Galactic Redshift (AQA A Level Physics): Revision Note

Exam code: 7408

Katie M

Written by: Katie M

Reviewed by: Tim

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Understand this topic with deeper explanations and understanding checks.

Galactic redshift

  • When spectral lines from a distant galaxy are redshifted, this means:

The lines have shifted towards a longer wavelength, or towards the red end of the spectrum

  • This shift can be observed by comparing the spectra from the distant galaxy to a spectrum produced by a nearby object, such as our Sun, or a laboratory sample

The distant galaxy’s dark lines are shifted towards the red end, or longer wavelengths, compared with the matching lines in the Sun’s spectrum.
Comparing the light spectrum produced by the Sun with light from a distant galaxy

An expanding Universe

  • After the discovery of redshift, astronomers began to realise that almost all the galaxies in the Universe are receding

    • This led to the idea that the space between the Earth and the galaxies must be expanding

  • This expansion stretches out the light waves as they travel through space, shifting them towards the red end of the spectrum

Two stages of an inflating balloon. As the blue balloon expands, its white dots become farther apart, illustrating space stretching between galaxies while the galaxies themselves do not move.
As space expands, galaxies move apart like dots on an inflating balloon
  • The expansion of the Universe can be compared to dots on an inflating balloon

    • As the balloon is inflated, the dots all move away from each other

    • In the same way, as the rubber stretches when the balloon is inflated, space itself is stretching out between galaxies

    • Just like the dots, the galaxies move away from each other, however, they themselves do not move

  • Another observation from looking at the light spectra produced by distant galaxies is that the greater the distance to the galaxy, the greater the redshift

    • This means that the greater the degree of redshift, the faster the galaxy is moving away from Earth

Five visible-light spectra labelled laboratory reference, nearby star, nearby galaxy, distant galaxy and very distant galaxy. Wavelength runs from 400 to 700 nanometres. Dark absorption lines progressively shift right towards red.
The further a galaxy is from Earth, the greater its redshift tends to be
Graph of redshift against distance. Galaxy symbols follow an upward trend, showing redshift increasing with distance, and this is shown by a straight sloped line through the origin.
The furthest galaxies appear to be redshifted the most and are receding the fastest

Worked Example

The spectra below show dark absorption lines against a continuous visible spectrum.

Two visible-light spectra labelled “light from a source in the laboratory” and “light from a distant galaxy”. Matching dark absorption lines in the galaxy spectrum shift left, towards lower frequency.

A particular line in the spectrum of light from a source in the laboratory has a frequency of 4.570 × 1014 Hz.

The same line in the spectrum of light from a distant galaxy is observed to have a frequency of 4.547 × 1014 Hz.

Calculate the speed of the distant galaxy, and state whether it is moving towards or away from the Earth.

[3]

Answer:

Step 1: Write down the known quantities

  • Observed frequency, f' = 4.547 × 1014 Hz

  • Original frequency, f = 4.570 × 1014 Hz

  • Change in frequency, ∆f = 4.547 × 1014 − 4.570 × 1014 = −2.3 × 1012 Hz

  • Speed of light, c = 3.0 × 108 m s−1

Step 2: Write down the Doppler redshift equation

∆ff = vc

Step 3: Rearrange for speed v, and calculate

v = c∆ff

v = (3.0 × 108) × (−2.3 × 1012)4.570 × 1014 [1 mark]

v = −1.51 × 106 m s−1 (3 s.f.) [1 mark]

Step 4: Write a concluding sentence

  • The relative velocity is negative, so the source is moving away from the Earth [1 mark]

OR 

  • The observed frequency is less than the emitted frequency (the light from a laboratory source), therefore, the source is receding, or moving away, from the Earth at 1.5 × 106 m s–1 [1 mark]

Examiner Tips and Tricks

Keep track of the minus signs in your calculation, as this gives you information about whether the object is moving away or towards the observer.

The speed of light is given in your data booklet, you will not need to memorise this value.

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Katie M

Author: Katie M

Expertise: Curriculum Expert

Katie has always been passionate about the sciences, and completed a degree in Astrophysics at Sheffield University. She decided that she wanted to inspire other young people, so moved to Bristol to complete a PGCE in Secondary Science. She particularly loves creating fun and absorbing materials to help students achieve their exam potential.

Tim

Reviewer: Tim

Expertise: Content Creator

Timothy graduated with a first class degree in Mathematics and Physics from the University of Warwick. After working as a postgraduate researcher, Timothy has worked as a content creator for various online revision platforms, creating physics resources for a range of levels and exam boards.