Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Virgo |
Right ascension | 14h 01m 38.79341s |
Declination | +01° 32′ 40.3145″ |
Apparent magnitude (V) | 4.2777±0.0007 |
Characteristics | |
Spectral type | A2IV/V |
U−B color index | +0.12 |
B−V color index | +0.11 |
Astrometry | |
Radial velocity (Rv) | −6.7±0.9 km/s |
Proper motion (μ) | RA: +17.49 mas/yr Dec.: −21.27 mas/yr |
Parallax (π) | 14.50 ± 0.18 mas |
Distance | 225 ± 3 ly (69.0 ± 0.9 pc) |
Absolute magnitude (MV) | +0.5 |
Details | |
Mass | 1.96 M☉ |
Radius | 1.6 R☉ |
Luminosity | 70 L☉ |
Surface gravity (log g) | 3.39 cgs |
Temperature | 8,413±286 K |
Metallicity [Fe/H] | −0.19 dex |
Rotational velocity (v sin i) | 186 km/s |
Age | 724 Myr |
Other designations | |
Database references | |
SIMBAD | data |
Tau Virginis (τ Vir, τ Virginis) is a single star in the zodiac constellation Virgo. With an apparent visual magnitude of 4.28, it is faintly visible to the naked eye. The distance to Tau Virginis, based upon parallax measurements, is approximately 225 light years with a margin of error of ±3 light years.
This star has a stellar classification of A2IV/V, which matches the spectrum of an A-type main sequence star mixed with spectral traits of a subgiant. It is about 700 million years old and is spinning rapidly with a projected rotational velocity of 186 km/s. The star has nearly double the mass of the Sun and about 160% of the Sun's radius. It shines with 70 times the luminosity of the Sun and has an effective temperature of 8413 K in its outer atmosphere.
Tau Virginis has multiple visual companions, listed below:
Companion | Visual Magnitude |
Angular Separation |
Position Angle |
Year Measured |
---|---|---|---|---|
B | 9.41 | 82.70″ | 287° | 2012 |
C | 13.10 | 176.70″ | 353° | 2000 |
D | 9.68 | 342.70″ | 85° | 2012 |
E | 12.00 | 14.6″ | 175° | 2009 |
References
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- ^ a b c d e f g David, Trevor J.; Hillenbrand, Lynne A. (2015), "The Ages of Early-Type Stars: Strömgren Photometric Methods Calibrated, Validated, Tested, and Applied to Hosts and Prospective Hosts of Directly Imaged Exoplanets", The Astrophysical Journal, 804 (2): 146, arXiv:1501.03154, Bibcode:2015ApJ...804..146D, doi:10.1088/0004-637X/804/2/146, S2CID 33401607.
- ^ a b Pasinetti Fracassini, L. E.; et al. (February 2001), "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS) - Third edition - Comments and statistics", Astronomy and Astrophysics, 367 (2): 521–524, arXiv:astro-ph/0012289, Bibcode:2001A&A...367..521P, doi:10.1051/0004-6361:20000451, S2CID 425754.
- ^ a b McDonald, I.; et al. (2012), "Fundamental Parameters and Infrared Excesses of Hipparcos Stars", Monthly Notices of the Royal Astronomical Society, 427 (1): 343–57, arXiv:1208.2037, Bibcode:2012MNRAS.427..343M, doi:10.1111/j.1365-2966.2012.21873.x, S2CID 118665352.
- ^ Morossi, C.; et al. (September 2002), "Metallicity Determinations from Ultraviolet-Visual Spectrophotometry. I. The Test Sample", The Astrophysical Journal, 577 (1): 377–388, Bibcode:2002ApJ...577..377M, doi:10.1086/342144.
- ^ a b Royer, F.; et al. (February 2007), "Rotational velocities of A-type stars. III. Velocity distributions", Astronomy and Astrophysics, 463 (2): 671–682, arXiv:astro-ph/0610785, Bibcode:2007A&A...463..671R, doi:10.1051/0004-6361:20065224, S2CID 18475298.
- ^ "* tau Vir". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2016-09-16.
- ^ 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.
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