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Beta Aquilae is a system in the equatorial 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 measurements, it is located at a distance of 44.4 . It is drifting closer to the Sun with a 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 , and adopted by the International Astronomical Union (IAU).

The system bore the traditional name Alshain derived from the Perso- term الشاهين, aš-šāhīn, meaning "the ", perhaps by from the šāhīn tarāzū (or possibly šāhīn tara zed; see ), the Persian name for the asterism , β and . 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 . 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 as Collum Corvi, meaning the crow's neck.

In Chinese, 河鼓 (Hé Gŭ), meaning River Drum, refers to an asterism consisting of Beta Aquilae, and . 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 河鼓一 (Hé Gŭ yī, ). 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 . The activity shows a cycle of . The star displays solar-like oscillations. Since 1943, the of this star has served as one of the stable anchor points by which other stars are classified.

This is an aging star that has exhausted the supply of hydrogen at its core and is evolving into a . Its has been precisely determined using interferometry at the Very Large Telescope and the , the average of both measurements, combined with its estimated distance, result in a radius 3.096 times the radius of the Sun. It has a mass 24% greater than , a luminosity 5.9 times that , and an effective temperature of 5,060 .

The 12th magnitude secondary companion, designated component B, is a double-lined spectroscopic binary, which is at an angular separation of 13 from the primary. It has a stellar classification of M2.5 V, matching a .


In culture
In the Chinese folk tale The Cowherd and the Weaver Girl, Beta and Gamma Aquilae are children of (牛郎, The Cowherd, ) and Zhinü (織女, The Princess, ).

The Koori people of Victoria knew Beta and Gamma Aquilae as the wives of Bunjil (Altair), the wedge-tailed eagle.

was a United States Navy ship.
     


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