Dubhe
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Dubhe is a multiple star system in the northern constellation of Ursa Major. It is formally designated Alpha Ursae Majoris, Latinised from α Ursae Majoris,<ref name=Kunitzsch/><ref name="IAU-CSN">{{#invoke:citation/CS1|citation |CitationClass=web }}</ref> Despite being designated "α" (alpha), it is the second-brightest object in the constellation. Alpha Ursae Majoris is the northern of the 'pointers' (or 'guards'), the second being Beta Ursae Majoris, or 'Merak' – this pair of stars point towards Polaris, the North Star.<ref name=Streicher2009/> α Ursae Majoris is located at a distance of approximately 123 light years from the Sun, based on parallax measurements.
Although it is part of the constellation of Ursa Major, it is not part of the Ursa Major Moving Group of stars that have a common motion through space.<ref name="motz">Template:Cite book</ref>
ComponentsEdit
Dubhe is a spectroscopic binary made up of the stars α Ursae Majoris A and α Ursae Majoris B. The pair orbit at a separation of about 23 astronomical units (AU),<ref name="msc"/> with a period of 44.5 years and an eccentricity of 0.44.<ref name=Gray2018/> There is another spectroscopic binary at an angular separation of 7.1 arcminutes, forming a 7th magnitude pair showing an F8 spectral type with an orbital period of 6.035 days and an eccentricity of 0.09. It is sometimes referred to as Alpha Ursae Majoris C, but is separately catalogued as HD 95638.<ref name="msc" /> Together they form a quadruple star system.<ref name=Eggleton_Tokovinin_2008/>
Component A is the system's primary, and it has a stellar classification of K0III.<ref name=guenther/> This is a giant star that has evolved away from the main sequence after consuming the hydrogen at its core. It is 280 million years old<ref name=Baines_et_al_2017/> with 3.7 times the Sun's mass<ref name=Gray2018/> and has expanded 27 times the radius of the Sun.<ref name=Baines2025/> The star is radiating 340 times the luminosity of the Sun from its enlarged photosphere<ref name="Luck2015"/> at an effective temperature of 4,800 K.<ref name=Baines2025/> The secondary star, component B, is an A-type main-sequence star that has a class of A5V.<ref name=Gray2018/> α Ursae Majoris has been reported to vary in brightness by about a thousandth of a magnitude. Ten radial oscillation modes have been detected, with periods between 6.4 hours and 6.4 days.<ref name="buzasi"/>
NomenclatureEdit
α Ursae Majoris (Latinised to Alpha Ursae Majoris) is the star system's Bayer designation.
It bore the traditional name Dubhe, which is derived from the Arabic for 'bear', Template:Transliteration, from the phrase {{#invoke:Lang|lang}} Template:Transliteration 'the back of the Greater Bear'. The ancient Egyptians called it Ak, meaning 'The Eye'.<ref name=allen1899>Template:Cite book</ref> In 2016, the International Astronomical Union organized a Working Group on Star Names (WGSN)<ref name="WGSN">{{#invoke:citation/CS1|citation |CitationClass=web }}</ref> to catalog and standardize proper names for stars. The WGSN's first bulletin of July 2016<ref name="WGSN1">{{#invoke:citation/CS1|citation |CitationClass=web }}</ref> included a table of the first two batches of names approved by the WGSN; which included Dubhe for the star α Ursae Majoris A.
The Hindus refer to the star as Kratu, one of the Seven Rishis.<ref name=allen1899/>
In Chinese, {{#invoke:Lang|lang}} Běi Dǒu, meaning Northern Dipper, refers to an asterism equivalent to the Big Dipper. Consequently, the Chinese name for Alpha Ursae Majoris itself is {{#invoke:Lang|lang}} Běi Dǒu yī, (Template:Langx) and {{#invoke:Lang|lang}} Tiān Shū, (Template:Langx).<ref>Template:In lang AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 6 月 15 日 Template:Webarchive</ref>
In cultureEdit
Dubhe is the official star of the State of Utah.<ref>{{#invoke:citation/CS1|citation |CitationClass=web }}</ref>
Dubhe was a ship in the United States Navy. The Danish National Home Guard Navy ship MHV806 is also named Dubhe.
See alsoEdit
ReferencesEdit
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