| NGC 88 | |
|---|---|
NGC 88 (center) surrounded by the other galaxies in Robert's Quartet | |
| Observation data (J2000 epoch) | |
| Constellation | Phoenix |
| Right ascension | 00h 21m 21.8s |
| Declination | −48° 38′ 25″ |
| Redshift | 0.011408 |
| Distance | 160 Mly |
| Apparent magnitude (V) | 14.1 |
| Characteristics | |
| Type | SB(s)a pec |
| Apparent size (V) | 0.8′ × 0.5′ |
| Other designations | |
| PGC 1370, ESO 194-G010 | |
NGC 88 is an interacting peculiar spiral galaxy located approximately 160 million light-years (49 Mpc) away in the constellation Phoenix. It is a physical member of Robert's Quartet (HCG 92), a compact group of four interacting galaxies. The galaxy has an apparent visual magnitude of 14.1.
NGC 88 features a faint, diffuse outer envelope of gas and dust that has been tidally extended due to ongoing gravitational interactions with its neighboring group members, particularly NGC 87 and NGC 89. High-resolution imaging obtained by the Very Large Telescope demonstrates that these interactions have induced mild star-forming regions within its distorted spiral arms. The galaxy has an apparent angular size of 0′.8 × 0′.5 arcminutes, which at its light-travel distance of 160 million light-years translates to a physical diameter of approximately 35,000 light-years.
NGC 88 was discovered by English astronomer John Herschel on September 30, 1834, using an 18.7-inch reflecting telescope at the Cape of Good Hope.