"Delta Bo\u00F6tis (\u03B4 Boo) \u2013 gwiazda podw\u00F3jna w gwiazdozbiorze Wolarza. Znajduje si\u0119 oko\u0142o 122 lata \u015Bwietlne od S\u0142o\u0144ca."@pl . . "BD+33 2561"@en . "0.87"^^ . . . . . "\u03B4 Bo\u00F6tis"@en . . . . "y"@en . "+0.951/"@en . . "Delta Bootis (Kurzform \u03B4 Boo, Flamsteed-Bezeichnung 49 Bootis) ist der vierthellste Stern im B\u00E4renh\u00FCter. Er stellt die linke Schulter des mythologischen Hirten Bootes dar, auf manchen Himmelsgloben auch seinen Hirtenstab. Der Stern 3. Gr\u00F6\u00DFe hat Spektralklasse G8. Er ist 117 Lichtjahre von uns entfernt und ist ein Doppelstern, der schon im Feldstecher deutlich trennbar ist: Winkeldistanz ca. 105\", Helligkeiten 3,5 und 8 mag."@de . . "\u20130.44"@en . . "Delta Bootis (\u03B4 Boo / 49 Bootis / HD 135722)\u200B es una estrella en la constelaci\u00F3n de Bootes de magnitud aparente +3,46.Sin nombre propio habitual, ocasionalmente es conocida como Princeps, \u00ABpr\u00EDncipe\u00BB o \u00ABprincipal\u00BB en lat\u00EDn.\u200BSe encuentra a 117 a\u00F1os luz de distancia del Sistema Solar. Delta Bootis es una gigante amarilla de tipo espectral G8III y 4990 K de temperatura, con una luminosidad 59 veces mayor que la del Sol. El valor de su di\u00E1metro, obtenido a partir de la medida de su di\u00E1metro angular, es 10,4 veces mayor que el del Sol. Su metalicidad es baja comparada a la solar, en torno al 40% de la misma; como resultado de ello, por su espectro est\u00E1 clasificada como una estrella con l\u00EDneas d\u00E9biles de CN (cian\u00F3geno).\u200B Delta Bootis tiene una compa\u00F1era estelar de magnitud +7,8, una enana de tipo espectral G0 similar al Sol. Sin embargo, su baja luminosidad \u2014un 80% de la solar\u2014 y su peque\u00F1o tama\u00F1o en relaci\u00F3n con su temperatura de 5900 K \u2014su radio equivale al 87% del radio solar\u2014, sugieren que puede ser una estrella subenana; ello concuerda con la baja metalicidad observada en Delta Bootis A. Visualmente est\u00E1n separadas casi 2 minutos de arco, lo que equivale a una separaci\u00F3n real de al menos a 3800 UA y un per\u00EDodo orbital de m\u00E1s de 120.000 a\u00F1os.\u200B"@es . . . . . . "\u0414\u0435\u043B\u044C\u0442\u0430 \u0412\u043E\u043B\u043E\u043F\u0430\u0441\u0430 (\u043B\u0430\u0442. \u03B4 Bo\u00F6tis), 49 \u0412\u043E\u043B\u043E\u043F\u0430\u0441\u0430 (\u043B\u0430\u0442. 49 Bo\u00F6tis), HD 135722 \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\u043B\u043E\u043F\u0430\u0441\u0430 \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 122 \u0441\u0432\u0435\u0442\u043E\u0432\u044B\u0445 \u043B\u0435\u0442 (\u043E\u043A\u043E\u043B\u043E 37,3 \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 2,18 \u043C\u043B\u0440\u0434 \u043B\u0435\u0442."@ru . . . . . . "3.09"^^ . . . . "Delta Bootis (Kurzform \u03B4 Boo, Flamsteed-Bezeichnung 49 Bootis) ist der vierthellste Stern im B\u00E4renh\u00FCter. Er stellt die linke Schulter des mythologischen Hirten Bootes dar, auf manchen Himmelsgloben auch seinen Hirtenstab. Der Stern 3. Gr\u00F6\u00DFe hat Spektralklasse G8. Er ist 117 Lichtjahre von uns entfernt und ist ein Doppelstern, der schon im Feldstecher deutlich trennbar ist: Winkeldistanz ca. 105\", Helligkeiten 3,5 und 8 mag."@de . . . . "\u0414\u0435\u043B\u044C\u0442\u0430 \u0412\u043E\u043B\u043E\u043F\u0430\u0441\u0430 (\u043B\u0430\u0442. \u03B4 Bo\u00F6tis), 49 \u0412\u043E\u043B\u043E\u043F\u0430\u0441\u0430 (\u043B\u0430\u0442. 49 Bo\u00F6tis), HD 135722 \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\u043B\u043E\u043F\u0430\u0441\u0430 \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 122 \u0441\u0432\u0435\u0442\u043E\u0432\u044B\u0445 \u043B\u0435\u0442 (\u043E\u043A\u043E\u043B\u043E 37,3 \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 2,18 \u043C\u043B\u0440\u0434 \u043B\u0435\u0442."@ru . "Delta Bo\u00F6tis (\u03B4 Boo / \u03B4 Bo\u00F6tis) merupakan salah satu bintang ganda pada rasi bintang Bo\u00F6tes. Bintang ini berada pada 117 tahun cahaya dari Bumi. Komponen primernya, \u03B4 Bo\u00F6tis A, adalah bintang kuning raksasa (yellow G-type giant) dengan magnitudo 3.46. Komponen lainnya, \u03B4 Bo\u00F6tis B, adalah bintang katai kuning (yellow G-type main sequence dwarf) dengan mangitudo 8.7."@in . "\u2013110.040"@en . . "Princeps (Delta Bo\u00F6tis/ \u03B4 Boo / \u03B4 Bo\u00F6tis) \u00E8 una stella binaria nella costellazione di Boote, dista circa 117 anni luce dal sistema solare."@it . . . "Delta Bootis (\u03B4 Boo, \u03B4 Bootis), som \u00E4r stj\u00E4rnans Bayerbeteckning, \u00E4r en dubbelstj\u00E4rna i den nordv\u00E4stra delen av stj\u00E4rnbilden Bj\u00F6rnvaktaren. Baserad p\u00E5 parallaxm\u00E4tningar, \u00E4r den bel\u00E4gen p\u00E5 ett avst\u00E5nd av omkring 121,8 ljus\u00E5r (37.3 parsecs) fr\u00E5n solen. Stj\u00E4rnan har en skenbar magnitud p\u00E5 3,5, vilket g\u00F6r den synlig f\u00F6r blotta \u00F6gat \u00E4ven under fullm\u00E5ne."@sv . . "Delta Bo\u00F6tis (Princeps, 49 Bo\u00F6tis) \u00E9 uma estrela na dire\u00E7\u00E3o da constela\u00E7\u00E3o de Bo\u00F6tes. Possui uma ascens\u00E3o reta de 15h 15m 30.10s e uma declina\u00E7\u00E3o de +33\u00B0 18\u2032 54.4\u2033. Sua magnitude aparente \u00E9 igual a 3.46. Considerando sua dist\u00E2ncia de 117 anos-luz em rela\u00E7\u00E3o \u00E0 Terra, sua magnitude absoluta \u00E9 igual a 0.69. Pertence \u00E0 classe espectral G8III."@pt . . "Delta Bo\u00F6tis"@pl . . "\u3046\u3057\u304B\u3044\u5EA7\u03B4\u661F\uFF08\u3046\u3057\u304B\u3044\u3056\u30C7\u30EB\u30BF\u305B\u3044\u3001\u03B4 Boo / \u03B4 Bo\u00F6tis\uFF09\u306F\u3001\u3046\u3057\u304B\u3044\u5EA7\u306E\u6052\u661F\u30673\u7B49\u661F\u3002 \u3053\u306E\u661F\u306F\u3001\u9023\u661F\u3067\u3042\u308B\u3002\u4E3B\u661F\u306F\u9EC4\u8272\u306E\u6E96\u5DE8\u661F\u3067\u3001\u4F34\u661F\u306F\u8996\u7B49\u7D1A+8.7\u306E\u9EC4\u8272\u306E\u4E3B\u7CFB\u5217\u661F\u3067\u3042\u308B\u3002\u6052\u661F\u9593\u306F3800\u5929\u6587\u5358\u4F4D\u96E2\u308C\u3066\u304A\u308A\u3001\u516C\u8EE2\u5468\u671F\u306F12\u4E07\u5E74\u3067\u3042\u308B\u3002"@ja . "G8 III"@en . "+0.656/"@en . . . . . . "Delta Bo\u00F6tis (Princeps, 49 Bo\u00F6tis) \u00E9 uma estrela na dire\u00E7\u00E3o da constela\u00E7\u00E3o de Bo\u00F6tes. Possui uma ascens\u00E3o reta de 15h 15m 30.10s e uma declina\u00E7\u00E3o de +33\u00B0 18\u2032 54.4\u2033. Sua magnitude aparente \u00E9 igual a 3.46. Considerando sua dist\u00E2ncia de 117 anos-luz em rela\u00E7\u00E3o \u00E0 Terra, sua magnitude absoluta \u00E9 igual a 0.69. Pertence \u00E0 classe espectral G8III."@pt . "ADS+9559"@en . "2903386"^^ . . "Delta Bootis"@es . "Delta Bootis"@de . "G0 V"@en . . . "\u2013111.58"@en . . . . . "Delta Bootis (\u03B4 Boo / \u03B4 Bootis) est une \u00E9toile binaire de la constellation du Bouvier. Elle est \u00E0 environ 122 ann\u00E9es-lumi\u00E8re de la Terre. La composante primaire, \u03B4 Bootis A, est une g\u00E9ante jaune de type G avec une magnitude apparente de +3,46. Sa compagne, \u03B4 Bootis B, est une naine jaune de la s\u00E9quence principale de type G avec une magnitude apparente de +8,7. Distantes d'environ 3800 UA, elles parcourent leur orbite en 120 000 ans environ."@fr . . . . . "Princeps (astronomia)"@it . . "BD+33 2562"@en . . . "Delta Bootis (\u03B4 Boo, \u03B4 Bootis), som \u00E4r stj\u00E4rnans Bayerbeteckning, \u00E4r en dubbelstj\u00E4rna i den nordv\u00E4stra delen av stj\u00E4rnbilden Bj\u00F6rnvaktaren. Baserad p\u00E5 parallaxm\u00E4tningar, \u00E4r den bel\u00E4gen p\u00E5 ett avst\u00E5nd av omkring 121,8 ljus\u00E5r (37.3 parsecs) fr\u00E5n solen. Stj\u00E4rnan har en skenbar magnitud p\u00E5 3,5, vilket g\u00F6r den synlig f\u00F6r blotta \u00F6gat \u00E4ven under fullm\u00E5ne."@sv . . "B"@en . . "+84.74"@en . "+0.02"@en . "\u3046\u3057\u304B\u3044\u5EA7\u03B4\u661F\uFF08\u3046\u3057\u304B\u3044\u3056\u30C7\u30EB\u30BF\u305B\u3044\u3001\u03B4 Boo / \u03B4 Bo\u00F6tis\uFF09\u306F\u3001\u3046\u3057\u304B\u3044\u5EA7\u306E\u6052\u661F\u30673\u7B49\u661F\u3002 \u3053\u306E\u661F\u306F\u3001\u9023\u661F\u3067\u3042\u308B\u3002\u4E3B\u661F\u306F\u9EC4\u8272\u306E\u6E96\u5DE8\u661F\u3067\u3001\u4F34\u661F\u306F\u8996\u7B49\u7D1A+8.7\u306E\u9EC4\u8272\u306E\u4E3B\u7CFB\u5217\u661F\u3067\u3042\u308B\u3002\u6052\u661F\u9593\u306F3800\u5929\u6587\u5358\u4F4D\u96E2\u308C\u3066\u304A\u308A\u3001\u516C\u8EE2\u5468\u671F\u306F12\u4E07\u5E74\u3067\u3042\u308B\u3002"@ja . "Delta Bo\u00F6tis"@pt . . . "13798"^^ . . . . . . "\u3046\u3057\u304B\u3044\u5EA7\u30C7\u30EB\u30BF\u661F"@ja . . "26.78"^^ . . . "3.6"^^ . . . "J2000"@en . "Delta Bo\u00F6tis"@in . . "\u0414\u0435\u043B\u044C\u0442\u0430 \u0412\u043E\u043B\u043E\u043F\u0430\u0441\u0430"@ru . . . "4847"^^ . . "Delta Bootis (\u03B4 Boo / \u03B4 Bootis) est une \u00E9toile binaire de la constellation du Bouvier. Elle est \u00E0 environ 122 ann\u00E9es-lumi\u00E8re de la Terre. La composante primaire, \u03B4 Bootis A, est une g\u00E9ante jaune de type G avec une magnitude apparente de +3,46. Sa compagne, \u03B4 Bootis B, est une naine jaune de la s\u00E9quence principale de type G avec une magnitude apparente de +8,7. Distantes d'environ 3800 UA, elles parcourent leur orbite en 120 000 ans environ."@fr . "Delta Bo\u00F6tis"@en . "0.16"^^ . . "Delta Bootis"@sv . "\u4E03\u516C\u4E03"@zh . . . . . "27.0648"^^ . . "A"@en . . "Delta Bo\u00F6tis (\u03B4 Boo) \u2013 gwiazda podw\u00F3jna w gwiazdozbiorze Wolarza. Znajduje si\u0119 oko\u0142o 122 lata \u015Bwietlne od S\u0142o\u0144ca."@pl . . . . . "+0.59"@en . "53.7"^^ . . "Delta Bo\u00F6tis (\u03B4 Boo / \u03B4 Bo\u00F6tis) merupakan salah satu bintang ganda pada rasi bintang Bo\u00F6tes. Bintang ini berada pada 117 tahun cahaya dari Bumi. Komponen primernya, \u03B4 Bo\u00F6tis A, adalah bintang kuning raksasa (yellow G-type giant) dengan magnitudo 3.46. Komponen lainnya, \u03B4 Bo\u00F6tis B, adalah bintang katai kuning (yellow G-type main sequence dwarf) dengan mangitudo 8.7."@in . . . "7.81"^^ . . "Delta del Bover"@ca . "1118784958"^^ . . . "+82.776"@en . . . "Delta Bootis (\u03B4 Boo / 49 Bootis / HD 135722)\u200B es una estrella en la constelaci\u00F3n de Bootes de magnitud aparente +3,46.Sin nombre propio habitual, ocasionalmente es conocida como Princeps, \u00ABpr\u00EDncipe\u00BB o \u00ABprincipal\u00BB en lat\u00EDn.\u200BSe encuentra a 117 a\u00F1os luz de distancia del Sistema Solar."@es . . . "\u7267\u592B\u5EA7Delta\uFF08\u7267\u592B\u5EA7\u03B4\uFF0C\u03B4 Boo\uFF09\u662F\u4E00\u4E2A\u4F4D\u4E8E\u5317\u5929\u661F\u5EA7\u7267\u592B\u5EA7\u7684\u53CC\u661F\u3002\u6839\u636E\u89C6\u5DEE\u6D4B\u91CF\uFF0C\u8FD9\u4E2A\u6052\u661F\u8DDD\u79BB\u5730\u7403\u5927\u7EA6122.5\u5149\u5E74\u3002\u4E2D\u6587\u661F\u5B98\u540D\u4E03\u516C\u4E03\u3002\u89C6\u661F\u7B493.5\uFF0C\u4F7F\u8BE5\u661F\u5728\u6EE1\u6708\u53EF\u4EE5\u7528\u8089\u773C\u770B\u89C1\u3002"@zh . . . . . . . . . "Delta Bo\u00F6tis"@nl . . . . . . . . . . "0.98"^^ . . . . . . . . "2.56"^^ . "Delta Bo\u00F6tis, Latinized from \u03B4 Bo\u00F6tis, is a double star in the northern constellation of Bo\u00F6tes, forming the easternmost member of the constellation's kite-shaped asterism of brighter stars. Based upon parallax measurements, it is located at a distance of approximately 121.8 light-years (37.3 parsecs) from the Earth. This star is sometimes called Princeps /\u02C8pr\u026Ans\u025Bps/, meaning prince or prime in Latin. The origin of this name is unclear, although it usually appears in an astrological context. The apparent visual magnitude of this star is 3.5, making it visible to the naked eye even during a Full Moon. The magnitude 7.81 companion can be viewed in binoculars or a small telescope."@en . . . "\u7267\u592B\u5EA7Delta\uFF08\u7267\u592B\u5EA7\u03B4\uFF0C\u03B4 Boo\uFF09\u662F\u4E00\u4E2A\u4F4D\u4E8E\u5317\u5929\u661F\u5EA7\u7267\u592B\u5EA7\u7684\u53CC\u661F\u3002\u6839\u636E\u89C6\u5DEE\u6D4B\u91CF\uFF0C\u8FD9\u4E2A\u6052\u661F\u8DDD\u79BB\u5730\u7403\u5927\u7EA6122.5\u5149\u5E74\u3002\u4E2D\u6587\u661F\u5B98\u540D\u4E03\u516C\u4E03\u3002\u89C6\u661F\u7B493.5\uFF0C\u4F7F\u8BE5\u661F\u5728\u6EE1\u6708\u53EF\u4EE5\u7528\u8089\u773C\u770B\u89C1\u3002"@zh . "Princeps (Delta Bo\u00F6tis/ \u03B4 Boo / \u03B4 Bo\u00F6tis) \u00E8 una stella binaria nella costellazione di Boote, dista circa 117 anni luce dal sistema solare."@it . . "Delta Bo\u00F6tis, Latinized from \u03B4 Bo\u00F6tis, is a double star in the northern constellation of Bo\u00F6tes, forming the easternmost member of the constellation's kite-shaped asterism of brighter stars. Based upon parallax measurements, it is located at a distance of approximately 121.8 light-years (37.3 parsecs) from the Earth. This star is sometimes called Princeps /\u02C8pr\u026Ans\u025Bps/, meaning prince or prime in Latin. The origin of this name is unclear, although it usually appears in an astrological context. The apparent visual magnitude of this star is 3.5, making it visible to the naked eye even during a Full Moon. The magnitude 7.81 companion can be viewed in binoculars or a small telescope. In Chinese, \u4E03\u516C (Q\u012B G\u014Dng), meaning Seven Excellencies, refers to an asterism consisting of \u03B4 Bo\u00F6tis, 42 Herculis, \u03C4 Herculis, \u03C6 Herculis, \u03C7 Herculis, \u03BD1 Bo\u00F6tis and \u03BC1 Bo\u00F6tis. Consequently, the Chinese name for \u03B4 Bo\u00F6tis itself is \u4E03\u516C\u4E03 (Q\u012B G\u014Dng q\u012B, English: the Seventh Star of Seven Excellencies.)"@en . "Delta Bootis"@fr . . "Delta Bo\u00F6tis is een dubbelster in het sterrenbeeld Ossenhoeder. de ster is vanuit de Benelux cricumpolaire wat betekent dat ze het hele jaar door te zien is. Het systeem bestaat uit twee type G sterren, een reuzenster en een hoofdreeksster die 3600 AE van elkaar verwijderd staan. De ster staat soms ook bekend als Princeps."@nl . "0.0307"^^ . . . . . "Delta Bo\u00F6tis is een dubbelster in het sterrenbeeld Ossenhoeder. de ster is vanuit de Benelux cricumpolaire wat betekent dat ze het hele jaar door te zien is. Het systeem bestaat uit twee type G sterren, een reuzenster en een hoofdreeksster die 3600 AE van elkaar verwijderd staan. De ster staat soms ook bekend als Princeps."@nl . . "Delta del Bover (\u03B4 Bootis) \u00E9s un estel a la constel\u00B7laci\u00F3 del Bover de magnitud aparent +3,46. Sense nom propi habitual, ocasionalment \u00E9s conegut com a Princeps, \u00ABpr\u00EDncep\u00BB o \u00ABprincipal\u00BB en llat\u00ED. S'hi troba a 117 anys llum de dist\u00E0ncia del sistema solar."@ca . "Delta del Bover (\u03B4 Bootis) \u00E9s un estel a la constel\u00B7laci\u00F3 del Bover de magnitud aparent +3,46. Sense nom propi habitual, ocasionalment \u00E9s conegut com a Princeps, \u00ABpr\u00EDncep\u00BB o \u00ABprincipal\u00BB en llat\u00ED. S'hi troba a 117 anys llum de dist\u00E0ncia del sistema solar. Delta del Bover \u00E9s una estrella gegant groga de tipus espectral G8III i 4.990 K de temperatura, amb una lluminositat 59 vegades major que la del Sol. El valor del seu di\u00E0metre, obtingut a partir de la mesura del seu di\u00E0metre angular, \u00E9s 10,4 vegades major que el del Sol. La seua metal\u00B7licitat \u00E9s baixa comparada a la solar, entorn del 40% de la mateixa; com a resultat d'aix\u00F2, pel seu espectre est\u00E0 classificada com un estel amb l\u00EDnies febles de CN (cianogen). Delta del Bover t\u00E9 una companya estel\u00B7lar de magnitud +7,8, una nana de tipus espectral G0 similar al Sol. No obstant aix\u00F2, la seva baixa lluminositat \u2014un 80% de la solar\u2014 i la seva petita grand\u00E0ria en relaci\u00F3 a la seva temperatura de 5.900 K \u2014el seu radi equival al 87% del radi solar, suggereixen que pot ser una estrella subnana; aix\u00F2 concorda amb la baixa metal\u00B7licitat observada en Delta del Bover A. Visualment estan separades gaireb\u00E9 2 minuts d'arc, cosa que equival a una separaci\u00F3 real d'almenys a 3.800 UA i un per\u00EDode orbital de m\u00E9s de 120.000 anys."@ca . . . . "3.482"^^ . "+0.700"@en . .