NGC 1011 是 鲸鱼座 的一個 星系。

NGC 1011 是 鯨魚座 的一個 星系。

NGC 1011 is a Spiral Galaxy in the Cetus constellation. NGC 1011 is situated close to the celestial equator and, as such, it is at least partly visible from both hemispheres in certain times of the year. Given its B magnitude of 15, NGC 1011 is visible with the help of a telescope having an aperture of 20 inches (500mm) or more.

Jan 20, 2020 · Historical Identification: Per Dreyer, NGC 1011 (= GC 5263, Stephan list VIII (#7), Swift list V (#31), 1860 RA 02 30 52, NPD 101 36.9) is "extremely faint, small, round, a little brighter middle" (described by Swift as 2nd of 3, the others being NGC 1010 (which is a duplicate of NGC 1006) and NGC 1017). The position precesses to RA 02 37 38.9 ...

NGC 1011 (također poznat kao MCG -2-7-45 i PGC 9955) je spiralna galaksija koja je udaljena oko 219 miliona sg od Zemlje i nalazi se u sazviježđu Kit. Najveći prečnik je 0,60 (38 hiljada sg) a najmanji 0,6 uglovnih minuta (38 hiljada sg).

< NGC List NGC 1011. NGC 1011 is a early spiral galaxy located in the constellation of Cetus. The NGC is a catalog of 7,840 nebulae, star clusters, and galaxies. Here are the key stats on NGC 1011:

IC 1011 is a barred spiral galaxy [1] with apparent magnitude of 14.7, [3] and with a redshift of z=0.02564 (SIMBAD) [1] or 0.025703 (NASA), [3] yielding a distance of 100 to 120 megaparsecs. [3] Its light takes 349.5 million years to reach Earth .

NGC 1011 est une galaxie lenticulaire (ou elliptique, mais certes pas spirale) située dans la constellation de la Baleine. Sa vitesse par rapport au fond diffus cosmologique est de 4 537 ± 23 km/s, ce qui correspond à une distance de Hubble de 66,9 ± 4,7 Mpc (∼218 millions d'al) [1].

NGC 1011 Galaxy in Cetus Dreyer's description: eF, S, R, lbM . Cross Identifications: GC 5263. Stephan VIII, Swift V.

NGC 1011 é uma galáxia espiral (Sa) localizada na direcção da constelação de Cetus. Possui uma declinação de -11° 00' 18" e uma ascensão recta de 2 horas, 37 minutos e 38,8 segundos. A galáxia NGC 1011 foi descoberta em 21 de Novembro de 1876 por Édouard Jean-Marie Stephan.