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32 Boötis

From Wikipedia, the free encyclopedia
Star in the constellation Boötes
32 Boötis
Observation data
Epoch J2000      Equinox J2000
ConstellationBoötes
Right ascension14h 41m 43.52071s[1]
Declination+11° 39′ 38.3820″[1]
Apparent magnitude (V)5.55[2]
Characteristics
Spectral typeG8 III[3]
B−Vcolor index0.941±0.002[2]
Astrometry
Radial velocity (Rv)−23.3±0.3[2] km/s
Proper motion (μ)RA: –159.787[1]mas/yr
Dec.: −112.732[1]mas/yr
Parallax (π)9.0120±0.2578 mas[1]
Distance360 ± 10 ly
(111 ± 3 pc)
Absolute magnitude (MV)0.09[2]
Details
Mass2.15[4] M
Radius12.06+0.09
−0.24
[1] R
Luminosity79.14±2.57[1] L
Surface gravity (log g)2.6±0.3[5] cgs
Temperature4,957.5+50.0
−17.5
[1] K
Metallicity [Fe/H]−23.3±0.3[2] dex
Rotational velocity (v sin i)2.6[6] km/s
Age1.46[4] Gyr
Other designations
32 Boo,BD+12°2729,FK5 1382,HD 129336,HIP 71837,HR 5481,SAO 120601,LTT 14344[7]
Database references
SIMBADdata

32 Boötis is a single[8]star in the northernconstellation ofBoötes,[7] located 360 light years away from the Sun.[1] It is visible to the naked eye as a faint, yellow-hued star with anapparent visual magnitude of 5.55.[2] This object is moving closer to the Earth with a heliocentricradial velocity of −23 km/s.[2] It has a relatively highproper motion, traversing thecelestial sphere at the rate of 0.195 arc seconds per annum.[9]

This is an aginggiant star with astellar classification of G8 III.[3] It is most likely on thehorizontal branch and is a candidatered clump giant.[5] The star is an estimated 1.46[4] billion years old with 2.15[4] times themass of the Sun. With the hydrogen at its core exhausted, it has expanded to 12[1] times theSun's radius. 32 Boötis is radiating 79[1] times theluminosity of the Sun from its swollenphotosphere at aneffective temperature of 4958 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. ^abcdefgAnderson, 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. ^abHarlan, E. A.; Taylor, D. C. (March 1970), "MK classification for F- and G-type stars. II",Astronomical Journal,75 (2):165–166,Bibcode:1970AJ.....75..165H,doi:10.1086/110956
  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. ^abAfşar, M.; et al. (July 2012), "Chemical Compositions of Thin-disk, High-metallicity Red Horizontal-branch Field Stars",The Astronomical Journal,144 (1): 20,arXiv:1205.3659,Bibcode:2012AJ....144...20A,doi:10.1088/0004-6256/144/1/20,S2CID 119249237, 20.
  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"32 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. ^Lépine, Sébastien; Shara, Michael M. (March 2005), "A Catalog of Northern Stars with Annual Proper Motions Larger than 0.15" (LSPM-NORTH Catalog)",The Astronomical Journal,129 (3):1483–1522,arXiv:astro-ph/0412070,Bibcode:2005AJ....129.1483L,doi:10.1086/427854,S2CID 2603568.
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