AQA · A-Level · Physics
Course version: 7408 · Version from Sept 2016
Qualitative treatment of Big Bang theory including evidence from…
Full specification wording
Hubble's law (A-level only): Qualitative treatment of Big Bang theory including evidence from cosmological microwave background radiation, and relative abundance of hydrogen and helium.
The Big Bang model describes an expanding Universe from a hot, dense early state.
Checked against the AQA 7408 specification (opens in a new tab) on .
- Point 2 of 2
- 4 key terms
Study notes
From the checked teaching notes for this specification point.
The idea
The Big Bang model describes an expanding Universe from a hot, dense early state. Qualitatively, expansion explains cosmological redshift: as space stretches, photon wavelengths increase, so distant galaxies appear redshifted. The cosmological microwave background radiation (CMBR) is thermal radiation at about 2.7 K filling all space; it is relic radiation from when the early Universe became transparent, and its near-uniform temperature with tiny ripples supports an initially hot, dense phase. The observed relative abundance of hydrogen and helium, roughly three parts hydrogen to one part helium by mass, matches predictions from Big Bang nucleosynthesis in the first minutes, when protons and neutrons fused mainly into helium. Together, redshift, the CMBR and light-element abundances provide independent evidence for the model.
What earns the marks
- States that the Universe is expanding and that the early Universe was much hotter and denser than it is now.
- Explains cosmological redshift qualitatively as stretching of photon wavelengths by expansion of space, not as a Doppler shift through a stationary medium.
- Identifies the CMBR as microwave radiation at about 2.7 K coming from all directions and interprets it as relic thermal radiation from the early Universe.
- Links the near-uniform temperature and small ripples in the CMBR to an initially hot, dense state that later cooled and clumped to form galaxies.
- Explains that Big Bang nucleosynthesis in the first minutes produced mainly hydrogen and helium, giving the observed relative abundance of about three parts hydrogen to one part helium by mass.
- Uses at least two independent pieces of evidence to support the Big Bang model rather than relying on a single observation.
Common mistakes and how to put them right
Treating cosmological redshift as a simple Doppler shift through space.
Put it right by describing expansion of space stretching photon wavelengths.
Describing the CMBR as coming only from the centre of the Universe or from a single direction.
Put it right by stating it is isotropic, arriving from all directions.
Claiming that all helium was made in stars.
Put it right by explaining that the observed primordial abundance is too large for stellar production alone and matches Big Bang nucleosynthesis.
Stating that the CMBR is the same as the light from the first stars.
Put it right by identifying it as thermal radiation released when the early Universe became transparent, long before stars formed.
Exam tips
- When asked for evidence, name the observation, state what is measured and explain how it supports the Big Bang model in one linked chain.
- Use the phrase 'expansion of space' rather than 'galaxies moving through space' when explaining cosmological redshift.
- For the CMBR, quote the approximate temperature 2.7 K and mention its near-uniformity and small ripples.
- For hydrogen and helium abundance, give the approximate mass ratio three to one and link it to nucleosynthesis in the first minutes.
Try the lesson
The start of the Hubble's law (A-level only): Qualitative treatment of Big Bang theory including evidence from cosmological microwave background radiation, and relative abundance of hydrogen and helium. lesson, made from checked teaching notes for this specification point.
Have a go first
Which observation provides direct evidence that the early Universe was hot and dense?
Listen
The Big Bang model describes an expanding Universe from a hot, dense early state. Qualitatively, expansion explains cosmological redshift: as space stretches, photon wavelengths increase, so distant galaxies appear redshifted. The cosmological microwave background radiation (CMBR) is thermal radiation at about 2.7 K filling all space; it is relic radiation from when the early Universe became transparent, and its near-uniform temperature with tiny ripples supports an initially hot, dense phase. The observed relative abundance of hydrogen and helium, roughly three parts hydrogen to one part helium by mass, matches predictions from Big Bang nucleosynthesis in the first minutes, when protons and neutrons fused mainly into helium. Together, redshift, the CMBR and light-element abundances provide independent evidence for the model. A strong answer earns marks for these points. States that the Universe is expanding and that the early Universe was much hotter and denser than it is now. Explains cosmological redshift qualitatively as stretching of photon wavelengths by expansion of space, not as a Doppler shift through a stationary medium. Identifies the CMBR as microwave radiation at about 2.7 K coming from all directions and interprets it as relic thermal radiation from the early Universe. Links the near-uniform temperature and small ripples in the CMBR to an initially hot, dense state that later cooled and clumped to form galaxies. A common slip: Treating cosmological redshift as a simple Doppler shift through space. Instead, describing expansion of space stretching photon wavelengths. Exam tip: When asked for evidence, name the observation, state what is measured and explain how it supports the Big Bang model in one linked chain.
Key words
Say what each word means before you turn the card.
Cosmological redshift
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Cosmological microwave background radiation
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Big Bang nucleosynthesis
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Expansion of the Universe
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See every definition
- Cosmological redshift
- As space stretches, photon wavelengths increase, so distant galaxies appear redshifted.
- Cosmological microwave background radiation
- Thermal radiation at about 2.7 K filling all space, relic radiation from when the early Universe became transparent.
- Big Bang nucleosynthesis
- In the first minutes, protons and neutrons fused mainly into helium, giving the observed relative abundance of hydrogen and helium.
- Expansion of the Universe
- The Big Bang model describes an expanding Universe from a hot, dense early state.
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