Astronomy:NGC 1585

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NGC 1585
NGC 1585 imaged by Legacy Surveys
Observation data (J2000 epoch)
ConstellationCaelum
Right ascension 04h 27m 33.0055s[1]
Declination−42° 09′ 54.502″[1]
Redshift0.015534[1]
Helio radial velocity4657 ± 31 km/s[1]
Distance223.0 ± 15.8 Mly (68.36 ± 4.83 Mpc)[1]
Apparent magnitude (V)13.5[1]
Characteristics
TypeSAc[1]
Size~129,400 ly (39.66 kpc) (estimated)[1]
Apparent size (V)1.2′ × 0.7′[1]
Other designations
ESO 303- G 018, IRAS 04259-4216, MCG-07-10-006, PGC 15150[1]

NGC 1585 is a spiral galaxy in the constellation of Caelum. Its velocity with respect to the cosmic microwave background is 4,635 ± 31 km/s, which corresponds to a Hubble distance of 68.4 ± 4.8 Mpc (~223 million light-years). It was discovered by British astronomer John Herschel on 1 December 1837.[2]

The SIMBAD database lists NGC 1585 as a Seyfert I Galaxy, i.e. it has a quasar-like nucleus with very high surface brightnesses whose spectra reveal strong, high-ionisation emission lines, but unlike quasars, the host galaxy is clearly detectable.[3]

Supernovae

Two supernovae have been observed in NGC 1585:

  • SN 2023vio (Type Iax [02cx-like], mag. 19.053) was discovered by ATLAS on 17 October 2023.[4]
  • SN 2025xes (Type Ia, mag. 16.81) was discovered by ATLAS on 10 September 2025.[5]

See also

References