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82 Virginis

From Wikipedia, the free encyclopedia
Star in the constellation Virgo
82 Virginis
Observation data
Epoch J2000      Equinox J2000
ConstellationVirgo
Right ascension13h 41m 36.770s[1]
Declination−08° 42′ 10.73″[1]
Apparent magnitude (V)5.01[2]
Characteristics
Evolutionary stageAGB[3]
Spectral typeM1III
Apparent magnitude (U)8.59[4]
Apparent magnitude (B)6.64[4]
Apparent magnitude (G)4.149[4]
Apparent magnitude (J)1.68[4]
Apparent magnitude (H)0.88[4]
Apparent magnitude (K)0.64[4]
B−Vcolor index1.623±0.009[5]
Astrometry
Radial velocity (Rv)−36.6±2[4] km/s
Proper motion (μ)RA: -91.65mas/yr[5]
Dec.: 40.28mas/yr[5]
Parallax (π)5.4376±0.2897 mas[1]
Distance600 ± 30 ly
(184 ± 10 pc)
Absolute magnitude (MV)−0.7[6]
Details
Mass6.5[7] M
Radius54[1] R
Luminosity812[8] L
Surface gravity (log g)0.714[2] cgs
Temperature3,675[2] K
Rotational velocity (v sin i)2.3±1[9] km/s
Age50[7] Myr
Other designations
m Vir,NSV 6390,BD−07 3674,HD 119149,HIP 66803,HR 5150,SAO 139490,TIC 743613,TYC 5546-1582-1,GSC 05546-01582,IRAS 13389-0827,2MASS J13413677-0842110
Database references
SIMBADdata

82 Virginis, also known asm Virginis, is a star in the constellationVirgo. It is located 160 pc (520light-years) from Earth based on a parallax of6.249±0.2611 mas fromGaia Data Release 3.[1] It is ared giant, based on itsspectral type of M1III.[4] Itsapparent magnitude is 5.01.[2]

Characteristics

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82 Virginis is ared giant star, based on its spectral type of M1III,[4] where M means that it is anM-type star and III is theluminosity class, meaning it is a giant star. The star is 54 times larger than the Sun.[1] Theeffective temperature of the star is3,675 K,[2] which is 2,197 degrees cooler than thesolar temperature of5,772 K. Itsrotational velocity is 2.3 km/s.[9] Theangular diameter of the star, as measured from the CHARM survey, is of4.48±0.28 mas.[10] At the current distance, this would lead to a radius of 77 R, somewhat larger than the radius derived by Gaia DR3.

The parallax of the star is measured at5.4376±0.2897 mas from Gaia DR3, translating to a distance of 184parsecs (600light-years) from Earth.[1] The star is moving towards Earth at a velocity of 36.6 km/s.[4] Itsapparent magnitude is 5.01,[2] making it visible to the naked eye.[a]

Notes

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  1. ^According to theBortle scale

References

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  1. ^abcdefgVallenari, A.; et al. (Gaia collaboration) (2023)."Gaia Data Release 3. Summary of the content and survey properties".Astronomy and Astrophysics.674: A1.arXiv:2208.00211.Bibcode:2023A&A...674A...1G.doi:10.1051/0004-6361/202243940.S2CID 244398875. Gaia DR3 record for this source atVizieR.
  2. ^abcdefGhosh, Supriyo; Mondal, Soumen; Das, Ramkrishna; Khata, Dhrimadri (2019-01-29)."Spectral Calibration of K$-$M Giants from medium resolution near-infrared HK-band spectra".Monthly Notices of the Royal Astronomical Society.arXiv:1901.09170.doi:10.1093/mnras/stz299.ISSN 0035-8711.
  3. ^Eggen, Olin J. (1992). "Asymptotic Giant Branch Stars Near the Sun".The Astronomical Journal.104: 275.Bibcode:1992AJ....104..275E.doi:10.1086/116239.
  4. ^abcdefghij"82 Vir".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2024-05-01.
  5. ^abvan Leeuwen, Floor (13 August 2007)."Validation of the new Hipparcos reduction".Astronomy & Astrophysics.474 (2):653–664.arXiv:0708.1752.Bibcode:2007A&A...474..653V.doi:10.1051/0004-6361:20078357.eISSN 1432-0746.ISSN 0004-6361. Hipparcos record for this source atVizieR.
  6. ^Pace, G.; Pasquini, L.; Ortolani, S. (2003). "The Wilson-Bappu effect: A tool to determine stellar distances".Astronomy and Astrophysics.401 (3): 997.arXiv:astro-ph/0301637.Bibcode:2003A&A...401..997P.doi:10.1051/0004-6361:20030163.
  7. ^abBorisov, Sviatoslav B.; Chilingarian, Igor V.; Rubtsov, Evgenii V.; Ledoux, Cédric; Melo, Claudio; Grishin, Kirill A.; Katkov, Ivan Yu.; Goradzhanov, Vladimir S.; Afanasiev, Anton V.; Kasparova, Anastasia V.; Saburova, Anna S. (2023)."New Generation Stellar Spectral Libraries in the Optical and Near-infrared. I. The Recalibrated UVES-POP Library for Stellar Population Synthesis".The Astrophysical Journal Supplement Series.266 (1): 11.arXiv:2211.09130.Bibcode:2023ApJS..266...11B.doi:10.3847/1538-4365/acc321.
  8. ^McDonald, I.; Zijlstra, A. A.; Boyer, M. L. (2012)."Fundamental parameters and infrared excesses of Hipparcos stars".Monthly Notices of the Royal Astronomical Society.427 (1): 343.arXiv:1208.2037.Bibcode:2012MNRAS.427..343M.doi:10.1111/j.1365-2966.2012.21873.x.
  9. ^abZamanov, R. K.; Bode, M. F.; Melo, C. H. F.; Stateva, I. K.; Bachev, R.; Gomboc, A.; Konstantinova-Antova, R.; Stoyanov, K. A. (2008-10-11)."Rotational velocities of the giants in symbiotic stars: III. Evidence of fast rotation in S-type symbiotics".Monthly Notices of the Royal Astronomical Society.390 (1):377–382.arXiv:0807.3817.Bibcode:2008MNRAS.390..377Z.doi:10.1111/j.1365-2966.2008.13751.x.
  10. ^Richichi, A.; Percheron, I. (2002-05-01)."CHARM: A Catalog of High Angular Resolution Measurements".Astronomy and Astrophysics.386 (2):492–503.Bibcode:2002A&A...386..492R.doi:10.1051/0004-6361:20020236.hdl:1887/7492.ISSN 0004-6361.
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