Cosmological Red Shift (WJEC GCSE Physics)

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Katie M

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Katie M

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Cosmological Redshift

  • Usually, when an object emits waves, they spread out symmetrically
  • If the source of the waves moves, the waves can become squashed together or spread out
  • If a source of light moves towards an observer, the waves become squashed, causing the wavelength to decrease
    • The wavelength of light shifts towards the blue end of the spectrum
    • This is called blueshift
  • If a source of light moves away from an observer, the waves spread out, causing the wavelength to increase
    • The wavelength of light shifts towards the red end of the spectrum
    • This is called redshift

Redshift and Blueshift of Light

Light Doppler Shift, downloadable AS & A Level Physics revision notes

When light moves away from an observer, they observe redshift and when light moves towards an observer, they observe blueshift

  • When astronomers compare the absorption spectra of light from distant galaxies with spectra from nearby objects, such as the Sun, they observe the dark lines are shifted towards the red end of the spectrum
  • This means the wavelength has increased as the light travelled from the galaxy to the Earth
  • This shows that distant stars and galaxies are moving away from the Earth

Redshift of Light from a Distant Galaxy

2-6-comparing-absorption-spectra

Comparing the absorption spectra produced by the Sun and a distant galaxy shows the light from the distant galaxy has been shifted towards red wavelengths (it has stretched) due to it moving away

Examiner Tip

You need to know that in the visible light spectrum, red light has the longest wavelength and the smallest frequency.

Absorption spectra usually display wavelength as increasing from left to right, so the red end (longer wavelength) is usually on the right and the violet end (shorter wavelength) is usually on the left

The Expanding Universe

  • Cosmological redshift indicates that distant galaxies are moving away from us
  • If galaxies are moving away from us, this means the Universe must be expanding

Expansion of the Universe

2-6-redshift-and-universe-expansion

Observations of light from galaxies show they are moving away from us which means the Universe is expanding

  • When Edwin Hubble looked at the absorption spectra of distant galaxies, he determined a relationship between the speed of a galaxy and its distance from Earth

Comparing Redshifts of Galaxies

Redshift of Galaxies

Hubble discovered that all galaxies show redshift, but the galaxies that are further away show a greater increase in redshift

  • This is Hubble's law, which states

The speed of recession is proportional to the distance of the galaxy away from Earth

  • 'Recession' speed means the speed at which something is moving away
  • This means that the further away a galaxy is from Earth:
    • The faster it is moving away
    • The greater the increase in redshift

Relationship between Redshift and Galaxy Distance

2-6-hubble-law-graph

Hubble's law tells us the greater the distance to a galaxy, the greater the redshift, or the speed it moves away from Earth

Examiner Tip

Make sure that you understand that the stretching of the wavelength of light is due to the expansion of the Universe, not the motion of stars and galaxies themselves.

This can be visualised by imagining a balloon with equally spaced points on it. The balloon represents space and the points represent galaxies.

Big Bang Balloon Analogy, downloadable IGCSE & GCSE Physics revision notes

When the balloon is deflated (i.e. the Universe was smaller), the points (galaxies) are closer together and are at an equal distance apart.

As the balloon (Universe) expands, all the points (galaxies) become further apart by the same amount.

This is because the space between the galaxies itself has expanded.

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Katie M

Author: Katie M

Expertise: Physics

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.