Gamma Eridani Explained

Gamma Eridani (γ Eridani, abbreviated Gamma Eri, γ Eri), formally named Zaurak, is a variable star in the constellation of Eridanus. It is visible to the naked eye with an apparent visual magnitude that varies around 2.9, and lies at a distance of about 203 light years from the Sun, as determined by the Hipparcos astrometry satellite.

Description

Gamma Eridani has been defined as a standard star for the spectral class M0III-IIIb. It is a red giant on the asymptotic giant branch, fusing hydrogen and helium in separate shells outside its core. Observations published in 1960 showed it to vary in brightness by a few hundredths of a magnitude. In 1977, it was officially listed as a variable star in the General Catalogue of Variable Stars although the class of variable is uncertain.

The Gaia EDR3 data identified a comoving companion star of Gamma Eridani, at a projected separation of . It is likely that there is an additional red dwarf companion that at a distance within, too close to resolve from the primary.[1]

Nomenclature

Gamma Eridani is the star's Bayer designation. It has the traditional name Zaurak, alternatively spelled Zaurac, which is one of the Persian words for 'boat'. In 2016, the International Astronomical Union organized a Working Group on Star Names (WGSN) to catalog and standardize proper names for stars. The WGSN's first bulletin of July 2016 included a table of the first two batches of names approved by the WGSN; which included Zaurak for this star.

In Chinese, Chinese: 天苑 (Chinese: Tiān Yuàn), meaning Celestial Meadows, refers to an asterism consisting of γ Eridani, δ Eridani, π Eridani, ε Eridani, ζ Eridani, η Eridani, π Ceti, τ1 Eridani, τ2 Eridani, τ3 Eridani, τ4 Eridani, τ5 Eridani, τ6 Eridani, τ7 Eridani, τ8 Eridani and τ9 Eridani.[2] Consequently, the Chinese name for γ Eridani itself is Chinese: 天苑一 (Chinese: Tiān Yuàn yī, English: the First [Star] of Celestial Meadows.)[3]

USS Zaurak (AK-117) was a United States Navy Crater class cargo ship named after the star.

Notes and References

  1. Kervella . Pierre . Arenou . Frédéric . Thévenin . Frédéric . Stellar and substellar companions from Gaia EDR3: Proper-motion anomaly and resolved common proper-motion pairs (Corrigendum) . Astronomy & Astrophysics . April 2024 . 684 . C2 . 10.1051/0004-6361/202450066e. free . 2024A&A...684C...2K .
  2. 中國星座神話, written by 陳久金. Published by 台灣書房出版有限公司, 2005, .
  3. 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.