Delta Draconis Explained

Delta Draconis (δ Draconis, abbreviated Delta Dra, δ Dra), formally named Altais,[1] is a yellow star in the constellation of Draco. It has an apparent visual magnitude of 3.0, making it easily visible to the naked eye. Based on parallax measurements obtained during the Hipparcos mission, it is approximately 97.4abbr=offNaNabbr=off from the Sun.

Nomenclature

δ Draconis (Latinised to Delta Draconis) is the star's Bayer designation.

It bore the traditional names Aldib, Altais (the goat) and Nodus Secundus. The title Altais was derived from Arabic Al Tāis "the Goat", the association of this star, along with Pi Draconis, Rho Draconis and Epsilon Draconis (Tyl). According to a 1971 NASA catalog of stars, Al Tāis or Tais were the title for three stars : Delta Draconis as Altais, Pi Draconis as Tais I and Rho Draconis as Tais II (exclude Epsilon Draconis). In 2016, the International Astronomical Union organized a Working Group on Star Names (WGSN) to catalogue and standardize proper names for stars. The WGSN approved the name Altais for this star on 21 August 2016 and it is now so included in the List of IAU-approved Star Names.[1]

In Chinese, Chinese: 天廚 (Chinese: Tiān Chú, Tien Choo), meaning Celestial Kitchen or Heaven's Kitchen, refers to an asterism consisting of Delta Draconis, Sigma Draconis, Epsilon Draconis, Rho Draconis, 64 Draconis and Pi Draconis.[2] Consequently, the Chinese name for Delta Draconis itself is Chinese: 天廚一 (Chinese: Tiān Chú yī, English: the First Star of Celestial Kitchen).[3]

Properties

Delta Draconis is a giant star with a stellar classification of G9 III. This indicates that, at an estimated age of 800 million years, it has exhausted the supply of hydrogen at its core and entered a later stage in its evolution. The angular diameter of the star is estimated as . At a parallax of 32.54 mas, this corresponds to a physical radius equal to 11 times the solar radius. It is radiating 59 times the luminosity of the Sun from its outer atmosphere at an effective temperature of 4,820 K. At this temperature, it is giving off the yellow-hued glow of a G-type star. With a mass 2.32 times that of the Sun, this star will end its life as a white dwarf.

Pole star

Delta Draconis is the northern pole star of Ceres, lying 1.5 degrees from the true pole.[4]

Notes and References

  1. Web site: Naming Stars . IAU.org . 4 March 2018.
  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.
  4. Web site: Dawn explores Ceres: Results from the survey orbit . 2017-03-30 . 2015-09-05 . https://web.archive.org/web/20150905125337/http://nesf2015.arc.nasa.gov/sites/default/files/downloads/pdf/05.pdf . dead .