| NGC 1164 | |
|---|---|
| NGC 1164 (Sloan Digital Sky Survey) | |
| Observation data (J2000.0 epoch) | |
| Constellation | Perseus [1] |
| Right ascension | 03h 01m 59.84s [2] |
| Declination | +42° 35′ 05.8″ [2] |
| Redshift | 0.013926 [2] |
| Heliocentric radial velocity | 4175±10 km/s [2] |
| Distance | 59 Mpc [2] |
| Apparent magnitude (V) | ~13 [3] |
| Apparent magnitude (B) | 14.4 [4] |
| Characteristics | |
| Type | (R')SAB(s)ab [2] |
| Apparent size (V) | 102.70" [2] |
| Other designations | |
| PGC 11441, MCG+07-07-016, UGC 2490 [4] | |
NGC 1164 is a barred spiral galaxy located in the constellation Perseus, approximately 60 million parsecs from Earth. It was discovered by the astronomer John Herschel in 1828. [3] NGC 1164 is classified as a (R')SAB(s)ab type spiral galaxy, with a prominent central bar structure and well-defined spiral arms. [2]
Two supernovae have been observed in NGC 1164: