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Theta Arietis, Latinised from θ Arietis, is the Bayer designation for a binary star system in the northern constellation of Aries. It is faintly visible to the naked eye with an apparent visual magnitude of 5.58. With an annual parallax shift of 7.61 mas, the distance to this star is an estimated 429 light-years (132 parsecs) with a 10-light-year margin of error. It is drifting further away with a radial velocity of +6 km/s. In 2016, a solar-mass companion was reported in close orbit around this star, based on observations using adaptive optics with the Gemini North Telescope.

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rdf:type
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  • Theta d'Àries (ca)
  • Theta Arietis (it)
  • Theta Arietis (pt)
  • Theta Arietis (en)
  • Theta Arietis (sv)
  • 娄宿增十三 (zh)
rdfs:comment
  • Theta d'Àries (θ Arietis) és una estrella de la constel·lació d'Àries. És una nana de la seqüència principal blanca del tipus A de la magnitud aparent +5,58. Està aproximadament a 387 anys-llum de la Terra. (ca)
  • Theta Arietis (θ Ari / θ Arietis) è una stella bianca nella sequenza principale di magnitudine 5,58 situata nella costellazione dell'Ariete. Dista 387 anni luce dal sistema solare. (it)
  • Theta Arietis (θ Ari, θ Arietis) är Bayerbeteckning för en stjärna nära mitten av stjärnbilden Väduren. Det är svagt synlig för blotta ögat med en skenbar magnitud på 5,58. Baserat på en årlig parallaxförskjutning på 7,29 mas, befinner sig denna stjärna på ett beräknat avstånd av ungefär 450 ljusår (140 parsek) från solen. (sv)
  • Theta Arietis (22 Arietis) é uma estrela na direção da constelação de Aries. Possui uma ascensão reta de 02h 18m 07.55s e uma declinação de +19° 54′ 04.2″. Sua magnitude aparente é igual a 5.58. Considerando sua distância de 387 anos-luz em relação à Terra, sua magnitude absoluta é igual a 0.21. Pertence à classe espectral A1Vn. (pt)
  • 娄宿增十三,即白羊座θ (θ Ari),是一颗位于白羊座的恒星,距离地球约387光年。 娄宿增十三是一颗A-型主序星,视星等为+5.58。 (zh)
  • Theta Arietis, Latinised from θ Arietis, is the Bayer designation for a binary star system in the northern constellation of Aries. It is faintly visible to the naked eye with an apparent visual magnitude of 5.58. With an annual parallax shift of 7.61 mas, the distance to this star is an estimated 429 light-years (132 parsecs) with a 10-light-year margin of error. It is drifting further away with a radial velocity of +6 km/s. In 2016, a solar-mass companion was reported in close orbit around this star, based on observations using adaptive optics with the Gemini North Telescope. (en)
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  • θ Arietis (en)
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  • http://commons.wikimedia.org/wiki/Special:FilePath/Aries_constellation_map.svg
  • http://commons.wikimedia.org/wiki/Special:FilePath/Red_circle.svg
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