Astronomy:NGC 2642

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NGC 2642
NGC 2642 imaged by SDSS
Observation data (J2000 epoch)
ConstellationHydra
Right ascension 08h 40m 44.3818s[1]
Declination−04° 07′ 18.011″[1]
Redshift0.014473[1]
Helio radial velocity4339 ± 5 km/s[1]
Distance222.8 ± 15.6 Mly (68.32 ± 4.79 Mpc)[1]
Apparent magnitude (V)12.6[1]
Characteristics
TypeSB(r)bc[1]
Size~140,800 ly (43.17 kpc) (estimated)[1]
Apparent size (V)2.0′ × 1.8′[1]
Other designations
IRAS 08382-0356, MCG-01-22-033, PGC 24395[1]

NGC 2642 is a barred spiral galaxy in the constellation of Hydra. Its velocity with respect to the cosmic microwave background is 4632 ± 21 km/s, which corresponds to a Hubble distance of 68.32 ± 4.79 Mpc (~223 million light-years).[1] It was discovered by British astronomer John Herschel on 19 February 1830.[2]

According to the SIMBAD database, NGC 2642 is a Seyfert I galaxy, i.e. it has a quasar-like nuclei with very high surface brightnesses whose spectra reveal strong, high-ionisation emission lines, but unlike quasars, the host galaxy is clearly detectable.[3]

Supernovae

Three supernovae have been observed in NGC 2642:

  • SN 2002fj (Type IIn, mag. 15.8) was discovered by Libert "Berto" Monard on 12 September 2002.[4][5]
  • SN 2008bh (Type II, mag. 16.3) was discovered by the Lick Observatory Supernova Search (LOSS) and by The CHilean Automatic Supernova sEarch (CHASE) on 23 March 2008.[6][7]
  • SN 2023aaby (Type Ic, mag. 17.943) was discovered by ATLAS on 14 December 2023.[8]

See also

References