A blueshift is any decrease in wavelength (increase in frequency); 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 
Doppler blueshift is caused by movement of a source toward the observer. The term applies to any decrease in wavelength (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.
Doppler blueshift is used in astronomy to determine relative motion:
- The Andromeda Galaxy is moving toward our own Milky Way galaxy within the Local Group; thus, when observed from earth, its light is undergoing a blueshift.
- Components of a binary star system will be blueshifted when moving towards Earth
- When observing spiral galaxies, the side spinning toward us will have a slight blueshift relative to the side spinning away from us (see Tully–Fisher relation).
- Blazars are known to propel relativistic jets toward us, emitting synchrotron radiation and bremsstrahlung that appears blueshifted.
- Nearby stars such as Barnard's Star are moving toward us, resulting in a very small blueshift.
- Doppler blueshift of distant objects (high z) can be subtracted from the much larger cosmological redshift to determine relative motion in the expanding universe.
Gravitational blueshift 
An observer at a lower gravitational potential than a source ("downhill") will observe radiation to be blueshifted to shorter wavelengths. This 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.
Blue outliers 
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. These types of galaxies are called "blue outliers".
See also 
- Kuhn, Karl F.; Theo Koupelis (2004). In Quest of the Universe. Jones & Bartlett Publishers. pp. 122–3. ISBN 0-7637-0810-0.
- Aoki, Kentaro; Toshihiro Kawaguchi, and Kouji Ohta (2005-01). "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.
- Taylor, Edwin F.; Wheeler, John Archibald (2000). Exploring black holes: introduction to general relativity. Addison Wesley Longman. ISBN 978-0-201-38423-9.
- Bonometto, Silvio; Gorini, Vittorio; Moschella, Ugo (2002). Modern Cosmology. CRC Press. ISBN 978-0-7503-0810-6.