Back رأس الثعبان (نجم) Arabic Alwaid AST Beta Əjdaha Azerbaijani Alwaid Czech Alwaid German Ρασταμπάν Greek Alwaid Spanish بتا اژدها Persian Beta Draconis French רסטבן HE

Beta Draconis

β Draconis
Location of β Draconis (circled)
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Draco
Right ascension 17h 30m 25.96170s[1]
Declination +52° 18′ 04.9993″[1]
Apparent magnitude (V) 2.79[2]
Characteristics
Spectral type G2Ib-IIa[3]
U−B color index +0.954±0.007[4]
B−V color index +0.98[5]
R−I color index +0.48[5]
Astrometry
Radial velocity (Rv)−21.00±0.23[4] km/s
Proper motion (μ) RA: −15.89[1] mas/yr
Dec.: +12.28[1] mas/yr
Parallax (π)8.58 ± 0.10 mas[1]
Distance380 ± 4 ly
(117 ± 1 pc)
Absolute magnitude (MV)–2.457[6]
Details
Mass6.0±0.2[2] M☉
Radius40[7] R☉
Luminosity996[7] L☉
Surface gravity (log g)1.86±0.04[8] cgs
Temperature5,160±150[8] K
Metallicity [Fe/H]0.02±0.10[8] dex
Rotational velocity (v sin i)10.7[8] km/s
Age65[2] Myr
Other designations
Rastaban, Rastaben, Alwaid, Asuia, NGCA-V25, β Dra, 23 Dra, BD+52°2065, FK5 653, HD 159181, HIP 85670, HR 6536, SAO 30429, ADS 10611, WDS 17304+5218AB[9]
Database references
SIMBADdata

Beta Draconis (β Draconis, abbreviated Beta Dra, β Dra) is a binary star system[10] and the third-brightest star in the northern circumpolar constellation of Draco. The two components are designated Beta Draconis A (officially named Rastaban /ˈræstəbæn/, “head to sole of foot”, the traditional name of the system)[11] and B respectively. With a combined apparent visual magnitude of 2.79,[2] it is bright enough to be easily seen with the naked eye. Based upon parallax measurements from the Hipparcos astrometry satellite,[12][13] it lies at a distance of about 380 light-years (120 parsecs) from the Sun.[1] The system is drifting closer with a radial velocity of −21 km/s.[4]

The binary system consists of a bright giant orbited by a dwarf companion once every four millennia or so.[14] The companion is about 11 magnitudes fainter than the primary star,[15] and the two are separated by 4.2″.[10]

The spectrum of the primary, Beta Draconis A, matches a stellar classification of G2Ib-IIa,[3] showing mixed features of a bright giant and a supergiant star, and is listed as a standard star for that spectral class.[16] It is about 65 million years old[2] and is currently undergoing its first convective dredge-up.[17] Compared to the Sun, Beta Draconis A is an enormous star with six times the mass and roughly 40 times the radius. At this size, it is emitting about 950 times the luminosity of the Sun from its outer envelope at an effective temperature of 5,160 K,[2] giving it the yellow hue of a G-type star.[18] The star has a particularly strong chromospheric emission that is generating X-ray[19][20] and far-UV radiation.[21] There is a detectable magnetic field with a longitudinal field strength of −1.16±0.25 G.[22]

Beta Draconis lies on or near the cepheid instability strip,[23] yet only appears to be a microvariable with a range of about 1/100th of a magnitude.[24][25] It was confirmed as a variable star with a range of about 1/100th of a magnitude by Gabriel Cristian Neagu using data from the TESS and Hipparcos missions.[24][25] The variability was reported to the AAVSO (American Association of Variable Star Observers), in the Variable Star Index.[26]

  1. ^ a b c d e f Cite error: The named reference aaa474_2_653 was invoked but never defined (see the help page).
  2. ^ a b c d e f Cite error: The named reference mnras402_2_1369 was invoked but never defined (see the help page).
  3. ^ a b Cite error: The named reference keenan1980 was invoked but never defined (see the help page).
  4. ^ a b c Cite error: The named reference Anderson_Francis_2012 was invoked but never defined (see the help page).
  5. ^ a b Cite error: The named reference bsc1 was invoked but never defined (see the help page).
  6. ^ Cite error: The named reference katz2011 was invoked but never defined (see the help page).
  7. ^ a b Cite error: The named reference mcdonald2017 was invoked but never defined (see the help page).
  8. ^ a b c d Cite error: The named reference Marfil_et_al_2020 was invoked but never defined (see the help page).
  9. ^ Cite error: The named reference SIMBAD was invoked but never defined (see the help page).
  10. ^ a b Cite error: The named reference Eggleton_Tokovinin_2008 was invoked but never defined (see the help page).
  11. ^ Cite error: The named reference IAU-LSN was invoked but never defined (see the help page).
  12. ^ Cite error: The named reference aaa323_L49 was invoked but never defined (see the help page).
  13. ^ Cite error: The named reference GSM was invoked but never defined (see the help page).
  14. ^ Cite error: The named reference kaler was invoked but never defined (see the help page).
  15. ^ Cite error: The named reference wds was invoked but never defined (see the help page).
  16. ^ Cite error: The named reference perkins was invoked but never defined (see the help page).
  17. ^ Cite error: The named reference Kovtyukh_et_al_2005 was invoked but never defined (see the help page).
  18. ^ Cite error: The named reference csiro was invoked but never defined (see the help page).
  19. ^ Cite error: The named reference Evans_et_al_2010 was invoked but never defined (see the help page).
  20. ^ Cite error: The named reference Skinner_Brown_1996 was invoked but never defined (see the help page).
  21. ^ Cite error: The named reference Brown_et_al_1984 was invoked but never defined (see the help page).
  22. ^ Cite error: The named reference Grunhut_et_al_2010 was invoked but never defined (see the help page).
  23. ^ Cite error: The named reference Butler1998 was invoked but never defined (see the help page).
  24. ^ a b Cite error: The named reference ricker2014 was invoked but never defined (see the help page).
  25. ^ a b Cite error: The named reference perryman1997 was invoked but never defined (see the help page).
  26. ^ Cite error: The named reference vsx was invoked but never defined (see the help page).

Developed by StudentB