NGC 2 is an intermediate spiral galaxy with the morphological type of Sab, located in the constellation of Pegasus. NGC 2 was discovered by Lawrence Parsons, 4th Earl of Rosse on 20 August 1873.[2]
| NGC 2 | |
|---|---|
 NGC 2 by the DESI Legacy Surveys | |
| Observation data (J2000 epoch) | |
| Constellation | Pegasus |
| Right ascension | 00h 07m 17.1s[1] |
| Declination | +27° 40′ 42″[1] |
| Redshift | 0.025214[1] |
| Heliocentric radial velocity | 7559 km/s[1] |
| Galactocentric velocity | 7720 km/s[1] |
| Distance | 305 ± 10 Mly (93.738 ± 3.28 Mpc)[1] |
| Apparent magnitude (V) | +15.0[1] |
| Absolute magnitude (V) | -22.58[1] |
| Characteristics | |
| Type | Sab[1] |
| Size | ~106,700 ly (32.72 kpc) (estimated)[1] |
| Apparent size (V) | 1′.0 × 0′.6[1] |
| Notable features | - |
| Other designations | |
| GC 6246, MCG+04-01-026, UGC 59, PGC 567[1] | |
Observational History
editNGC 2 was first observed by Lawrence Parsons, 4th Earl of Rosse on 24 August 1873, and was described as "very faint, small, south of GC 1."[2]
Properties
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NGC 2 is located about 345 million light-years from the Solar System, with a magnitude of +14.2, while the distance to NGC 1 is 210 million light-years. Although visually close in the sky, NGC 1 and NGC 2 are at very different distances; were they stars, they would be referred to as an "optical double" as seen from Earth.[2]
AGC 102559, a spiral galaxy 60,000 light-years in diameter, is the closest galaxy to NGC 2, only 1.8 million light-years from it. Although it is quite close to NGC 1, the latter is closer and unrelated to NGC 2.
NGC 2 is a spiral galaxy with a diameter of about 60 thousand light-years, smaller than the size of the Milky Way.[3]
Listing in astronomical catalogues
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See also
editReferences
editExternal links
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Media related to NGC 2 at Wikimedia Commons- Source: NGC/IC Project
- NGC 2 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
