| IC 755 | |
|---|---|
| | |
| Observation data (J2000 epoch) | |
| Constellation | Coma Berenices |
| Right ascension | 12h 01m 10.382s [2] |
| Declination | +14° 06′ 16.25″ [2] |
| Redshift | 0.00511 [3] |
| Heliocentric radial velocity | 1528 km/s [3] |
| Distance | 60.3 ± 4.9 Mly (18.5 ± 1.5 Mpc) [4] |
| Group or cluster | Virgo Cluster [5] |
| Apparent magnitude (B) | 13.9 [3] |
| Characteristics | |
| Type | SBb? edge-on [6] |
| Other designations | |
| NGC 4019, UGC 7001, MCG +02-31-014, PGC 37912 [3] | |
IC 755, also known as NGC 4019, [3] is a barred spiral galaxy. [6] It lies about 60 million light-years away (18 Megaparsecs) [4] in the northern constellation of Coma Berenices. It is a member of the Virgo Cluster. [5]
In 1999 a star within IC 755 was seen to explode as a supernova and named SN 1999an. [4] Supernovae like SN 1999an are classified as Type II [4] and they are dramatic events that mark the end of the lives of massive stars. The supernova was discovered by the Beijing Astronomical Observatory Supernova Survey.