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Spiral galaxy in the constellation Cetus From Wikipedia, the free encyclopedia
NGC 345 is a spiral galaxy located in the constellation Cetus. It was discovered on September 27, 1864 by Albert Marth. It was described by Dreyer as "very faint, very small, gradually brighter middle."[2]
| NGC 345 | |
|---|---|
SDSS image of NGC 345 | |
| Observation data (J2000 epoch) | |
| Constellation | Cetus |
| Right ascension | 01h 01m 22.1s[1] |
| Declination | −06° 53′ 03″[1] |
| Redshift | 0.017592[1] |
| Heliocentric radial velocity | 5,274 km/s[1] |
| Apparent magnitude (V) | 14.86[1] |
| Characteristics | |
| Type | SA(s)a[1] |
| Apparent size (V) | 1.2' × 0.8'[1] |
| Other designations | |
| MCG -01-03-064, 2MASX J01012211-0653034, 2MASXi J0101221-065303, 6dF J0101221-065303, PGC 3665.[1] | |
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