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Pi Sagittarii

Pi Sagittarii is a triple star system in the zodiac constellation of Sagittarius. It has an apparent visual magnitude of +2.89, bright enough to be readily seen with the naked eye. Based upon parallax measurements, it is roughly 510 light-years from the Sun.

Nomenclature
π Sagittarii (Latinised to Pi Sagittarii) is the system's Bayer designation. The designations of the three constituents as Pi Sagittarii A, B and C, derive from the convention used by the Washington Multiplicity Catalog (WMC) for multiple star systems, and adopted by the International Astronomical Union (IAU). The system bore the traditional name Albaldah, to catalog and standardize proper names for stars. The WGSN decided to attribute proper names to individual stars rather than entire multiple systems. It approved the name Albaldah for the component Pi Sagittarii A on 5 September 2017 and it is now so included in the List of IAU-approved Star Names. In Chinese, (), meaning Establishment, refers to an asterism consisting of Pi Sagittarii, Xi2 Sagittarii, Omicron Sagittarii, 43 Sagittarii, Rho1 Sagittarii and Upsilon Sagittarii. Consequently, the Chinese name for Pi Sagittarii itself is (, ). == Properties ==
Properties
The spectrum of the system's primary, Pi Sagitarii A, matches a stellar classification of F2 II. ==References==
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