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Astronomy

  • 5 subtopics
  • 15 things to know
  • Unit AS 2

What Astronomy covers

Astronomy is examined in Unit AS 2, Waves, Photons and Astronomy, and drawn on again in Unit AS 3, Practical Techniques and Data Analysis. It covers the classical Doppler effect, the red shift parameter z, cosmological red shift and Doppler red shift, Hubble's law and the age of the universe.

Where it is assessed

Unit AS 2

Waves, Photons and Astronomy, and again in Unit AS 3, Practical Techniques and Data Analysis.

Check the CCEA specification ↗

The 5 subtopics

Each one has its own page. CCEA AS Physics students sit this topic in the first year.

What you need to know

Answer each one before you reveal it.

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Key term

State the classical equation for the wavelength received by a stationary observer from an approaching source.

Key term

State the classical Doppler equation in terms of frequency for a moving source and a stationary observer.

Numbers

A line measured at 486 nm in the laboratory appears at 492 nm in the spectrum of a galaxy. Calculate the red shift parameter.

Numbers

A line of laboratory wavelength 656 nm is observed at 670 nm in a galaxy's spectrum. Calculate the red shift parameter and the recession speed.

Numbers

A source with a laboratory wavelength of 500 nm is observed with a red shift parameter of 0.010. Calculate the observed wavelength.

Numbers

A galaxy has a red shift parameter of 0.030. Calculate its distance, taking the Hubble constant as 2.4 × 10⁻¹⁸ s⁻¹.

Key term

Why must the distance to a galaxy be found by a method independent of its red shift?

Key term

Why is the assumption behind the 1/H₀ estimate of the age of the universe not exactly correct?

Key term

How does the finite age of the universe limit how much of it can be observed?

Key term

How would evidence that the expansion of the universe is speeding up affect the estimate of its age?

Key term

What causes a Doppler red shift?

Key term

What causes a cosmological red shift?

Key term

Explain in terms of wavefronts why an approaching source produces a shorter wavelength.

Key term

At what point in the light's journey does the stretching that produces a cosmological red shift occur?

Key term

State Hubble's law, defining each symbol with its unit.

Take Astronomy further

The same content, four other ways.

Commonly confused

Pairs that lose marks when they are blurred together.

  • Red shift vs Blue shift

    Red shift: the received wavelengths are longer than the laboratory values and the separation is increasing. Blue shift: they are shorter and the separation is decreasing.

Questions from this topic

Each one with the model answer underneath.

  1. 1

    What is the Doppler effect?

    Model answer

    The Doppler effect is the change in the observed frequency and wavelength of a wave that occurs when the source and the observer are moving relative to one another.

  2. 2

    Describe what is heard as an ambulance siren approaches, passes and drives away.

    Model answer

    The note is heard at a higher pitch than normal while the ambulance approaches, drops suddenly as it passes, and is heard at a lower pitch than normal as it recedes.

  3. 3

    Explain in terms of wavefronts why an approaching source produces a shorter wavelength.

    Model answer

    The source moves forward between emitting one wavefront and the next, so each new wavefront starts from a point closer to the observer and the wavefronts ahead of the source are bunched together.

  4. 4

    Explain in terms of wavefronts why a receding source produces a longer wavelength.

    Model answer

    The source moves away between emitting successive wavefronts, so each new wavefront starts further from the observer and the wavefronts behind the source are stretched apart.

  5. 5

    State the classical equation for the wavelength received by a stationary observer from a receding source, defining each symbol.

    Model answer

    λ' = λ(c + v)/c, where λ' is the received wavelength in metres, λ is the wavelength emitted by the source at rest in metres, v is the speed of the source in m s⁻¹ and c is the speed of the wave in the medium in m s⁻¹.

  6. 6

    State the classical equation for the wavelength received by a stationary observer from an approaching source.

    Model answer

    λ' = λ(c − v)/c, where λ' is the received wavelength, λ is the wavelength emitted by the source at rest, v is the speed of the approaching source and c is the wave speed, all in SI units.

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Astronomy revision questions

Is Astronomy examined at AS in CCEA Physics?
Yes. It sits in Unit AS 2, which you take in the first year, so it is on the AS paper as well as counting towards the full A level.
What does Astronomy cover in CCEA AS-Level Physics?
5 subtopics: the classical doppler effect, the red shift parameter z, cosmological red shift and doppler red shift, hubble's law and the age of the universe. Each one has its own page with questions and model answers.
How is Astronomy organised?
By the CCEA 1210 specification, subtopic by subtopic, so it matches the order you are taught it in.

Every question in Astronomy, on a schedule.

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