Mu Draconis

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μ Draconis
Draco constellation map.svg
Red circle.svg
Location of μ Draconis (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Draco
Right ascension 17h 05m 20.12403s[1]
Declination +54° 28′ 12.0994″[1]
Apparent magnitude (V) 4.92[2]
(5.66 / 5.69)[3]
Spectral type F7V
U−B color index −0.01[4]
B−V color index +0.47[4]
Radial velocity (Rv) −17.30 ± 0.5[5] km/s
Proper motion (μ) RA: −58.16[1] mas/yr
Dec.: 67.87[1] mas/yr
Parallax (π) 36.45 ± 0.46[1] mas
Distance 89 ± 1 ly
(27.4 ± 0.3 pc)
Absolute magnitude (MV) +2.73[6]
Primary μ Dra A
Companion μ Dra B
Period (P) 812.0 ± 70.5 yr
Semi-major axis (a) 4.48 ± 0.03″
Eccentricity (e) 0.5139 ± 0.029
Inclination (i) 142.2 ± 1.3°
Longitude of the node (Ω) 282.85 ± 0.80°
Periastron epoch (T) 1946.19 ± 0.72
Argument of periastron (ω)
193.31 ± 0.083°
μ Dra A
Mass 1.35[7] M
Metallicity [Fe/H] −0.01[6] dex
μ Dra B
Mass 1.30[7] M
Age 2.2[6] Gyr
Other designations
21 Draconis, GJ 9584, BD+54° 1857, SAO 30239, HIP 83608
A: Alrakis, HR 6370, HD 154906
B: HR 6369, HD 154905
Database references
μ Dra A
μ Dra B

Mu Draconis (μ Draconis, abbreviated Mu Dra, μ Dra) is a multiple star system near the head of the constellation of Draco. With a combined magnitude of 4.92,[2] it is visible to the naked eye. Based on parallax estimates by the Hipparcos spacecraft, it is located approximately 89 light-years from the Sun.[1]

The system consists of a single primary star (designated Mu Draconis A, also named Arrakis[8]), a secondary binary pair (Mu Draconis B) and a further single star (C). B's two components are designated Mu Draconis Ba and Bb.

Mu Draconis A and Ba are nearly identical F-type main-sequence stars, with masses of 1.35 M and 1.30 M, respectively.[7] Both have the spectral class of F5V, and have similar apparent magnitude, at 5.66 and 5.69, respectively.[3] The secondary, Mu Draconis B, has a drifting radial velocity, and is itself a spectroscopic binary with an orbital period of 2,270 days.[9] The smaller component, Mu Draconis Bb, has a mass of 0.2 M. Mu Draconis C is a 14th magnitude common-proper-motion companion 13.2" away from the bright pair, with a mass of 0.29 M.[7]


μ Draconis (Latinised to Mu Draconis) is the star's Bayer designation. The designations of the three constituents as Mu Draconis A, B and C, and those of B's components - Mu Draconis Ba and Bb - derive from the convention used by the Washington Multiplicity Catalog (WMC) for multiple star systems, and adopted by the International Astronomical Union (IAU).[10]

It bore the traditional name Alrakis (also written as Arrakis and Errakis), which is derived from name given to it in Arabic by Arabian stargazers, al-Rāqiṣ, "the Trotting Camel"[11][12] or "the Dancer".[13][12] In 2016, the International Astronomical Union organized a Working Group on Star Names (WGSN)[14] to catalogue and standardize proper names for stars. The WGSN approved the name Alrakis for the component Mu Draconis A on February 1, 2017 and it is now so included in the List of IAU-approved Star Names.[8]

This star, along with Beta Draconis (Rastaban), Gamma Draconis (Eltanin), Nu Draconis ('Kuma') and Xi Draconis (Grumium) were Al ʽAwāïd "the Mother Camels", which was later known as the Quinque Dromedarii.[15]

Cultural references[edit]

Science fiction writer Frank Herbert chose Arrakis as the name of the primary planet in his famous Dune series of novels, aware that the word "Arrakis" is the transliteration into English of the Arabic words for "the Dancer" (al-Raqis). However, Herbert uses the name not to describe Mu Draconis A, but the fictional planet Arrakis as the third planet of the star Canopus (α Carinae) in the constellation Carina.[citation needed]


  1. ^ a b c d e f van Leeuwen, F.; et al. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics. 474 (2): 653–664. arXiv:0708.1752Freely accessible. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357. 
  2. ^ a b "* mu Dra". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 16 May 2017. 
  3. ^ a b c "Sixth Catalog of Orbits of Visual Binary Stars". United States Naval Observatory. Retrieved 16 May 2017. 
  4. ^ a b Mermilliod, J.-C. (1986). "Compilation of Eggen's UBV data, transformed to UBV (unpublished)". Catalogue of Eggen's UBV data. Bibcode:1986EgUBV........0M. 
  5. ^ Holmberg, J.; Nordström, B.; Andersen, J. (2007). "The Geneva-Copenhagen survey of the Solar neighbourhood II". Astronomy and Astrophysics. 475 (2): 519. arXiv:0707.1891Freely accessible. Bibcode:2007A&A...475..519H. doi:10.1051/0004-6361:20077221. 
  6. ^ a b c Holmberg, J.; Nordström, B.; Andersen, J. (2009). "The Geneva-Copenhagen survey of the solar neighbourhood. III. Improved distances, ages, and kinematics". Astronomy and Astrophysics. 501 (3): 941. arXiv:0811.3982Freely accessible. Bibcode:2009A&A...501..941H. doi:10.1051/0004-6361/200811191. 
  7. ^ a b c d Tokovinin, Andrei (2014). "From Binaries to Multiples. II. Hierarchical Multiplicity of F and G Dwarfs". The Astronomical Journal. 147 (4): 87. arXiv:1401.6827Freely accessible. Bibcode:2014AJ....147...87T. doi:10.1088/0004-6256/147/4/87. 
  8. ^ a b "Naming Stars". Retrieved 16 December 2017. 
  9. ^ Pourbaix, D.; et al. (2004). "SB9: The ninth catalogue of spectroscopic binary orbits". Astronomy and Astrophysics. 424 (2): 727. arXiv:astro-ph/0406573Freely accessible. Bibcode:2004A&A...424..727P. doi:10.1051/0004-6361:20041213.  (SB9 catalog entry)
  10. ^ Hessman, F. V.; Dhillon, V. S.; Winget, D. E.; Schreiber, M. R.; Horne, K.; Marsh, T. R.; Guenther, E.; Schwope, A.; Heber, U. (2010). "On the naming convention used for multiple star systems and extrasolar planets". arXiv:1012.0707Freely accessible [astro-ph.SR]. 
  11. ^ Kunitzsch, P.; Smart, T. (2006). A Dictionary of Modern star Names: A Short Guide to 254 Star Names and Their Derivations (2nd rev. ed.). Cambridge, MA: Sky Pub. p. 35. ISBN 978-1-931559-44-7. 
  12. ^ a b Allen, R. H. (1963). Star Names: Their Lore and Meaning (rep. ed.). New York, NY: Dover Publications Inc. p. 211. ISBN 0-486-21079-0. 
  13. ^ Davis Jr., G. A. (1971). Pronunciations, Derivations, and Meanings of a Selected List of Star Names (rep. ed.). Cambridge, Massachusetts: Sky Pub. Corp. p. 13. 
  14. ^ "International Astronomical Union | IAU". Retrieved 2017-03-31. 
  15. ^ Allen, R. H. (1963). Star Names: Their Lore and Meaning (Reprint ed.). New York, NY: Dover Publications Inc. p. 207. ISBN 0-486-21079-0. Retrieved 2010-12-12.