NGC 3947 | |
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Observation data (J2000 epoch) | |
Constellation | Leo |
Right ascension | 11h 53m 20.3208s[1] |
Declination | +20° 45′ 06.184″[1] |
Redshift | 0.020698 [1] |
Heliocentric radial velocity | 6205 ± 2 km/s[1] |
Distance | 314.0 ± 22.0 Mly (96.28 ± 6.75 Mpc)[1] |
Group or cluster | NGC 3947 Group, Leo Cluster |
Apparent magnitude (V) | 13.2[1] |
Characteristics | |
Type | (R)SB(rs)b[1] |
Size | ~153,100 ly (46.93 kpc) (estimated)[1] |
Apparent size (V) | 1.4' x 1.2'[1] |
Other designations | |
IRAS 11507+2101, 2MASX J11532031+2045055, UGC 6863, MCG +04-28-088, PGC 37264, CGCG 127-095[1] |
NGC 3947 is a barred spiral galaxy in the constellation of Leo. Its velocity with respect to the cosmic microwave background is 6528 ± 23 km/s, which corresponds to a Hubble distance of 314.0 ± 22.0 Mly (96.28 ± 6.75 Mpc).[1] In addition, three non redshift measurements give a distance of 284.67 ± 12.90 Mly (87.28 ± 3.956 Mpc).[2] It was discovered by German-British astronomer William Herschel on 26 April 1785.[3]