CCEA AS-Level Physics 1210
Physical Quantities, Scalars and Vectors
Moments and Equilibrium
Linear Motion and Dynamics
Newton's Laws of Motion
Linear Momentum and Impulse
Work, Energy and Power
Current, Charge and Potential Difference
Resistance and Resistivity
Internal Resistance and Potential Dividers
Waves
Refraction
Lenses
Superposition, Interference and Diffraction
Quantum Physics
Wave-Particle Duality
Astronomy
Practical Skills and Data Analysis
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.
- The classical Doppler effectRecall questions on what the Doppler effect is and the ambulance siren as the everyday case, the wavefront explanation for an approaching and a receding source, the wavelength and frequency equations, worked calculations both ways, whether the emitted frequency itself changes, the null result for transverse motion, and the derivation of Δλ/λ = v/c.Open →
- The red shift parameter zRed shift and blue shift.Open →
- Cosmological red shift and Doppler red shiftRecall questions on what causes each kind of shift and the essential difference between them, where in the light's journey the stretching happens, which applies to a distant galaxy and which to an orbiting star, why Andromeda is blue-shifted, the inflating balloon analogy, and why the Earth is not at the centre.Open →
- Hubble's lawHubble's law, defining each symbol with its unit and value of the Hubble constant with its unit.Open →
- The age of the universeRecall questions on the estimate t ≈ 1/H₀ and how it follows from Hubble's law, worked calculations in seconds and in years, the assumption of a constant expansion rate and why it is not exactly right, the effect of a larger Hubble constant, why the oldest stars must be younger than the estimate, and the observable limit a finite age imposes.Open →
What you need to know
Answer each one before you reveal it.
State the classical Doppler equation in terms of frequency for a moving source and a stationary observer.
A line measured at 486 nm in the laboratory appears at 492 nm in the spectrum of a galaxy. Calculate the red shift parameter.
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.
A source with a laboratory wavelength of 500 nm is observed with a red shift parameter of 0.010. Calculate the observed wavelength.
A galaxy has a red shift parameter of 0.030. Calculate its distance, taking the Hubble constant as 2.4 × 10⁻¹⁸ s⁻¹.
Why must the distance to a galaxy be found by a method independent of its red shift?
Why is the assumption behind the 1/H₀ estimate of the age of the universe not exactly correct?
How does the finite age of the universe limit how much of it can be observed?
How would evidence that the expansion of the universe is speeding up affect the estimate of its age?
What causes a Doppler red shift?
What causes a cosmological red shift?
Explain in terms of wavefronts why an approaching source produces a shorter wavelength.
At what point in the light's journey does the stretching that produces a cosmological red shift occur?
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
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
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
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
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
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
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.
What is inside Levo
Six ways to work the same material.
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.
Attempt a question from memory, write the correct version, then attempt it again. Levo records the jump between your first attempt and your last, and brings each question back on the day you are due to forget it.
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