Astronomy:Theta Virginis

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Short description: Multiple star system in the constellation of Virgo
θ Virginis
Virgo constellation map.svg
Red circle.svg
Location of θ Virginis (circled)
Observation data
Equinox J2000.0]] (ICRS)
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[1] mas
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
SIMBADdata

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. 1.0 1.1 1.2 1.3 1.4 van Leeuwen, F. (2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics 474 (2): 653–664, doi:10.1051/0004-6361:20078357, Bibcode2007A&A...474..653V. 
  2. 2.0 2.1 2.2 2.3 Mermilliod, J.-C. (1986), "Compilation of Eggen's UBV data, transformed to UBV (unpublished)", Catalogue of Eggen's UBV Data (SIMBAD), Bibcode1986EgUBV........0M. 
  3. 3.0 3.1 3.2 3.3 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, doi:10.1111/j.1365-2966.2008.13596.x, Bibcode2008MNRAS.389..869E. 
  4. 4.0 4.1 4.2 4.3 4.4 Landstreet, J. D. et al. (September 2009), "Atmospheric velocity fields in tepid main sequence stars", Astronomy and Astrophysics 503 (3): 973–984, doi:10.1051/0004-6361/200912083, Bibcode2009A&A...503..973L. 
  5. Wilson, R. E. (1953), "General Catalogue of Stellar Radial Velocities", Carnegie Institute Washington D.C. Publication (Carnegie Institute of Washington, D.C.), Bibcode1953GCRV..C......0W. 
  6. Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters 38 (5): 331, doi:10.1134/S1063773712050015, Bibcode2012AstL...38..331A. 
  7. 7.0 7.1 Zorec, J.; Royer, F. (January 2012), "Rotational velocities of A-type stars. IV. Evolution of rotational velocities", Astronomy & Astrophysics 537: A120, doi:10.1051/0004-6361/201117691, Bibcode2012A&A...537A.120Z. 
  8. "tet Vir". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=tet+Vir. 
  9. 9.0 9.1 Tokovinin, Andrei (2018). "The Updated Multiple Star Catalog". The Astrophysical Journal Supplement Series 235 (1): 6. doi:10.3847/1538-4365/aaa1a5. Bibcode2018ApJS..235....6T. 
  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, doi:10.1051/aas:1997105, Bibcode1997A&AS..125..497A. 
  11. Scholz, G. et al. (September 1998), "Spectroscopic and photometric investigations of MAIA candidate stars", Astronomy and Astrophysics 337: 447–459, Bibcode1998A&A...337..447S. 

External links