| NGC 4477 | |
|---|---|
| SDSS image of NGC 4477 | |
| Observation data (J2000 epoch) | |
| Constellation | Coma Berenices [1] |
| Right ascension | 12h 30m 02.2s [2] |
| Declination | 13° 38′ 12″ [2] |
| Redshift | 0.004463 [2] |
| Heliocentric radial velocity | 1,338 km/s [1] |
| Distance | 54.8 Mly (16.8 Mpc) |
| Group or cluster | Virgo Cluster |
| Apparent magnitude (V) | 10.4 [1] |
| Characteristics | |
| Type | SB0(s) [2] |
| Size | ~69,340 ly (estimated) [2] |
| Apparent size (V) | 3.7′ × 3.3′ [1] |
| Other designations | |
| VCC 1253, IRAS 12275+1354, UGC 7638, MCG 2-32-97, PGC 41260, CGCG 70-129 [2] | |
NGC 4477 is a barred lenticular galaxy [3] [4] in the constellation of Coma Berenices. [5] It is classified as a type 2 Seyfert galaxy. [3] This galaxy was discovered by German-British astronomer William Herschel on April 8, 1784. [6] NGC 4477 is located about 55 million light-years away, [7] where it is a member of Markarian's Chain in the Virgo Cluster of galaxies. [8]
NGC 4477 has a very well-defined bar which is imbedded within an extensive lens-like envelope. It has a fairly sharp edge and is slightly enhanced near the rim, and is classified as a ring-like feature. Surrounding the ring, two broad, diffuse incomplete arcs appear to bracket the galaxy around the bar. It is suggested that NGC 4477 has a highly evolved double ring morphology. Also, both ring features are exceedingly washed out. [4]