{{Short description|Star in the constellation Taurus}} {{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=132 Tauri |x=40|y=292 }} | caption = Location of 132 Tauri (circled in red) }} {{Starbox observe | epoch = J2000 | constell = Taurus | ra = {{RA|05|49|00.96598}}<ref name=vanLeeuwen2007/> | dec = {{DEC|+24|34|03.1220}}<ref name=vanLeeuwen2007/> | appmag_v = 4.89 {{nowrap|(5.07 + 9.09)}}<ref name=Eggleton2008/> }} {{Starbox character | class = G9&nbsp;III<ref name=Keenan1999/> | b-v = 1.021<ref name=Anderson2012/> | u-b = | r-i = | variable = }} {{Starbox astrometry | radial_v = {{Val|+15.8|0.6}}<ref name=deBruijne2012/> | prop_mo_ra = +10.44<ref name=vanLeeuwen2007/> | prop_mo_dec = −8.30<ref name=vanLeeuwen2007/> | parallax = 8.97 | p_error = 1.98 | parallax_footnote = <ref name=vanLeeuwen2007/> | absmag_v = }} {{Starbox detail | source = | component1 = 132 Tau Aa | mass = | radius = | luminosity = | gravity = {{Val|2.74|0.11}}<ref name=Prugniel2011/> | temperature = {{Val|4853|47|fmt=commas}}<ref name=Prugniel2011/> | metal_fe = {{Val|0.18|0.05}}<ref name=Prugniel2011/> | rotational_velocity = | age_myr = }} {{Starbox catalog | names = {{odlist | F=132 Tau | BD=+24°970 | FK5=2435 | HD=38751 | HIP=27468 | HR=2002 | SAO=77592 | WDS=J05490+2434AB }}<ref name=SIMBAD/> }} {{Starbox reference | Simbad = 132+Tau }} {{Starbox end}}

'''132 Tauri''' is a binary star<ref name=Eggleton2008/> system in the constellation Taurus. It is faintly visible to the naked eye with an apparent visual magnitude of 4.89.<ref name=Eggleton2008/> Based upon a poorly constrained annual parallax shift of {{Val|8.97|1.98|ul=mas}},<ref name=vanLeeuwen2007/> it is located roughly 360&nbsp;light years from the Sun. The system is moving further away with a heliocentric radial velocity of +16&nbsp;km/s.<ref name=deBruijne2012/> It lies near the ecliptic and thus is subject to occultation by the Moon. One such event was observed September 3, 1991.<ref name=Meyer1995/>

This system forms a wide double star with an angular separation of {{Val|3.8|ul=arcsec}} along a position angle of 230°, as of 1991. The brighter star, component A, has an apparent magnitude of 4.99 while the fainter secondary, component B, is of magnitude 9.09. The primary is itself an unresolved binary<ref name=WDSC2014/> with a combined stellar classification of G9&nbsp;III,<ref name=Keenan1999/> which matches an aging G-type giant star that has exhausted the hydrogen at its core and evolved away from the main sequence.

==References== <references> <ref name=SIMBAD>{{cite simbad | title=132 Tau | access-date=2018-03-27 }}</ref>

<ref name=vanLeeuwen2007>{{citation | title=Validation of the new Hipparcos reduction | last1=van Leeuwen | first1=F. | postscript=. | 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 }}</ref>

<ref name=Anderson2012>{{citation | title=XHIP: An extended hipparcos compilation | last1=Anderson | first1=E. | last2=Francis | first2=Ch. | journal=Astronomy Letters | volume=38 | issue=5 | pages=331 | year=2012 | bibcode=2012AstL...38..331A | doi=10.1134/S1063773712050015 | arxiv=1108.4971 | s2cid=119257644 | postscript=. }}</ref>

<ref name=Meyer1995>{{citation | title=Observations of lunar occultations at Observatoire de la Cote d'Azur | display-authors=1 | last1=Meyer | first1=C. | last2=Rabbia | first2=Y. | last3=Froeschle | first3=M. | last4=Helmer | first4=G. | last5=Amieux | first5=G. | journal=Astronomy and Astrophysics Supplement | volume=110 | page=107 | date=April 1995 | bibcode=1995A&AS..110..107M }}</ref>

<ref name=Keenan1999>{{citation | last1=Keenan | first1=Philip C. | last2=Barnbaum | first2=Cecilia | title=Revision and Calibration of MK Luminosity Classes for Cool Giants by HIPPARCOS Parallaxes | journal=The Astrophysical Journal | postscript=. | issue=2 | pages=859–865 | date=June 1999 | volume=518 | doi=10.1086/307311 | bibcode=1999ApJ...518..859K| s2cid=121902473 | doi-access=free }}</ref>

<ref name=Prugniel2011>{{citation | display-authors=1 | last1=Prugniel | first1=Ph. | last2=Vauglin | first2=I. | last3=Koleva | first3=M. | title=The atmospheric parameters and spectral interpolator for the MILES stars | journal=Astronomy & Astrophysics | volume=531 | page=A165 | date=July 2011 | doi=10.1051/0004-6361/201116769 | bibcode=2011A&A...531A.165P | postscript=. | arxiv=1104.4952 | s2cid=54940439 }}</ref>

<ref name=Eggleton2008>{{citation | last1=Eggleton | first1=P. P. | last2=Tokovinin | first2=A. A. | title=A catalogue of multiplicity among bright stellar systems | journal=Monthly Notices of the Royal Astronomical Society | volume=389 | issue=2 | pages=869–879 | date=September 2008 | doi=10.1111/j.1365-2966.2008.13596.x | doi-access=free | bibcode=2008MNRAS.389..869E | postscript=. | arxiv=0806.2878 | s2cid=14878976 }}</ref>

<ref name=deBruijne2012>{{citation | last1=de Bruijne | first1=J. H. J. | last2=Eilers | first2=A.-C. | title=Radial velocities for the HIPPARCOS-Gaia Hundred-Thousand-Proper-Motion project | journal=Astronomy & Astrophysics | volume=546 | id=A61 | pages=14 | date=October 2012 | doi=10.1051/0004-6361/201219219 | bibcode=2012A&A...546A..61D | arxiv=1208.3048 | s2cid=59451347 | postscript=. }}</ref>

<ref name=WDSC2014>{{citation | display-authors=1 | last1=Mason | first1=B. D. | last2=Wycoff | first2=G. L. | last3=Hartkopf | first3=W. I. | last4=Douglass | first4=G. G. | last5=Worley | first5=C. E. | title=The Washington Visual Double Star Catalog | journal=The Astronomical Journal | year=2014 | volume=122 | issue=6 | page=3466 | bibcode=2001AJ....122.3466M | doi=10.1086/323920 | doi-access=free }}</ref> </references>

{{Stars of Taurus}}

Category:G-type giants Category:Suspected variables Category:Taurus (constellation) BD+24 0970 Tauri, 132 038751 027468 2002