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NGC 1585

Coordinates: Sky map 04h 27m 33.0055s, −42° 09′ 54.502″
From Wikipedia, the free encyclopedia
NGC 1585
BERJAYA
NGC 1585 imaged by Legacy Surveys
Observation data (J2000 epoch)
ConstellationCaelum
Right ascension04h 27m 33.0055s[1]
Declination−42° 09 54.502[1]
Redshift0.015534[1]
Heliocentric 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, 2MASX J04273300-4209549, 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

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Two supernovae have been observed in NGC 1585:

See also

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References

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  1. 1 2 3 4 5 6 7 8 9 10 "Results for object NGC 1585". NASA/IPAC Extragalactic Database. NASA and Caltech. Retrieved 19 July 2024.
  2. Seligman, Courtney. "New General Catalogue Objects: NGC 1585". Celestial Atlas. Retrieved 12 December 2024.
  3. "NGC 1585". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 12 December 2024.
  4. "SN 2023vio". Transient Name Server. IAU. Retrieved 12 December 2024.
  5. "SN 2025xes". Transient Name Server. IAU. Retrieved 26 September 2025.
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  • Wikimedia Commons logo Media related to NGC 1585 at Wikimedia Commons
  • NGC 1585 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images