Epsilon Boötis (ε Boötis, abbreviated Epsilon Boo, ε Boo), officially named Izar ( ), is a binary star in the northern constellation of Boötes. The star system can be viewed with the unaided eye at night, but resolving the pair with a small telescope is challenging; an aperture of or greater is required. Nomenclature ε Boötis (Latinised to Epsilon Boötis) is the star's Bayer designation. It bore the traditional names Izar, Mirak and Mizar, and was named by Friedrich Georg Wilhelm von Struve. Izar, Mirak and Mizar are from the ('veil') and ('the loins'); is Latin for 'loveliest'. In 2016, the International Astronomical Union organized a Working Group on Star Names (WGSN) to catalogue and standardize proper names for stars. The WGSN approved the name Izar for this star on 21 August 2016 and it is now so entered in the IAU Catalog of Star Names. In the catalogue of stars in the Calendarium of Al Achsasi Al Mouakket, this star was designated ( ), which was translated into Latin as , meaning 'belt of barker'. In Chinese astronomy, ('Celestial Lance'), refers to an asterism consisting of Epsilon Boötis, Sigma Boötis and Rho Boötis. Consequently, the Chinese name for Epsilon Boötis itself is ('the First Star of Celestial Lance'). Properties Epsilon Boötis consists of a pair of stars with an angular separation of at a position angle of . The brighter component (A) has an apparent visual magnitude of 2.37, making it readily visible to the naked eye at night. The fainter component (B) is at magnitude 5.12, which by itself would also be visible to the naked eye. Parallax measurements from the Hipparcos astrometry satellite put the system at a distance of about from the Earth. This means the pair has a projected separation of 185 Astronomical Units, and they orbit each other with a period of at least 1,000 years. The brighter member has a stellar classification of K0 II-III, which means it is a fairly late-stage star well into its stellar evolution, having already exhausted its supply of hydrogen fuel at the core. With more than four times the mass of the Sun, it has expanded to about 33 times the Sun's radius and is emitting 501 times the luminosity of the Sun. This energy is being radiated from its outer envelope at an effective temperature of 4,550 K, giving it the orange hue of a K-type