| NGC 3455 | |
|---|---|
 NGC 3455 spiral galaxy taken byHubble Space Telescope. | |
| Observation data (J2000epoch) | |
| Constellation | Leo |
| Right ascension | 10h 54m 31.066s[1] |
| Declination | +17° 17′ 04.59″[1] |
| Redshift | 0.003730[1] |
| Heliocentric radial velocity | 1117[1] |
| Distance | 65 millionly |
| Apparent magnitude (B) | 13.1[1] |
| Characteristics | |
| Type | SABb[1] |
| Other designations | |
| MCG+03-28-031, Z 95-62, [M98c] 105151.6+173308, IRAS 10518+1733, PSCz Q10518+1733, Z 1051.9+1733, [T76] 25B, KPG 257b, QDOT B1051512+173306, [BEC2010] HRS 30,LEDA 32767, UGC 6028, [CHM2007] HDC 632 J105431.06+1717045,2MASX J10543106+1717045, UZC J105431.1+171704, [CHM2007] LDC 778 J105431.06+1717045 | |
NGC 3455 is anintermediate spiral galaxy located 65 million light-years away in the constellation ofLeo.[2] It is a member of theNGC 3370 Group of galaxies, which is a member of theLeo II Groups, a series of galaxies andgalaxy clusters strung out from the right edge of theVirgo Supercluster.[3]
Media related toNGC 3455 at Wikimedia Commons | Thisspiral galaxy article is astub. You can help Wikipedia byexpanding it. |
