Alpha Crateris

Alpha Crateris, officially named Alkes, is a star in the constellation of Crater. It is a cool giant star about away.

Nomenclature

α Crateris is the star's Bayer designation.
It bore the traditional name Alkes, from the Arabic الكاس alkās or الكأس alka's "the cup". In the catalogue of stars in the Calendarium of Al Achsasi al Mouakket, this star was designated Aoul al Batjna, which was translated into Latin as Prima Crateris, meaning "first of the Cup". In 2016, the International Astronomical Union organized a IAU [Working Group on Star Names|Working Group on Star Names] to catalogue and standardize proper names for stars. The WGSN approved the name Alkes for this star on 12 September 2016 and it is now so included in the List of IAU-approved Star Names.
In Chinese, 翼宿, meaning Wings , refers to an asterism consisting of Alpha Crateris, Gamma Crateris, Zeta Crateris, Lambda Crateris, Nu Hydrae, Eta Crateris, Delta Crateris, Iota Crateris, Kappa Crateris, Epsilon Crateris, HD 95808, HD 93833, Theta Crateris, HD 102574, HD 100219, Beta Crateris, HD 99922, HD 100307, HD 96819, Chi¹ Hydrae, HD 102620 and HD 103462. Consequently, Alpha Crateris itself is known as 翼宿一.

was a United States Navy named after the star.

Alpha Crateris is an orange giant of spectral type K1III. It has an apparent magnitude of 4.07, and is 174 light-years from Earth. It is thought to be a horizontal branch star, meaning it is fusing helium in its core after a helium flash. Cool horizontal branch stars are often called red clump giants as they form a noticeable grouping near the hot edge of the red giant branch in the H–R diagrams of clusters with near-solar metallicity. On this basis it is calculated to have a mass of, a luminosity of, and an age around two billion years. Its surface temperature is 4691 K. Or it might be a red-giant branch star, still fusing hydrogen in a shell around an inert helium core, in which case it would be slightly less massive, older, cooler, larger, and more luminous.