Zeta Ceti Explained

Zeta Ceti (ζ Ceti, abbreviated Zeta Cet, ζ Cet) is a binary star in the equatorial constellation of Cetus. It has a combined apparent visual magnitude of 3.74, which is bright enough to be seen with the naked eye. Based upon parallax measurements taken during the Hipparcos mission, it is approximately 235 light-years from the Sun.

Zeta Ceti is the primary or 'A' component of a double star system designated WDS J01515-1020 (the secondary or 'B' component is HD 11366).[1] Zeta Ceti's two components are therefore designated WDS J01515-1020 Aa and Ab. Aa is officially named Baten Kaitos, the traditional name of the entire system.[2]

Nomenclature

ζ Ceti (Latinised to Zeta Ceti) is the binary pair's Bayer designation. WDS J01515-1020 A is its designation in the Washington Double Star Catalog. The designations of the two components as WDS J01515-1020 Aa and Ab derive from the convention used by the Washington Multiplicity Catalog (WMC) for multiple star systems, and adopted by the International Astronomical Union (IAU).[3]

It bore the traditional name Baten Kaitos, derived from the Arabic بطن قيطس batn qaytus "belly of the sea monster". In 2016, the International Astronomical Union 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.[4] It approved the name Baten Kaitos for the component WDS J01515-1020 Aa on 12 September 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 Rabah al Naamat رابع ألنعامة raabi3 al naʽāmāt, which was translated into Latin as Quarta Struthionum, meaning "the fourth ostrich". This star, along with Eta Ceti (Deneb Algenubi), Theta Ceti (Thanih Al Naamat), Tau Ceti (Thalath Al Naamat), and Upsilon Ceti, formed Al Naʽāmāt ('ألنعامة), "the Hen Ostriches".[5]

In Chinese, Chinese: 天倉 (Chinese: Tiān Cāng), meaning Square Celestial Granary, refers to an asterism consisting of Zeta Ceti, Iota Ceti, Theta Ceti, Eta Ceti, Tau Ceti and 57 Ceti.[6] Consequently, the Chinese name for Zeta Ceti itself is Chinese: 天倉四 (Chinese: Tiān Cāng sì, English: the Fourth Star of Square Celestial Granary).[7]

Properties

Zeta Ceti is a single-lined spectroscopic binary system with an orbital period of 4.5 years and an eccentricity of 0.59. The primary, Baten Kaitos, is an evolved K-type giant star with a stellar classification of . The suffix notation indicates this is a weak barium star, showing slightly stronger than normal lines of singly-ionized barium. This star has an estimated 2.34 times the mass of the Sun and, at an estimated age of 1.24 billion years, has expanded to 25 times the Sun's radius.

HD 11366 (WDS J01515-1020B), of spectral type K0 III, is further away (419 parsecs, compared to WDS J01515-1020A's 72 parsecs), and is therefore not a member of the system but a chance alignment - this is referred to as an optical companion.[8]

Notes and References

  1. Web site: Washington Double Star Catalog . United States Naval Observatory . 23 February 2018.
  2. Book: Kunitzsch . Paul . Smart . Tim . 2006 . 2nd rev. . A Dictionary of Modern star Names: A Short Guide to 254 Star Names and Their Derivations . Sky Pub . Cambridge, Massachusetts . 978-1-931559-44-7.
  3. On the naming convention used for multiple star systems and extrasolar planets . 2010 . 1012.0707 . astro-ph.SR . Hessman . F. V. . Dhillon . V. S. . Winget . D. E. . Schreiber . M. R. . Horne . K. . Marsh . T. R. . Guenther . E. . Schwope . A. . Heber . U. .
  4. Web site: WG Triennial Report (2015-2018) - Star Names . 5 . 2018-07-14.
  5. [Eta Ceti]
  6. 中國星座神話, written by 陳久金. Published by 台灣書房出版有限公司, 2005, .
  7. 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.
  8. News: HD 11366. 2018-09-23.