Astronomy:NGC 4477

From HandWiki
Short description: Galaxy in the constellation Coma Berenices
NGC 4477
SDSS NGC 4477.jpg
SDSS image of NGC 4477
Observation data (J2000 epoch)
ConstellationComa Berenices
Right ascension 12h 30m 02.2s[1]
Declination13° 38′ 12″[1]
Redshift0.004463/1338 km/s[1]
Distance54.8 Mly
Group or clusterVirgo Cluster
Apparent magnitude (V)11.38[1]
Characteristics
TypeSB0(s) [1]
Size~69,340 ly (estimated)[1]
Apparent size (V)3.8 x 3.5[1]
Other designations
CGCG 70-129, IRAS 12275+1354, MCG 2-32-97, PGC 41260, UGC 7638, VCC 1253[1]

NGC 4477 is a barred lenticular galaxy[2][3] located about 55 million light-years away[4] in the constellation of Coma Berenices.[5] NGC 4477 is classified as a type 2 Seyfert galaxy.[2] The galaxy was discovered by astronomer William Herschel on April 8, 1784.[6] NGC 4477 is a member of Markarian's Chain which forms part of the larger Virgo Cluster.[7]

Physical characteristics

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.[3]

See also

Gallery

References

External links