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θ Virginis
Location of θ Virginis (circled)
Observation data
Epoch J2000.0       Equinox J2000.0
Constellation Virgo
Right ascension 13h 09m 56.99067s [1]
Declination −05° 32′ 20.4185″ [1]
Apparent magnitude (V) 4.37 [2] (4.49 + 6.83 + 9.4 + 10.4) [3]
Characteristics
Spectral type A1Vs [4] + ? + A9m + ? [3]
U−B color index +0.00 [2]
B−V color index −0.02 [2]
Astrometry
Radial velocity (Rv)−2.9 [5] km/s
Proper motion (μ) RA: −36.28 [1]  mas/ yr
Dec.: −31.22 [1]  mas/ yr
Parallax (π)10.33 ± 1.09  mas [1]
Distanceapprox. 320  ly
(approx. 100  pc)
Absolute magnitude (MV)−0.52 [6]
Details
θ Vir Aa
Mass3.11±0.11 [7]  M
Luminosity190 [7]  L
Surface gravity (log g)3.4 [4]  cgs
Temperature9,250 [4]  K
Rotational velocity (v sin i)4±1 [4] km/s
Other designations
51 Virginis, θ Vir, BD−04°3430, FK5 490, HD 114330, HIP 64238, HR 4963, SAO 139189. [8]
Database references
SIMBAD data

Theta Virginis (θ Vir, θ Virginis) is a multiple star system in the zodiac constellation of Virgo. Based upon parallax measurements, it is about 320  light years from the Sun. The three [9] stars in this system have a combined apparent visual magnitude of 4.37, [2] bright enough to be seen with the naked eye.

The primary component, Theta Virginis Aa, is a white-hued A-type main sequence star with a stellar classification of A1Vs. [4] It is part of a spectroscopic binary [10] whose components, Aa and Ab, have visual magnitudes of +4.49 and +6.83 respectively. The system has an orbital period of about 33.04 years with an eccentricity of 0.9. [3] The brighter member of this pair shows photometric and radial velocity periodicities with a cycle time of 0.7 days, which may indicate its rotation period. [11]

The inner pair is orbited by the 9.4 magnitude B component, at an angular separation of 7.1  arcseconds. A fourth component C, 69.6 arcseconds away, has an apparent magnitude of 10.4. [3] However, component C is an optical companion: it is physically unrelated and only appears close in the sky. [9]

References

  1. ^ a b c d e van Leeuwen, F. (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. ^ a b c d Mermilliod, J.-C. (1986), "Compilation of Eggen's UBV data, transformed to UBV (unpublished)", Catalogue of Eggen's UBV Data, SIMBAD, Bibcode: 1986EgUBV........0M.
  3. ^ a b c d 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.
  4. ^ a b c d e Landstreet, J. D.; et al. (September 2009), "Atmospheric velocity fields in tepid main sequence stars", Astronomy and Astrophysics, 503 (3): 973–984, arXiv: 0906.3824, Bibcode: 2009A&A...503..973L, doi: 10.1051/0004-6361/200912083, S2CID  53423301.
  5. ^ Wilson, R. E. (1953), "General Catalogue of Stellar Radial Velocities", Carnegie Institute Washington D.C. Publication, Carnegie Institute of Washington, D.C., Bibcode: 1953GCRV..C......0W.
  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. ^ a b Zorec, J.; Royer, F. (January 2012), "Rotational velocities of A-type stars. IV. Evolution of rotational velocities", Astronomy & Astrophysics, 537: A120, arXiv: 1201.2052, Bibcode: 2012A&A...537A.120Z, doi: 10.1051/0004-6361/201117691, S2CID  55586789.
  8. ^ "tet Vir". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2016-09-05.{{ cite web}}: CS1 maint: postscript ( link)
  9. ^ a b Tokovinin, Andrei (2018). "The Updated Multiple Star Catalog". The Astrophysical Journal Supplement Series. 235 (1): 6. arXiv: 1712.04750. Bibcode: 2018ApJS..235....6T. doi: 10.3847/1538-4365/aaa1a5. S2CID  119047709.
  10. ^ Adelman, Saul J. (November 1997), "On the possible variability of the main sequence A stars theta Virginis and 109 Virginis", Astronomy & Astrophysics Supplement Series, 125 (3): 497–499, Bibcode: 1997A&AS..125..497A, doi: 10.1051/aas:1997105.
  11. ^ Scholz, G.; et al. (September 1998), "Spectroscopic and photometric investigations of MAIA candidate stars", Astronomy and Astrophysics, 337: 447–459, Bibcode: 1998A&A...337..447S.

External links