NGC 2342 explained

NGC 2342
Constellation Name:Gemini
Epoch:J2000
Type:S pec[1]
Dist Ly:NaNMpc
Z:0.017652
H Radial V:5292 ± 4 km/s
Appmag V:12.6
Size V:1.4' x 1.3'
Size:~45.74kpc (estimated)

NGC 2342 is a spiral galaxy in the constellation of Gemini. Its velocity with respect to the cosmic microwave background is 5445 ± 11 km/s, which corresponds to a Hubble distance of 80.31 ± 5.62 Mpc (∼262 million light-years). It was discovered by German astronomer Albert Marth on 10 November 1864.[2]

NGC 2342 is also a luminous infrared galaxy (LIRG). Together with NGC 2341, they both form a gravitationally bound galaxy pair called HOLM 301.[3]

One supernova has been observed in NGC 2342: SN 2023vck (type Ib, mag 19.9).[4]

See also

Notes and References

  1. Web site: NASA/IPAC Extragalactic Database . Results for NGC 2342 . 4 August 2024.
  2. https://cseligman.com/text/atlas/ngc23.htm#2342 Celestial Atlas entry for NGC 2342.
  3. Holmberg . Erik . 1937-01-01 . A Study of Double and Multiple Galaxies Together with Inquiries into some General Metagalactic Problems . Annals of the Observatory of Lund . 6 . 1–173. 4 August 2024.
  4. https://www.wis-tns.org/object/2023vck Transient Name Server entry for SN 2023vck.