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This image is a derivative work of the following images: File:Centaurus_constellation_map.png licensed with Cc-by-sa-3.0-migrated, GFDL 2004-12-12T18:00:49Z Alfio 2559x2559 (372805 Bytes) Centaurus constellation map; Uploaded with derivativeFX
Centaurus / s ɛ n ˈ t ɔːr ə s,-ˈ t ɑːr-/ is a bright constellation in the southern sky. One of the largest constellations , Centaurus was included among the 48 constellations listed by the 2nd-century astronomer Ptolemy , and it remains one of the 88 modern constellations .
Constellation map Subcategories. This category has the following 2 subcategories, out of 2 total. ... Pages in category "Centaurus" The following 200 pages are in ...
Map showing the location of NGC 3766. NGC 3766 (also known as Caldwell 97) is an open star cluster in the southern constellation Centaurus.It is located in the vast star-forming region known as the Carina molecular cloud, and was discovered by Nicolas Louis de Lacaille during his astrometric survey in 1751–1752. [2]
NGC 4230 is a loosely scattered open cluster in the constellation of Centaurus. [1] [3] It was discovered by John Herschel on April 5, 1837. [4] The ESO catalog (and SIMBAD database) misidentify ESO 171-SC14 as NGC 4230. [4]
NGC 3918 is a bright planetary nebula in the constellation Centaurus, nicknamed the "Blue Planetary" or "The Southerner". It is the brightest of the far southern planetary nebulae. This nebula was discovered by Sir John Herschel in March 1834 and is easily visible through small telescopes.
The depictions of the constellations in Urania's Mirror are redrawings from those in Alexander Jamieson's A Celestial Atlas, published about three years earlier, and include unique attributes differing from Jamieson's sky atlas, including the new constellation of Noctua the owl, and Norma Nilotica – a measuring device for the Nile floods – held by Aquarius the water bearer.
NGC 5408 is an irregular galaxy in the constellation Centaurus. ... M83 Subgroup of the Centaurus A/M83 ... , Sky Map, Articles and images This page ...
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