| NGC 579 | |
|---|---|
NGC 579 imaged by SDSS | |
| Observation data (J2000 epoch) | |
| Constellation | Triangulum |
| Right ascension | 01h 31m 46.5375s |
| Declination | +33° 36′ 55.954″ |
| Redshift | 0.016655±0.0000130 |
| Heliocentric radial velocity | 4,993±4 km/s |
| Distance | 226.9 ± 15.9 Mly (69.57 ± 4.88 Mpc) |
| Group or cluster | NGC 507 Group (LGG 26) |
| Apparent magnitude (V) | 13.9 |
| Characteristics | |
| Type | Scd |
| Size | ~119,500 ly (36.65 kpc) (estimated) |
| Apparent size (V) | 1.1′ × 1.0′ |
| Other designations | |
| IRAS 01289+3321, 2MASX J01314651+3336560, UGC 1089, MCG +05-04-064, PGC 5691, CGCG 502-103 | |
NGC 579 is a spiral galaxy in the constellation of Triangulum. Its velocity with respect to the cosmic microwave background is 4,717±20 km/s, which corresponds to a Hubble distance of 226.9 ± 15.9 Mly (69.57 ± 4.88 Mpc). It was discovered by British astronomer John Herschel on 22 November 1827.
NGC 579 has a possible active galactic nucleus, i.e. it has a compact region at the center of a galaxy that emits a significant amount of energy across the electromagnetic spectrum, with characteristics indicating that this luminosity is not produced by the stars.
NGC 579 is a member of the NGC 507 group (also known as LGG 26). This large group contains 42 galaxies, of which 21 are in the NGC catalogue, and 5 are in the IC catalogue.
One supernova has been observed in NGC 579:
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