"\u304E\u3087\u3057\u3083\u5EA7\u03C81\u661F\u306F\u3001\u592A\u967D\u304B\u3089\u7D044,000\u5149\u5E74\u96E2\u308C\u305F\u3068\u3053\u308D\u306B\u3042\u308B \u8D64\u8272\u8D85\u5DE8\u661F\u3002\u5B66\u540D\u306F\u03C81Aurigae\uFF08\u7565\u79F0\u306F\u03C81Aur\uFF09\u3067\u3001\u5149\u5EA6\u306F\u592A\u967D\u306E\u7D0463,000\u500D\u3042\u308B\u3068\u3055\u308C\u3066\u3044\u308B\u3002\u3053\u306E\u6052\u661F\u306F\u304E\u3087\u3057\u3083\u5EA7\u306E\u4E2D\u306B\u4F4D\u7F6E\u3057\u3066\u304A\u308A\u30014.54\u7B49\u30685.7\u7B49\u306E\u9593\u3092\u5909\u5149\u3059\u308BLC\u578B\u306E\u8108\u52D5\u5909\u5149\u661F\u3067\u3042\u308B\u3002"@ja . . . . "14.4"^^ . "+4.7"@en . . . . "K5-M1Iab-Ib"@en . . . "4.91"^^ . . "726"^^ . "Psi1 Aurigae"@es . . . "Psi1 Aurigae (\u03C81 Aur, \u03C81 Aurigae) is a star in the northern constellation of Auriga. It is faintly visible to the naked eye with an apparent visual magnitude of 4.91. Based upon a measured annual parallax shift of 0.44 mas, it is approximately 7,500 light-years (2,300 parsecs) distant from the Earth. It is receding from the Sun with a radial velocity of +4.7 km/s. This is a massive supergiant star with a stellar classification of K5-M1Iab-Ib. It is a slow irregular variable of the LC type, with its brightness varying in magnitude by 0.44. The star is more than 14 times as massive as the Sun and is blazing with 63,579 times the Sun's luminosity. This energy is being radiated into outer space from its outer atmosphere at an effective temperature of 3,750 K, giving it the orange-red hue of a cool M-type star."@en . "\u5EA7\u65D7\u589E\u4E00"@zh . . . . . "\u041F\u0441\u0438\u00B9 \u0412\u043E\u0437\u043D\u0438\u0447\u0435\u0433\u043E"@ru . . "Psi1 Aurigae (\u03C81 Aur / \u03C81 Aurigae) adalah salah satu bintang di rasi Auriga. \u03C81 Aurigae adalah bintang supraraksasa jingga tipe K (orange K-type supergiant) dengan magnitudo rata-rata 4.92. Bintang ini berada pada jarak 3835 tahun cahaya dari Bumi."@in . . . . . . "J2000"@en . . "Psi1 Aurigae"@it . "\u5EA7\u65D7\u589E\u4E00\uFF08\u03C81Aurigae/\u5FA1\u592B\u5EA7\u03C81\uFF09\uFF0C\u662F\u5FA1\u592B\u5EA7\u7684\u4E00\u9897\u6052\u661F\u3002\u89C6\u661F\u7B494.91\uFF0C\u88F8\u773C\u89C2\u6D4B\u663E\u5F97\u5FAE\u4EAE\u3002\u6BCF\u5E74\u6D4B\u91CF\u7684\u65F6\u5DEE\u6570\u636E\u4E3A0.82\uFF0C\u6839\u636E\u8FD9\u4E2A\u6570\u636E\u53EF\u4EE5\u63A8\u5BFC\u51FA\u8DDD\u79BB\u5730\u74034000\u5149\u5E74\uFF081200\u79D2\u5DEE\u8DDD\uFF09\u3002 \u7531\u6052\u661F\u5149\u8C31\u53EF\u5F97\u5EA7\u65D7\u589E\u4E00\u4E3A\u4E00\u9897M\u578B\u7EA2\u5DE8\u661F\u3002\u5E76\u4E14\u5EA7\u65D7\u589E\u4E00\u662F\u4E00\u9897\u4EAE\u5EA6\u53D8\u5316\u5E45\u5EA6\u4E3A0.44\u7684LC\u578B\u6162\u4E0D\u89C4\u5219\u53D8\u661F\uFF0C \u5B83\u7684\u8D28\u91CF\u662F\u592A\u9633\u768414\u500D\uFF0C\u4EAE\u5EA6\u662F\u592A\u9633\u768463,579\u500D\uFF0C\u5176\u5916\u5927\u6C14\u5C42\u6709\u6548\u6E29\u5EA63750K\uFF0C\u56E0\u6B64\u663E\u793A\u51FA\u6A58\u7EA2\u8272\u3002"@zh . "Psi1 Aurigae (\u03C81 Aurigae / 46 Aurigae)\u200B es una estrella en la constelaci\u00F3n de la Auriga.Comparte la denominaci\u00F3n de Bayer \u00ABPsi\u00BB con otras nueve estrellas y tiene magnitud aparente +4,97.Es una estrella muy lejana cuya paralaje medida por Hipparcos (0,82 \u00B1 0,28 milisegundos de arco) es poco fiable.Un estudio la sit\u00FAa a una distancia aproximada de 817 p\u00E1rsecs (2660 a\u00F1os luz) del Sistema Solar.\u200B Psi1 Aurigae figura catalogada en la base de datos SIMBAD como una supergigante anaranjada de tipo espectral K5,\u200B pero recientemente se la ha reclasificado como supergigante roja de tipo M0I.\u200BTiene una temperatura efectiva entre 3750 y 3984 K\u200B\u200B\u200B y su luminosidad es 63.600 veces superior a la luminosidad solar.\u200BA partir de su di\u00E1metro angular \u20144,9 milisegundos de arco\u2014,\u200B se puede estimar su verdadero di\u00E1metro.Considerando que la distancia que nos separa de ella es de 817 p\u00E1rsecs, se puede estimar su di\u00E1metro real, siendo su valor aproximado 600 veces m\u00E1s grande que el di\u00E1metro solar.Por otra parte, presenta una metalicidad superior a la solar ([Fe/H] = +0,20).\u200BEs una estrella masiva de 14,4 masas solares,\u200B\u200B cifra que la sit\u00FAa claramente por encima del l\u00EDmite a partir del cual las estrellas finalizan su vida explosionando como supernovas.Tiene una edad de 12,3 \u00B1 0,4 millones de a\u00F1os.\u200B Psi1 Aurigae puede tener una o dos compa\u00F1eras estelares de las que nada se sabe.\u200BSu supuesta \u00ABvariabilidad\u00BB puede deberse a la presencia de una compa\u00F1era estelar cercana.\u200B"@es . ""@en . . . "+1.97"@en . . . . . . . . . "1124777439"^^ . "0.4426"^^ . . "Psi1 Aurigae"@in . . "Psi1 Aurigae"@en . . "8917"^^ . . . . "+2.29"@en . . . "+0.08"@en . "Psi1 Aurigae"@sv . . . . . . . . "0.1103"^^ . "63579"^^ . . . "Psi1 Aurigae (\u03C81 Aurigae, f\u00F6rkortat Psi1 Aur, \u03C81 Aur) som \u00E4r stj\u00E4rnans Bayerbeteckning, \u00E4r en ensam stj\u00E4rna bel\u00E4gen i den nord\u00F6stra delen av stj\u00E4rnbilden Kusken. Den har en skenbar magnitud p\u00E5 4,91 och \u00E4r svagt synlig f\u00F6r blotta \u00F6gat d\u00E4r ljusf\u00F6roreningar ej f\u00F6rekommer. Baserat p\u00E5 parallaxm\u00E4tning inom Hipparcosuppdraget p\u00E5 ca 0,82 mas, ber\u00E4knas den befinna sig p\u00E5 ett avst\u00E5nd p\u00E5 ca 4 000 ljus\u00E5r (ca 1 200 parsek) fr\u00E5n solen. Den \u00E4r en l\u00E5ngsam irregulj\u00E4r variabel av LC-typ, vars magnitud varierar i storleksordningen 0,44."@sv . . "12.3"^^ . "Psi1 Aurigae (\u03C81 Aur, \u03C81 Aurigae) is a star in the northern constellation of Auriga. It is faintly visible to the naked eye with an apparent visual magnitude of 4.91. Based upon a measured annual parallax shift of 0.44 mas, it is approximately 7,500 light-years (2,300 parsecs) distant from the Earth. It is receding from the Sun with a radial velocity of +4.7 km/s."@en . . . . . . "3750"^^ . "Psi1 Aurigae"@pt . . . . "Psi1 Aurigae (\u03C81 Aur / \u03C81 Aurigae) \u00E8 una stella supergigante arancione di magnitudine 4,97 situata nella costellazione dell'Auriga. Dista 3837 anni luce dal sistema solare."@it . "\u304E\u3087\u3057\u3083\u5EA7\u30D7\u30B5\u30A41\u661F"@ja . . "\u20132.131"@en . "Psi1 Aurigae (\u03C81 Aurigae, f\u00F6rkortat Psi1 Aur, \u03C81 Aur) som \u00E4r stj\u00E4rnans Bayerbeteckning, \u00E4r en ensam stj\u00E4rna bel\u00E4gen i den nord\u00F6stra delen av stj\u00E4rnbilden Kusken. Den har en skenbar magnitud p\u00E5 4,91 och \u00E4r svagt synlig f\u00F6r blotta \u00F6gat d\u00E4r ljusf\u00F6roreningar ej f\u00F6rekommer. Baserat p\u00E5 parallaxm\u00E4tning inom Hipparcosuppdraget p\u00E5 ca 0,82 mas, ber\u00E4knas den befinna sig p\u00E5 ett avst\u00E5nd p\u00E5 ca 4 000 ljus\u00E5r (ca 1 200 parsek) fr\u00E5n solen. Den \u00E4r en l\u00E5ngsam irregulj\u00E4r variabel av LC-typ, vars magnitud varierar i storleksordningen 0,44."@sv . "\u304E\u3087\u3057\u3083\u5EA7\u03C81\u661F\u306F\u3001\u592A\u967D\u304B\u3089\u7D044,000\u5149\u5E74\u96E2\u308C\u305F\u3068\u3053\u308D\u306B\u3042\u308B \u8D64\u8272\u8D85\u5DE8\u661F\u3002\u5B66\u540D\u306F\u03C81Aurigae\uFF08\u7565\u79F0\u306F\u03C81Aur\uFF09\u3067\u3001\u5149\u5EA6\u306F\u592A\u967D\u306E\u7D0463,000\u500D\u3042\u308B\u3068\u3055\u308C\u3066\u3044\u308B\u3002\u3053\u306E\u6052\u661F\u306F\u304E\u3087\u3057\u3083\u5EA7\u306E\u4E2D\u306B\u4F4D\u7F6E\u3057\u3066\u304A\u308A\u30014.54\u7B49\u30685.7\u7B49\u306E\u9593\u3092\u5909\u5149\u3059\u308BLC\u578B\u306E\u8108\u52D5\u5909\u5149\u661F\u3067\u3042\u308B\u3002"@ja . . . . . "Psi1 Aurigae (46 Aurigae) \u00E9 uma estrela na dire\u00E7\u00E3o da constela\u00E7\u00E3o de Auriga. Possui uma ascens\u00E3o reta de 06h 24m 53.90s e uma declina\u00E7\u00E3o de +49\u00B0 17\u2032 16.4\u2033. Sua magnitude aparente \u00E9 igual a 4.92. Considerando sua dist\u00E2ncia de 3835 anos-luz em rela\u00E7\u00E3o \u00E0 Terra, sua magnitude absoluta \u00E9 igual a \u22125.43. Pertence \u00E0 classe espectral K5Iabvar. \u00C9 componente do sistema psi Aurigae."@pt . . . "\u041F\u0441\u0438\u00B9 \u0412\u043E\u0437\u043D\u0438\u0447\u0435\u0433\u043E (\u043B\u0430\u0442. \u03C8\u00B9 Aurigae), 46 \u0412\u043E\u0437\u043D\u0438\u0447\u0435\u0433\u043E (\u043B\u0430\u0442. 46 Aurigae), HD 44537 \u2014 \u043E\u0434\u0438\u043D\u043E\u0447\u043D\u0430\u044F \u043F\u0435\u0440\u0435\u043C\u0435\u043D\u043D\u0430\u044F \u0437\u0432\u0435\u0437\u0434\u0430 \u0432 \u0441\u043E\u0437\u0432\u0435\u0437\u0434\u0438\u0438 \u0412\u043E\u0437\u043D\u0438\u0447\u0435\u0433\u043E \u043D\u0430 \u0440\u0430\u0441\u0441\u0442\u043E\u044F\u043D\u0438\u0438 (\u0432\u044B\u0447\u0438\u0441\u043B\u0435\u043D\u043D\u043E\u043C \u0438\u0437 \u0437\u043D\u0430\u0447\u0435\u043D\u0438\u044F \u043F\u0430\u0440\u0430\u043B\u043B\u0430\u043A\u0441\u0430) \u043F\u0440\u0438\u0431\u043B\u0438\u0437\u0438\u0442\u0435\u043B\u044C\u043D\u043E 5 559 \u0441\u0432\u0435\u0442\u043E\u0432\u044B\u0445 \u043B\u0435\u0442 (\u043E\u043A\u043E\u043B\u043E 1 704 \u043F\u0430\u0440\u0441\u0435\u043A\u043E\u0432) \u043E\u0442 \u0421\u043E\u043B\u043D\u0446\u0430. \u0412\u0438\u0434\u0438\u043C\u0430\u044F \u0437\u0432\u0451\u0437\u0434\u043D\u0430\u044F \u0432\u0435\u043B\u0438\u0447\u0438\u043D\u0430 \u0437\u0432\u0435\u0437\u0434\u044B \u2014 \u043E\u0442 +4,68m \u0434\u043E +5,7m. \u0412\u043E\u0437\u0440\u0430\u0441\u0442 \u0437\u0432\u0435\u0437\u0434\u044B \u043E\u0446\u0435\u043D\u0438\u0432\u0430\u0435\u0442\u0441\u044F \u043A\u0430\u043A \u043E\u043A\u043E\u043B\u043E 12,3 \u043C\u043B\u043D \u043B\u0435\u0442."@ru . . . ""@en . "1.07"^^ . . . . . "\u041F\u0441\u0438\u00B9 \u0412\u043E\u0437\u043D\u0438\u0447\u0435\u0433\u043E (\u043B\u0430\u0442. \u03C8\u00B9 Aurigae), 46 \u0412\u043E\u0437\u043D\u0438\u0447\u0435\u0433\u043E (\u043B\u0430\u0442. 46 Aurigae), HD 44537 \u2014 \u043E\u0434\u0438\u043D\u043E\u0447\u043D\u0430\u044F \u043F\u0435\u0440\u0435\u043C\u0435\u043D\u043D\u0430\u044F \u0437\u0432\u0435\u0437\u0434\u0430 \u0432 \u0441\u043E\u0437\u0432\u0435\u0437\u0434\u0438\u0438 \u0412\u043E\u0437\u043D\u0438\u0447\u0435\u0433\u043E \u043D\u0430 \u0440\u0430\u0441\u0441\u0442\u043E\u044F\u043D\u0438\u0438 (\u0432\u044B\u0447\u0438\u0441\u043B\u0435\u043D\u043D\u043E\u043C \u0438\u0437 \u0437\u043D\u0430\u0447\u0435\u043D\u0438\u044F \u043F\u0430\u0440\u0430\u043B\u043B\u0430\u043A\u0441\u0430) \u043F\u0440\u0438\u0431\u043B\u0438\u0437\u0438\u0442\u0435\u043B\u044C\u043D\u043E 5 559 \u0441\u0432\u0435\u0442\u043E\u0432\u044B\u0445 \u043B\u0435\u0442 (\u043E\u043A\u043E\u043B\u043E 1 704 \u043F\u0430\u0440\u0441\u0435\u043A\u043E\u0432) \u043E\u0442 \u0421\u043E\u043B\u043D\u0446\u0430. \u0412\u0438\u0434\u0438\u043C\u0430\u044F \u0437\u0432\u0451\u0437\u0434\u043D\u0430\u044F \u0432\u0435\u043B\u0438\u0447\u0438\u043D\u0430 \u0437\u0432\u0435\u0437\u0434\u044B \u2014 \u043E\u0442 +4,68m \u0434\u043E +5,7m. \u0412\u043E\u0437\u0440\u0430\u0441\u0442 \u0437\u0432\u0435\u0437\u0434\u044B \u043E\u0446\u0435\u043D\u0438\u0432\u0430\u0435\u0442\u0441\u044F \u043A\u0430\u043A \u043E\u043A\u043E\u043B\u043E 12,3 \u043C\u043B\u043D \u043B\u0435\u0442."@ru . "Psi1 Aurigae (46 Aurigae) \u00E9 uma estrela na dire\u00E7\u00E3o da constela\u00E7\u00E3o de Auriga. Possui uma ascens\u00E3o reta de 06h 24m 53.90s e uma declina\u00E7\u00E3o de +49\u00B0 17\u2032 16.4\u2033. Sua magnitude aparente \u00E9 igual a 4.92. Considerando sua dist\u00E2ncia de 3835 anos-luz em rela\u00E7\u00E3o \u00E0 Terra, sua magnitude absoluta \u00E9 igual a \u22125.43. Pertence \u00E0 classe espectral K5Iabvar. \u00C9 componente do sistema psi Aurigae."@pt . . . . . . . . . . . . . "Psi1 Aurigae"@en . . . . "\u5EA7\u65D7\u589E\u4E00\uFF08\u03C81Aurigae/\u5FA1\u592B\u5EA7\u03C81\uFF09\uFF0C\u662F\u5FA1\u592B\u5EA7\u7684\u4E00\u9897\u6052\u661F\u3002\u89C6\u661F\u7B494.91\uFF0C\u88F8\u773C\u89C2\u6D4B\u663E\u5F97\u5FAE\u4EAE\u3002\u6BCF\u5E74\u6D4B\u91CF\u7684\u65F6\u5DEE\u6570\u636E\u4E3A0.82\uFF0C\u6839\u636E\u8FD9\u4E2A\u6570\u636E\u53EF\u4EE5\u63A8\u5BFC\u51FA\u8DDD\u79BB\u5730\u74034000\u5149\u5E74\uFF081200\u79D2\u5DEE\u8DDD\uFF09\u3002 \u7531\u6052\u661F\u5149\u8C31\u53EF\u5F97\u5EA7\u65D7\u589E\u4E00\u4E3A\u4E00\u9897M\u578B\u7EA2\u5DE8\u661F\u3002\u5E76\u4E14\u5EA7\u65D7\u589E\u4E00\u662F\u4E00\u9897\u4EAE\u5EA6\u53D8\u5316\u5E45\u5EA6\u4E3A0.44\u7684LC\u578B\u6162\u4E0D\u89C4\u5219\u53D8\u661F\uFF0C \u5B83\u7684\u8D28\u91CF\u662F\u592A\u9633\u768414\u500D\uFF0C\u4EAE\u5EA6\u662F\u592A\u9633\u768463,579\u500D\uFF0C\u5176\u5916\u5927\u6C14\u5C42\u6709\u6548\u6E29\u5EA63750K\uFF0C\u56E0\u6B64\u663E\u793A\u51FA\u6A58\u7EA2\u8272\u3002"@zh . . "\u20130.155"@en . . . . . "Psi1 Aurigae (\u03C81 Aur / \u03C81 Aurigae) adalah salah satu bintang di rasi Auriga. \u03C81 Aurigae adalah bintang supraraksasa jingga tipe K (orange K-type supergiant) dengan magnitudo rata-rata 4.92. Bintang ini berada pada jarak 3835 tahun cahaya dari Bumi."@in . . "Psi1 Aurigae (\u03C81 Aur / \u03C81 Aurigae) \u00E8 una stella supergigante arancione di magnitudine 4,97 situata nella costellazione dell'Auriga. Dista 3837 anni luce dal sistema solare."@it . . . . . . . . "Psi1 Aurigae (\u03C81 Aurigae / 46 Aurigae)\u200B es una estrella en la constelaci\u00F3n de la Auriga.Comparte la denominaci\u00F3n de Bayer \u00ABPsi\u00BB con otras nueve estrellas y tiene magnitud aparente +4,97.Es una estrella muy lejana cuya paralaje medida por Hipparcos (0,82 \u00B1 0,28 milisegundos de arco) es poco fiable.Un estudio la sit\u00FAa a una distancia aproximada de 817 p\u00E1rsecs (2660 a\u00F1os luz) del Sistema Solar.\u200B Psi1 Aurigae puede tener una o dos compa\u00F1eras estelares de las que nada se sabe.\u200BSu supuesta \u00ABvariabilidad\u00BB puede deberse a la presencia de una compa\u00F1era estelar cercana.\u200B"@es . "4989444"^^ . . "\u22125.53"@en .