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This article is about the physical phenomenon. For the term as used in photochemistry, see hypsochromic shift. For other uses of "blueshift" or "blue shift", see Blueshift (disambiguation).
Doppler redshift and blueshift

A blueshift is any decrease in wavelength, with a corresponding increase in frequency, of electromagnetic waves; the opposite effect is referred to as redshift. In visible light, this shifts the color from the red end of the spectrum to the blue end. The term also applies when photons outside the visible spectrum (e.g., X rays and radio waves) are shifted toward shorter wavelengths, as well as to shifts in the de Broglie wavelength of particles. Blueshift is most commonly caused by relative motion toward the observer, described by the Doppler effect. An observer in a gravity well will also see infalling radiation gravitationally blueshifted, described by General Relativity in the same way as gravitational redshift. In a contracting universe, cosmological blueshift would be observed; the expanding universe gives a cosmological redshift, and the expansion is observed to be accelerating.

Doppler blueshift[edit]

Doppler blueshift is caused by movement of a source towards the observer. The term applies to any decrease in wavelength and increase in frequency caused by relative motion, even outside the visible spectrum. Only objects moving at near-relativistic speeds toward the observer are noticeably bluer to the naked eye, but the wavelength of any reflected or emitted photon or other particle is shortened in the direction of travel.[1]

Doppler blueshift is used in astronomy to determine relative motion:

Gravitational blueshift[edit]

Matter waves (protons, electrons, photons, etc.) falling into a gravity well become more energetic and undergo observer-independent blueshifting.

Unlike the apparent Doppler blueshift, caused by movement of a source towards the observer and thus dependent on the received angle of the photon, gravitational blueshift is real and does not depend on the received angle of the photon:

Photons climbing out of a gravitating object become less energetic. This loss of energy is known as a "redshifting", as photons in the visible spectrum would appear more red. Similarly, photons falling into a gravitational field become more energetic and exhibit a blueshifting. ... Note that the magnitude of the redshifting (blueshifting) effect is not a function of the emitted angle or the received angle of the photon—it depends only on how far radially the photon had to climb out of (fall into) the potential well.[3][4]

It is a natural consequence of conservation of energy and mass–energy equivalence, and was confirmed experimentally in 1959 with the Pound–Rebka experiment. Gravitational blueshift contributes to cosmic microwave background (CMB) anisotropy via the Sachs–Wolfe effect: when a gravitational well evolves while a photon is passing, the amount of blueshift on approach will differ from the amount of gravitational redshift as it leaves the region.[5]

Blue outliers[edit]

There are faraway active galaxies that show a blueshift in their [O III] emission lines. One of the largest blueshifts is found in the narrow-line quasar, PG 1543+489, which has a relative velocity of -1150 km/s.[2] These types of galaxies are called "blue outliers".[2]

See also[edit]


  1. ^ Kuhn, Karl F.; Theo Koupelis (2004). In Quest of the Universe. Jones & Bartlett Publishers. pp. 122–3. ISBN 0-7637-0810-0. 
  2. ^ a b c Aoki, Kentaro; Toshihiro Kawaguchi; Kouji Ohta (January 2005). "The Largest Blueshifts of the [O III] Emission Line in Two Narrow-Line Quasars". Astrophysical Journal 618 (2): 601–608. arXiv:astro-ph/0409546. Bibcode:2005ApJ...618..601A. doi:10.1086/426075. 
  3. ^ R.J. Nemiroff (1993). "Gravitational Principles and Mathematics". NASA. 
  4. ^ R.J. Nemiroff (1993). "Visual distortions near a neutron star and black hole". American Journal of Physics 61 (7): 619-632. arXiv:astro-ph/9312003v1. Bibcode:1993AmJPh..61..619N. doi:10.1119/1.17224. 
  5. ^ Bonometto, Silvio; Gorini, Vittorio; Moschella, Ugo (2002). Modern Cosmology. CRC Press. ISBN 978-0-7503-0810-6.