tau Tauri
{{Short description|Star system in the constellation Taurus}}{{distinguish|T Tauri}}
{{Starbox begin}}
{{Starbox image
|image=
{{Location mark
|image=Taurus constellation map.svg|alt=|float=center|width=280
|label=|position=right
|mark=Red circle.svg|mark_width=10|mark_link=Tau Tauri
|x=457|y=363
}}
| caption = Location of τ Tauri (circled)
}}
{{Starbox observe
| epoch = J2000
| constell = Taurus
}}
{{Starbox character
| type =
| class = B3V + ? + A0V–A2V + A1V
| variable =
}}
{{Starbox astrometry
| parallax = 8.19
| p_error = 0.88
}}
{{Starbox orbit
| primary = Aa
| period_unitless = {{Val|2.956549|0.000002|u=days}}
| axis =
| axis_unitless = ≤ {{Convert|2176000|km|AU|disp=out}}
| eccentricity = {{Val|0.051|0.019}}
| periastron = {{Val|2436424.207|0.009|ul=JD|fmt=commas}}
| periarg = {{Val|126.7|21.8}}
| k1 = {{Val|53.6|1.0}}
}}
{{Starbox detail
| component1 = Aa
| radius =
| age_gyr =
}}
{{Starbox catalog
| names = {{odlist | B=τ Tau | F=94 Tauri | BD=+22°739 | FK5=174 | HD=29763 | HIP=21881 | HR=1497 | SAO=76721 | GC=5716 | CCDM=J04422+2257AB | GSC=01830-02129 | WDS=J04422+2257A }}
}}
{{Starbox reference
| Simbad = tau+Tau
}}
{{Starbox end}}
Tau Tauri, Latinized from τ Tauri, is a quadruple star system in the constellation Taurus. It is visible to the naked eye as a faint point of light with a combined apparent visual magnitude of 4.33. The distance to this system is approximately about 400 light years based on parallax. The system is moving further from the Earth with a heliocentric radial velocity of +14.6 km/s, and it is a member of the Taurion OB association, located between Orion and Taurus. It is located 0.7 degree north of the ecliptic, and thus is subject to lunar occultations.
The blue-white hued primary, component Aa, is a B-type main-sequence star with a stellar classification of B3V. It was found to be a close spectroscopic binary in 1903 by American astronomers Edwin B. Frost and Walter S. Adams. The pair have an orbital period of 2.96 days and eccentricity of 0.05. A second companion, white-hued component Ab, has magnitude 6.97 and angular separation 0.2" from the primary in a 58-year orbit. This is a probably A-type main-sequence star with a class of A0V–A2V. The more distant component B is a type A1V star with magnitude 7.2 and separation 62.8".
References
{{reflist|refs=
{{cite simbad | title=tau Tau | access-date=2016-10-18 | postscript=. }}
| title=The spectroscopic binary Boss 1107
| last1=Petrie | first1=R. M. | last2=Ebbighausen | first2=E. G.
| journal=Publications of the Dominion Astrophysical Observatory Victoria
| volume=11 | pages=385–394 | date=1961
| bibcode=1961PDAO...11..385P }}
| title=Cosmography of OB stars in the solar neighbourhood
| last1=Bouy | first1=H. | last2=Alves | first2=J.
| journal=Astronomy & Astrophysics
| volume=584 | id=A26 | pages=13 | date=December 2015
| doi=10.1051/0004-6361/201527058
| bibcode=2015A&A...584A..26B | doi-access=free }}
| title=New binary stars discovered by lunar occultations
| display-authors=1 | last1=Richichi | first1=A.
| last2=Calamai | first2=G. | last3=Leinert | first3=C.
| journal=Astronomy and Astrophysics
| volume=286 | pages=829–837 | date=June 1994
| bibcode=1994A&A...286..829R }}
| title=Validation of the new Hipparcos reduction
| last1=Van Leeuwen | first1=F.
| journal=Astronomy and Astrophysics
| volume=474 | issue=2 | pages=653–664 | year=2007
| arxiv=0708.1752 | bibcode=2007A&A...474..653V
| doi=10.1051/0004-6361:20078357
| s2cid=18759600 }} [http://vizier.u-strasbg.fr/viz-bin/VizieR-S?HIP%2021881 Vizier catalog entry]
{{cite journal | last=Wilson | first=R. E. | year=1953 | title=General Catalogue of Stellar Radial Velocities | journal=Carnegie Institute Washington D.C. Publication | publisher=Carnegie Institution for Science | bibcode=1953GCRV..C......0W | isbn=9780598216885 | lccn=54001336 }}
}}
{{Stars of Taurus}}
{{DEFAULTSORT:Tau Tauri}}
Category:B-type main-sequence stars
Category:A-type main-sequence stars
Category:Spectroscopic binaries