JentooPhysics 2

AP® Physics 2: Algebra-Based · Unit 14 · Topic 14.5

The Doppler Effect

The Doppler effect is the shift in observed frequency caused by relative motion between a wave source and a listener: wavefronts bunch up ahead of an approaching source and spread out behind a receding one.

A source emits sound waves as expanding spheres of compression and rarefaction, each new wavefront starting from wherever the source currently is. If the source moves, it chases its own outgoing waves. Ahead of it, successive wavefronts get crowded together, so the wavelength shrinks and the listener there hears a higher frequency. Behind it, the source is pulling away from the waves it already sent, so they stretch out, giving a longer wavelength and a lower frequency. The source's own vibration frequency never changes; only the spacing of the waves in space changes.

Moving the listener instead of the source gives a similar shift but for a different reason: the listener's own motion changes how fast they sweep through wavefronts, without altering the wavelength in the air at all. A listener moving toward a stationary source meets each crest sooner than if they stood still, so they detect a higher rate of arrivals. The two cases are not identical in formula, since the wave medium (air) is the fixed reference, but at everyday speeds they produce very similar shifts.

The same idea applies to light. Galaxies moving away from us stretch their light to longer, redder wavelengths, called redshift. Because almost every distant galaxy shows redshift, and more distant ones show more of it, the universe must be expanding, with space itself carrying galaxies apart.

Key terms

Doppler effect
The change in observed frequency of a wave caused by relative motion between the source and the observer.
Wavefront
A surface connecting points of a wave that are in the same phase, such as a crest, as it expands from the source.
Redshift
A stretching of light to longer wavelengths, seen when the light source is moving away from the observer.
Relative velocity
The speed and direction of one object as measured from the reference frame of another, which is what determines the Doppler shift.

Watch it explained

  1. How it worksHow does a moving source bunch up the wavefronts ahead of it and stretch them out behind?
  2. How it worksCompare what happens when the source moves toward a still listener with when the listener moves instead.
  3. Common mistakeWhy isn't the pitch higher the whole time an ambulance is driving toward you and getting louder?
  4. Going furtherHow does redshift in the light from distant galaxies tell us the universe is expanding?

Check yourself

Your turn1 of 2
Find the frequency heard by a stationary listener as a 757 Hz source approaches at 68 m/s, with sound at 343 m/s.

End of topic.