Beta Aquilae

Beta Aquilae, Latinized from β Aquilae, is a binary star system in the equatorial constellation of Aquila. It is visible to the naked eye as a point-like source with an apparent visual magnitude of 3.87. Based on parallax measurements obtained during the Hipparcos mission, it is located at a distance of approximately 44.7 light-years from the Sun. It is drifting closer to the Sun with a radial velocity of −40 km/s.
Its two components are designated Beta Aquilae A (formally named Alshain , the traditional name for the system) and B.
Nomenclature.
"β Aquilae" (Latinised to "Beta Aquilae") is the system's Bayer designation. The designations of the two components as "Beta Aquilae A" and "B" 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 "Alshain" derived from the Perso-Arabic term الشاهين, "aš-šāhīn", meaning "the (peregrine) falcon", perhaps by folk etymology from the Persian "šāhīn tarāzū" (or possibly "šāhīn tara zed"; see Gamma Aquilae), the Persian name for the asterism α, β and γ Aquilae. In 2016, the IAU organized a Working Group on Star Names (WGSN) to catalogue 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 "Alshain" for the component Beta Aquilae A on 21 August 2016 and it is now so included in the List of IAU-approved Star Names.
In the catalogue of stars in the "Calendarium" of Al Achsasi al Mouakket, this star was designated "Unuk al Ghyrab" (عنق ألغراب - "únuq al-ghuraab"), which was translated into Latin as "Collum Corvi", meaning "the crow's neck".
In Chinese, (), meaning "River Drum", refers to an asterism consisting of Beta Aquilae, Altair and Gamma Aquilae. Consequently, the Chinese name for Beta Aquilae itself is (, ).
Namesake.
 was a United States navy ship.
Properties.
The primary (Beta Aquilae A) is of magnitude 3.71 and spectral class G8IV. It has a very low level of surface magnetic activity and may be in a state similar to a Maunder minimum. Since 1943, the spectrum of this star has served as one of the stable anchor points by which other stars are classified. A subgiant with a mass 26% greater than the Sun's, a luminosity six times that of the Sun, and a radius about thrice solar.
The secondary (Beta Aquilae B) is a 12th magnitude companion which is 13 arcseconds away in the sky. It is a class M red dwarf with a mass a third that of the Sun and a luminosity 2.5% the Sun's.
In culture.
In Chinese mythology, The Princess and the Cowherd, Beta and Gamma Aquilae are children of Niulang (牛郎, The Cowherd, Altair) and Zhinü (織女, The Princess, Vega).
The Koori people of Victoria knew Beta and Gamma Aquilae as the black swan wives of "Bunjil" (Altair), the wedge-tailed eagle.