NGC 493 explained

NGC 493
Upright:1.35
Epoch:J2000
Constellation Name:Cetus
Z:0.007799 ± 0.000017
H Radial V:(+2329 ± 5) km/s
Dist Ly:90 Mly
Type:SAB(s)cd?
Appmag V:12.2
Size V:4.3′ × 1.7′
Names: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]

Two supernovae have been observed in NGC 493: SN 1971S (mag. 15.5)[4] and SN 2016hgm (type II, mag. 17.9).[5]

See also

External links

Notes and References

  1. Web site: Revised NGC Data for NGC 493. spider.seds.org. 2017-10-05.
  2. Web site: Your NED Search Results. ned.ipac.caltech.edu. 2017-10-05.
  3. Web site: astronomy-mall.com/Adventures.In.Deep.Space/NGC%201-7840%20complete.htm. Astronomy Mall.
  4. https://www.wis-tns.org/object/1971S Transient Name Server entry for SN 1971S.
  5. https://www.wis-tns.org/object/2016hgm Transient Name Server entry for SN 2016hgm.