| NGC 575 | |
|---|---|
 SDSS image | |
| Observation data (J2000epoch) | |
| Constellation | Pisces |
| Right ascension | 01h 30m 46.6s[1] |
| Declination | +21° 26′ 26″[1] |
| Redshift | 0.010434 ± 0.000017 |
| Heliocentric radial velocity | 3128 ± 5 km/s |
| Distance | 145 ± 10 kly (44.4 ± 3.1 kpc)h−1 0.73 |
| Apparent magnitude (V) | 12.9 |
| Apparent magnitude (B) | 13.6 |
| Characteristics | |
| Type | SB(rs)c[1] |
| Apparent size (V) | 1.7 × 1.6arcseconds[2] |
| Other designations | |
| IC 1710,[1]MCG+03-04-051,[1]PGC 5634,[1]UGC 1081 | |
NGC 575 is abarred spiral galaxy ofHubble type SB(rs)c in the constellationPisces. It is approximately 145 million light years from theMilky Way and has a diameter of about 70,000light years.
The object was discovered on October 17, 1876, byÉdouard Stephan (listed as NGC 575) and on January 18, 1896, byStéphane Javelle (listed as IC 1710).[3]
Media related toNGC 575 at Wikimedia Commons | Thisspiral galaxy article is astub. You can help Wikipedia byexpanding it. |
