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Single dish radio telescopes, I-R, U-V and X-ray telescopes: AQA A‑Level Physics questions

AQA A-Level Physics past-paper questions on 3.9.1.3 Single dish radio telescopes, I-R, U-V and X-ray telescopes, 2008–2025, with mark schemes and examiner’s reports where available.

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  3. Q01.3

    June 2019 · Paper 3 Astrophysics

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  6. Q2(c)

    June 2012 · PHYA5 Astrophysics (old spec)

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  7. Q3(a)

    June 2010 · PHYA5 Astrophysics (old spec)

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All 7 questions on Single dish radio telescopes, I-R, U-V and X-ray telescopes, as a list
  1. November 2021, Paper 3 Astrophysics, Q05.2 (3 marks): A telescope uses wavelengths in the range 90 nm to 120 nm. Explain why this telescope must be located in space. Go on to discuss one advantage that this telesco
  2. November 2021, Paper 3 Astrophysics, Q05.3 (3 marks): Table 1 shows information about two telescopes. Table 1 Telescope Diameter / m Dish shape Arecibo 305 spherical Lovell 76 parabolic Each telescope detects radio
  3. June 2019, Paper 3 Astrophysics, Q01.3 (6 marks): Table 1 contains information about two telescopes, A and B. Each telescope is planned to be the biggest of its type in the world. Table 1 Telescope A B Type Opt
  4. Specimen, Paper 3 Astrophysics, Q01.2 (6 marks): The concave mirrors used in some reflecting telescopes can suffer from spherical aberration. 0 1 The International Ultraviolet Explorer (IUE) and the Gran Teles
  5. June 2013, PHYA5 Astrophysics (old spec), Q2(c)(i) (2 marks): Calculate the minimum angular separation which could be resolved by a radio telescope of diameter 5000km detecting waves of frequency 230GHz. angular separation
  6. June 2012, PHYA5 Astrophysics (old spec), Q2(c) (6 marks): Different types of telescope are used to detect the various parts of the electromagnetic spectrum. Discuss with reference to three different parts of the electr
  7. June 2010, PHYA5 Astrophysics (old spec), Q3(a) (1 mark): Explain why X-ray telescopes need to be in orbit. (1 mark)

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