NGC 6920 is a Lenticular Galaxy in the Octans constellation. NGC 6920 is situated close to the southern celestial pole and, as such, it is easilty visible for most part of the year from the southern hemisphere.

2023年8月21日 · Historical Identification: Per Dreyer, NGC 6920 (= GC 4579 = JH 3829, 1860 RA 20 22 36, NPD 170 28.8) is "pretty bright, considerably small, round, pretty suddenly much brighter middle". Physical Information: Apparent size 1.8 by 1.5? arcmin

NGC 6920 (također poznat kao ESO 26-4 i PGC 65273) je spiralna galaksija koja je udaljena oko 119 miliona sg od Zemlje i nalazi se u sazviježđu Oktant. Najveći prečnik je 1,80 (63 hiljade sg) a najmanji 1,5 uglovnih minuta (52 hiljade sg). Prvo otkriće je napravio John Frederick William Herschel 21. jula 1835. godine. [2] [4] [5]

OBJECT #636 NGC 6920 Constellation Octans Right ascension 20h44m Declination –808000. Magnitude 12.4 Size 1.80by 1.5 Type Spiral galaxy. You’ll find our next target only 108 from the South Celestial Pole, 3.88 southwest of magnitude 3.7 Nu (n) Octantis. Although spiral, NGC 6920 doesn’t hint at spiral structure through amateur tele- scopes.

NGC 6920 . NGC 6920 is a lenticular galaxy located in the constellation Octans. Some key stats include:

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2022年1月15日 · NGC 6920 -- Interacting Galaxies The astronomical object called NGC 6920 is a Interacting Galaxies: Origin of the objects types : (Ref) Object type as listed in the reference "Ref" (acronym) Object type linked to the acronym according to the original reference Anterior to 2007, before we can link the objet type to a reference, or given by the ...

NGC 6920 (NGC6920) is a lenticular galaxy that has a distance from Earth of light years. It can be found in the constellation of Octans.

The distance from the Sun to NGC 6920: based on the amount of redshift (z) - 36.6 Mpc; Other names of the object NGC 6920 : PGC 65273, ESO 26-4, AM 2036-801 Nearby objects: NGC 6918 , NGC 6919 , NGC 6921 , NGC 6922

Redshift-Distance Survey of Early-Type Galaxies: Spectroscopic Data We present central velocity dispersions and Mg2 line indicesfor an all-sky sample of ~1178 elliptical and S0 galaxies, of which 984had no previous measures.