L 0 2 4 6 8 10 12 14 16 18 20 t / days 29 W. Show that the mean luminosi
  7. January 2025, Unit 5, Q16(b)(ii) (2 marks): When viewed from Earth, the mean intensity of this Cepheid variable star is –4 W m –2. 5.1 × 10 Determine the distance of this Cepheid variable star from Earth.
  8. June 2024, Unit 5, Q2 (1 mark): Which of the following can be used to determine the distance to a nearby star? A Doppler shift B Hertzsprung–Russell diagram C Hubble’s law D Trigonometric para
  9. January 2024, Unit 5, Q2 (1 mark): Astronomers can use stellar parallax to determine the distances to stars. Which of the following statements is correct? A Measurements are made against more dis
  10. January 2024, Unit 5, Q18(b) (4 marks): Kruger B can be used as a standard candle. Describe how standard candles can be used to determine the distance to galaxies. (4)
  11. October 2023, Unit 5, Q2 (1 mark): Astronomers use stellar parallax to determine the distances to nearby stars. Which of the following must be known to use stellar parallax? A distance between th
  12. June 2023, Unit 5, Q3 (1 mark): The distances to stars can be determined using trigonometric parallax. Star X has twice the parallax angle of Star Y. Which of the following statements is corre
  13. June 2023, Unit 5, Q20(c) (4 marks): In the early 20th century, Edwin Hubble observed the Andromeda Nebula. He saw stars similar to the stars in our galaxy. One star he saw was a standard candle kn
  14. January 2023, Unit 5, Q18(a)(i) (4 marks): Describe how stellar parallax is used by astronomers. (4)
  15. January 2023, Unit 5, Q18(a)(ii) (1 mark): Tycho Brahe concluded that the Earth was motionless at the centre of the universe, as he was not able to detect any stellar parallax. Suggest why he was not abl
  16. January 2023, Unit 5, Q18(b)(i) (1 mark): State what is meant by a standard candle. (1)
  17. January 2023, Unit 5, Q18(b)(ii) (3 marks): Describe how standard candles can be used to determine the distance to nearby galaxies. (3)
  18. October 2022, Unit 5, Q13 (6 marks): *13 The average distance between galaxies is many times greater than the size of our galaxy. Astronomers use standard candles to determine the distances to othe
  19. June 2022, Unit 5, Q11 (3 marks): A standard candle in the galaxy M81 has a luminosity 14 800 times the luminosity of the Sun. The intensity of radiation received from the standard candle, measu
  20. June 2022, Unit 5, Q18(a)(i) (2 marks): The parallax angle was 2.01 × 10–6 rad. Calculate the distance, in metres, of Wolf 359 from Earth. mean distance from Earth to Sun = 1.50 × 1011 m (2) Distance
  21. June 2022, Unit 5, Q18(a)(ii) (2 marks): Explain why parallax measurements can only be used to determine the distances to a relatively small number of stars. (2)
  22. January 2022, Unit 5, Q19(a) (3 marks): Using parallax measurements, astronomers can determine distances to all stars with a parallax angle larger than 2.4 × 10–7 rad. The variable star Alpha Cephei i
  23. January 2022, Unit 5, Q19(b) (3 marks): Cepheids are a type of standard candle. Describe how standard candles can be used to determine distances to stars. (3)
  24. October 2021, Unit 5, Q1 (1 mark): Which of the following describes a standard candle? A a star of known distance B a star of known intensity C a star of known luminosity D a star of known mass
  25. October 2021, Unit 5, Q17(a) (3 marks): Describe how trigonometric parallax can be used to determine the distance to a nearby star. (3)
  26. June 2021, Unit 5, Q12(a) (1 mark): State what is meant by a standard candle. (1)
  27. January 2021, Unit 5, Q20(b)(ii) (3 marks): Dust in space around a star may affect how bright the star appears to be. It is claimed that dust around a standard candle would lead to the conclusion that the

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