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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 .
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]
Constellation map Subcategories. This category has the following 2 subcategories, out of 2 total. ... Pages in category "Centaurus" The following 200 pages are in ...
High-resolution image of Centaurus A showing the discrete elements of galactic core; Centaurus A at UniverseToday.com; NGC5128 Centaurus A; NGC 5128 at DOCdb (Deep Sky Observer's Companion) Centaurus A on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images; Centaurus A at Constellation Guide
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]
Omega Centauri (ω Cen, NGC 5139, or Caldwell 80) is a globular cluster in the constellation of Centaurus that was first identified as a non-stellar object by Edmond Halley in 1677. Located at a distance of 17,090 light-years (5,240 parsecs), it is the largest known globular cluster in the Milky Way at a diameter of roughly 150 light-years. [10]
The spiral galaxy NGC 4622 lies approximately 111 million light years away from Earth in the constellation Centaurus. NGC 4622 is an example of a galaxy with leading spiral arms. [2] Each spiral arm winds away from the center of the galaxy and ends at an outermost tip that "points" in a certain direction (away from the arm).
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