NGC 4680

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NGC 4680
NGC4680 - HST - Potw2123a.jpg
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]

Contents

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]

See also

References

  1. 1 2 3 4 5 6 "NASA/IPAC Extragalactic Database". Results for NGC 4680. Retrieved 2024-03-26.
  2. information@eso.org. "A Spiral Amongst Friends". www.spacetelescope.org. Retrieved 2024-04-20.
  3. "NGC 4680 – Lenticular Galaxy in Corvus | TheSkyLive.com". theskylive.com. Retrieved 2024-04-20.
  4. "New General Catalog Objects: NGC 4650–4699". cseligman.com. Retrieved 2024-04-20.
  5. Marples, P.; Evans, R.; Phillips, M.; Schlegel, D. J.; Filippenko, A. V.; Leonard, D. C.; Wang, L.; Wheeler, J. C.; Garnavich, P.; Challis, P.; Kirshner, R.; Grogin, N. (1 April 1997). "Supernova 1997bp in NGC 4680". International Astronomical Union Circular. 6613: 1. ISSN   0081-0304.
  6. "SN 1997bp". Transient Name Server. IAU . Retrieved 6 December 2024.