Coordinates: Sky map 10h 48m 27.9204s, +12° 31′ 59.897″

NGC 3389

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NGC 3389
File:NGC3389 - SDSS DR14.jpg
NGC 3389 imaged by SDSS
Observation data (J2000 epoch)
ConstellationLeo
Right ascension10h 48m 27.9204s[1]
Declination+12° 31′ 59.897″[1]
Redshift0.004346±0.000007[1]
Heliocentric radial velocity1,303±2 km/s[1]
Distance71.70 ± 3.01 Mly (21.983 ± 0.924 Mpc)[1]
Group or clusterHOLM 212, NGC 3338 Group (LGG 214)
Apparent magnitude (V)12.3B[1]
Characteristics
TypeSA(s)c[1]
Size~81,000 ly (24.83 kpc) (estimated)[1]
Apparent size (V)2.8′ × 1.3′[1]
Other designations
HOLM 212C, NGC 3373, UGC 5914, MCG +02-28-013, PGC 32306, CGCG 066-022[1]

NGC 3389 is a spiral galaxy in the constellation of Leo. Its velocity with respect to the cosmic microwave background is 1,651±24 km/s, which corresponds to a Hubble distance of 79.4 ± 5.7 Mly (24.35 ± 1.74 Mpc).[1] However, 24 non-redshift measurements give a closer mean distance of 71.70 ± 3.01 Mly (21.983 ± 0.924 Mpc).[2] It was discovered by German-British astronomer William Herschel on 11 March 1784.[3] It was also observed by John Herschel on 23 March 1830, causing it to be listed a second time in the New General Catalogue as NGC 3373.[3]

Holm 212 and NGC 3338 groups

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NGC 3389, Messier 105, and NGC 3384 are listed together as Holm 212 in Erik Holmberg's A Study of Double and Multiple Galaxies Together with Inquiries into some General Metagalactic Problems, published in 1937.[4]

According to A. M. Garcia, NGC 3389 is a member of the NGC 3338 Group (also known as LGG 214). In addition to NGC 3338, this galaxy group includes at least three other galaxies: NGC 3346, UGC 5832, and MRK 1263.[5]

Supernovae

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Two supernovae have been observed in NGC 3389.

See also

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References

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  • Error creating thumbnail: File missing Media related to Lua error in Module:Commons_link at line 62: attempt to index field 'wikibase' (a nil value). at Wikimedia Commons
  • NGC 3389 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images