This article needs more citations. (February 2017) |
| NGC 87 | |
|---|---|
NGC 87, a warped galaxy in Robert's Quartet | |
| Observation data (J2000 epoch) | |
| Constellation | Phoenix |
| Right ascension | 00h 21m 14.2133s |
| Declination | −48° 37′ 42.81″ |
| Redshift | 0.011391 |
| Heliocentric radial velocity | 3415 ± 23 km/s |
| Distance | 154.7 ± 11.0 Mly (47.44 ± 3.36 Mpc) |
| Apparent magnitude (V) | 14.1 |
| Characteristics | |
| Type | IBm pec |
| Size | ~51,500 ly (15.80 kpc) (estimated) |
| Apparent size (V) | 0.9′ × 0.7′ |
| Other designations | |
| ESO 194-G008, PGC 1357 | |
NGC 87 is a diffuse, irregular galaxy located approximately 155 million light-years away in the southern constellation of Phoenix. It was discovered on September 30, 1834, by the English astronomer John Herschel.
NGC 87 is classified morphologically as a diffuse irregular galaxy, displaying a lack of a distinct central nucleus or organized spiral structure. At its distance of 155 million light-years, its angular size corresponds to a physical diameter of roughly 42,000 light-years, making it about 40% the size of the Milky Way.
Unlike its spiral and lenticular companions, NGC 87 contains significant reservoirs of cold neutral hydrogen gas and active H II regions. Its asymmetric appearance and chaotic star-forming areas are driven by tidal interactions with nearby galactic companions.
The galaxy is a member of Robert's Quartet, a compact galaxy group located in Phoenix that also includes NGC 88, NGC 89, and NGC 90. The four member galaxies reside within a region spanning roughly 150,000 light-years across and exhibit active gravitational interactions.
One supernova has been observed in NGC 87: