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NGC 2342

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Galaxy in the constellation Gemini

NGC 2342
The spiral galaxy NGC 2342 imaged by the Hubble Space Telescope
Observation data (J2000 epoch)
ConstellationGemini
Right ascension07 09 18.0802
Declination+20° 38′ 09.762″
Redshift0.017652
Heliocentric radial velocity5291 ± 2 km/s
Distance261.9 ± 18.3 Mly (80.29 ± 5.62 Mpc)
Apparent magnitude (V)12.6
Characteristics
TypeS pec
Size~149,200 ly (45.73 kpc) (estimated)
Apparent size (V)1.4′ × 1.3′
Other designations
HOLM 086A, IRAS 07063+2043, 2MASX J07091808+2038092, UGC 3709, MCG +03-19-004, PGC 20265, CGCG 086-007

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.

NGC 2342 is a luminous infrared galaxy (LIRG). Together with NGC 2341, they both form a gravitationally bound galaxy pair listed as HOLM 86.

One supernova has been observed in NGC 2342: SN 2023vck (type Ib, mag 19.917) was discovered by the Zwicky Transient Facility on 15 October 2023.

See also

References

  1. ^ "Results for NGC 2342". NASA/IPAC Extragalactic Database. NASA and Caltech. Retrieved 4 August 2024.
  2. Seligman, Courtney. "New General Catalogue Objects: NGC 2342". Celestial Atlas. Retrieved 14 December 2024.
  3. Holmberg, Erik (1 January 1937). "A Study of Double and Multiple Galaxies Together with Inquiries into some General Metagalactic Problems". Annals of the Observatory of Lund. 6: 1–173. Retrieved 4 August 2024.
  4. "SN 2023vck". Transient Name Server. IAU. Retrieved 15 December 2024.

External links

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