NGC 4469 | |
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![]() NGC 4469 imaged by the Vera C. Rubin Observatory | |
Observation data (J2000 epoch) | |
Constellation | Virgo |
Right ascension | 12h 29m 28.0300s [1] |
Declination | +08° 45′ 00.622″ [1] |
Redshift | 0.001962±0.00000803 [1] |
Heliocentric radial velocity | 588±2 km/s [1] |
Distance | 54.63 ± 0.16 Mly (16.750 ± 0.050 Mpc) [1] |
Group or cluster | Virgo Cluster |
Apparent magnitude (V) | 12.0 [1] |
Characteristics | |
Type | SB(s)0/a, LINER [1] |
Size | ~68,000 ly (20.85 kpc) (estimated) [1] |
Apparent size (V) | 2.50′ × 1.04′ [1] |
Other designations | |
VCC 1190, IRAS 12269+0901, UGC 7622, MCG +02-32-089, PGC 41164, CGCG 070-121 [1] |
NGC 4469 is a nearly edge-on spiral galaxy [2] located about 55 million light-years away [3] in the constellation of Virgo. [4] It is also classified as a LINER galaxy. [3] NGC 4469 was discovered by German-British astronomer William Herschel on April 15, 1784. [5] It is a member of the Virgo Cluster. [6]
NGC 4469 has an X or peanut-shaped bulge, betraying the presence of a bar which generates such structures. [2] [7] NGC 4469 may also have an axisymmetric structure. [8]
NGC 4469 has dust lanes that cross the Earth's line of sight. [6]