Jump to content

NGC 458

From Wikipedia, the free encyclopedia

This is an old revision of this page, as edited by Monkbot (talk | contribs) at 21:01, 12 January 2021 (Task 18 (cosmetic): eval 2 templates: hyphenate params (1×);). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.

NGC 458
NGC 458
NGC 458 as seen by the DSS
Credit: DSS
Observation data (J2000 epoch)
Right ascension01h 14m 53.36s[1]
Declination−71° 32′ 58.7″[1]
Apparent magnitude (V)11.86[1]
Apparent dimensions (V)2.6′ × 2.3′[1]
Physical characteristics
Other designationsKron 69, Lindsay 96, ESO 51-26, RZ2005 197.[1]
Associations
ConstellationTucana
See also: Open cluster, List of open clusters

NGC 458 is an open cluster located in the constellation Tucana. It was discovered on September 6, 1826, by James Dunlop. It was also observed by John Herschel and DeLisle Stewart. It was described by Dreyer as "pretty faint, large, round, very gradually brighter middle." It was also noted in the second Index Catalogue that it was "probably a cluster, extremely small, close, no nebulosity seen by D.S. (DeLisle Stewart)."[2]

References

  1. ^ a b c d e "NGC 458". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 21 May 2017.
  2. ^ "New General Catalog Objects: NGC 450 - 499". Cseligman. Retrieved May 21, 2017.
  • Media related to NGC 458 at Wikimedia Commons