NGC 120
Galaxy in the constellation Cetus
From Wikipedia, the free encyclopedia
NGC 120 is a lenticular galaxy of type SB0? with an apparent magnitude of 13.4 located in the constellation Cetus.[5] It was discovered on 27 September 1880 by Wilhelm Tempel.[5]
Right ascension00h 27m 30.09072s[1]
Declination−01° 30′ 48.4591″[1]
| NGC 120 | |
|---|---|
legacy surveys DR9 image of NGC 120 | |
| Observation data (J2000 epoch) | |
| Constellation | Cetus |
| Right ascension | 00h 27m 30.09072s[1] |
| Declination | −01° 30′ 48.4591″[1] |
| Redshift | 0.0136[2] |
| Heliocentric radial velocity | 4057 km/s[2] |
| Distance | 168.0 Mly (51.52 Mpc)[3] |
| Apparent magnitude (B) | 14.8[2] |
| Characteristics | |
| Type | SB00:[4] |
| Other designations | |
| UGC 267, MCG +00-02-033, PGC 1693[2] | |
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