Kappa Velorum (κ Velorum, abbreviated Kappa Vel or κ Vel; proper name Markeb ) is star system in the southern constellation of Vela. It is binary star consisting of two components, designated A and B; κ Vel A is by far the brighter of the two, so dominates the combined light. From parallax measurements, this system is located at a distance of roughly 572 light-years (175 parsecs) from the Sun. The apparent visual magnitude is 2.48, making it readily visible to the naked eye in the southern hemisphere. It forms part of an asterism known as the False Cross along with Delta Velorum, Iota Carinae and Epsilon Carinae, so called because it is sometimes mistaken for the Southern Cross, causing errors in astronavigation.
Nomenclature κ Velorum (Latinised to Kappa Velorum) is the system's Bayer designation. The designations of the two components as Kappa Velorum A and B derives from the convention used by the Washington Multiplicity Catalog (WMC) for multiple star systems, and adopted by the International Astronomical Union (IAU). The system had a traditional name Markab, from the Arabic مركب, markab meaning "something to ride". It was often spelled Markeb to distinguish it from similarly named stars such as Alpha Pegasi. In 2016, the IAU organized a Working Group on Star Names (WGSN) to catalog and standardize proper names for stars. The WGSN approved the name Markeb for Kappa Velorum A on 5 September 2017. Markab had previously been approved for Alpha Pegasi on 30 June 2016. Both are now included in the List of IAU-approved Star Names. In Chinese, 天社 (Tiān Shè), meaning Celestial Earth God's Temple, refers to an asterism consisting of Kappa Velorum, Gamma2 Velorum, b Velorum and Delta Velorum. Consequently, Kappa Velorum itself is known as 天社五 (Tiān Shè wǔ), "the Fifth Star of Celestial Earth God's Temple".
Properties Kappa Velorum is a spectroscopic binary system consisting of a pair of stars that complete an orbit around each other with a period of 116.80 days, a semi-major axis of 1.28 AU and an eccentricity of 0.1761. The primary's stellar classification of the pair is B2 V – IV, which matches the class of a B-type star that is exhausting the hydrogen at its core and has begun to evolve into a subgiant star. It is about 13 times more massive than the Sun, with a photospheric radius twelve times larger, irradiating 13,000 times more luminosity than the Sun at an effective temperature of 18,000 K, which give Kappa Velorum A the blue-white hue typical of B-type stars. The secondary is a B-type main-sequence star much less luminous than the primary. It has 7.7 times the mass of the Sun and an effective temperature of 19,000 K, also giving it a blue-white hue.
Interstellar medium Analysis of the spectrum of Kappa Velorum shows absorption lines due to the interstellar medium between Earth and the star. Observation of these features over many years has shown that the lines vary in strength, probably caused by a small dense cloud extending 100–1,000 au moving across the line of sight.
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External links "The path of the Southern Celestial Pole": The System of W. B. Yeats's A Vision [1] Diagram of the southern precession circle, showing Markeb as the South Pole Star in 9000 AD. Kaler, James B., "MARKEB (Kappa Velorum)", Stars, University of Illinois, retrieved 2012-01-08


