OCR · A-Level · Physics

    Course version: H556 · Version from Sept 2015

    Cosmology: (e) Doppler effect; Doppler shift of electromagnetic radiation

    The Doppler effect is the change in observed frequency and wavelength when a source of waves moves relative to an observer.

    Checked against the OCR H556 specification (opens in a new tab) on .

    • Point 7 of 17
    • 3 key terms

    Study notes

    From the checked teaching notes for this specification point.

    The idea

    The Doppler effect is the change in observed frequency and wavelength when a source of waves moves relative to an observer. For electromagnetic radiation, a source moving away from the observer has its observed wavelength stretched, producing a red shift; a source moving towards the observer has its wavelength compressed, producing a blue shift. The size of the shift depends on the relative speed along the line of sight. In cosmology, nearly all distant galaxies show red shift, which is evidence that they are receding. You should be able to identify the direction of motion from the sign of the shift and distinguish red shift from blue shift in spectra.

    What earns the marks

    • Doppler effect is the change in observed frequency or wavelength due to relative motion between source and observer.
    • For electromagnetic radiation, motion away from the observer increases observed wavelength (red shift).
    • Motion towards the observer decreases observed wavelength (blue shift).
    • The shift depends on the component of relative velocity along the line of sight.
    • Red shift of galactic spectra is evidence for recession of galaxies.

    Common mistakes and how to put them right

    • Thinking red shift means the galaxy is actually red in colour.

      Put it right: Red shift refers to the position of spectral lines shifted towards longer wavelengths.

    • Confusing the direction of shift.

      Put it right: Away means red shift, towards means blue shift.

    • Assuming the Doppler shift depends on distance rather than relative velocity.

      Put it right: The shift depends on the relative speed along the line of sight.

    • Believing the Doppler effect only applies to sound.

      Put it right: It applies to all waves, including electromagnetic radiation.

    Exam tips

    • Read the question carefully to identify whether the source is moving towards or away from the observer.
    • Remember that red shift means longer wavelength and lower frequency; blue shift means shorter wavelength and higher frequency.
    • In multiple-choice questions, eliminate options that confuse red shift with blue shift or that link shift directly to distance.

    Try the lesson

    The start of the Cosmology: (e) Doppler effect; Doppler shift of electromagnetic radiation lesson, made from checked teaching notes for this specification point.

    Listen

    The Doppler effect is the change in observed frequency and wavelength when a source of waves moves relative to an observer. For electromagnetic radiation, a source moving away from the observer has its observed wavelength stretched, producing a red shift; a source moving towards the observer has its wavelength compressed, producing a blue shift. The size of the shift depends on the relative speed along the line of sight. In cosmology, nearly all distant galaxies show red shift, which is evidence that they are receding. You should be able to identify the direction of motion from the sign of the shift and distinguish red shift from blue shift in spectra. A strong answer earns marks for these points. Doppler effect is the change in observed frequency or wavelength due to relative motion between source and observer. For electromagnetic radiation, motion away from the observer increases observed wavelength (red shift). Motion towards the observer decreases observed wavelength (blue shift). The shift depends on the component of relative velocity along the line of sight. A common slip: Thinking red shift means the galaxy is actually red in colour. Instead, red shift refers to the position of spectral lines shifted towards longer wavelengths. Exam tip: Read the question carefully to identify whether the source is moving towards or away from the observer.

    See it

    A top-down flowchart. The first node states that the source moves relative to the observer, leading to a node defining the Doppler effect as a change in observed frequency and wavelength. This branches into two paths: motion away from the observer leads to wavelength being stretched (increased), which leads to red shift; motion towards the observer leads to wavelength being compressed (decreased), which leads to blue shift. A separate node from the Doppler effect states that the size of the shift depends on the relative speed along the line of sight. The red shift node leads to a final node stating that red shift of distant galaxies is evidence they are receding.
    It shows how relative motion of a source produces either a red shift (motion away) or a blue shift (motion towards), with the shift size depending on the speed along the line of sight.

    Key words

    Say what each word means before you turn the card.

    Doppler effect

    Try answering aloud or in your head before turning the card.

    Red shift

    Try answering aloud or in your head before turning the card.

    Blue shift

    Try answering aloud or in your head before turning the card.

    See every definition
    Doppler effect
    The change in observed frequency and wavelength when a source of waves moves relative to an observer.
    Red shift
    A source moving away from the observer has its observed wavelength stretched, producing a red shift.
    Blue shift
    A source moving towards the observer has its wavelength compressed, producing a blue shift.

    Label the diagram

    Some boxes have lost their names. Pick the right name for each number.

    The diagram again, with 3 boxes numbered instead of named. A top-down flowchart. The first node states that the source moves relative to the observer, leading to a node defining the Doppler effect as a change in observed frequency and wavelength. This branches into two paths: motion away from the observer leads to wavelength being stretched (increased), which leads to red shift; motion towards the observer leads to wavelength being compressed (decreased), which leads to blue shift. A separate node from the Doppler effect states that the size of the shift depends on the relative speed along the line of sight. The red shift node leads to a final node stating that red shift of distant galaxies is evidence they are receding.
    • 1Box 1

    • 2Box 2

    • 3Box 3

    0 of 3 labelled

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