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Tau3 Eridani

From Wikipedia, the free encyclopedia
A-type star in the constellation Eridanus
For other star systems with thisBayer designation, seeTau Eridani.
τ3 Eridani
Observation data
EpochJ2000.0      EquinoxJ2000.0 (ICRS)
ConstellationEridanus
Right ascension03h 02m 23.49939s[1]
Declination−23° 37′ 28.0936″[1]
Apparent magnitude (V)4.10[2]
Characteristics
Spectral typeA3 IV-V[3]
U−Bcolor index+0.08[2]
B−Vcolor index+0.16[2]
Astrometry
Radial velocity (Rv)−9.8[4] km/s
Proper motion (μ)RA: −147.25[1]mas/yr
Dec.: −55.28[1]mas/yr
Parallax (π)36.80±0.18 mas[1]
Distance88.6 ± 0.4 ly
(27.2 ± 0.1 pc)
Absolute magnitude (MV)+1.91[5]
Details
Mass1.78[6] M
Radius1.9[7] R
Luminosity13.7[8] L
Surface gravity (log g)4.17[6] cgs
Temperature8,251±281[6] K
Metallicity [Fe/H]−0.21[3] dex
Rotational velocity (v sin i)133[9] km/s
Age476[6] Myr
Other designations
τ3 Eridani, τ3 Eri,11 Eridani,CD-24° 1387,HD 18978,HIP 14146,HR 919,SAO 168249.[10]
Database references
SIMBADdata

Tau3 Eridani,Latinized fromτ3 Eridani, is astar in theconstellationEridanus. It is visible to the naked eye with anapparent visual magnitude of 4.10.[2] Using theparallax method,[1] the distance to this star can be estimated as 88.6 light years. In 2001 it was reported as a candidateVega-like star, meaning it appears to radiate aninfrared excess from an orbitingcircumstellar disk.[11] However, this has not been confirmed.[12]

This is anA-type star with astellar classification of A3 IV-V.[3] Theluminosity class of IV-V indicates the spectrum displays traits intermediate between amain sequence andsubgiant star. It is around 476[6] million years old and is spinning rapidly with aprojected rotational velocity of 133 km/s.[9] This is creating an equatorial bulge that might be 7% wider than the polar radius.[13] Tau3 Eridani has 178%[6] of theSun's mass and nearly double theradius of the Sun.[7] The star shines with 13.7 times thesolar luminosity from anouter atmosphere at aneffective temperature of 8,251 K.[6]

References

[edit]
  1. ^abcdefvan 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. ^abcdMermilliod, J.-C. (1986), "Compilation of Eggen's UBV data, transformed to UBV (unpublished)",Catalogue of Eggen's UBV Data,SIMBAD,Bibcode:1986EgUBV........0M.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. ^abcGray, R. O.; et al. (July 2006), "Contributions to the Nearby Stars (NStars) Project: spectroscopy of stars earlier than M0 within 40 pc-The Southern Sample",The Astronomical Journal,132 (1):161–170,arXiv:astro-ph/0603770,Bibcode:2006AJ....132..161G,doi:10.1086/504637,S2CID 119476992.
  4. ^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.
  5. ^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.
  6. ^abcdefgDavid, Trevor J.; Hillenbrand, Lynne A. (May 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): 38,arXiv:1501.03154,Bibcode:2015ApJ...804..146D,doi:10.1088/0004-637X/804/2/146,S2CID 33401607, 146.
  7. ^abPasinetti 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.
  8. ^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.
  9. ^abRoyer, 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.
  10. ^"tau03 Eri".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2016-10-13.{{cite web}}: CS1 maint: postscript (link)
  11. ^Song, Inseok; et al. (January 2001), "Ages of A-Type Vega-like Stars from uvbyβ Photometry",The Astrophysical Journal,546 (1):352–357,arXiv:astro-ph/0010102,Bibcode:2001ApJ...546..352S,doi:10.1086/318269,S2CID 18154947.
  12. ^Gáspár, András; et al. (May 2013), "The Collisional Evolution of Debris Disks",The Astrophysical Journal,768 (1): 29,arXiv:1211.1415,Bibcode:2013ApJ...768...25G,doi:10.1088/0004-637X/768/1/25,S2CID 119295265, 25.
  13. ^Van Belle, Gerard T. (2012), "Interferometric observations of rapidly rotating stars",The Astronomy and Astrophysics Review,20 (1): 51,arXiv:1204.2572,Bibcode:2012A&ARv..20...51V,doi:10.1007/s00159-012-0051-2,S2CID 119273474.
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