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Lenticular galaxy in the constellation Pisces From Wikipedia, the free encyclopedia
NGC 473 is a lenticular galaxy in the constellation of Pisces.[2] Its velocity with respect to the cosmic microwave background is 1819 ± 22 km/s, which corresponds to a Hubble distance of 87.5 ± 6.2 Mly (26.82 ± 1.91 Mpc).[1] In addition, one non redshift measurement gives a distance of 97 Mly (29.8 Mpc).[3] It was discovered on December 20, 1786 by William Herschel.[2]
NGC 473 | |
---|---|
Observation data (J2000 epoch) | |
Constellation | Pisces |
Right ascension | 01h 19m 55.0731s[1] |
Declination | +16° 32′ 41.668″[1] |
Redshift | 0.007118[1] |
Heliocentric radial velocity | 2,134 km/s[1] |
Distance | 29.8 Mpc[1] |
Apparent magnitude (V) | 12.5[2] |
Characteristics | |
Type | SABo(r)a[2] |
Size | ~73,500 ly (22.54 kpc) (estimated)[1] |
Apparent size (V) | 1.9' x 1.2'[2] |
Other designations | |
IRAS 01172+1616, UGC 859, MCG +03-04-022, PGC 4785, CGCG 459-030 |
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