NGC 5938 is a Barred Spiral Galaxy in the Triangulum Australe constellation. NGC 5938 is situated south of the celestial equator and, as such, it is more easily visible from the southern hemisphere. Given its B magnitude of 11.9, NGC 5938 is visible with the help of a telescope having an aperture of 8 inches (200mm) or more.

NGC 5938 is an Elliptical Galaxy located in the constellation of Triangulum Australe in the southern hemisphere. NGC 5938's distance from Earth is 96,085,668.87 light years. NGC 5938 is called NGC 5938 in the New General Catalogue (NGC).

< NGC List NGC 5938. NGC 5938 is a barred spiral galaxy located in the constellation of Triangulum Australe. The NGC is a catalog of 7,840 nebulae, star clusters, and galaxies. Here are the key stats on NGC 5938:

2022年4月5日 · Historical Identification: Per Dreyer, NGC 5938 (= GC 4107 = JH 3605, 1860 RA 15 23 30, NPD 156 22.6) is "faint, small, among stars". Physical Information: Apparent size 2.8 by 2.5 arcmin

海因兹2-138是11视星等的行星状星云，比ngc 5979小。 NGC 5938位于南三角座ε以南五度，是非常遥远的 螺旋星系 ，距地球约有三亿光年。 ESO 69-6由两个逐渐合并的星系组成，距地球约六亿光年，合并过程还令星系拖出长长的尾巴。

2022年2月2日 · NGC 5938 -- Galaxy The astronomical object called NGC 5938 is a Galaxy: 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 CDS team in some particular ...

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New General Catalogue (NGC) [See all groups] Observation and Astrometry data. Constellation: Triangulum Australe: Right ascension: 15 h 36 m 25.80 s: Declination:-66°51'38.0" Aparent dimensions: 2.455′ × 1.66′ Catalogs and designations: Proper Names : …

2023年7月17日 · NGC 5938 is a very rarely imaged barred spiral galaxy 171 million light years away in the constellation Triangulum Australe. The galaxy has a bright central core region and relatively loose arms with star forming regions indicating possible past …

NGC 5938 galaxia bat da, Triangulum Australe konstelazioan [1]. John Herschelek aurkitu zuen 1836ko ekainaren 9an [2].