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CAIE A-Level Physics 25.3.1 Shifted Spectral Lines

Practise identifying redshift by comparing observed and known spectral lines, then explaining how recession changes wavelength or frequency.

Syllabus
2028–2030
Course
Physics 9702
Level
A2

Exam points

  • identify redshift by comparing observed spectral-line positions with known emission or absorption lines
  • explain how recession changes observed wavelength or frequency

25.3.1—The lines in the emission and absorption spectra question 1

[Maximum number: 2]

The lines in Fig. 10.1 have been corrected for redshift.

Explain how cosmologists are able to determine that light from a distant star has undergone redshift.

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