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NGC 493

From Wikipedia, the free encyclopedia
(Redirected from UGC 914)
NGC 493
NGC 493
SDSS view of NGC 493
Observation data (J2000 epoch)
ConstellationCetus
Right ascension01h 22m 09.54s
Declination+00° 56 47.5
Redshift0.007799 ± 0.000017
Heliocentric radial velocity(+2329 ± 5) km/s
Distance90 Mly
Apparent magnitude (V)12.2
Characteristics
TypeSAB(s)cd?
Apparent size (V)4.3′ × 1.7′
Other designations
PGC 4979, GC 281, UGC 914, 2MASS J01220898+0056432, Z 385.84, MGC +00-04-099, IRAS 01195+0041, H 3.594, h 105

NGC 493, also occasionally referred to as PGC 4979 or GC 281, is a barred spiral galaxy in the constellation Cetus.[1] It is located approximately 90 million light-years from Earth and was discovered on December 20, 1786 by astronomer William Herschel.[2] It was later also observed by his son, John Herschel. John Dreyer, creator of the New General Catalogue, described the galaxy as "very faint, large, much extended 60°" with "a little brighter middle".[3]

Supernovae

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Three supernovae have been observed in NGC 493:

See also

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References

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  1. "Revised NGC Data for NGC 493". spider.seds.org. Retrieved 2017-10-05.
  2. "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2017-10-05.
  3. "astronomy-mall.com/Adventures.In.Deep.Space/NGC%201-7840%20complete.htm". Astronomy Mall.
  4. Rosino, L.; Pigatto (22 November 1971). Marsden, Brian G. (ed.). "SUPERNOVA IN NGC 493". Central Bureau for Astronomical Telegrams. 2371. Smithsonian Astrophysical Observatory, IAU: 1. Retrieved 4 August 2025.
  5. "SN 1971S". Transient Name Server. IAU. Retrieved 3 December 2024.
  6. "SN 2016hgm". Transient Name Server. IAU. Retrieved 3 December 2024.
  7. "SN 2022ywf". Transient Name Server. IAU. Retrieved 3 December 2024.
[edit]
  • Wikimedia Commons logo Media related to NGC 493 at Wikimedia Commons
  • NGC 493 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
  • SEDS