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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 .
Print/export Download as PDF; ... Constellation map Subcategories. This category has the following 2 subcategories, out of 2 total. ... Pages in category "Centaurus"
The Alpha Centaurids are a meteor shower in the constellation Centaurus, peaking in early February each year. The average magnitude is around 2.5, with a peak of about three meteors an hour. [2] They have been observed since 1969, with a single possible recorded observation in 1938. [3]
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
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]
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 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.
It is a proper motion member of the Lower Centaurus–Crux sub-group in the Scorpius–Centaurus OB association, the nearest such association of co-moving massive stars to the Sun. [3] The primary component of this system is a B-type main-sequence star with a stellar classification of B3 V. [ 3 ] It is about 24 [ 6 ] million years old with a ...
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