. "Zeta Bootis (\u03B6 Bootis, f\u00F6rkortad Zeta Boo, \u03B6 Boo), som \u00E4r stj\u00E4rnans Bayer-beteckning, \u00E4r en dubbelstj\u00E4rna i s\u00F6dra delen av stj\u00E4rnbilden Bj\u00F6rnvaktaren. Den har en kombinerad skenbar magnitud av 3,78 och \u00E4r synlig f\u00F6r blotta \u00F6gat d\u00E4r ljusf\u00F6roreningar inte f\u00F6rekommer. Baserat p\u00E5 parallaxm\u00E4tning inom Hipparcosuppdraget p\u00E5 cirka 18,1 mas, ber\u00E4knas den befinna sig p\u00E5 ett avst\u00E5nd av cirka 180 ljus\u00E5r (55 parsek) fr\u00E5n solen."@sv . "Zeta Bootis (\u03B6 Bootis, f\u00F6rkortad Zeta Boo, \u03B6 Boo), som \u00E4r stj\u00E4rnans Bayer-beteckning, \u00E4r en dubbelstj\u00E4rna i s\u00F6dra delen av stj\u00E4rnbilden Bj\u00F6rnvaktaren. Den har en kombinerad skenbar magnitud av 3,78 och \u00E4r synlig f\u00F6r blotta \u00F6gat d\u00E4r ljusf\u00F6roreningar inte f\u00F6rekommer. Baserat p\u00E5 parallaxm\u00E4tning inom Hipparcosuppdraget p\u00E5 cirka 18,1 mas, ber\u00E4knas den befinna sig p\u00E5 ett avst\u00E5nd av cirka 180 ljus\u00E5r (55 parsek) fr\u00E5n solen."@sv . "Zeta del Bover"@ca . . "2737331"^^ . . . "\u0632\u064A\u062A\u0627 \u0627\u0644\u0639\u0648\u0627\u0621 \u0647\u0648 \u0646\u062C\u0645 \u0645\u0632\u062F\u0648\u062C \u064A\u0642\u0639 \u0641\u064A \u0643\u0648\u0643\u0628\u0629 \u0627\u0644\u0639\u0648\u0627\u0621 .\u064A\u062A\u0643\u0648\u064E\u0651\u0646\u064F \u0645\u0646 \u0646\u062C\u0645\u0627\u0646 \u0639\u0645\u0644\u0627\u0642\u0627\u0646 \u0648 \u0645\u0646 \u0646\u0641\u0633 \u0627\u0644\u062A\u0635\u0646\u064A\u0641 \u0627\u0644\u0646\u062C\u0645\u064A A2III ,\u0648\u064A\u0628\u0639\u062F\u0627\u0646 \u0647\u0630\u0627\u0646 \u0627\u0644\u0646\u062C\u0645\u0627\u0646 \u0639\u0646\u0627 180 \u0633\u0646\u0629 \u0636\u0648\u0626\u064A\u0629 ,\u0648 \u0628\u0642\u062F\u0631 \u0638\u0627\u0647\u0631\u064A +3,78 ,\u0648 \u0628\u0633\u0631\u0639\u0629 \u0634\u0639\u0627\u0639\u064A\u0629 \u062A\u0635\u0644 \u0625\u0644\u0649 \u22125,5 \u0643\u0645/\u062B\u0627 ,\u0648\u062A\u0628\u0644\u063A \u062D\u0631\u0627\u0631\u0629 \u0633\u0637\u062D\u0647 8750 \u0643\u0644\u0641\u0646 ,\u0648 \u0636\u064A\u0627\u0624\u0647 \u0623\u0642\u0648\u0649 \u062838 \u0645\u0631\u0629 \u0639\u0646 \u0636\u064A\u0627\u0621 \u0627\u0644\u0634\u0645\u0633 , \u0648 \u0643\u062A\u0644\u062A\u0647 2,3 \u0643\u062A\u0644\u0629 \u0634\u0645\u0633\u064A\u0629."@ar . . . . . . "Zeta Bo\u00F6tes is een dubbelster in het sterrenbeeld Ossenhoeder. Het systeem bestaat uit twee reuzensterren met de spectraalklasse A2 III. Terwijl de sterren een gezamenlijke magnitude van 3,78 hebben, hebben ze afzonderlijk een magnitude van 4,43 (Zeta Bo\u00F6tis A) en 4,83 (Zeta Bo\u00F6tis B)."@nl . . . . . . . . . . . "Zeta Bo\u00F6tis"@en . . . . "10095"^^ . "Zeta Bo\u00F6tes is een dubbelster in het sterrenbeeld Ossenhoeder. Het systeem bestaat uit twee reuzensterren met de spectraalklasse A2 III. Terwijl de sterren een gezamenlijke magnitude van 3,78 hebben, hebben ze afzonderlijk een magnitude van 4,43 (Zeta Bo\u00F6tis A) en 4,83 (Zeta Bo\u00F6tis B)."@nl . . "B"@en . . . . . . . "-11.08"^^ . "Zeta Bo\u00F6tis (\u03B6 Boo / \u03B6 Bo\u00F6tis) \u00E8 una stella binaria bianca nella sequenza principale di magnitudine 3,79 situata nella costellazione di Boote. Dista 180 anni luce dal sistema solare."@it . "Zeta Bo\u00F6tis"@in . "\u0632\u064A\u062A\u0627 \u0627\u0644\u0639\u0648\u0627\u0621"@ar . . . . "18.07"^^ . "A1V"@en . . . "\u0414\u0437\u0435\u0442\u0430 \u0412\u043E\u043B\u043E\u043F\u0430\u0441\u0430 (\u043B\u0430\u0442. \u03B6 Bo\u00F6tis), 30 \u0412\u043E\u043B\u043E\u043F\u0430\u0441\u0430 (\u043B\u0430\u0442. 30 Bo\u00F6tis) \u2014 \u0442\u0440\u043E\u0439\u043D\u0430\u044F \u0437\u0432\u0435\u0437\u0434\u0430 \u0432 \u0441\u043E\u0437\u0432\u0435\u0437\u0434\u0438\u0438 \u0412\u043E\u043B\u043E\u043F\u0430\u0441\u0430 \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 176 \u0441\u0432\u0435\u0442\u043E\u0432\u044B\u0445 \u043B\u0435\u0442 (\u043E\u043A\u043E\u043B\u043E 53,9 \u043F\u0430\u0440\u0441\u0435\u043A\u043E\u0432) \u043E\u0442 \u0421\u043E\u043B\u043D\u0446\u0430. \u0412\u043E\u0437\u0440\u0430\u0441\u0442 \u0437\u0432\u0435\u0437\u0434\u044B \u043E\u043F\u0440\u0435\u0434\u0435\u043B\u0451\u043D \u043A\u0430\u043A \u043E\u043A\u043E\u043B\u043E 320 \u043C\u043B\u043D \u043B\u0435\u0442."@ru . "Zeta Bootis"@sv . "B"@en . . "+0.05"@en . . . "1079517975"^^ . "Zeta Bootis"@es . . . . . . . "\u0414\u0437\u0435\u0442\u0430 \u0412\u043E\u043B\u043E\u043F\u0430\u0441\u0430"@ru . . . "Zeta Bo\u00F6tis, Latinized from \u03B6 Bo\u00F6tis, is a binary star system in the constellation of Bo\u00F6tes. They have the Flamsteed designation 30 Bo\u00F6tis; Zeta Bo\u00F6tis is the Bayer designation. This system is visible to the naked eye with a combined apparent magnitude of +3.78. The individual magnitudes differ slightly, with component A having a magnitude of 4.46 and component B at the slightly dimmer magnitude 4.55. It is located at a distance of approximately 180 light years from the Sun based on parallax, but is drifting closer with a radial velocity of \u22129 km/s."@en . "Zeta Bootis"@fr . "\u0414\u0437\u0435\u0442\u0430 \u0412\u043E\u043B\u043E\u043F\u0430\u0441\u0430 (\u043B\u0430\u0442. \u03B6 Bo\u00F6tis), 30 \u0412\u043E\u043B\u043E\u043F\u0430\u0441\u0430 (\u043B\u0430\u0442. 30 Bo\u00F6tis) \u2014 \u0442\u0440\u043E\u0439\u043D\u0430\u044F \u0437\u0432\u0435\u0437\u0434\u0430 \u0432 \u0441\u043E\u0437\u0432\u0435\u0437\u0434\u0438\u0438 \u0412\u043E\u043B\u043E\u043F\u0430\u0441\u0430 \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 176 \u0441\u0432\u0435\u0442\u043E\u0432\u044B\u0445 \u043B\u0435\u0442 (\u043E\u043A\u043E\u043B\u043E 53,9 \u043F\u0430\u0440\u0441\u0435\u043A\u043E\u0432) \u043E\u0442 \u0421\u043E\u043B\u043D\u0446\u0430. \u0412\u043E\u0437\u0440\u0430\u0441\u0442 \u0437\u0432\u0435\u0437\u0434\u044B \u043E\u043F\u0440\u0435\u0434\u0435\u043B\u0451\u043D \u043A\u0430\u043A \u043E\u043A\u043E\u043B\u043E 320 \u043C\u043B\u043D \u043B\u0435\u0442."@ru . . "Zeta Bo\u00F6tis"@it . . . . . "\u3046\u3057\u304B\u3044\u5EA7\u03B6\u661F(\u03B6 Boo, \u03B6 Bootis)\u306F\u3001\u3046\u3057\u304B\u3044\u5EA7\u306B\u3042\u308B\u9023\u661F\u3067\u3042\u308A\u30012\u3064\u306E\u6052\u661F\u306F\u3069\u3061\u3089\u3082A2III\u578B\u3067\u3042\u308B\u3002\u30D5\u30E9\u30E0\u30B9\u30C6\u30A3\u30FC\u30C9\u756A\u53F7\u3067\u306F\u3001\u3046\u3057\u304B\u3044\u5EA730\u756A\u661F\u3068\u3044\u3046\u3002\u3053\u306E\u9023\u661F\u7CFB\u306F\u3001\u5730\u7403\u304B\u3089\u7D04180\u5149\u5E74\u96E2\u308C\u3001\u5408\u8A08\u306E\u8996\u7B49\u7D1A\u306F+3.78\u3067\u3042\u308B\u3002\u5404\u3005\u306E\u7B49\u7D1A\u306F\u82E5\u5E72\u7570\u306A\u308A\u3001A\u661F\u306F+4.43\u7B49\u7D1A\u3001B\u661F\u306F+4.83\u7B49\u7D1A\u3067\u3042\u308B\u3002 \u9023\u661F\u7CFB\u306E\u6027\u8CEA\u306F\u30011796\u5E74\u304B\u3089\u8ABF\u3079\u3089\u308C\u7D9A\u3051\u3066\u304A\u308A\u3001\u8ECC\u9053\u5468\u671F\u306F45,460\u65E5\uFF08124.46\u5E74\uFF09\u3067\u3042\u308B\u3002\u6B21\u56DE\u306F\u30012023\u5E748\u6708\u306B\u6700\u63A5\u8FD1\u3059\u308B\u30020.9977\u3068\u975E\u5E38\u306B\u9AD8\u3044\u8ECC\u9053\u96E2\u5FC3\u7387\u3067\u3042\u308A\u3001\u6700\u63A5\u8FD1\u3057\u305F\u6642\u306E\u8DDD\u96E2\u306F\u30010.3\u5929\u6587\u5358\u4F4D\u4EE5\u5185\u3067\u3042\u308B\u3002 \n* Zeta Bootis imaged with the 2000\u5E745\u670813\u65E5\u306B\u5317\u6B27\u5149\u5B66\u671B\u9060\u93E1\u3067\u3092\u7528\u3044\u3066\u64AE\u5F71\u3055\u308C\u305F\u5199\u771F\u3002\u6052\u661F\u306E\u5468\u308A\u306E\u30A8\u30A2\u30EA\u30FC\u30C7\u30A3\u30B9\u30AF\u306F\u30012.56m\u306E\u53E3\u5F84\u304B\u3089\u306E\u56DE\u6298\u3067\u3042\u308B\u3002 \n* \u30B9\u30DA\u30C3\u30AF\u30EB\u30FB\u30A4\u30E1\u30FC\u30B8\u30F3\u30B0\u3092\u7528\u3044\u3066\u77ED\u6642\u9593\u9732\u5149\u3067\u64AE\u5F71\u3055\u308C\u305F\u5199\u771F"@ja . "+51.95"@en . . . "A2III + A2III"@en . "Zeta Bootis (\u03B6 Boo / 30 Bootis / HIP 71795) es una estrella binaria de magnitud aparente +3,78 en la constelaci\u00F3n de Bootes, el pastor, cuyas componentes est\u00E1n separadas actualmente algo menos de 1 segundo de arco. Se encuentra a 180 a\u00F1os luz de distancia del Sistema Solar. Las dos componentes del sistema son dos estrellas blancas de tipo espectral A2 o A3 clasificadas como gigantes\u200B o subgigantes,\u200Baunque la relaci\u00F3n entre luminosidad y temperatura parece indicar que son estrellas de la secuencia principal.\u200B Las dos estrellas son muy similares: de brillo casi id\u00E9ntico (magnitudes +4,52 y +4,55), su temperatura superficial es de 8750 K y la luminosidad de cada una de ellas es 38 veces mayor que la del Sol.\u200B La separaci\u00F3n media entre las dos estrellas es 33 UA con un per\u00EDodo orbital de 123 a\u00F1os. La \u00F3rbita tiene una excentricidad muy alta, una de las mayores que se conocen, lo que hace que la distancia entre las componentes var\u00EDe entre 1,4 y 64 UA. Cuando la distancia es m\u00E1xima las estrellas se pueden separar con telescopio, mientras que con m\u00EDmina separaci\u00F3n (acaecida en 1897 y que vuelve a tener lugar en 2021) no se pueden resolver.\u200B"@es . . "1.24"^^ . . . . . . "+0.05"@en . "3.78"^^ . . "\u5DE6\u6444\u63D0\u4E09\uFF08\u7267\u592B\u5EA7\u03B6\uFF0C\u03B6 Boo\uFF09\u662F\u4E00\u500B\u4F4D\u4E8E\u7267\u592B\u5EA7\u7684\u4EAE\u96D9\u661F\u7CFB\u7D71\u3002\u5176\u4F9D\u7167\u4F5B\u6C0F\u547D\u540D\u6CD5\u4E5F\u7A31\u7232\u7267\u592B\u5EA730\uFF0830 Bo\u00F6tis\uFF09\u3002\u7267\u592B\u5EA7\u03B6\u5927\u7D04\u8DDD\u96E2\u5730\u7403181\u5149\u5E74\uFF0C\u5176\u7D44\u6210\u7684\u5169\u9846\u661F\u7D50\u5408\u7684\u8996\u661F\u7B49\u70BA+3.78\u3002\u7267\u592B\u5EA7\u03B6\u88AB\u8A8D\u7232\u5C6C\u65BC\u5927\u718A\u5EA7\u79FB\u52D5\u661F\u7FA4\u3002 \u76EE\u524D\uFF0C\u7267\u592B\u5EA7\u03B6\u7684\u5169\u9846\u661F\u4E4B\u9593\u7684\u89D2\u5EA6\u8DDD\u96E2\u70BA0.8\"\uFF08\u6B64\u6578\u5B57\u5728\u5169\u9846\u6046\u661F\u4E92\u76F8\u516C\u8F49\u6642\u6703\u6709\u6240\u8B8A\u52D5\uFF09\uFF0C\u56E0\u6B64\u7267\u592B\u5EA7\u03B6\u5E38\u88AB\u7528\u4F5C\u6E2C\u8A66\u65B0\u7684\u9AD8\u7CBE\u5EA6\u62CD\u651D\u6280\u8853\u3002\u5176\u7D44\u6210\u7684\u5169\u9846\u6046\u661F\u90FD\u662F\u767D\u8272\u7684A\u578B\u5DE8\u661F\uFF0C\u8996\u661F\u7B49\u5206\u5225\u70BA+4.43\u548C+4.83\u3002"@zh . . . . . . . "J2000"@en . . . "Zeta Bootis (\u03B6 Boo / 30 Bootis / HIP 71795) es una estrella binaria de magnitud aparente +3,78 en la constelaci\u00F3n de Bootes, el pastor, cuyas componentes est\u00E1n separadas actualmente algo menos de 1 segundo de arco. Se encuentra a 180 a\u00F1os luz de distancia del Sistema Solar."@es . . . . . . . "Zeta Bo\u00F6tis (\u03B6 Boo / \u03B6 Bo\u00F6tis) adalah bintang ganda yang cemerlang di rasi Bo\u00F6tes. Bintang ini berada pada jarak 180 tahun cahaya dari Bumi dan memiliki magnitudo kombinasi 3.78. Kedua komponennya adalah bintang raksasa putih tipe A (A-type giant star) dengan magnitudo masing-masing +4.43 dan +4.83. \n* Zeta Bootis imaged with the on 13 May 2000 using the method. (The around the stars is from the 2.56m telescope aperture.) \n* Typical short-exposure image of a binary star, as seen using through the Earth's atmosphere."@in . . . "Zeta Bo\u00F6tis (\u03B6 Boo / \u03B6 Bo\u00F6tis) \u00E8 una stella binaria bianca nella sequenza principale di magnitudine 3,79 situata nella costellazione di Boote. Dista 180 anni luce dal sistema solare."@it . . . . . . "Zeta Bo\u00F6tis"@nl . . . . . "Zeta Bootis (\u03B6 Boo, \u03B6 Bootis) est une \u00E9toile binaire de la constellation du Bouvier constitu\u00E9e de deux \u00E9toiles g\u00E9antes de m\u00EAme type spectral A2III. Elles portent la d\u00E9signation de Flamsteed 30 Bootis. Ce syst\u00E8me est \u00E0 environ 180 ann\u00E9es-lumi\u00E8re de la Terre et a une magnitude apparente combin\u00E9e de +3,78. Les magnitudes individuelles diff\u00E8rent l\u00E9g\u00E8rement, la composante A ayant une magnitude de 4,43 et la composante B une magnitude l\u00E9g\u00E8rement plus \u00E9lev\u00E9e de 4,83. La nature binaire de ce syst\u00E8me est connue depuis 1796. Elles accomplissent une orbite en environ 45460 jours, soit 124,46 ans. Le prochain rapprochement aura lieu en ao\u00FBt 2023. L'orbite de cette paire a une tr\u00E8s forte excentricit\u00E9 de 0,9977, amenant les \u00E9toiles \u00E0 moins de 0,3 UA l'une de l'autre. \n* Zeta Bootis photographi\u00E9e par le Nordic Optical Telescope le 13 mai 2000 avec la m\u00E9thode de lucky imaging (les disques d'Airy autour des \u00E9toiles proviennent de la diffraction due \u00E0 l'ouverture de 2,56 m du t\u00E9lescope). \n* Image typique \u00E0 courte pose d'une \u00E9toile binaire, vue par interf\u00E9rom\u00E9trie des tavelures \u00E0 travers l'atmosph\u00E8re terrestre."@fr . "+0.13"@en . . . . . . . "Zeta del Bover (\u03B6 Bootis) \u00E9s un estel binari de magnitud aparent +3,78 en la constel\u00B7laci\u00F3 del Bover, el pastor, les components del qual estan separades actualment una poc menys d'1 segon d'arc. Es troba a 180 anys llum de dist\u00E0ncia del Sistema Solar."@ca . "Zeta Bo\u00F6tis (\u03B6 Boo / \u03B6 Bo\u00F6tis) adalah bintang ganda yang cemerlang di rasi Bo\u00F6tes. Bintang ini berada pada jarak 180 tahun cahaya dari Bumi dan memiliki magnitudo kombinasi 3.78. Kedua komponennya adalah bintang raksasa putih tipe A (A-type giant star) dengan magnitudo masing-masing +4.43 dan +4.83. \n* Zeta Bootis imaged with the on 13 May 2000 using the method. (The around the stars is from the 2.56m telescope aperture.) \n* Typical short-exposure image of a binary star, as seen using through the Earth's atmosphere."@in . . "\u5DE6\u6444\u63D0\u4E09"@zh . "\u03B6 Bo\u00F6tis"@en . . . . . . . "Zeta del Bover (\u03B6 Bootis) \u00E9s un estel binari de magnitud aparent +3,78 en la constel\u00B7laci\u00F3 del Bover, el pastor, les components del qual estan separades actualment una poc menys d'1 segon d'arc. Es troba a 180 anys llum de dist\u00E0ncia del Sistema Solar. Les dues components del sistema s\u00F3n dos estels blancs de tipus espectral A2 o A3 classificats com a gegants o subgegants, encara que la relaci\u00F3 entre lluminositat i temperatura sembla indicar que s\u00F3n estels de la seq\u00FC\u00E8ncia principal. Els dos estels s\u00F3n molt similars: de lluentor gaireb\u00E9 id\u00E8ntica (magnituds +4,52 i +4,55), la seva temperatura superficial \u00E9s de 8750 K i la lluminositat de cadascun d'ells \u00E9s 38 vegades major que la del Sol. La separaci\u00F3 mitjana entre els dos estels \u00E9s 33 ua amb un per\u00EDode orbital de 123 anys. L'\u00F2rbita t\u00E9 una excentricitat molt alta, una de les majors que es coneixen, la qual cosa fa que la dist\u00E0ncia entre les components vari\u00EF entre 1,4 i 64 ua. Quan la dist\u00E0ncia \u00E9s m\u00E0xima els estels es poden separar amb telescopi, mentre que amb m\u00EDmina separaci\u00F3 (esdevinguda en 1897 i que torna a tenir lloc en 2021) no es poden resoldre."@ca . "Zeta Bo\u00F6tis (30 Bo\u00F6tis) \u00E9 uma estrela dupla na dire\u00E7\u00E3o da constela\u00E7\u00E3o de Bo\u00F6tes. Possui uma ascens\u00E3o reta de 14h 41m 08.92s e uma declina\u00E7\u00E3o de +13\u00B0 43\u2032 42.0\u2033. Sua magnitude aparente \u00E9 igual a 3.78. Considerando sua dist\u00E2ncia de 180 anos-luz em rela\u00E7\u00E3o \u00E0 Terra, sua magnitude absoluta \u00E9 igual a 0.06. Pertence \u00E0 classe espectral A3IVn."@pt . "Zeta Bo\u00F6tis"@pt . "A"@en . . . . . . . . . . . "Zeta Bootis (\u03B6 Boo, \u03B6 Bootis) est une \u00E9toile binaire de la constellation du Bouvier constitu\u00E9e de deux \u00E9toiles g\u00E9antes de m\u00EAme type spectral A2III. Elles portent la d\u00E9signation de Flamsteed 30 Bootis. Ce syst\u00E8me est \u00E0 environ 180 ann\u00E9es-lumi\u00E8re de la Terre et a une magnitude apparente combin\u00E9e de +3,78. Les magnitudes individuelles diff\u00E8rent l\u00E9g\u00E8rement, la composante A ayant une magnitude de 4,43 et la composante B une magnitude l\u00E9g\u00E8rement plus \u00E9lev\u00E9e de 4,83. \n* \n* Image typique \u00E0 courte pose d'une \u00E9toile binaire, vue par interf\u00E9rom\u00E9trie des tavelures \u00E0 travers l'atmosph\u00E8re terrestre."@fr . "Zeta Bo\u00F6tis, Latinized from \u03B6 Bo\u00F6tis, is a binary star system in the constellation of Bo\u00F6tes. They have the Flamsteed designation 30 Bo\u00F6tis; Zeta Bo\u00F6tis is the Bayer designation. This system is visible to the naked eye with a combined apparent magnitude of +3.78. The individual magnitudes differ slightly, with component A having a magnitude of 4.46 and component B at the slightly dimmer magnitude 4.55. It is located at a distance of approximately 180 light years from the Sun based on parallax, but is drifting closer with a radial velocity of \u22129 km/s. The duplicity of this star was discovered by English astronomer William Herschel in 1796, and their changing positions have been tracked from 1823 onward. They complete an orbit roughly every 124.5 years (45,460 days). The orbit of this pair has a very high eccentricity of 0.9977, bringing the stars within 0.3 AU at their closest approach. The next close approach will occur during August 2023. In 1976, T. W. Edwards found a stellar classification of A2III for both components, suggesting they may be evolved A-type giant stars. Helmut A. Abt reported a class of A2V in 1981, which matches an A-type main-sequence star. Abt and Nidia Morrell updated the classification to A1V in 1995. Considering the extreme nature of their orbit, it is unlikely that any companion exoplanets could have stable orbits around either star."@en . . "81"^^ . . . . . . "\u3046\u3057\u304B\u3044\u5EA7\u03B6\u661F(\u03B6 Boo, \u03B6 Bootis)\u306F\u3001\u3046\u3057\u304B\u3044\u5EA7\u306B\u3042\u308B\u9023\u661F\u3067\u3042\u308A\u30012\u3064\u306E\u6052\u661F\u306F\u3069\u3061\u3089\u3082A2III\u578B\u3067\u3042\u308B\u3002\u30D5\u30E9\u30E0\u30B9\u30C6\u30A3\u30FC\u30C9\u756A\u53F7\u3067\u306F\u3001\u3046\u3057\u304B\u3044\u5EA730\u756A\u661F\u3068\u3044\u3046\u3002\u3053\u306E\u9023\u661F\u7CFB\u306F\u3001\u5730\u7403\u304B\u3089\u7D04180\u5149\u5E74\u96E2\u308C\u3001\u5408\u8A08\u306E\u8996\u7B49\u7D1A\u306F+3.78\u3067\u3042\u308B\u3002\u5404\u3005\u306E\u7B49\u7D1A\u306F\u82E5\u5E72\u7570\u306A\u308A\u3001A\u661F\u306F+4.43\u7B49\u7D1A\u3001B\u661F\u306F+4.83\u7B49\u7D1A\u3067\u3042\u308B\u3002 \u9023\u661F\u7CFB\u306E\u6027\u8CEA\u306F\u30011796\u5E74\u304B\u3089\u8ABF\u3079\u3089\u308C\u7D9A\u3051\u3066\u304A\u308A\u3001\u8ECC\u9053\u5468\u671F\u306F45,460\u65E5\uFF08124.46\u5E74\uFF09\u3067\u3042\u308B\u3002\u6B21\u56DE\u306F\u30012023\u5E748\u6708\u306B\u6700\u63A5\u8FD1\u3059\u308B\u30020.9977\u3068\u975E\u5E38\u306B\u9AD8\u3044\u8ECC\u9053\u96E2\u5FC3\u7387\u3067\u3042\u308A\u3001\u6700\u63A5\u8FD1\u3057\u305F\u6642\u306E\u8DDD\u96E2\u306F\u30010.3\u5929\u6587\u5358\u4F4D\u4EE5\u5185\u3067\u3042\u308B\u3002 \n* Zeta Bootis imaged with the 2000\u5E745\u670813\u65E5\u306B\u5317\u6B27\u5149\u5B66\u671B\u9060\u93E1\u3067\u3092\u7528\u3044\u3066\u64AE\u5F71\u3055\u308C\u305F\u5199\u771F\u3002\u6052\u661F\u306E\u5468\u308A\u306E\u30A8\u30A2\u30EA\u30FC\u30C7\u30A3\u30B9\u30AF\u306F\u30012.56m\u306E\u53E3\u5F84\u304B\u3089\u306E\u56DE\u6298\u3067\u3042\u308B\u3002 \n* \u30B9\u30DA\u30C3\u30AF\u30EB\u30FB\u30A4\u30E1\u30FC\u30B8\u30F3\u30B0\u3092\u7528\u3044\u3066\u77ED\u6642\u9593\u9732\u5149\u3067\u64AE\u5F71\u3055\u308C\u305F\u5199\u771F"@ja . . . . . . . ""@en . "\u0632\u064A\u062A\u0627 \u0627\u0644\u0639\u0648\u0627\u0621 \u0647\u0648 \u0646\u062C\u0645 \u0645\u0632\u062F\u0648\u062C \u064A\u0642\u0639 \u0641\u064A \u0643\u0648\u0643\u0628\u0629 \u0627\u0644\u0639\u0648\u0627\u0621 .\u064A\u062A\u0643\u0648\u064E\u0651\u0646\u064F \u0645\u0646 \u0646\u062C\u0645\u0627\u0646 \u0639\u0645\u0644\u0627\u0642\u0627\u0646 \u0648 \u0645\u0646 \u0646\u0641\u0633 \u0627\u0644\u062A\u0635\u0646\u064A\u0641 \u0627\u0644\u0646\u062C\u0645\u064A A2III ,\u0648\u064A\u0628\u0639\u062F\u0627\u0646 \u0647\u0630\u0627\u0646 \u0627\u0644\u0646\u062C\u0645\u0627\u0646 \u0639\u0646\u0627 180 \u0633\u0646\u0629 \u0636\u0648\u0626\u064A\u0629 ,\u0648 \u0628\u0642\u062F\u0631 \u0638\u0627\u0647\u0631\u064A +3,78 ,\u0648 \u0628\u0633\u0631\u0639\u0629 \u0634\u0639\u0627\u0639\u064A\u0629 \u062A\u0635\u0644 \u0625\u0644\u0649 \u22125,5 \u0643\u0645/\u062B\u0627 ,\u0648\u062A\u0628\u0644\u063A \u062D\u0631\u0627\u0631\u0629 \u0633\u0637\u062D\u0647 8750 \u0643\u0644\u0641\u0646 ,\u0648 \u0636\u064A\u0627\u0624\u0647 \u0623\u0642\u0648\u0649 \u062838 \u0645\u0631\u0629 \u0639\u0646 \u0636\u064A\u0627\u0621 \u0627\u0644\u0634\u0645\u0633 , \u0648 \u0643\u062A\u0644\u062A\u0647 2,3 \u0643\u062A\u0644\u0629 \u0634\u0645\u0633\u064A\u0629."@ar . "\u5DE6\u6444\u63D0\u4E09\uFF08\u7267\u592B\u5EA7\u03B6\uFF0C\u03B6 Boo\uFF09\u662F\u4E00\u500B\u4F4D\u4E8E\u7267\u592B\u5EA7\u7684\u4EAE\u96D9\u661F\u7CFB\u7D71\u3002\u5176\u4F9D\u7167\u4F5B\u6C0F\u547D\u540D\u6CD5\u4E5F\u7A31\u7232\u7267\u592B\u5EA730\uFF0830 Bo\u00F6tis\uFF09\u3002\u7267\u592B\u5EA7\u03B6\u5927\u7D04\u8DDD\u96E2\u5730\u7403181\u5149\u5E74\uFF0C\u5176\u7D44\u6210\u7684\u5169\u9846\u661F\u7D50\u5408\u7684\u8996\u661F\u7B49\u70BA+3.78\u3002\u7267\u592B\u5EA7\u03B6\u88AB\u8A8D\u7232\u5C6C\u65BC\u5927\u718A\u5EA7\u79FB\u52D5\u661F\u7FA4\u3002 \u76EE\u524D\uFF0C\u7267\u592B\u5EA7\u03B6\u7684\u5169\u9846\u661F\u4E4B\u9593\u7684\u89D2\u5EA6\u8DDD\u96E2\u70BA0.8\"\uFF08\u6B64\u6578\u5B57\u5728\u5169\u9846\u6046\u661F\u4E92\u76F8\u516C\u8F49\u6642\u6703\u6709\u6240\u8B8A\u52D5\uFF09\uFF0C\u56E0\u6B64\u7267\u592B\u5EA7\u03B6\u5E38\u88AB\u7528\u4F5C\u6E2C\u8A66\u65B0\u7684\u9AD8\u7CBE\u5EA6\u62CD\u651D\u6280\u8853\u3002\u5176\u7D44\u6210\u7684\u5169\u9846\u6046\u661F\u90FD\u662F\u767D\u8272\u7684A\u578B\u5DE8\u661F\uFF0C\u8996\u661F\u7B49\u5206\u5225\u70BA+4.43\u548C+4.83\u3002"@zh . . . . . "Zeta Bo\u00F6tis (30 Bo\u00F6tis) \u00E9 uma estrela dupla na dire\u00E7\u00E3o da constela\u00E7\u00E3o de Bo\u00F6tes. Possui uma ascens\u00E3o reta de 14h 41m 08.92s e uma declina\u00E7\u00E3o de +13\u00B0 43\u2032 42.0\u2033. Sua magnitude aparente \u00E9 igual a 3.78. Considerando sua dist\u00E2ncia de 180 anos-luz em rela\u00E7\u00E3o \u00E0 Terra, sua magnitude absoluta \u00E9 igual a 0.06. Pertence \u00E0 classe espectral A3IVn."@pt . "\u3046\u3057\u304B\u3044\u5EA7\u30BC\u30FC\u30BF\u661F"@ja . .