| NGC 5579 | |
|---|---|
SDSS image of NGC 5579 | |
| Observation data (J2000 epoch) | |
| Constellation | Boötes |
| Right ascension | 14h 20m 26.484s |
| Declination | +35° 11′ 19.66″ |
| Redshift | 0.01199±0.00001 |
| Heliocentric radial velocity | 3,608 km/s |
| Distance | 179 ± 14 Mly (54.9 ± 4.3 Mpc) |
| Apparent magnitude (B) | 14.7 |
| Characteristics | |
| Type | SABcd |
| Apparent size (V) | 1.22′ × 0.93′ |
| Notable features | Singular, disturbed |
| Other designations | |
| GC 3852, IRAS 14183+3524, 2MASX J14202656+3511188, NGC 5579, Arp 69, UGC 9180, LEDA 51236, MCG +06-32-002, PGC 51236, CGCG 191.080, 192.003, VV 142a | |
NGC 5579 is an intermediate spiral galaxy in the northern constellation of Boötes. It was discovered on May 1, 1785) by German-British astronomer William Herschel. The galaxy is located at a distance of 179 ± 14 million light-years (54.9 ± 4.3 Mpc) from the Milky Way, and is receding with a heliocentric radial velocity of 3,608 km/s. It is entry 69 in Halton Arp's Atlas of Peculiar Galaxies.

On Dec. 17, 2006, a supernova designated SN 2006ss was discovered 22.7″ north and 11.9″ east of the galactic center. It was determined to be a type IIb supernova based on the spectrum.