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Theta Scorpii
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{{Short description|Star in the constellation Scorpius}} {{Starbox begin }} {{Starbox image | image= {{Location mark | image=Scorpius constellation map.svg | float=center | width=250 | position=right | mark=Red circle.svg | mark_width=10 | mark_link=θ Sco | x%=24.6 | y%=87.6 }} | caption=Location of θ Scorpii (circled) }} {{Starbox observe | epoch = J2000 | ra = {{RA|17|37|19.12985}}<ref name=aaa474_2_653/> | dec = {{DEC|-42|59|52.1808}}<ref name=aaa474_2_653/> | appmag_v = 1.84 {{nowrap|(1.862 + 6.22)<ref name=hog/>}} | constell = [[Scorpius]] }} {{Starbox character | class = F0Ib-F1III<ref name="ayres2018" /> or F0 II<ref name=houk1978/> | b-v = +0.40<ref name=clpl4_99/> | u-b = +0.21<ref name=clpl4_99/> | variable = }} {{Starbox astrometry | radial_v = +1.4<ref name=gcsrv/> | prop_mo_ra = +5.54<ref name=aaa474_2_653/> | prop_mo_dec = −3.12<ref name=aaa474_2_653/> | parallax = 9.90 | p_error = 0.26 | parallax_footnote = <ref name=Lewis/> | absmag_v = −2.71<ref name=Anderson2012/> }} {{Starbox detail | mass = {{val|3.10|+0.37|-0.32}}<ref name=Lewis/> | radius = 26.3 - 35.5<ref name=Lewis/> | luminosity = 1,400<ref name=Lewis/> | temperature = 6,294<ref name=Lewis/> | metal_fe = | gravity = {{val|2.4|0.2}}<ref name=ap28_3_335/> | rotational_velocity = 125<ref name="AAR20_1_51"/> | rotation = 16.60<ref name=Lewis/> [[day|d]] | age_myr = }} {{Starbox catalog | names={{odlist | name=Sargas | name2=Girtab | name3=[[Gould designation|160 G.]] Scorpii | B=θ Sco | CD=−42°12312 | FK5=654 | HD=159532 | HIP=86228 | HR=6553 | SAO=228201 | CCDM=J17373−4300 }}<ref name=SIMBAD/> }} {{Starbox reference | Simbad = tet+Sco }} {{Starbox end}} '''Theta Scorpii''' ('''θ Scorpii''', abbreviated '''Theta Sco''', '''θ Sco''') is a [[binary star]] in the [[Southern celestial hemisphere|southern]] [[zodiac]] [[constellation]] of [[Scorpius]]. The [[apparent visual magnitude]] of this [[star]] is +1.87,<ref name=clpl4_99/> making it readily visible to the naked eye and one of the [[List of brightest stars|brightest stars]] in the [[night sky]]. It is sufficiently near that the distance can be measured directly using the [[stellar parallax|parallax]] technique and such measurements obtained during the ''[[Hipparcos]]'' mission yield an estimate of approximately {{Convert|101|pc|ly|abbr=off|lk=on|order=flip|sigfig=3}} from the [[Sun]]. The two components are designated '''θ Scorpii A''' (officially named '''Sargas''' {{IPAc-en|'|s|ɑr|g|æ|s}}, the traditional name for the system)<ref name=Kunitzsch/><ref name="IAU-LSN"/> and '''B'''.
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