Epsilon Scorpii Explained

Epsilon Scorpii (ε Scorpii, abbreviated Eps Sco, ε Sco), formally named Larawag,[1] is a star in the southern zodiac constellation of Scorpius. It has an apparent visual magnitude of +2.3, making it the fifth-brightest member of the constellation. Parallax measurements made during the Hipparcos mission provide an estimated distance to this star of around 63.7abbr=offNaNabbr=off from the Sun.

Epsilon Scorpii has a stellar classification of K1 III, which indicates it has exhausted the supply of hydrogen at its core and evolved into a giant star. Currently, it has expanded to 15.5 times the Sun's size and is emitting 54 times its luminosity. Presently it is generating energy through the nuclear fusion of helium at its core, which, considering the star's composition, places it along an evolutionary branch termed the red clump. The star's outer atmosphere has an effective temperature of 4,580 K, giving it the orange hue of a cool K-type star.

ε Scorpii is classified as a suspected variable star, although a study of Hipparcos photometry showed a variation of no more than 0.01–0.02 magnitudes. It is an X-ray source with a luminosity of .

Nomenclature

ε Scorpii (Latinised to Epsilon Scorpii) is the star's Bayer designation.

The star bore the traditional name Larawag in the culture of the Wardaman people of the Northern territory of Australia,[2] meaning clear sighting.[3] In 2016, the IAU organized a Working Group on Star Names (WGSN)[4] to catalog and standardize proper names for stars. The WGSN approved the name Larawag for Epsilon Scorpii on 19 November 2017 and it is now so included in the List of IAU-approved Star Names.[1]

Patrick Moore introduced the name Wei as Chinese name for this star. However, this seems to be a misreading, as Chinese Chinese: 尾宿 (Chinese: Wěi Xiù, English Tail) refers to an asterism (i.e. Chinese constellation) consisting of Epsilon Scorpii, Mu¹ Scorpii, Zeta¹ Scorpii and Zeta² Scorpii, Eta Scorpii, Theta Scorpii, Iota² Scorpii and Iota¹ Scorpii, Kappa Scorpii, Lambda Scorpii and Upsilon Scorpii.[5] Consequently, the name for Epsilon Scorpii itself is Chinese: 尾宿二 (Chinese: Wěi Xiù èr), which means "the Second Star of Tail".[6] [7]

In culture

Epsilon Scorpii appears on the flag of Brazil, symbolising the state of Ceará.[8]

Notes and References

  1. Web site: Naming Stars . IAU.org . 16 December 2017.
  2. IAU Approves 86 New Star Names From Around the World . IAU.org . 11 December 2017.
  3. IAU Working Group on Star Names (WGSN) . IAU.org.
  4. Web site: IAU Working Group on Star Names (WGSN). 22 May 2016.
  5. 中國星座神話, written by 陳久金. Published by 台灣書房出版有限公司, 2005, .
  6. 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.
  7. [Ian Ridpath|Ridpath, Ian]
  8. Web site: Astronomy of the Brazilian Flag . FOTW Flags Of The World website .