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[[Fasciculus:Redshift.svg|thumb|Spectral lines in the [[Spectrum visuale|visible spectrum]] of a supercluster of distant galaxies (right), as compared to absorption lines in the visible spectrum of the [[Sol|Sun]] (left). Arrows indicate redshift. Wavelength increases up towards the red and beyond (frequency decreases).]]
'''Motus ad rubrum''' in [[physica]] est incrementum [[longitudo undae|longitudinis undae]], vel motus ad rubram [[spectrum|spectri]] extremitatem, [[lux|lucis]] vel aliae [[radiatio electromagnetica|radiationis electromagneticae]]. "Rubrior" significat auctam undae longitudinem, utrum radiatio intra [[spectrum visuale]] iacet an non. Secundum theorias [[lux|lucis]] radiatio rubrior etiam habet minorem [[frequentia]]m et energiam [[photon]]um.
'''Motus ad rubrum'''
<!--In [[Physica|physics]], '''redshift''' happens when light or other [[Radiatio electromagnetica|electromagnetic radiation]] from an object is increased in [[Longitudo undae|wavelength]], or shifted to the red end of the spectrum. In general, whether or not the radiation is within the [[Spectrum visuale|visible spectrum]], "redder" means an increase in wavelength – equivalent to a lower [[Frequentia|frequency]] and a lower [[photon]] energy, in accordance with, respectively, the [[Lux|wave]] and [[Lux|quantum]] theories of light.
 
<!--Some redshifts are an example of the [[Effectus Doppler|Doppler effect]], familiar in the change of apparent pitches of sirens and frequency of the [[Sonus (physica)|sound waves]] emitted by speeding vehicles. A redshift occurs whenever a light source moves away from an observer. A special instance of this is the [[Cosmologia|cosmological]] redshift, which is due to the expansion of the universe, and sufficiently distant light sources (generally more than a few million [[Annus luce mensus|light years]] away) show redshift corresponding to the rate of increase in their distance from Earth. Finally, gravitational redshift is a [[Relativitas generalis|relativistic]] effect observed in electromagnetic radiation moving out of gravitational fields. Conversely, a decrease in wavelength is called blueshift and is generally seen when a light-emitting object moves toward an observer or when electromagnetic radiation moves into a gravitational field. However, redshift is a more common term and sometimes blueshift is referred to as negative redshift.
 
Knowledge of redshifts and blueshifts has been applied to develop several terrestrial technologies such as Doppler radar and radar guns.<ref>See Feynman, Leighton and Sands (1989) or any introductory undergraduate (and many high school) [//en.wikipedia.org/wiki/Physics/Further_reading physics textbooks]. </ref> Redshifts are also seen in the spectroscopic observations of [[Astronomia|astronomical]] objects.<ref name="basicastronomy">See Binney and Merrifeld (1998), Carroll and Ostlie (1996), Kutner (2003) for applications in astronomy.</ref> Its value is represented by the letter ''z.''