Beta Aquilae is a triple star system in the equatorial constellation of Aquila. Its name is a Bayer designation that is Latinized from β Aquilae, and abbreviated Beta Aql or β Aql. This system is visible to the naked eye as a point-like source with an apparent visual magnitude of 3.87. Based on parallax measurements, it is located at a distance of 44.4 light-years. It is drifting closer to the Sun with a radial velocity of −40 km/s, and is predicted to approach to within in roughly 207,000 years.
Its two visible components are designated Beta Aquilae A and B. The former is formally named Alshain , the traditional name for the system.
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 Persian shāhīn-i tarazu "the scale beam", the Persian name for the asterism of α, β and γ Aquilae, itself a translation of the Arabic al-mizan "the balance". The name Tarazed for γ Aquilae is derived from the same Persian term. 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. 中國星座神話, written by 陳久金. Published by 台灣書房出版有限公司, 2005, . Consequently, the Chinese name for Beta Aquilae itself is (, ). 香港太空館 - 研究資源 - 亮星中英對照表 , Hong Kong Space Museum. Accessed on line November 26, 2008.
Properties The primary, component 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. The activity shows a cycle of . The star displays solar-like oscillations. Since 1943, the spectrum of this star has served as one of the stable anchor points by which other stars are classified.
This is an aging subgiant star that has exhausted the supply of hydrogen at its core and is evolving into a giant. Its angular diameter has been precisely determined using interferometry at the CHARA array, which combined with its estimated distance, result in a radius 3.123 times the radius of the Sun. It has a mass 24% greater than the Sun's, a luminosity 6.2 times that of the Sun, and an effective temperature of 5,163 K.
The 12th magnitude secondary companion, designated component B, is a double-lined spectroscopic binary, which is at an angular separation of 13 arcseconds from the primary. It has a stellar classification of M2.5 V, matching a class M red dwarf.
In culture In the Chinese folk tale The Cowherd and the Weaver Girl, 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.
was a United States Navy ship.
References .
External links
ARICNS Image β Aquilae Stellar Catalog entry for Beta Aquilae.