Xi Tauri
{{short description|Star system in the constellation Taurus}}
{{Starbox begin
| name = ξ Tauri
}}
{{Starbox image
| image = 250px
| caption = A light curve for Xi Tauri plotted from TESS data
}}
{{Starbox observe
| epoch = J2000.0
| constell = Taurus
}}
{{Starbox character
| class = B9Vn + B9V + B5V + F5V
| appmag_1_passband =
| appmag_1 =
| r-i =
| v-r =
| b-v =
| u-b =
| variable = Algol
}}
{{Starbox astrometry
| radial_v =
| prop_mo_ra = {{val|50.58|1.48}}
| prop_mo_dec = {{val|-39.54|1.40}}
| parallax = 15.60
| p_error = 1.04
| absmag_v =
}}
{{Starbox orbit
|primary=ξ Tau Aa
|name=ξ Tau Ab
|period_unitless={{val|7.146651|0.000010|u=d}}
|periastron=JD {{val|2448299.075|0.010}}
|eccentricity={{val|0.0|0.05}}
|inclination={{val|86.2|0.5}}
|node={{val|350.5|4.0}}
|periarg={{val|90|10}}
|k1={{val|89.1|10.0}}
}}
{{Starbox orbit
|primary=ξ Tau Aa-Ab
|name=ξ Tau B
|period_unitless={{val|145.12|0.055|u=d}}
|periastron=JD {{val|2453712.90|0.34}}
|eccentricity={{val|0.213|0.007}}
|periarg={{val|163.07|0.13}}
|k1={{val|38.02|5.0}}
|inclination={{val|87.07|0.19}}
|node={{val|328.63|0.38}}
|axis_unitless={{val|16.09|0.18|ul=mas}}
}}
{{Starbox detail
|component1=ξ Tau Aa
|temperature={{val|9400|500|fmt=commas}}
|gravity=4.2
|rotational_velocity={{val|33|2}}
|mass={{val|2.29|0.91}}
|radius={{val|2.0|0.2}}
|component2=ξ Tau Ab
|temperature2={{val|9200|500|fmt=commas}}
|gravity2=4.2
|rotational_velocity2={{val|34|2}}
|mass2={{val|2.20|0.78}}
|radius2={{val|1.5|0.2}}
}}
{{Starbox detail|no_heading=y
|component1=ξ Tau B
|mass={{val|3.08|1.24}}
|temperature={{val|15100|200|fmt=commas}}
|gravity={{val|4.3|0.1}}
|rotational_velocity={{val|246|10}}
}}
{{Starbox catalog
| names = 2 Tau, HR 1038, HD 21364, BD+09°439, HIP 16083, SAO 111195
}}
{{Starbox reference
|Simbad=xi+Tau
}}
{{Starbox end}}
Xi Tauri (ξ Tau, ξ Tauri) is a hierarchical quadruple system in the constellation Taurus.
Xi Tauri is a spectroscopic and eclipsing quadruple star. It consists of three blue-white B-type main sequence stars and an F-type main sequence star. Two of the stars form an eclipsing binary system and revolve around each other once every 7.15 days. These in turn orbit the third star once every 145 days. The fourth star is a F star that orbits the other three stars in a roughly fifty-year period and has been resolved optically. The brightest and most massive of the four stars is the "third" star, although the eclipsing pair have a greater combined mass and hence are generally considered to be the primary.
The typical combined apparent magnitude of the system is +3.73, but because the stars eclipse one another during their orbits, it is classified as a variable star, and its brightness varies from magnitude +3.73 to +3.81. Xi Tauri is approximately 210 light years from Earth.
Nomenclature for the four stars varies. Some sources refer to the faint resolved companion as component C, while others refer to it as B. Similarly, the inner three stars are respectively Aa, Ab, and B, or Aa, Ab, and Ac.
References
{{reflist|refs=
| title=MAST: Barbara A. Mikulski Archive for Space Telescopes
| url=https://mast.stsci.edu/portal/Mashup/Clients/Mast/Portal.html
| publisher=Space Telescope Science Institute |access-date=8 December 2021}}
{{cite web | url=http://simbad.u-strasbg.fr/simbad/sim-id?Ident=HR1038 | title=ksi Tau -- Star | website=SIMBAD Astronomical Database | publisher=Centre de données astronomiques de Strasbourg | access-date=2013-09-29}}
{{cite web |url=https://www.aavso.org/vsx/index.php?view=detail.top&oid=36241 |title=Xi Tau |access-date=2022-07-17 |publisher=AAVSO }}
}}
{{Stars of Taurus}}
{{DEFAULTSORT:Xi Tauri}}
Category:Spectroscopic binaries
Category:Taurus (constellation)