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Orbits and the Wider Universe

The Doppler shift of spectral lines and radial velocity

  • 3 things to know
  • Component 2

Overview

Recall questions on Δλ/λ = v/c, whether a line is shifted to the red or the blue for a receding or approaching source, worked speed calculations from a measured shift, why only the radial component is detected, and the periodic shift of a star in a binary.

What you need to know

Answer each one before you reveal it.

Your recallNot started
Key term

State the Doppler relationship used for light from a moving source, defining every symbol and its unit.

Numbers

A line emitted at 656.3 nm is observed at 656.45 nm. Calculate the star's radial velocity and state its direction.

Key term

What is observed in the spectrum of a star that is moving away from the Earth?

Questions from this subtopic

Each one with the model answer underneath.

  1. 1

    State the Doppler relationship used for light from a moving source, defining every symbol and its unit.

    Model answer

    The relationship is Δλ/λ = v/c, where Δλ is the change in wavelength in metres, λ is the emitted wavelength in metres, v is the radial velocity in m s⁻¹ and c is the speed of light, 3.00 × 10⁸ m s⁻¹.

  2. 2

    Under what condition is the Doppler relationship Δλ/λ = v/c valid?

    Model answer

    It is valid provided the source's speed is small compared with the speed of light.

  3. 3

    Define the radial velocity of a star.

    Model answer

    The radial velocity of a star is the component of its velocity along the line joining it to an observer on the Earth.

  4. 4

    What is observed in the spectrum of a star that is moving away from the Earth?

    Model answer

    Every spectral line is shifted to a longer wavelength, a red shift, by the same fractional amount.

  5. 5

    What is observed in the spectrum of a star that is moving towards the Earth?

    Model answer

    Every spectral line is shifted to a shorter wavelength, a blue shift, by the same fractional amount.

  6. 6

    How is the shift of a stellar spectral line identified, given that the star's true emitted wavelength cannot be measured directly?

    Model answer

    The pattern of lines is matched to the same element's pattern measured in a laboratory on Earth, and the shift of the whole pattern gives the change in wavelength.

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