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NGC 1590

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NGC 1590
NGC 1590 imaged by SDSS
Observation data (J2000 epoch)
ConstellationTaurus
Right ascension04h 31m 10.2655s[1]
Declination+07° 37′ 51.108″[1]
Redshift0.012999[1]
Heliocentric radial velocity3897 ± 6 km/s[1]
Distance184.1 ± 12.9 Mly (56.43 ± 3.95 Mpc)[1]
Group or clusterNGC 1762 Group (LGG 120)
Apparent magnitude (V)14.5[1]
Characteristics
TypeSbc D[1]
Size~64,000 ly (19.62 kpc) (estimated)[1]
Apparent size (V)0.9′ × 0.7′[1]
Other designations
IRAS 04284+0731, 2MASX J04311020+0737513, UGC 3071, MCG +01-12-008, PGC 15368, CGCG 419-014[1]

NGC 1590 is a spiral galaxy in the constellation of Taurus. Its velocity with respect to the cosmic microwave background is 3826 ± 8 km/s, which corresponds to a Hubble distance of 56.43 ± 3.95 Mpc (~184 million light-years).[1] It was discovered by German astronomer Heinrich d'Arrest on 28 October 1865.[2]

NGC 1762 Group

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NGC 1590 is part of the NGC 1762 Group (also known as LGG 120) that includes at least 27 galaxies, including IC 392 [fr], NGC 1633, NGC 1642, NGC 1691 [fr], NGC 1713 [fr], NGC 1719, and NGC 1762, among others.[3][4]

Supernova

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One supernova has been observed in NGC 1590:

See also

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References

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  1. ^ a b c d e f g h i j k "Results for object NGC 1590". NASA/IPAC Extragalactic Database. NASA and Caltech. Retrieved 4 August 2024.
  2. ^ Seligman, Courtney. "New General Catalogue Objects: NGC 1590". Celestial Atlas. Retrieved 15 December 2024.
  3. ^ Garcia, A. M. (1993). "General study of group membership. II. Determination of nearby groups". Astronomy and Astrophysics Supplement Series. 100: 47. Bibcode:1993A&AS..100...47G.
  4. ^ "LGG 120". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 26 December 2025.
  5. ^ Parisky, X.; Li, W. (2007). "Supernovae 2007ry and 2007rz". Central Bureau Electronic Telegrams (1158): 1. Bibcode:2007CBET.1158....1P.
  6. ^ "SN 2007rz". Transient Name Server. IAU. Retrieved 15 December 2024.
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