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Sigma Arietis, Latinized from σ Arietis, is the Bayer designation for a star in the northern constellation of Aries. It has an apparent visual magnitude of +5.52, which is bright enough for the star to be seen with the naked eye from dark suburban skies. The star is located at a distance of approximately 470 light-years (140 parsecs) from the Sun based on parallax, and is drifting further away with a radial velocity of +17 km/s. On November 20, 1952, it was observed being occulted by the planet Jupiter.

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  • Sigma d'Àries (ca)
  • Sigma Arietis (it)
  • Sigma Arietis (en)
  • Sigma Arietis (pt)
  • Sigma Arietis (sv)
  • 左更四 (zh)
rdfs:comment
  • Sigma d'Àries (σ Arietis) és una estrella de la constel·lació d'Àries. Sigma d'Àries és una nana de la seqüència principal blanca-blava del tipus B de la magnitud aparent +5,52. Està aproximadament a 480 anys-llum de la Terra. (ca)
  • Sigma Arietis (σ Ari / σ Arietis) è una stella bianco-azzurra nella sequenza principale di magnitudine 5,51 situata nella costellazione dell'Ariete. Dista 480 anni luce dal sistema solare. (it)
  • Sigma Arietis (σ Ari / σ Arietis) é uma estrela da constelação de Aries. É uma anã azul-branca da sequência principal e é da classe B. A sua magnitude aparente é +5,52 e está localizada a aproximadamente 480 anos-luz da Terra. (pt)
  • Sigma Arietis (σ Arietis förkortat Sigma Ari, σ Ari,) är Bayerbeteckning för en ensam stjärna i mellersta delen av stjärnbilden Väduren. Den har en skenbar magnitud på 5,52 och är synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätningar inom Hipparcos-uppdraget på 6,6 mas befinner den sig på ett beräknat avstånd av ca 490 ljusår (152 parsek) från solen. Den ingår sannolikt i Cassiopeiae Tau OB-föreningen av stjärnor som delar en gemensam rörelse genom rymden. (sv)
  • 左更四,即白羊座σ(σ Ari, σ Arietis),是一颗位于白羊座的恒星,它距离地球约480光年。 左更一是一颗蓝白色B-型主序星,视星等为+5.52。 白羊座σ在中国星官系统中属于西方白虎七宿中娄宿的星官左更第四星,因此被称为左更四。 (zh)
  • Sigma Arietis, Latinized from σ Arietis, is the Bayer designation for a star in the northern constellation of Aries. It has an apparent visual magnitude of +5.52, which is bright enough for the star to be seen with the naked eye from dark suburban skies. The star is located at a distance of approximately 470 light-years (140 parsecs) from the Sun based on parallax, and is drifting further away with a radial velocity of +17 km/s. On November 20, 1952, it was observed being occulted by the planet Jupiter. (en)
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  • σ 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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