NGC 2460 explained

NGC 2460
Credit:Adam Block/Mount Lemmon SkyCenter/University of Arizona
Epoch:J2000
Constellation Name:Camelopardalis
H Radial V:1446 km/s
Z:0.004837
Dist Ly:[1]
Type:SA(s)a
Appmag V:11.46
Absmag V:-21.0
Names:[2]
Sbrightness:22.5 mag/arcsec2

NGC 2460 is an unbarred spiral galaxy in the constellation Camelopardalis. It was discovered by German astronomer Wilhelm Tempel on August 11, 1882.[3]

It is also identified as an active nucleus galaxy. Its redshift of 0.004837 gives a distance of 22 megaparsecs, or approximately 70 million light-years.[1]

Physical characteristics

NGC 2460 has an absolute magnitude of -21.0, and an apparent magnitude of 11.46.[1] Several arms extend for long distances from the central galaxy, perhaps as a result of an interaction with nearby galaxy PGC 213434.[3] The galaxy has a radial velocity of 1446 km/s.[2]

Notes and References

  1. Web site: Results for object NGC 2460 (NGC 2460). NASA/IPAC Extragalactic Database. California Institute of Technology. 2021-02-13.
  2. NGC 2460. 2021-02-13.
  3. Web site: New General Catalogue objects: NGC 2450 - 2499. Seligman, Courtney. cseligman.com. 2021-02-13.