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Sigma Persei (Sigma Per, σ Persei, σ Per) is an orange K-type giant with an apparent magnitude of +4.36. It is approximately 360 light years from Earth. Sigma Persei is moving through the Galaxy at a speed of 17.4 km/s relative to the Sun. Its projected Galactic orbit carries it between 24,400 and 43,600 light years from the center of the Galaxy. It came closest to the Sun 5.1 million years ago when it had brightened to magnitude 3.11 from a distance of 202 light years. It has one reported planet, b, with a period of 580 days and a mass approximately 6.5 times that of Jupiter.

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  • Sigma Persei (pl)
  • Sigma Persei (pt)
  • Sigma Persei (en)
  • Сигма Персея (ru)
  • Sigma Persei (sv)
  • 天船增四 (zh)
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  • Sigma Persei (Sigma Per, σ Persei, σ Per) is an orange K-type giant with an apparent magnitude of +4.36. It is approximately 360 light years from Earth. Sigma Persei is moving through the Galaxy at a speed of 17.4 km/s relative to the Sun. Its projected Galactic orbit carries it between 24,400 and 43,600 light years from the center of the Galaxy. It came closest to the Sun 5.1 million years ago when it had brightened to magnitude 3.11 from a distance of 202 light years. It has one reported planet, b, with a period of 580 days and a mass approximately 6.5 times that of Jupiter. (en)
  • Sigma Persei (35 Persei) é uma estrela na direção da constelação de Perseus. Possui uma ascensão reta de 03h 30m 34.48s e uma declinação de +47° 59′ 42.6″. Sua magnitude aparente é igual a 4.36. Considerando sua distância de 353 anos-luz em relação à Terra, sua magnitude absoluta é igual a −0.93. Pertence à classe espectral K3III. (pt)
  • Sigma Persei (σ Persei, förkortat Sigma Per, σ Per) som är stjärnans Bayerbeteckning, är en jättestjärna belägen i den mellersta delen av stjärnbilden Perseus. Den har en skenbar magnitud på 4,36 och är synlig för blotta ögat. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 9,1 mas, beräknas den befinna sig på ett avstånd av ca 360 ljusår ( ca 110 parsek) från solen. (sv)
  • Sigma Persei (σ Per) – gwiazda w gwiazdozbiorze Perseusza, będąca olbrzymem o typie widmowym K3 III. Znajduje się około 360 lat świetlnych od Słońca. (pl)
  • 英仙座σ,又名BD+47 843,HD 21552、SAO 38890、HR 1052,是英仙座的一颗恒星,视星等为4.36,位于銀經148.48,銀緯-6.83,其B1900.0坐标为赤經3h 23m 31.2s,赤緯+47° -6.83′ 0″。 (zh)
  • Сигма Персея (σ Персея, Sigma Persei, σ Persei, сокращ. Sigma Per, σ Per) — звезда в северном созвездии Персея. Сигма Персея также находится в области массивных звёзд, хотя звезда вряд ли связана со скоплением Альфа Персея (которое находится на расстоянии 557−650 св. лет), а также другими скоплениями соседних массивных звёзд. Сигма Персея имеет видимую звёздную величину +4.36m, и, согласно шкале Бортля, видна невооружённым глазом даже на городском небе (англ. City sky). (ru)
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  • σ Persei (en)
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  • http://commons.wikimedia.org/wiki/Special:FilePath/Perseus_constellation_map.svg
  • http://commons.wikimedia.org/wiki/Special:FilePath/Red_circle.svg
  • http://commons.wikimedia.org/wiki/Special:FilePath/Sigma_Persei.jpg
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