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NGC 493

From Wikipedia, the free encyclopedia
Galaxy in the constellation Cetus
NGC 493
NGC 493
SDSS view of NGC 493
Observation data (J2000epoch)
ConstellationCetus
Right ascension01h 22m 09.54s
Declination+00° 56′ 47.5″
Redshift0.007799 ± 0.000017
Heliocentric radial velocity(+2329 ± 5) km/s
Distance90Mly
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 asPGC 4979 orGC 281, is abarred spiral galaxy in the constellationCetus.[1] It is located approximately 90 millionlight-years fromEarth and was discovered on December 20, 1786 by astronomerWilliam Herschel.[2] It was later also observed by his son,John Herschel.John Dreyer, creator of theNew General Catalogue, described the galaxy as "very faint, large, much extended 60°" with "a little brighter middle".[3]

Supernovae

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Threesupernovae 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. Retrieved2017-10-05.
  2. ^"Your NED Search Results".ned.ipac.caltech.edu. Retrieved2017-10-05.
  3. ^"astronomy-mall.com/Adventures.In.Deep.Space/NGC%201-7840%20complete.htm".Astronomy Mall.
  4. ^Marsden, Brian G. (22 November 1971)."Circular No. 2371".Central Bureau for Astronomical Telegrams. Smithsonian Astrophysical Observatory,IAU. Retrieved4 August 2025.
  5. ^"SN 1971S".Transient Name Server.IAU. Retrieved3 December 2024.
  6. ^"SN 2016hgm".Transient Name Server.IAU. Retrieved3 December 2024.
  7. ^"SN 2022ywf".Transient Name Server.IAU. Retrieved3 December 2024.

External links

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