Astronomy:Lambda Draconis

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Short description: Star in the constellation Draco
λ Draconis
Draco constellation map.svg
Red circle.svg
Location of λ Draconis (circled)
Observation data
Equinox J2000.0]] (ICRS)
Constellation Draco
Right ascension  11h 31m 24.22075s[1]
Declination +69° 19′ 51.8696″[1]
Apparent magnitude (V) +3.85[2]
Characteristics
Evolutionary stage asymptotic giant branch[3]
Spectral type M0III-IIIa Ca1[4]
U−B color index +1.97[2]
B−V color index +1.62[2]
Variable type slow irregular[5]
Astrometry
Radial velocity (Rv)+6.58±0.30[6] km/s
Proper motion (μ) RA: −40.97[1] mas/yr
Dec.: −19.19[1] mas/yr
Parallax (π)9.79 ± 0.15[1] mas
Distance333 ± 5 ly
(102 ± 2 pc)
Absolute magnitude (MV)−1.14±0.033[7]
Details
Mass1.7[8] M☉
Radius71[9] R☉
Luminosity834[10] L☉
Surface gravity (log g)1.10±0.05[11] cgs
Temperature3,958[10] K
Other designations
λ Dra, 1 Draconis, BD−70° 665, FK5 433, HD 100029, HIP 56211, HR 4434, SAO 15532[12]
Database references
SIMBADdata

Lambda Draconis (λ Draconis, abbreviated Lam Dra, λ Dra), also named Giausar (/ˈdʒɔːzɑːr/ JAW-zar),[13][14] is a solitary,[15] orange-red[16] star in the northern circumpolar constellation of Draco. It is visible to the naked eye with an apparent visual magnitude of +3.85.[2] Based upon an annual parallax shift of 9.79 mas as seen from the Earth,[1] the star is located around 333 light years from the Sun.

This is an evolved red giant star on the asymptotic giant branch[3] with a stellar classification of M0III-IIIa Ca1.[4] It is a suspected slow irregular variable with a periodicity of roughly 1,100 days.[5] The measured angular diameter, after correction for limb darkening, is 6.43±0.07 mas.[17] At the estimated distance of the star, this yields a physical size of about 53 times the radius of the Sun.[9] It has an estimated 1.7[8] times the mass of the Sun and is radiating 834 times the solar luminosity from its photosphere at an effective temperature of 3,958 K.[10]

Nomenclature

λ Draconis (Latinised to Lambda Draconis) is the star's Bayer designation.

It bore the traditional name Giausar[18] (also written as Gianfar, Giansar and Giauzar) and Juza. In 2016, the International Astronomical Union organized a Working Group on Star Names (WGSN)[19] to catalogue and standardize proper names for stars. The WGSN approved the name Giausar for this star on February 1, 2017 and it is now so included in the List of IAU-approved Star Names.[14]

In Chinese, 紫微右垣 (Zǐ Wēi Yòu Yuán), meaning Right Wall of Purple Forbidden Enclosure, refers to an asterism consisting of Lambda Draconis, Alpha Draconis, Kappa Draconis, 24 Ursae Majoris, 43 Camelopardalis, Alpha Camelopardalis and BK Camelopardalis.[20] Consequently, the Chinese name for Lambda Draconis itself is 紫微右垣三 (Zǐ Wēi Yòu Yuán sān, English: the Third Star of Right Wall of Purple Forbidden Enclosure.),[21] representing 上輔 (Shǎngfǔ), meaning First Minister.[22] 上輔 (Shǎngfǔ) was westernized into Sang Poo or Shaou Poo by R.H. Allen.[23]

Namesakes

USS Giansar (AK-111) was a United States Navy Crater class cargo ship named after the star.

References

  1. ↑ 1.0 1.1 1.2 1.3 1.4 1.5 van Leeuwen, F. (2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics 474 (2): 653–664, doi:10.1051/0004-6361:20078357, Bibcode: 2007A&A...474..653V. 
  2. ↑ 2.0 2.1 2.2 2.3 Johnson, H. L. et al. (1966), "UBVRIJKL photometry of the bright stars", Communications of the Lunar and Planetary Laboratory 4 (99): 99, Bibcode: 1966CoLPL...4...99J. 
  3. ↑ 3.0 3.1 Eggen, O. J. (1992). "Asymptotic giant branch stars near the sun". The Astronomical Journal 104: 275. doi:10.1086/116239. Bibcode: 1992AJ....104..275E. 
  4. ↑ 4.0 4.1 Keenan, Philip C.; McNeil, Raymond C. (1989), "The Perkins catalog of revised MK types for the cooler stars", Astrophysical Journal Supplement Series 71: 245, doi:10.1086/191373, Bibcode: 1989ApJS...71..245K. 
  5. ↑ 5.0 5.1 Samus, N. N.; Durlevich, O. V. et al. (2007), Combined General Catalogue of Variable Stars (GCVS4.2), http://www.sai.msu.su/gcvs/gcvs/, retrieved 2016-09-30. 
  6. ↑ Famaey, B. et al. (2009), "Spectroscopic binaries among Hipparcos M giants,. I. Data, orbits, and intrinsic variations", Astronomy and Astrophysics 498 (2): 627–640, doi:10.1051/0004-6361/200810698, Bibcode: 2009A&A...498..627F. 
  7. ↑ Park, Sunkyung et al. (2013), "Wilson-Bappu Effect: Extended to Surface Gravity", The Astronomical Journal 146 (4): 73, doi:10.1088/0004-6256/146/4/73, Bibcode: 2013AJ....146...73P. 
  8. ↑ 8.0 8.1 Gondoin, P. (December 1999), "Evolution of X-ray activity and rotation on G-K giants", Astronomy and Astrophysics 352: 217–227, Bibcode: 1999A&A...352..217G. 
  9. ↑ 9.0 9.1 Lang, Kenneth R. (2006), Astrophysical formulae, Astronomy and astrophysics library, 1 (3rd ed.), Birkhäuser, ISBN 3-540-29692-1, https://books.google.com/books?id=OvTjLcQ4MCQC&pg=PA41.  The radius (R*) is given by:
    [math]\displaystyle{ \begin{align} 2\cdot R_* & = \frac{(102.1\cdot 6.43\cdot 10^{-3})\ \text{AU}}{0.0046491\ \text{AU}/R_{\bigodot}} \\ & \approx 141.2\cdot R_{\bigodot} \end{align} }[/math]
  10. ↑ 10.0 10.1 10.2 McDonald, I. et al. (2012), "Fundamental parameters and infrared excesses of Hipparcos stars", Monthly Notices of the Royal Astronomical Society 427 (1): 343–357, doi:10.1111/j.1365-2966.2012.21873.x, Bibcode: 2012MNRAS.427..343M. 
  11. ↑ Takagi, Yuhei et al. (June 2011), "Age Determinations of Early-M Type Pre-Main Sequence Stars Using a High-Resolution Near-Infrared Spectroscopic Method", Publications of the Astronomical Society of Japan 63 (3): 677–684, doi:10.1093/pasj/63.3.677, Bibcode: 2011PASJ...63..677T. 
  12. ↑ "lam Dra". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=lam+Dra. 
  13. ↑ Kunitzsch, Paul; Smart, Tim (2006). A Dictionary of Modern star Names: A Short Guide to 254 Star Names and Their Derivations (2nd rev. ed.). Cambridge, Massachusetts: Sky Pub. ISBN 978-1-931559-44-7. 
  14. ↑ 14.0 14.1 "Naming Stars". IAU.org. https://www.iau.org/public/themes/naming_stars/. Retrieved 16 December 2017. 
  15. ↑ Eggleton, P. P.; Tokovinin, A. A. (September 2008), "A catalogue of multiplicity among bright stellar systems", Monthly Notices of the Royal Astronomical Society 389 (2): 869–879, doi:10.1111/j.1365-2966.2008.13596.x, Bibcode: 2008MNRAS.389..869E. 
  16. ↑ Moore, Patrick (2013), The Observer's Year: 366 Nights of the Universe, The Patrick Moore Practical Astronomy Series, Springer Science & Business Media, p. 285, ISBN 978-1447136132, https://books.google.com/books?id=p87TBwAAQBAJ&pg=PA182 
  17. ↑ Richichi, A. et al. (February 2005), "CHARM2: An updated Catalog of High Angular Resolution Measurements", Astronomy and Astrophysics 431 (2): 773–777, doi:10.1051/0004-6361:20042039, Bibcode: 2005A&A...431..773R. 
  18. ↑ Kaler, James B., Giausar, http://stars.astro.illinois.edu/sow/giausar.html, retrieved 2017-05-28. 
  19. ↑ "International Astronomical Union | IAU". https://www.iau.org/science/scientific_bodies/working_groups/280/. 
  20. ↑ (in Chinese) 中國星座神話, written by 陳久金. Published by 台灣書房出版有限公司, 2005, ISBN:978-986-7332-25-7.
  21. ↑ (in Chinese) 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.
  22. ↑ English-Chinese Glossary of Chinese Star Regions, Asterisms and Star Name , Hong Kong Space Museum. Accessed on line November 23, 2010.
  23. ↑ Allen, Richard Hinckley (1963), Star Names — Their Lore and Meaning: Draco, the Dragon, https://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Draco*.html, retrieved 2017-05-28. 




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