OCR A-Level Physics A H556
Practical Skills in the Written Papers
The Practical Endorsement
Physical Quantities and Units
Making Measurements and Analysing Data
Nature of Quantities
Motion
Forces in Action
Work, Energy and Power
Materials
Newton’s Laws of Motion and Momentum
Charge and Current
Energy, Power and Resistance
Electrical Circuits
Waves
Quantum Physics
Thermal Physics
Oscillations
Gravitational Fields
Astrophysics and Cosmology
Capacitors
Electric Fields
Electromagnetism
Nuclear and Particle Physics
Astrophysics and Cosmology
Doppler shift and Hubble's law
- 3 things to know
- Papers 1, 2 and 3
Overview
Recall questions on the Doppler effect for electromagnetic radiation, recession velocity from redshift, Hubble's law and the Hubble constant, with calculations.
What you need to know
Answer each one before you reveal it.
What happens to the observed wavelength of electromagnetic radiation when the source moves away from the observer?
Calculate the recession velocity when change in wavelength = 19 nm, rest wavelength = 460 nm, speed of light = 3.00 × 10⁸ m s⁻¹.
Questions from this subtopic
Each one with the model answer underneath.
- 1
Define the Doppler effect.
Model answer
The Doppler effect is the change in observed frequency or wavelength of a wave when there is relative motion between the source and the observer.
- 2
What happens to the observed frequency of electromagnetic radiation when the source moves towards the observer?
Model answer
The observed frequency increases, causing a blueshift.
- 3
What happens to the observed wavelength of electromagnetic radiation when the source moves away from the observer?
Model answer
The observed wavelength increases, causing a redshift.
- 4
State the Doppler equation for electromagnetic radiation and define each term.
Model answer
Δf/f = Δλ/λ ≈ v/c, where Δf is the change in frequency, f is the original frequency, Δλ is the change in wavelength, λ is the original wavelength, v is the relative velocity of the source, and c is the speed of light.
- 5
How can the recession velocity of a galaxy be determined from observations?
Model answer
By measuring the redshift of the galaxy's spectral lines and applying the Doppler equation to calculate the recession velocity.
- 6
State Hubble's law and define each term in the equation.
Model answer
v ≈ H₀d, where v is the recession velocity of a galaxy, H₀ is the Hubble constant, and d is the distance to the galaxy.
Other ways to work this
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