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This is the list of notable stars in the constellation Vela, sorted by decreasing brightness.. This constellation's Bayer designations (Greek-letter star names) were given while it was still considered part of the constellation of Argo Navis.
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 .
In 2016, the International Astronomical Union (IAU) organized a Working Group on Star Names (WGSN) [2] to catalog and standardize proper names for stars. The WGSN's first bulletin, dated July 2016, [3] included a table of 125 stars comprising the first two batches of names approved by the WGSN (on 30 June and 20 July 2016) together with names of stars adopted by the IAU Executive Committee ...
Gamma Velorum is a quadruple star system in the constellation Vela.This name is the Bayer designation for the star, which is Latinised from γ Velorum and abbreviated γ Vel.At a combined magnitude of +1.72, it is one of the brightest stars in the night sky, and contains by far the closest and brightest Wolf–Rayet star.
Lambda Velorum (λ Velorum, abbreviated Lambda Vel, λ Vel), officially named Suhail / ˈ s uː h eɪ l /, [11] is a star in the southern constellation of Vela.With a mean apparent visual magnitude of 2.21, [2] this is the third-brightest star in the constellation and one of the brighter stars in the sky.
HR 3562 (HD 76566) is a visual binary consisting of a bluish-white hued variable star and a Sun-like secondary star in the southern constellation of Vela. It has the variable-star designation IY Velorum (abbreviated to IY Vel). With an apparent magnitude of 6.26, the brighter primary is near the limit for naked eye visibility.
Omicron Velorum (ο Vel, ο Velorum) is a star in the constellation Vela. It is the brightest member of the loose naked eye open cluster IC 2391, also known as the ο Velorum Cluster. A light curve for Omicron Velorum, plotted from TESS data [9] Omicron Velorum is a blue-white B-type star with a mean apparent magnitude of +3.60.
There are 372 probable member stars within the angular radius of the cluster and 115 within the central part of the cluster. [4] The tidal radius of the cluster is 9.0 - 11.6 parsecs (29 - 38 light years) and represents the average outer limit of IC 2488, beyond which a star is unlikely to remain gravitationally bound to the cluster core. [ 3 ]