| NGC 37 | |
|---|---|
 | |
| Observation data (J2000epoch) | |
| Constellation | Phoenix |
| Right ascension | 00h 11m 22.93s |
| Declination | −56° 57′ 26.4″ |
| Redshift | 0.032606[1] |
| Heliocentric radial velocity | 9775 ± 45km/s[1] |
| Distance | 151.36Mpc[1] (493,68 millionly) Redshift-based |
| Apparent magnitude (V) | 14.66[1] |
| Characteristics | |
| Type | (RL)SAB00 |
| Apparent size (V) | 1.1′ × 0.7'[1] |
| Other designations | |
| PGC 801,ESO 149-22,2MASX J00112290-5657264, SGC 000855-5714.1,6dFGS gJ001122.9-565726, [CHM2007] LDC 7 J001122.90-5657264Gaia DR3 4919494715236325504 | |
NGC 37 is alenticular galaxy located in thePhoenix constellation. It is approximately 42kiloparsecs (137,000light-years) in diameter and about 12.9billion years old.[1]
It may have a companion galaxy calledPGC 95382.[2] Its redshift and radial velocity (z=0.03007 & V=8880 km/s) are really similar so it can be situated quite close to NGC 37.
NGC 37 is a member ofSCG2 0009-5713,[3] a compact galaxy group. Its other members arePGC 128413, a spiral galaxy,PGC 128414, a lenticular galaxy similar to NGC 37 and PGC 95382. The galaxy group's redshift is probably around 0.031000 because most of its members have a similar value.
Media related toNGC 37 at Wikimedia Commons.jpg) | Thislenticular galaxy article is astub. You can help Wikipedia byexpanding it. |
