NGC 460
In this article, we will thoroughly explore the topic of NGC 460, a topic that has captured the attention of people of all ages and walks of life. From its importance in history to its relevance today, NGC 460 has been the subject of study and interest for researchers, academics and enthusiasts alike. Through a comprehensive analysis, we will examine the various aspects related to NGC 460, from its origins to its impact on modern society. With the intention of providing a complete and detailed overview of NGC 460, this article will delve into its many facets, offering a broad and enriching perspective to understand its true meaning and scope.
| NGC 460 | |
|---|---|
 NGC 460 imaged by the Hubble Space Telescope | |
| Observation data (J2000 epoch) | |
| Right ascension | 01h 14m 41.6s[1] |
| Declination | −73° 17′ 51″[1] |
| Physical characteristics | |
| Other designations | Kron 66, Lindsay 97, IRAS 01133-7333, LI-SMC 201.[1] |
| Associations | |
| Constellation | Tucana |
NGC 460 is an open cluster with a nebula located in the constellation Tucana. It was possibly observed on August 1, 1826, by James Dunlop, though it was officially discovered on April 11, 1834, by John Herschel. Dreyer described it as "very faint (in Nubecular Minor)," with Nubecular Minor referring to the Small Magellanic Cloud. DeLisle Stewart described it as "faint, pretty large, irregularly round, gradually brighter middle, mottled but not resolved, 2nd of several."[2]
Image gallery
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NGC 465 and NGC 460 imaged by DSS
See also
References
- ^ a b c "NGC 460". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 26 May 2017.
- ^ "New General Catalog Objects: NGC 450 - 499". Cseligman. Retrieved May 26, 2017.
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