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NGC 3261 is a barred spiral galaxy in the constellation Vela. The galaxy lies about 110 million light years away from Earth based on redshift, which means, given its apparent dimensions, that NGC 3261 is approximately 130,000 light years across. [1] It was discovered by John Herschel on March 15, 1836. [3]
Vela is a constellation in the southern sky, which contains the Vela Supercluster. Its name is Latin for the sails of a ship, and it was originally part of a larger constellation, the ship Argo Navis , which was later divided into three parts, the others being Carina and Puppis .
This constellation's Bayer designations (Greek-letter star names) were given while it was still considered part of the constellation of Argo Navis. After Argo Navis was broken up into Carina , Vela, and Puppis , these Greek-letter designations were kept, so that Vela does not have a full complement of Greek-letter designations.
HD 91324 is a likely binary [4] star system in the southern constellation of Vela. It is visible to the naked eye with an apparent visual magnitude of 4.89. [2] The distance to HD 91324, as determined from its annual parallax shift of 45.6 mas, [1] is 71.5 light years. It is moving further from the Earth with a heliocentric radial velocity of ...
IC 2488 is an open cluster in the constellation Vela. It was discovered by Nicolas-Louis de Lacaille in 1752. [ 5 ] It is located approximately 3,700 light years away from Earth.
RCW 36 (also designated Gum 20) [5] is an emission nebula containing an open cluster in the constellation Vela.This H II region is part of a larger-scale star-forming complex known as the Vela Molecular Ridge (VMR), a collection of molecular clouds in the Milky Way that contain multiple sites of ongoing star-formation activity. [1]
HD 79940 is a single [9] star in the southern constellation of Vela.It has the Bayer designation of k 1 Velorum; HD 79940 is the identifier from the Henry Draper Catalogue.This star has a yellow-white hue and is faintly visible to the naked eye as a point light source with an apparent visual magnitude of 4.63. [2]
NGC 2659 is an open cluster in the constellation Vela. It was discovered by John Herschel on 3 February, 1835. It is of Trumpler class III3m. It is a young cluster, with age nearly 8 million years. The core of the cluster is 1.93 parsec (6.3 light years) across and the total radius is 3.6 pc (11.7 light years).