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Omega² Scorpio

Omega 2 Scorpio ( ω 2 Scorpii , ω 2 Sco ) is a star in the zodiac constellation Scorpio . Probably [10] is a variable star. It is a component of the visual double star Omega Scorpio; bright enough to be visible to the naked eye: the apparent magnitude is of +4.320. [2] The distance to this star estimated by the parallax measurement method [1] is about 291 light years . The apparent stellar magnitude of this star changes by 0.38 due to extinction by interstellar dust . [five]

Omega 2 Scorpio
Star
Observational data
( Age J2000 )
Right ascension16 h 07 m 24.32818 s [1]
Declination-20 ° 52 ′ 07.5518 ″ [1]
Distance
Visible magnitude ( V )+4,320 [2]
Constellation
Astrometry
Radial velocity ( R v )−5.4 [3] km / s
Own movement (μ)RA: +44.81 [1]
Dec: −45.42 [1]
Parallax (π)11.22 ± 0.32 [1] mas
Absolute magnitude (V)−0.62 [5]
Specifications
Spectral classG6 / 8III [6]
Color Index ( B - V )+0.850 [2]
Color Index ( U - B )+0.494 [2]
physical characteristics
Weight3.27 [5] M ☉
Radius15,6 [7] R ☉
Age282 [5] million years
Temperature5363 ± 42 [8] K
Luminosity141 [9] L ☉
Metallicity+0.03 ± 0.05 [8]
Other designations
Jabhat al Akrab, ω 2 Sco , 10 Scorpii, BD −20 ° 4408 , HD 144608, HIP 78990, HR 5997, SAO 184135.
Database Information
SIMBADdata

Omega 2 Scorpio is a giant star of the spectral class G: G6 / 8III. [6] The age is estimated at 282 Ma, [5] the star is in the late stages of evolution, belongs to a thin disk and is at the stage of a horizontal branch . [11] The angular diameter of the star, measured by interferometry methods, is 1.63 ± 0.10 mas , [12] which, at a known distance from the object, corresponds to a radius 16 times greater than the solar one. [7] The mass exceeds the solar 3.27 times, [5] the luminosity is equal to 141 luminosity of the Sun. [9] The effective temperature of the outer part of the atmosphere is 5363 K. [eight]


Notes

  1. ↑ 1 2 3 4 5 6 van Leeuwen, F. (2007), " Validation of the new Hipparcos reduction ", Astronomy and Astrophysics T. 474 (2): 653–664 , DOI 10.1051 / 0004-6361: 20078357  
  2. ↑ 1 2 3 4 Kozok, JR (September 1985), "Photometric observations of emission B-stars in the southern Milky Way", Astronomy and Astrophysics Supplement Series T. 61: 387–405  
  3. ↑ Wilson, RE (1953), General Catalog of Stellar Radial Velocities , Carnegie Institute of Washington DC  
  4. ↑ 1 2 3 4 5 Gaia Data Release 2 - 2018.
    <a href=" https://wikidata.org/wiki/Track:Q51905050 "> </a>
  5. ↑ 1 2 3 4 5 6 Takeda, Yoichi; Sato, Bun'ei & Murata, Daisuke (August 2008), " Stellar Parameters and Elemental Abundances of Late-G Giants ", Publications of the Astronomical Society of Japan T. 60 (4): 781–802 , DOI 10.1093 / pasj / 60.4.781  
  6. ↑ 1 2 Houk, N. & Smith-Moore, M. (1988), Michigan Catalog of Two-dimensional Spectral Types for the HD Stars. Declinations -26 ° .0 to -12 ° .0 , vol. four  
  7. ↑ 1 2 Lang, Kenneth R. (2006), Astrophysical formulae , vol. 1 (3 ed.), Astronomy and astrophysics library, Birkhäuser, ISBN 3-540-29692-1 , < https://books.google.com/books?id=OvTjLcQ4MCQC&pg=PA41 >   . The value of the radius (R * ) is given by
    2⋅R∗=(89⋅1.63⋅ten-3)a.e.0.0046491a.e./R⨀≈31.2⋅R⨀{\ displaystyle {\ begin {aligned} 2 \ cdot R _ {*} & = {\ frac {(89 \ cdot 1.63 \ cdot 10 ^ {- 3}) \ {\ text {AU}}} {0.0046491 \ {\ text {AU}} / R _ {\ bigodot}}} \\ & \ approx 31.2 \ cdot R _ {\ bigodot} \ end {aligned}}}  
  8. ↑ 1 2 3 Prugniel, P .; Vauglin, I. & Koleva, M. (2011), " The atmospheric parameters and spectral interpolator for the MILES stars ", Astronomy & Astrophysics T. 531: A165 , DOI 10.1051 / 0004-6361 / 201116769  
  9. ↑ 1 2 McDonald, I .; Zijlstra, AA & Boyer, ML (2012), " Fundamental Parameters and Infrared Excesses of Hipparcos Stars ", Monthly Notices of the Royal Astronomical Society T. 427 (1): 343–57 , DOI 10.1111 / j.1365-2966.2012.21873 .x  
  10. ↑ Sterken, C. (January 1977), "uvby Photometry of the Suspected Variable omega2 Sco", Information Bulletin on Variable Stars T. 1230: 1  
  11. ↑ Afşar, M .; Sneden, C. & For, B.-Q. (July 2012), " Chemical Compositions of Thin-disk, High-metallicity Red Horizontal-branch Field Stars ", The Astronomical Journal T. 144 (1): 20, 20 , DOI 10.1088 / 0004-6256 / 144/1/20  
  12. ↑ Richichi, A. & Percheron, I. (May 2002), " CHARM: A Catalog of High Angular Resolution Measurements ", Astronomy and Astrophysics T. 386: 492-503 , DOI 10.1051 / 0004-6361: 20020236  

Links

  • Kaler, James B. (September 9, 2016), Omega-1 and Omega-2 Scorpii , University of Illinois , < http://stars.astro.illinois.edu/sow/omegasco.html > . Retrieved September 26, 2016.  
Source - https://ru.wikipedia.org/w/index.php?title=Omega²_Scorpion&oldid=90673486


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