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31 Boötis

From Wikipedia, the free encyclopedia
Star in the constellation Boötes
31 Boötis
Observation data
Epoch J2000      Equinox J2000
ConstellationBoötes
Right ascension14h 41m 38.75049s[1]
Declination+08° 09′ 42.3409″[1]
Apparent magnitude (V)4.86[2]
Characteristics
Spectral typeG7 IIIa[3]
B−Vcolor index0.992±0.038[2]
Astrometry
Radial velocity (Rv)−16.5±1.8[2] km/s
Proper motion (μ)RA: −9.589[1]mas/yr
Dec.: +3.906[1]mas/yr
Parallax (π)6.8757±0.2796 mas[1]
Distance470 ± 20 ly
(145 ± 6 pc)
Absolute magnitude (MV)−1.22[2]
Details
Mass3.27[4] M
Radius23.25+0.40
−0.49
[1] R
Luminosity274.9±12.6[1] L
Surface gravity (log g)2.60[5] cgs
Temperature4,874+53
−41
[1] K
Metallicity[Fe/H]−0.10[5] dex
Rotational velocity (v sin i)6.5[6] km/s
Age370[4] Myr
Other designations
31 Boo,NSV 6769,BD+08°2903,FK5 3163,GC 19789,HD 129312,HIP 71832,HR 5480,SAO 120601[7]
Database references
SIMBADdata

31 Boötis is a single[8]star in the northernconstellation ofBoötes,[7] located 470 light years from the Sun.[1] It is visible to the naked eye as a faint, yellow-hued star with anapparent visual magnitude of 4.86.[2] The object is moving closer to the Earth with a heliocentricradial velocity of −16.5 km/s.[2] It was known to be part of a constellation between Virgo and Boötes namedMons Maenalus, it was also the brightest star in the constellation.

This is anevolvedgiant star with astellar classification of G7 IIIa.[3] It is a suspectedvariable star of unknown type,[9] and is anX-ray source.[10] The star is 370[4] million years old with 3.27[4] times themass of the Sun. Having exhausted the hydrogen at its core, the star has expanded to 23[1] times theSun's radius. It is radiating 275[1] times theluminosity of the Sun from its swollenphotosphere at aneffective temperature of 4,874 K.[1]

References

[edit]
  1. ^abcdefghijklBrown, A. G. A.; et al. (Gaia collaboration) (August 2018)."Gaia Data Release 2: Summary of the contents and survey properties".Astronomy & Astrophysics.616. A1.arXiv:1804.09365.Bibcode:2018A&A...616A...1G.doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source atVizieR.
  2. ^abcdefAnderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation",Astronomy Letters,38 (5): 331,arXiv:1108.4971,Bibcode:2012AstL...38..331A,doi:10.1134/S1063773712050015,S2CID 119257644.
  3. ^abKeenan, Philip C.; McNeil, Raymond C. (1989), "The Perkins Catalog of Revised MK Types for the Cooler Stars",The Astrophysical Journal Supplement Series,71: 245,Bibcode:1989ApJS...71..245K,doi:10.1086/191373.
  4. ^abcdLuck, R. Earle (2015), "Abundances in the Local Region. I. G and K Giants",Astronomical Journal,150 (3), 88,arXiv:1507.01466,Bibcode:2015AJ....150...88L,doi:10.1088/0004-6256/150/3/88,S2CID 118505114.
  5. ^abHekker, S.; Meléndez, J. (2007), "Precise radial velocities of giant stars. III. Spectroscopic stellar parameters",Astronomy and Astrophysics,475 (3): 1003,arXiv:0709.1145,Bibcode:2007A&A...475.1003H,doi:10.1051/0004-6361:20078233,S2CID 10436552.
  6. ^De Medeiros, J. R.; et al. (November 2000), "Rotation and lithium in single giant stars",Astronomy and Astrophysics,363:239–243,arXiv:astro-ph/0010273,Bibcode:2000A&A...363..239D.
  7. ^ab"31 Boo".SIMBAD.Centre de données astronomiques de Strasbourg. RetrievedMay 10, 2019.
  8. ^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,arXiv:0806.2878,Bibcode:2008MNRAS.389..869E,doi:10.1111/j.1365-2966.2008.13596.x,S2CID 14878976.
  9. ^Samus, N. N.; et al. (2017), "General Catalogue of Variable Stars",Astronomy Reports, 5.1,61 (1):80–88,Bibcode:2017ARep...61...80S,doi:10.1134/S1063772917010085,S2CID 125853869.
  10. ^Haakonsen, Christian Bernt; Rutledge, Robert E. (September 2009), "XID II: Statistical Cross-Association of ROSAT Bright Source Catalog X-ray Sources with 2MASS Point Source Catalog Near-Infrared Sources",The Astrophysical Journal Supplement,184 (1):138–151,arXiv:0910.3229,Bibcode:2009ApJS..184..138H,doi:10.1088/0067-0049/184/1/138,S2CID 119267456.

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