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Sigma Virginis

From Wikipedia, the free encyclopedia
Star in the constellation Virgo
σ Virginis
Location of σ Virginis (circled)
Observation data
Epoch J2000      Equinox J2000
ConstellationVirgo
Right ascension13h 17m 36.28327s[1]
Declination+05° 28′ 11.5221″[1]
Apparent magnitude (V)4.86[2]
Characteristics
Spectral typeM1 III[3]
U−Bcolor index+1.86[2]
B−Vcolor index+1.62[2]
Variable typesuspected[4]
Astrometry
Radial velocity (Rv)−28.26±0.30[5] km/s
Proper motion (μ)RA: −6.06[1]mas/yr
Dec.: +9.14[1]mas/yr
Parallax (π)4.83±0.19 mas[1]
Distance680 ± 30 ly
(207 ± 8 pc)
Absolute magnitude (MV)−1.80[6]
Details
Radius98[7] R
Luminosity1,610[7] L
Surface gravity (log g)0.42[7] cgs
Temperature3,690[7] K
Other designations
σ Vir,60 Virginis,BD+06°2722,FK5 1344,HD 115521,HIP 64852,HR 5015,SAO 119855[8]
Database references
SIMBADdata

Sigma Virginis (σ Vir, σ Virginis) is astar in thezodiacconstellation ofVirgo. It can be faintly seen with the naked eye with a baselineapparent visual magnitude of 4.86.[2] Based uponparallax measurements, the distance to this star is roughly 680 light-years.

Alight curve for Sigma Virginis, plotted fromHipparcos data[9]

This is an evolvedred giant star with astellar classification of M1 III.[3] It is a suspectedvariable star with a brightness that ranges from magnitude +4.77 to +4.86.[4] This variation has pulsation periods of 23.4, 24.3, 27.9 and 34.1 days.[3] Theeffective temperature of thestellar atmosphere is around 3,800 K, and it shines with 1,734 times theluminosity of the Sun.[7]

References

[edit]
  1. ^abcdevan Leeuwen, F. (November 2007), "Validation of the new Hipparcos reduction",Astronomy and Astrophysics,474 (2):653–664,arXiv:0708.1752,Bibcode:2007A&A...474..653V,doi:10.1051/0004-6361:20078357,S2CID 18759600.
  2. ^abcdMermilliod, J.-C. (1986), "Compilation of Eggen's UBV data, transformed to UBV (unpublished)",Catalogue of Eggen's UBV Data,SIMBAD,Bibcode:1986EgUBV........0M.
  3. ^abcTabur, V.; Bedding, T. R. (2009), "Long-term photometry and periods for 261 nearby pulsating M giants",Monthly Notices of the Royal Astronomical Society,400 (4):1945–61,arXiv:0908.3228,Bibcode:2009MNRAS.400.1945T,doi:10.1111/j.1365-2966.2009.15588.x,S2CID 15358380.
  4. ^abKukarkin, B. V.; et al. (1981), "Nachrichtenblatt der Vereinigung der Sternfreunde e.V. (Catalogue of suspected variable stars)",Nachrichtenblatt der Vereinigung der Sternfreunde, Moscow: Academy of Sciences USSR Shternberg,Bibcode:1981NVS...C......0K.
  5. ^Famaey, B.; et al. (2005), "Local kinematics of K and M giants from CORAVEL/Hipparcos/Tycho-2 data. Revisiting the concept of superclusters",Astronomy and Astrophysics,430:165–186,arXiv:astro-ph/0409579,Bibcode:2005A&A...430..165F,doi:10.1051/0004-6361:20041272,S2CID 17804304.
  6. ^Anderson, 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.
  7. ^abcdeMcDonald, I.; Zijlstra, A. A.; Watson, R. A. (2017), "Fundamental parameters and infrared excesses of Tycho-Gaia stars",Monthly Notices of the Royal Astronomical Society,471 (1): 770,arXiv:1706.02208,Bibcode:2017MNRAS.471..770M,doi:10.1093/mnras/stx1433,S2CID 73594365.
  8. ^"sig Vir",SIMBAD,Centre de données astronomiques de Strasbourg, retrieved2016-09-16.
  9. ^"/ftp/cats/more/HIP/cdroms/cats",Centre de Données astronomiques de Strasbourg, Strasbourg astronomical Data Center, retrieved15 October 2022.
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