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Tau1 Hydrae

From Wikipedia, the free encyclopedia
Triple star system in the constellation Hydra
For other stars with this Bayer designation, seeτ Hydrae.
Tau1 Hydrae
Location of τ1 Hydrae (circled in red)
Observation data
EpochJ2000.0      EquinoxJ2000.0 (ICRS)
ConstellationHydra
Right ascension09h 29m 08.89655s[1]
Declination−02° 46′ 08.2649″[1]
Apparent magnitude (V)+4.59(4.60 + 7.15)[2]
Characteristics
Spectral typeF6 V + ? + K0[3]
B−Vcolor index+0.411±0.015[2]
Astrometry
Radial velocity (Rv)+10.85±0.28[4] km/s
Absolute magnitude (MV)+3.28[5]
τ1 Hydrae A
Proper motion (μ)RA: +107.115[6]mas/yr
Dec.: −29.652[6]mas/yr
Parallax (π)56.2938±0.5309 mas[6]
Distance57.9 ± 0.5 ly
(17.8 ± 0.2 pc)
τ1 Hydrae B
Proper motion (μ)RA: +138.487[7]mas/yr
Dec.: −17.371[7]mas/yr
Parallax (π)55.3675±0.0638 mas[7]
Distance58.91 ± 0.07 ly
(18.06 ± 0.02 pc)
Orbit[8]
Period (P)2,807±23 d
Eccentricity (e)0.33±0.12
Periastronepoch (T)2445260 ± 150 JD
Semi-amplitude (K1)
(primary)
2.98±0.39 km/s
Details
τ1 Hydrae A
Mass1.20[9] M
Radius1.4[10] R
Luminosity (bolometric)3.369[2] L
Surface gravity (log g)4.12±0.14[9] cgs
Temperature6,473±220[9] K
Metallicity[Fe/H]−0.01[2] dex
Rotational velocity (v sin i)30.4±1.5[5] km/s
Age3.61[2] Gyr
τ1 Hydrae B
Mass0.86[11] M
Radius0.81[10] R
Luminosity0.435[7] L
Temperature5,197[7] K
Other designations
τ1 Hya,31 Hydrae,BD−02°2901,GJ 348,HD 81997,HIP 46509,HR 3759,SAO 136895,WDS J09291-0246[12]
Database references
SIMBADτ1 Hya AB
τ1 Hya A
τ1 Hya B

Tau1 Hydrae is atriple star[3] system in the equatorialconstellation ofHydra. Based upon the annualparallax shift of the two visible components as seen from Earth,[1] they are located about 18 parsecs (59 ly) from theSun. The system has a combinedapparent visual magnitude of +4.59,[2] which is bright enough to be visible to the naked eye at night.

The inner pair of stars form a single-linedspectroscopic binary with anorbital period of about 2,807 days and aneccentricity of 0.33.[8] The visible member of the pair, component A, is a visual magnitude 4.60[2]F-type main sequence star with astellar classification of F6 V.[3] During the 1990s, it was thought to be aGamma Doradus variable, but this was later discounted as it shows no short-termphotometric variability. The star does show some long-term variability, possibly as a result of amagnetic activity cycle similar to thesolar cycle.[13]

The tertiary member, component B, is a visual magnitude 7.15[2]K-type star with a class of K0.[3] It lies at a separation of 1,120 AU from the primary.[14] As of 2012, it was positioned at anangular separation of 67.5 arc seconds along aposition angle of 4°.[15]

This star along withτ2 Hydrae,ι Hydrae and33 Hydrae (A Hydrae) were traditionally known as Ukdah, Arabic for "knot".[16] The name Ukdah is now officially applied to ι Hydrae.

References

[edit]
  1. ^abcvan 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. ^abcdefghMontesinos, B.; et al. (September 2016), "Incidence of debris discs around FGK stars in the solar neighbourhood",Astronomy & Astrophysics,593: 31,arXiv:1605.05837,Bibcode:2016A&A...593A..51M,doi:10.1051/0004-6361/201628329,S2CID 55251562, A51.
  3. ^abcdEggleton, 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. ^de Bruijne, J. H. J.; Eilers, A.-C. (October 2012), "Radial velocities for the HIPPARCOS-Gaia Hundred-Thousand-Proper-Motion project",Astronomy & Astrophysics,546: 14,arXiv:1208.3048,Bibcode:2012A&A...546A..61D,doi:10.1051/0004-6361/201219219,S2CID 59451347, A61.
  5. ^abReiners, Ansgar (January 2006), "Rotation- and temperature-dependence of stellar latitudinal differential rotation",Astronomy and Astrophysics,446 (1):267–277,arXiv:astro-ph/0509399,Bibcode:2006A&A...446..267R,doi:10.1051/0004-6361:20053911,S2CID 8642707
  6. ^abcBrown, A. G. A.; et al. (Gaia collaboration) (August 2018)."Gaia Data Release 2: Summary of the contents and survey properties".Astronomy & Astrophysics.616. A1.arXiv:1804.09365.Bibcode:2018A&A...616A...1G.doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source atVizieR.
  7. ^abcdeBrown, A. G. A.; et al. (Gaia collaboration) (August 2018)."Gaia Data Release 2: Summary of the contents and survey properties".Astronomy & Astrophysics.616. A1.arXiv:1804.09365.Bibcode:2018A&A...616A...1G.doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source atVizieR.
  8. ^abPourbaix, D.; et al. (September 2004), "SB9: The ninth catalogue of spectroscopic binary orbits",Astronomy and Astrophysics,424:727–732,arXiv:astro-ph/0406573,Bibcode:2004A&A...424..727P,doi:10.1051/0004-6361:20041213,S2CID 119387088.
  9. ^abcDavid, 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.
  10. ^abPasinetti Fracassini, L. E.; et al. (February 2001), "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS)",Astronomy and Astrophysics,367 (3rd ed.):521–524,arXiv:astro-ph/0012289,Bibcode:2001A&A...367..521P,doi:10.1051/0004-6361:20000451,S2CID 425754.
  11. ^Tokovinin, Andrei (2014), "From Binaries to Multiples. II. Hierarchical Multiplicity of F and G Dwarfs",The Astronomical Journal,147 (4): 14,arXiv:1401.6827,Bibcode:2014AJ....147...87T,doi:10.1088/0004-6256/147/4/87,S2CID 56066740, 87.
  12. ^"tau01 Hya".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2017-03-22.{{cite web}}: CS1 maint: postscript (link)
  13. ^Henry, G. W.; et al. (March 1999), "tau1 Hydrae: NOT A gamma DORADUS VARIABLE",Information Bulletin on Variable Stars,4688 (4688): 1,Bibcode:1999IBVS.4688....1H.
  14. ^Allen, Peter R.; et al. (August 2012), "Low-mass Tertiary Companions to Spectroscopic Binaries. I. Common Proper Motion Survey for Wide Companions Using 2MASS",The Astronomical Journal,144 (2): 12,arXiv:1206.4289,Bibcode:2012AJ....144...62A,doi:10.1088/0004-6256/144/2/62,S2CID 51051184, 62.
  15. ^Mason, B. D.; et al. (2014), "The Washington Visual Double Star Catalog",The Astronomical Journal,122 (6):3466–3471,Bibcode:2001AJ....122.3466M,doi:10.1086/323920.
  16. ^Allen, R. H. (1963).Star Names: Their Lore and Meaning (Reprint ed.). New York, NY: Dover Publications Inc. p. 250.ISBN 0-486-21079-0. Retrieved2010-12-12.{{cite book}}:ISBN / Date incompatibility (help)
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