Quantum redactiones paginae "Motus ad rubrum" differant

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'''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.
 
Aliqui motus ad robrum sunt exempla [[effectus Doppler|effectûs Doppler]], notiore in mutatione altitudinis vel frequentiae [[sonus (physica)|soni]] [[tramen|traminibus]], [[arcera|arceris]], aliisque vehiculis celeribus emissi.<!--A redshiftMotus occursad wheneverrubrum afit lightquandocumque sourcelumen movesab awayobservatore from an observerabit. AExemplum specialhuius instanceest ofmotus thisad is therubrum [[Cosmologiacosmologia|cosmologicalcosmologicus]] redshift, whichquae isex dueexpansione to the expansion of the universe,universi evenit.<!--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.''