WJEC A-Level Physics 1420QS
Basic Physics
Kinematics
Dynamics
Energy Concepts
Solids Under Stress
Using Radiation to Investigate Stars
Particles and Nuclear Structure
Conduction of Electricity
Resistance
D.C. Circuits
The Nature of Waves
Wave Properties
Refraction of Light
Photons
Lasers
Circular Motion
Vibrations
Kinetic Theory
Thermal Physics
Nuclear Decay
Nuclear Energy
Capacitance
Electrostatic and Gravitational Fields of Force
Orbits and the Wider Universe
Magnetic Fields
Electromagnetic Induction
Option A: Alternating CurrentsOption A
Option B: Medical PhysicsOption B
Option C: The Physics of SportsOption C
Option D: Energy and the EnvironmentOption D
Mathematical Requirements (Appendix C)
Orbits and the Wider Universe
Radial velocity and the Doppler shift of spectral lines
- 3 things to know
- A2 Unit 4 Section A
Overview
Recall questions on Radial velocity and the Doppler shift of spectral lines.
What you need to know
Answer each one before you reveal it.
Give the Doppler relationship used for a star's radial velocity and define every symbol.
Which way is a spectral line shifted for a receding star?
Questions from this subtopic
Each one with the model answer underneath.
- 1
Define the radial velocity of a star.
Model answer
Radial velocity is the component of a star's velocity along the line joining it to an observer on the Earth.
- 2
Give the Doppler relationship used for a star's radial velocity and define every symbol.
Model answer
Δλ/λ = v/c, where Δλ is the shift in wavelength, λ the emitted wavelength, v the radial velocity and c the speed of light.
- 3
Which way is a spectral line shifted for a receding star?
Model answer
Towards longer wavelengths, so the line is red-shifted.
- 4
Which way is it shifted for an approaching star?
Model answer
Towards shorter wavelengths, so the line is blue-shifted.
- 5
How is the shift measured in practice?
Model answer
The wavelength of a known absorption line in the star's spectrum is compared with the wavelength of the same line measured in a laboratory source.
- 6
A line of laboratory wavelength 486.1 nm is observed at 486.4 nm. Calculate the radial velocity.
Model answer
Δλ/λ = 0.3 ÷ 486.1 = 6.17 × 10⁻⁴, so v = 6.17 × 10⁻⁴ × 3.00 × 10⁸, which is 1.85 × 10⁵ m s⁻¹ of recession.
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