Definition
The Doppler shift is the change in frequency and wavelength of a propagating wave (acoustic, electromagnetic, etc.), caused by the movement of the source emitting the wave relative to the observer. This effect is named after the Austrian physicist Christian Doppler who proposed it in 1842. In France, the effect is currently called Doppler–Fizeau, because the French physicist Hippolyte Fizeau proposed it for electromagnetic waves in 1848. If the source is moving away from the observer, the wavelength appears stretched while frequencies are shifted toward lower values, and if the source is approaching, the wavelength appears compressed and frequencies shifted toward higher values. In the case of light, the effect is called redshift (receding source) and blueshift (approaching source), respectively. This effect is of great importance in astronomy because it allows direct determination of the radial speed of celestial objects and of the distance of remote galaxies (because of...
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Rouan, D. (2014). Doppler Shift. In: Amils, R., et al. Encyclopedia of Astrobiology. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-27833-4_455-2
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DOI: https://doi.org/10.1007/978-3-642-27833-4_455-2
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Publisher Name: Springer, Berlin, Heidelberg
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