NGC 2491 explained

NGC 2491
Constellation Name:Canis Minor
Z:0.039290
H Radial V:18,476 km/s
Dist Ly:583 Mly (178.74 Mpc)
Sbrightness:11.75
Ra:07h 58m 27.37s
Appmag V:14.8
Size:130,000 ly
Type:S
Dec:+07d 59m 01.74s
Names:PGC 22353, 2MASX J07582739+0759018, SDSS J075827.37+075901.7, CGCG 031-007, 2MASS J07582738+0759019, NPM1G+08.0123, LEDA 22353
Epoch:J2000
Appmag B:15.6
Size V:0.3' x 0.2'

NGC 2491 is a spiral galaxy located in Canis Minor constellation.[1] It is located 580 million light-years from Earth and has an approximate diameter of 130,000 light-years.[2]

Details

NGC 2491 was discovered by American astronomer Lewis Swift on November 15, 1885.[3] Swift described it as extremely faint, small, with a round irregular shape, and a bright star to the west. With a surface brightness of magnitude of 11.75, NGC 2491 is classified as a high surface brightness galaxy.[4]

References

  1. Web site: Revised NGC Data for NGC 2491 . 2024-04-23 . spider.seds.org.
  2. Web site: Your NED Search Results . 2024-04-23 . ned.ipac.caltech.edu.
  3. Web site: New General Catalog Objects: NGC 2450 - 2499 . 2024-04-23 . cseligman.com.
  4. Web site: Data from NGC and IC catalogue by Wolfgang Steinickle from NGC 2400-2499 . 2024-04-23 . astrovalleyfield.ca.