"\u2265"@en . . . . . "Delta Aurigae (\u03B4 Aur/\u03B4 Aurigae) est une \u00E9toile binaire de la constellation du Cocher situ\u00E9e approximativement \u00E0 140 al de la Terre. Situ\u00E9e sur l'ascension droite 6h (comme \u03C0, \u03B2 et \u03B8 Aurigae) et ayant une d\u00E9clinaison de plus de 54\u00B0N, Delta Aurigae est th\u00E9oriquement circumpolaire d\u00E8s la latitude 36\u00B0N."@fr . . . . "Delta Aurigae"@es . . "\u304E\u3087\u3057\u3083\u5EA7\u30C7\u30EB\u30BF\u661F"@ja . "Delta Aurigae (\u03B4 Aur/\u03B4 Aurigae) est une \u00E9toile binaire de la constellation du Cocher situ\u00E9e approximativement \u00E0 140 al de la Terre. Situ\u00E9e sur l'ascension droite 6h (comme \u03C0, \u03B2 et \u03B8 Aurigae) et ayant une d\u00E9clinaison de plus de 54\u00B0N, Delta Aurigae est th\u00E9oriquement circumpolaire d\u00E8s la latitude 36\u00B0N."@fr . "\u2013142.928"@en . . "\u304E\u3087\u3057\u3083\u5EA7\u03B4\u661F\uFF08\u304E\u3087\u3057\u3083\u3056\u30C7\u30EB\u30BF\u305B\u3044\u3001\u03B4 Aur / \u03B4 Aurigae\uFF09\u306F\u3001\u304E\u3087\u3057\u3083\u5EA7\u306B\u4F4D\u7F6E\u3059\u308B\u591A\u91CD\u661F\u3067\u3042\u308B\u3002 \u300C\u4E3B\u661F\u300D\u306EA\u306F\u6A59\u8272\u306EK\u578B\u5DE8\u661F\u3067\u3001+3.83\u7B49\u7D1A\u3067\u3042\u308B\u3002\u300C\u4F34\u661F\u300D\u306F\u3001B\u304C+10.6\u7B49\u7D1A\u3067124.4\u79D2\u96E2\u308C\u3066\u304A\u308A\u3001C\u304C+10.1\u7B49\u7D1A\u3067195.5\u79D2\u96E2\u308C\u3066\u3044\u308B\u3002\u66F4\u306B\u3001C\u3082\u4E8C\u91CD\u661F\u3067\u300194.3\u79D2\u96E2\u308C\u305F+11.4\u7B49\u306E\u300C\u4F34\u661F\u300DD\u304C\u3042\u308B\u3002\u3053\u308C\u3089\u306F\u5168\u3066\u898B\u304B\u3051\u306E\u91CD\u661F\u3067\u3001\u7269\u7406\u7684\u306A\u95A2\u4FC2\u306F\u306A\u3044\u3068\u8003\u3048\u3089\u308C\u308B\u3002 \u4E00\u65B9\u3067\u3001\u304E\u3087\u3057\u3083\u5EA7\u03B4\u661F\u306F\u5206\u5149\u9023\u661F\u3067\u3042\u308B\u3002\u591A\u6570\u306E\u5206\u5149\u89B3\u6E2C\u304B\u3089\u6C42\u3081\u305F\u8996\u7DDA\u901F\u5EA6\u306E\u5468\u671F\u7684\u306A\u5909\u52D5\u3092\u5206\u6790\u3057\u305F\u7D50\u679C\u3001\u516C\u8EE2\u5468\u671F\u306F1283.4\u65E5\u3001\u8ECC\u9053\u96E2\u5FC3\u7387\u306F0.231\u3068\u898B\u7A4D\u3082\u3089\u308C\u3066\u3044\u308B\u3002"@ja . . . . "Delta Aurigae"@pt . . . "Delta del Cotxer (\u03B4 Aurigae) \u00E9s un sistema estel\u00B7lar de la constel\u00B7laci\u00F3 del Cotxer. Est\u00E0 aproximadament a uns 140 anys llum de la Terra. El component primari, \u03B4 Aurigae A, \u00E9s una estrella gegant taronja del tipus K amb magnitud aparent +3,72. T\u00E9 tres companyes: \u03B4 Aurigae B, amb una magnitud aparent de +9,7, distant a 115,4 segons d'arc; a 197,1 segons d'arc de A es troba \u03B4 Aurigae C, que tamb\u00E9 t\u00E9 magnitud +9,7. Finalment, C \u00E9s, per ella mateixa, una bin\u00E0ria, amb una companya de magnitud 11a a 93,5 segons d'arc."@ca . . . "Delta Aurigae je hv\u011Bzda v souhv\u011Bzd\u00ED Vozky. Jedn\u00E1 se o astrometrickou dvojhv\u011Bzdu, tj. hv\u011Bzdu, kter\u00E1 se pohybuje po identifikovan\u00E9 ob\u011B\u017En\u00E9 dr\u00E1ze, ale bez viditeln\u00E9ho spole\u010Dn\u00EDka. Nav\u00EDc jde z\u0159ejm\u011B o sou\u010D\u00E1st komplikovan\u00E9ho syst\u00E9mu slo\u017Een\u00E9ho nejm\u00E9n\u011B ze \u010Dty\u0159 hv\u011Bzd. Delta Aurigae je hv\u011Bzda spektr\u00E1ln\u00ED klasifikace K0III, jde tedy o oran\u017Eov\u00E9ho obra o polom\u011Bru zhruba 11kr\u00E1t v\u011Bt\u0161\u00EDm ne\u017E m\u00E1 Slunce, z\u00E1\u0159iv\u00FD v\u00FDkon odpov\u00EDd\u00E1 zhruba 62n\u00E1sobku z\u00E1\u0159ivosti Slunce. Povrchov\u00E1 teplota je odhadov\u00E1na na 4786 kelvin\u016F, co\u017E je o n\u011Bco m\u00E9n\u011B ne\u017E u Slunce. Delta Aurigae se nach\u00E1z\u00ED zhruba 126 sv\u011Bteln\u00FDch let od Zem\u011B."@cs . . . . "23.0557"^^ . . "+1.017"@en . . "11516"^^ . "Delta Aurigae (Prijipati, Praja, 33 Aurigae) \u00E9 uma estrela na dire\u00E7\u00E3o da constela\u00E7\u00E3o de Auriga. Possui uma ascens\u00E3o reta de 05h 59m 31.55s e uma declina\u00E7\u00E3o de +54\u00B0 17\u2032 05.9\u2033. Sua magnitude aparente \u00E9 igual a 3.72. Considerando sua dist\u00E2ncia de 140 anos-luz em rela\u00E7\u00E3o \u00E0 Terra, sua magnitude absoluta \u00E9 igual a 0.55. Pertence \u00E0 classe espectral K0III."@pt . "\u304E\u3087\u3057\u3083\u5EA7\u03B4\u661F\uFF08\u304E\u3087\u3057\u3083\u3056\u30C7\u30EB\u30BF\u305B\u3044\u3001\u03B4 Aur / \u03B4 Aurigae\uFF09\u306F\u3001\u304E\u3087\u3057\u3083\u5EA7\u306B\u4F4D\u7F6E\u3059\u308B\u591A\u91CD\u661F\u3067\u3042\u308B\u3002 \u300C\u4E3B\u661F\u300D\u306EA\u306F\u6A59\u8272\u306EK\u578B\u5DE8\u661F\u3067\u3001+3.83\u7B49\u7D1A\u3067\u3042\u308B\u3002\u300C\u4F34\u661F\u300D\u306F\u3001B\u304C+10.6\u7B49\u7D1A\u3067124.4\u79D2\u96E2\u308C\u3066\u304A\u308A\u3001C\u304C+10.1\u7B49\u7D1A\u3067195.5\u79D2\u96E2\u308C\u3066\u3044\u308B\u3002\u66F4\u306B\u3001C\u3082\u4E8C\u91CD\u661F\u3067\u300194.3\u79D2\u96E2\u308C\u305F+11.4\u7B49\u306E\u300C\u4F34\u661F\u300DD\u304C\u3042\u308B\u3002\u3053\u308C\u3089\u306F\u5168\u3066\u898B\u304B\u3051\u306E\u91CD\u661F\u3067\u3001\u7269\u7406\u7684\u306A\u95A2\u4FC2\u306F\u306A\u3044\u3068\u8003\u3048\u3089\u308C\u308B\u3002 \u4E00\u65B9\u3067\u3001\u304E\u3087\u3057\u3083\u5EA7\u03B4\u661F\u306F\u5206\u5149\u9023\u661F\u3067\u3042\u308B\u3002\u591A\u6570\u306E\u5206\u5149\u89B3\u6E2C\u304B\u3089\u6C42\u3081\u305F\u8996\u7DDA\u901F\u5EA6\u306E\u5468\u671F\u7684\u306A\u5909\u52D5\u3092\u5206\u6790\u3057\u305F\u7D50\u679C\u3001\u516C\u8EE2\u5468\u671F\u306F1283.4\u65E5\u3001\u8ECC\u9053\u96E2\u5FC3\u7387\u306F0.231\u3068\u898B\u7A4D\u3082\u3089\u308C\u3066\u3044\u308B\u3002"@ja . "Delta Aurigae"@fr . . "0.5600000000000001"^^ . . "K0 IIIb"@en . "+0.837"@en . . . . . . . . . "\u516B\u7A40\u4E00\uFF0C\u5373\u5FA1\u592B\u5EA7\u03B4\uFF08\u03B4 Aur, \u03B4 Aurigae\uFF09\u662F\u4E00\u4E2A\u4F4D\u4E8E\u5FA1\u592B\u5EA7\u7684\u53CC\u661F\u7CFB\u7EDF\uFF0C\u8DDD\u79BB\u5730\u7403\u7EA6140\u5149\u5E74\u3002 \u516B\u7A40\u4E00\u7684\u4E3B\u661F\u662F\u4E00\u9897\u6A59\u8272K-\u578B\u5DE8\u661F\uFF0C\u89C6\u661F\u7B49\u4E3A+3.72\u3002\u5B83\u7684\u4F34\u661F\u89C6\u661F\u7B49\u4E3A+9.7\uFF0C\u8DDD\u79BB\u4E3B\u661F115.4\u89D2\u79D2\u3002 \u5728\u4E2D\u56FD\u53E4\u4EE3\u661F\u5B98\u7CFB\u7EDF\u4E2D\uFF0C\u5B83\u5C5E\u4E8E\u4E09\u57A3\u7D2B\u5FAE\u57A3\u7684\u661F\u5B98\u516B\u7A40\u7B2C\u4E00\u661F\uFF0C\u8FD9\u4E5F\u662F\u516B\u7A40\u4E00\u540D\u5B57\u7684\u6765\u7531\u3002\u5728\u5370\u5EA6\u5929\u6587\u5B66\u4E2D\uFF0C\u516B\u7A40\u4E00\u88AB\u79F0\u4E3APraj\u0101pati (\u092A\u094D\u0930\u091C\u093E\u092A\u0924\u093F), \u610F\u601D\u4E3A\u201C\u9020\u7269\u4E3B\u201D\u3002"@zh . . . . . "Delta Aurigae"@en . "2.7"^^ . . . "3.26"^^ . "Delta Aurigae (\u03B4 Aur / 33 Aurigae / HD 40035) es una estrella en la constelaci\u00F3n de Auriga de magnitud aparente +3,72, ocasionalmente conocida con el nombre de Prijipati. Se encuentra a 140 a\u00F1os luz de distancia del Sistema Solar. Dos compa\u00F1eras visuales de magnitud 10 y 11, esta \u00FAltima a su vez una estrella doble, no son compa\u00F1eras reales sino estrellas en la misma l\u00EDnea de visi\u00F3n."@es . "Delta Aurigae (\u03B4 Aurigae, f\u00F6rkortat Delta Aur, \u03B4 Aur) som \u00E4r stj\u00E4rnans Bayerbeteckning, \u00E4r en dubbelstj\u00E4rna bel\u00E4gen i den norra delen av stj\u00E4rnbilden Kusken. Den har en skenbar magnitud p\u00E5 3,72 och \u00E4r synlig f\u00F6r blotta \u00F6gat d\u00E4r ljusf\u00F6roreningar ej f\u00F6rekommer. Baserat p\u00E5 parallaxm\u00E4tning inom Hipparcosuppdraget p\u00E5 ca 25,9 mas, ber\u00E4knas den befinna sig p\u00E5 ett avst\u00E5nd p\u00E5 ca 126 ljus\u00E5r (ca 39 parsek) fr\u00E5n solen."@sv . "0.4512"^^ . . . . . . . . "Delta Aurigae (\u03B4 Aur / \u03B4 Aurigae) adalah suatu sistem bintang pada rasi bintang Auriga. Bintang ini berada pada jarak 140 tahun cahaya dari Bumi. Komponen primernya, \u03B4 Aurigae A, adalah bintang raksasa jingga (orange K-type giant) dengan magnitudo 3.72. Komponen lainnya, \u03B4 Aurigae B, dengan magnitudo +9.7, terpisah 115.4 arcseconds dari A. Pada jarak 197.1 arcseconds dari A, adalah \u03B4 Aurigae C, yang juga bermagnitudo 9.7. C sendiri merupakan bintang ganda dan pasangannya yang merupakan bintang dengan magnituo tingkat kesebelas magnitude terpisah 93.5 arcseconds dari C."@in . . "Delta Aurigae (Prijipati, Praja, 33 Aurigae) \u00E9 uma estrela na dire\u00E7\u00E3o da constela\u00E7\u00E3o de Auriga. Possui uma ascens\u00E3o reta de 05h 59m 31.55s e uma declina\u00E7\u00E3o de +54\u00B0 17\u2032 05.9\u2033. Sua magnitude aparente \u00E9 igual a 3.72. Considerando sua dist\u00E2ncia de 140 anos-luz em rela\u00E7\u00E3o \u00E0 Terra, sua magnitude absoluta \u00E9 igual a 0.55. Pertence \u00E0 classe espectral K0III."@pt . . "\u0414\u0435\u043B\u044C\u0442\u0430 \u0412\u043E\u0437\u043D\u0438\u0447\u0435\u0433\u043E (\u043B\u0430\u0442. \u03B4 Aurigae), 33 \u0412\u043E\u0437\u043D\u0438\u0447\u0435\u0433\u043E (\u043B\u0430\u0442. 33 Aurigae), HD 40035 \u2014 \u043A\u0440\u0430\u0442\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 \u043F\u0440\u0438\u0431\u043B\u0438\u0437\u0438\u0442\u0435\u043B\u044C\u043D\u043E 142 \u0441\u0432\u0435\u0442\u043E\u0432\u044B\u0445 \u043B\u0435\u0442 (\u043E\u043A\u043E\u043B\u043E 43 \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 +3,72m. \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 1,3 \u043C\u043B\u0440\u0434 \u043B\u0435\u0442."@ru . . "Delta Aurigae (\u03B4 Aur / \u03B4 Aurigae) \u00E8 una stella gigante arancione di magnitudine 3,74 situata nella costellazione dell'Auriga. Dista 140 anni luce dal sistema solare."@it . . . . "Delta Aurigae is een dubbelster in het sterrenbeeld Voerman. Een van de twee componenten is een reuzenster."@nl . . . "3.715"^^ . . . . "\uB9C8\uCC28\uBD80\uC790\uB9AC \uB378\uD0C0\uB294 \uACA8\uC6B8\uCCA0 \uBCC4\uC790\uB9AC\uC778 \uB9C8\uCC28\uBD80\uC790\uB9AC\uC758 \uB378\uD0C0 \uBCC4\uC774\uB2E4. \uC774 \uBCC4\uC758 \uB0A8\uCABD\uC5D0 \uC758 \uBCF5\uC0AC\uC810\uC774 \uC788\uB2E4. \uD0DC\uC591\uBCF4\uB2E4 11\uBC30 \uD070 \uBC18\uC9C0\uB984\uC744 \uAC00\uC9C0\uACE0 \uC788\uB294 \uAC70\uC131\uC774\uB2E4."@ko . "Delta Aurigae (\u03B4 Aur / \u03B4 Aurigae) adalah suatu sistem bintang pada rasi bintang Auriga. Bintang ini berada pada jarak 140 tahun cahaya dari Bumi. Komponen primernya, \u03B4 Aurigae A, adalah bintang raksasa jingga (orange K-type giant) dengan magnitudo 3.72. Komponen lainnya, \u03B4 Aurigae B, dengan magnitudo +9.7, terpisah 115.4 arcseconds dari A. Pada jarak 197.1 arcseconds dari A, adalah \u03B4 Aurigae C, yang juga bermagnitudo 9.7. C sendiri merupakan bintang ganda dan pasangannya yang merupakan bintang dengan magnituo tingkat kesebelas magnitude terpisah 93.5 arcseconds dari C."@in . "Delta Aurigae"@sv . . . . . . "\u0414\u0435\u043B\u044C\u0442\u0430 \u0412\u043E\u0437\u043D\u0438\u0447\u0435\u0433\u043E (\u043B\u0430\u0442. \u03B4 Aurigae), 33 \u0412\u043E\u0437\u043D\u0438\u0447\u0435\u0433\u043E (\u043B\u0430\u0442. 33 Aurigae), HD 40035 \u2014 \u043A\u0440\u0430\u0442\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 \u043F\u0440\u0438\u0431\u043B\u0438\u0437\u0438\u0442\u0435\u043B\u044C\u043D\u043E 142 \u0441\u0432\u0435\u0442\u043E\u0432\u044B\u0445 \u043B\u0435\u0442 (\u043E\u043A\u043E\u043B\u043E 43 \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 +3,72m. \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 1,3 \u043C\u043B\u0440\u0434 \u043B\u0435\u0442."@ru . "Delta Aurigae (\u03B4 Aur / 33 Aurigae / HD 40035) es una estrella en la constelaci\u00F3n de Auriga de magnitud aparente +3,72, ocasionalmente conocida con el nombre de Prijipati. Se encuentra a 140 a\u00F1os luz de distancia del Sistema Solar. Delta Aurigae es una gigante naranja de tipo espectral K0III con una temperatura superficial de 4825 K. Es una de las muchas estrellas de este tipo visibles a simple vista en cuyo interior se produce la fusi\u00F3n nuclear del helio. Con una luminosidad 47 veces mayor que la del Sol, su radio es 12 veces m\u00E1s grande que el radio solar. Su metalicidad es similar a la que posee el Sol. Tiene una masa aproximada de 2 masas solares y su edad se estima en 1300 millones de a\u00F1os. Delta Aurigae, Menkalinan (\u03B2 Aurigae) y \u03B8 Aurigae \u2014las tres en perfecta alineaci\u00F3n\u2014 se hallan a pocos minutos de arco del coluro solsticial, meridiano celeste que pasa a trav\u00E9s de los polos y de los dos solsticios situados en Sagitario y G\u00E9minis. Debido al movimiento de precesi\u00F3n de la Tierra su posici\u00F3n relativa al coluro ha ido cambiando con el tiempo, marcando la posici\u00F3n exacta del mismo a mediados de 2005. Dos compa\u00F1eras visuales de magnitud 10 y 11, esta \u00FAltima a su vez una estrella doble, no son compa\u00F1eras reales sino estrellas en la misma l\u00EDnea de visi\u00F3n."@es . "2893395"^^ . "\u516B\u7A40\u4E00"@zh . . . . "4786"^^ . . . "0.5"^^ . "1092407374"^^ . "Delta del Cotxer (\u03B4 Aurigae) \u00E9s un sistema estel\u00B7lar de la constel\u00B7laci\u00F3 del Cotxer. Est\u00E0 aproximadament a uns 140 anys llum de la Terra. El component primari, \u03B4 Aurigae A, \u00E9s una estrella gegant taronja del tipus K amb magnitud aparent +3,72. T\u00E9 tres companyes: \u03B4 Aurigae B, amb una magnitud aparent de +9,7, distant a 115,4 segons d'arc; a 197,1 segons d'arc de A es troba \u03B4 Aurigae C, que tamb\u00E9 t\u00E9 magnitud +9,7. Finalment, C \u00E9s, per ella mateixa, una bin\u00E0ria, amb una companya de magnitud 11a a 93,5 segons d'arc."@ca . . . . . . "Delta Aurigae"@cs . . . "\u0414\u0435\u043B\u044C\u0442\u0430 \u0412\u043E\u0437\u043D\u0438\u0447\u0435\u0433\u043E"@ru . "Delta Aurigae je hv\u011Bzda v souhv\u011Bzd\u00ED Vozky. Jedn\u00E1 se o astrometrickou dvojhv\u011Bzdu, tj. hv\u011Bzdu, kter\u00E1 se pohybuje po identifikovan\u00E9 ob\u011B\u017En\u00E9 dr\u00E1ze, ale bez viditeln\u00E9ho spole\u010Dn\u00EDka. Nav\u00EDc jde z\u0159ejm\u011B o sou\u010D\u00E1st komplikovan\u00E9ho syst\u00E9mu slo\u017Een\u00E9ho nejm\u00E9n\u011B ze \u010Dty\u0159 hv\u011Bzd. Delta Aurigae je hv\u011Bzda spektr\u00E1ln\u00ED klasifikace K0III, jde tedy o oran\u017Eov\u00E9ho obra o polom\u011Bru zhruba 11kr\u00E1t v\u011Bt\u0161\u00EDm ne\u017E m\u00E1 Slunce, z\u00E1\u0159iv\u00FD v\u00FDkon odpov\u00EDd\u00E1 zhruba 62n\u00E1sobku z\u00E1\u0159ivosti Slunce. Povrchov\u00E1 teplota je odhadov\u00E1na na 4786 kelvin\u016F, co\u017E je o n\u011Bco m\u00E9n\u011B ne\u017E u Slunce. Delta Aurigae se nach\u00E1z\u00ED zhruba 126 sv\u011Bteln\u00FDch let od Zem\u011B."@cs . "Delta Aurigae, Latinized from \u03B4 Aurigae, is the Bayer designation for an astrometric binary star in the northern constellation of Auriga. It is visible to the naked eye with an apparent visual magnitude of 3.715. Based upon its annual parallax shift of 23.06 mas, it is some 141 light-years (43 parsecs) distant from the Earth, give or take a three light-year margin of error. It is drifting further away with a radial velocity of +10 km/s. This star is the namesake for the Delta Aurigids, a meteor shower that occurs between October 6\u201315. The radiant point for this shower passes several degrees to the south of the star."@en . . "\u20130.15"@en . . "\uB9C8\uCC28\uBD80\uC790\uB9AC \uB378\uD0C0\uB294 \uACA8\uC6B8\uCCA0 \uBCC4\uC790\uB9AC\uC778 \uB9C8\uCC28\uBD80\uC790\uB9AC\uC758 \uB378\uD0C0 \uBCC4\uC774\uB2E4. \uC774 \uBCC4\uC758 \uB0A8\uCABD\uC5D0 \uC758 \uBCF5\uC0AC\uC810\uC774 \uC788\uB2E4. \uD0DC\uC591\uBCF4\uB2E4 11\uBC30 \uD070 \uBC18\uC9C0\uB984\uC744 \uAC00\uC9C0\uACE0 \uC788\uB294 \uAC70\uC131\uC774\uB2E4."@ko . . . . . . . . . "3.9"^^ . "+85.814"@en . "\u516B\u7A40\u4E00\uFF0C\u5373\u5FA1\u592B\u5EA7\u03B4\uFF08\u03B4 Aur, \u03B4 Aurigae\uFF09\u662F\u4E00\u4E2A\u4F4D\u4E8E\u5FA1\u592B\u5EA7\u7684\u53CC\u661F\u7CFB\u7EDF\uFF0C\u8DDD\u79BB\u5730\u7403\u7EA6140\u5149\u5E74\u3002 \u516B\u7A40\u4E00\u7684\u4E3B\u661F\u662F\u4E00\u9897\u6A59\u8272K-\u578B\u5DE8\u661F\uFF0C\u89C6\u661F\u7B49\u4E3A+3.72\u3002\u5B83\u7684\u4F34\u661F\u89C6\u661F\u7B49\u4E3A+9.7\uFF0C\u8DDD\u79BB\u4E3B\u661F115.4\u89D2\u79D2\u3002 \u5728\u4E2D\u56FD\u53E4\u4EE3\u661F\u5B98\u7CFB\u7EDF\u4E2D\uFF0C\u5B83\u5C5E\u4E8E\u4E09\u57A3\u7D2B\u5FAE\u57A3\u7684\u661F\u5B98\u516B\u7A40\u7B2C\u4E00\u661F\uFF0C\u8FD9\u4E5F\u662F\u516B\u7A40\u4E00\u540D\u5B57\u7684\u6765\u7531\u3002\u5728\u5370\u5EA6\u5929\u6587\u5B66\u4E2D\uFF0C\u516B\u7A40\u4E00\u88AB\u79F0\u4E3APraj\u0101pati (\u092A\u094D\u0930\u091C\u093E\u092A\u0924\u093F), \u610F\u601D\u4E3A\u201C\u9020\u7269\u4E3B\u201D\u3002"@zh . . "Delta del Cotxer"@ca . . . "Delta Aurigae is een dubbelster in het sterrenbeeld Voerman. Een van de twee componenten is een reuzenster."@nl . . . . . . . . . . . . . . . . . "J2000"@en . . . "11"^^ . . . . "Delta Aurigae"@it . . . . . . "Delta Aurigae"@nl . . . "Delta Aurigae (\u03B4 Aurigae, f\u00F6rkortat Delta Aur, \u03B4 Aur) som \u00E4r stj\u00E4rnans Bayerbeteckning, \u00E4r en dubbelstj\u00E4rna bel\u00E4gen i den norra delen av stj\u00E4rnbilden Kusken. Den har en skenbar magnitud p\u00E5 3,72 och \u00E4r synlig f\u00F6r blotta \u00F6gat d\u00E4r ljusf\u00F6roreningar ej f\u00F6rekommer. Baserat p\u00E5 parallaxm\u00E4tning inom Hipparcosuppdraget p\u00E5 ca 25,9 mas, ber\u00E4knas den befinna sig p\u00E5 ett avst\u00E5nd p\u00E5 ca 126 ljus\u00E5r (ca 39 parsek) fr\u00E5n solen."@sv . "Delta Aurigae, Latinized from \u03B4 Aurigae, is the Bayer designation for an astrometric binary star in the northern constellation of Auriga. It is visible to the naked eye with an apparent visual magnitude of 3.715. Based upon its annual parallax shift of 23.06 mas, it is some 141 light-years (43 parsecs) distant from the Earth, give or take a three light-year margin of error. It is drifting further away with a radial velocity of +10 km/s. This star is the namesake for the Delta Aurigids, a meteor shower that occurs between October 6\u201315. The radiant point for this shower passes several degrees to the south of the star. The variable radial velocity of this system was not recognized until 1999, more than a century following the first measurement in 1897. Delta Aurigae is a single-lined spectroscopic binary: periodic Doppler shifts in the star's spectrum indicate orbital motion. The pair have an orbital period of 1,283.4 days (3.514 years) and an eccentricity of 0.231. Based on the small amplitude of the radial velocity variation, the companion is most likely a small K- or early M-type main-sequence star with around half the mass of the Sun. The visible component of this system is an evolved giant star with a stellar classification of K0 IIIb. It is a member of the so-called \"red clump\", indicating that it is generating energy through helium fusion at its core. The star is 3.26 billion years old and is spinning with a projected rotational velocity of 4 km/s. It has 1.63 times the mass of the Sun and has expanded to 11 times the Sun's radius. The star is radiating 62 times the Sun's luminosity from the star's photosphere at an effective temperature of 4,786 K. This heat gives the star the orange-hued glow of a K-type star."@en . . . "\uB9C8\uCC28\uBD80\uC790\uB9AC \uB378\uD0C0"@ko . . . . . . "Delta Aurigae (\u03B4 Aur / \u03B4 Aurigae) \u00E8 una stella gigante arancione di magnitudine 3,74 situata nella costellazione dell'Auriga. Dista 140 anni luce dal sistema solare."@it . "Delta Aurigae"@in . . . . . . . . . . . . . . . . . . . . . . . "1.63"^^ . . . "62"^^ .