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Beta Gruis
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Beta Gruis ( β Gruis, abbreviated Beta Gru, β Gru), formally named Tiaki , is the second brightest in the southern of Grus. It was once considered the rear star in the tail of the constellation of the (Southern) Fish, : it, with , , , , and , belonged to Piscis Austrinus in medieval Arabic astronomy.


Nomenclature
β Gruis (Latinised to Beta Gruis) is the star's Bayer designation.

It bore the traditional name of Tiaki. In 2016, the IAU organized a Working Group on Star Names (WGSN) to catalog and standardize proper names for stars. The WGSN approved the name Tiaki for this star on 5 September 2017 and it is now so included in the List of IAU-approved Star Names.

In , 鶴 (Hè), meaning Crane, refers to an asterism consisting of Beta Gruis, , , , , , , , Delta² Gruis and Mu¹ Gruis. 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, Beta Gruis itself is known as 鶴二 (Hè èr, ). 香港太空館 - 研究資源 - 亮星中英對照表 , Hong Kong Space Museum. Accessed on line November 23, 2010. The Chinese name gave rise to another English name, Ke. Richard Hinckley Allen: Star Names — Their Lore and Meaning: Grus


Properties
Beta Gruis is a star on the asymptotic giant branch with an estimated mass of about 2.4 times that of and a surface temperature of approximately 3,500 , just over half the surface temperature of the Sun. This low temperature accounts for the dull red color of an M-type star. The total luminosity is about 3,200 times that of , and it has 150 times the .

It is one of the brightest stars at and near-infrared wavelenghts. At the K band, it is the fifth-brightest star in the night sky.

Alan William James Cousins announced that Beta Gruis is a in 1952. Beta Gruis is a semiregular variable (SRb) star that varies in magnitude by about 0.4. It varies between intervals when it displays regular changes with a 37-day periodicity and times when it undergoes slow irregular variability.


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