Doppler Shift

01Doppler Shift

Doppler effect of light

This section covers how relative motion between a light source and observer changes the observed frequency and wavelength.

Doppler effect: relative motion between a source and an observer changes the frequency and wavelength measured by the observer.

For a moving source, successive wavefronts are closer together in the direction of motion and further apart behind the source. An observer in front therefore measures a shorter wavelength and higher frequency, whereas an observer behind measures a longer wavelength and lower frequency.

For a light source moving at a speed much less than the speed of light, vcv\ll c:

Δff=vc\displaystyle \frac{\Delta f}{f}=\frac{v}{c}

Here ff is the reference frequency, Δf\Delta f is its measured change, vv is the relative velocity along the line joining source and observer, and cc is the speed of light.

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Reference and observed wavelength

If λ\lambda is the reference wavelength and λ\lambda' is the wavelength measured by the observer, the change is

Δλ=λλ\displaystyle \Delta\lambda=\lambda'-\lambda

If source and observer velocities are measured along the same line, their relative velocity can be written as

v=vsvo\displaystyle v=v_s-v_o

For observations made from Earth, the observer is usually treated as stationary, so vo=0v_o=0 and the relative velocity is the source velocity along the viewing direction.

Since wavelength and frequency are inversely related, increasing the observed wavelength decreases the observed frequency, while decreasing the wavelength increases the frequency.

Exam Tip: Before using the Doppler approximation, check that the source speed is much smaller than cc. Keep the signs of Δf\Delta f, Δλ\Delta\lambda and vv consistent with the direction convention used in the question.

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