Comoving and proper distances
In standard cosmology, comoving distance and proper distance are two closely related distance measures used by cosmologists to define distances between objects. Proper distance roughly corresponds to where a distant object would be at a specific moment of cosmological time, which can change over time due to the expansion of the universe. Comoving distance factors out the expansion of the universe, giving a distance that does not change in time due to the expansion of space (though this may change due to other, local factors, such as the motion of a galaxy within a cluster).
3C 1473C 2363C 2953C 3213C 353C 473C 483C 66A3C 793C 961 CygniA1689-zD1A1689B11APM 08279+5255Abell 1835 IR1916Angular diameter distanceBaryon acoustic oscillationsBig BangBullet ClusterChronology of the universeCo-moving distanceComoving coordinatesComoving distanceComoving observerComoving timeCosmic microwave backgroundCosmological horizonCosmological perturbation theoryCosmological proper distanceCosmos Redshift 7Dark energyDistance measures (cosmology)EGS-zs8-1Edwin HubbleEvent horizonExpansion of the universeFaster-than-lightFriedmann–Lemaître–Robertson–Walker metricGN-108036GN-z11
Link from a Wikipage to another Wikipage
primaryTopic
Comoving and proper distances
In standard cosmology, comoving distance and proper distance are two closely related distance measures used by cosmologists to define distances between objects. Proper distance roughly corresponds to where a distant object would be at a specific moment of cosmological time, which can change over time due to the expansion of the universe. Comoving distance factors out the expansion of the universe, giving a distance that does not change in time due to the expansion of space (though this may change due to other, local factors, such as the motion of a galaxy within a cluster).
has abstract
Em cosmologia padrão, estando ...... mpo, como o Modelo Lambda-CDM.
@pt
En cosmologia, la distància co ...... vidida per un factor d'escala.
@ca
In cosmologia la distanza como ...... ta l'espansione dell'universo.
@it
In standard cosmology, comovin ...... ing distance remains constant.
@en
Jarak comoving (disingkat menj ...... mentara Jarak co-moving tidak.
@in
La distance comobile est une c ...... suit l'expansion de l'univers.
@fr
Współrzędne współporuszające s ...... ędnych współporuszających się.
@pl
Сопутствующее расстояние и соб ...... и этом расширении не меняется.
@ru
يطلق مصطلح مسافة مسايرة أو مسا ...... س ذات أهمية كبرى في علم الكون.
@ar
在宇宙学中，共动距离和普通距离是两种很相关的距离测量方式，用 ...... 间普通距离随时间以宇宙標度因子变化，而共动距离一直保持不变。
@zh
Link from a Wikipage to an external page
Wikipage page ID
page length (characters) of wiki page
Wikipage revision ID
1,018,486,546
Link from a Wikipage to another Wikipage
wikiPageUsesTemplate
comment
Em cosmologia padrão, estando ...... nte usada a distância comóvel.
@pt
En cosmologia, la distància co ...... gueix l'expansió de l'univers.
@ca
In cosmologia la distanza como ...... ta l'espansione dell'universo.
@it
In standard cosmology, comovin ...... of a galaxy within a cluster).
@en
Jarak comoving (disingkat menj ...... meskipun alam semesta meluas.
@in
La distance comobile est une c ...... suit l'expansion de l'univers.
@fr
Współrzędne współporuszające s ...... czy pamiętać o czynniku skali.
@pl
Сопутствующее расстояние и соб ...... ремя. Таким образом, эти два р
@ru
يطلق مصطلح مسافة مسايرة أو مسا ...... س ذات أهمية كبرى في علم الكون.
@ar
在宇宙学中，共动距离和普通距离是两种很相关的距离测量方式，用 ...... 间普通距离随时间以宇宙標度因子变化，而共动距离一直保持不变。
@zh
label
Comoving and proper distances
@en
Coordinate comoventi
@it
Distance comobile
@fr
Distància comòbil
@ca
Distância comóvel
@pt
Jarak comoving
@in
Kunmova distanco
@eo
Współrzędne współporuszające się
@pl
Сопутствующее расстояние
@ru
مسافة مسايرة
@ar