| NGC 4477 | |
|---|---|
SDSS image of NGC 4477 | |
| Observation data (J2000 epoch) | |
| Constellation | Coma Berenices |
| Right ascension | 12h 30m 02.2s |
| Declination | 13° 38′ 12″ |
| Redshift | 0.004463 |
| Heliocentric radial velocity | 1,338 km/s |
| Distance | 54.8 Mly (16.8 Mpc) |
| Group or cluster | Virgo Cluster |
| Apparent magnitude (V) | 10.4 |
| Characteristics | |
| Type | SB0(s) |
| Size | ~69,340 ly (estimated) |
| Apparent size (V) | 3.7′ × 3.3′ |
| Other designations | |
| VCC 1253, IRAS 12275+1354, UGC 7638, MCG 2-32-97, PGC 41260, CGCG 70-129 | |
NGC 4477 is a barred lenticular galaxy in the constellation of Coma Berenices. It is classified as a type 2 Seyfert galaxy. This galaxy was discovered by German-British astronomer William Herschel on April 8, 1784. NGC 4477 is located about 55 million light-years away, where it is a member of Markarian's Chain in the Virgo Cluster of galaxies.
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.