NGC 4680 | |
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![]() NGC 4680 imaged by the Hubble Space Telescope | |
Observation data | |
Constellation | Virgo |
Right ascension | 12h 46m 54.7221s [1] |
Declination | −11° 38′ 12.899″ [1] |
Redshift | 0.008312 ± 0.000030 [1] |
Heliocentric radial velocity | (2492 ± 9) km/s |
Apparent magnitude (V) | 12,8 mag |
Apparent magnitude (B) | 13,7 mag |
Characteristics | |
Type | Pec [1] |
Size | ~50,700 ly (15.56 kpc) (estimated) [1] |
Apparent size (V) | 1.4′ × 1.2′ |
Other designations | |
IRAS 12443-1121, MCG -02-33-007, PGC 43118 [1] |
NGC 4680 is a spiral/lenticular galaxy in the constellation Virgo. [2] It is estimated to be 106 million light-years from the Milky Way and has a diameter of about 45,000 ly. [3] In the same area of the sky there are, among other things: the galaxies NGC 4700 and NGC 4708.[ citation needed ] NGC 4680 was discovered on May 27, 1835, by John Herschel using an 18-inch reflecting telescope, who described it as "eF, S, has one or two small stars entangled in it". [4]
One supernova has been observed in NGC 4680. SN 1997bp (type Ia, mag. 13.8) was discovered by Robert Evans on 6 April 1997. [5] [6]