NGC 47 | |
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NGC 47 (2MASS) |
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Observation data (J2000 epoch) | |
Constellation | Cetus |
Right ascension | 00h 14m 30.6s[1] |
Declination | -07° 10′ 03″[1] |
Redshift | 0.019013[1] |
Helio radial velocity | 5700 ± 3 km/s[1] |
Distance | ~236 Mly (redshift) |
Type | SB(rs)bc[1] |
Apparent dimensions (V) | 2′.2 × 2′.1[1] |
Apparent magnitude (V) | 13.5[1] |
Notable features | none |
Other designations | |
NGC 58,[1] PGC 967,[1] MCG 1-1-55,[1] IRAS 00119-0726[1] | |
See also: Galaxy, List of galaxies |
NGC 47 (also known as NGC 58, MCG -1-1-55, IRAS00119-0726 and PGC 967) is a barred spiral galaxy in the constellation Cetus, discovered in 1886 by Ernst Wilhelm Leberecht Tempel. Its alternate name NGC 58 is due to the observation by Lewis Swift, who was unaware that Tempel had already discovered the object earlier. It appears as a small, faint spiral nebula with a bright core and is slightly oval.
It is approximately 236 million light years from Earth, measured by way of a generic "redshift estimate".[1]
Astronomical catalogs | ||
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NGC: | NGC 45 - NGC 46 - NGC 47 - NGC 48 - NGC 49 | |
NGC 56 - NGC 57 - NGC 58 - NGC 59 - NGC 60 | ||
PGC: | PGC 965 - PGC 966 - PGC 967 - PGC 968 - PGC 969 |