@prefix dbo: .
@prefix dbr: .
dbr:List_of_brightest_natural_objects_in_the_sky dbo:wikiPageWikiLink dbr:Eta_Sagittarii .
dbr:Epsilon_Sagittarii dbo:wikiPageWikiLink dbr:Eta_Sagittarii .
dbr:Gamma2_Sagittarii dbo:wikiPageWikiLink dbr:Eta_Sagittarii .
dbr:Delta_Sagittarii dbo:wikiPageWikiLink dbr:Eta_Sagittarii .
@prefix foaf: .
@prefix wikipedia-en: .
wikipedia-en:Eta_Sagittarii foaf:primaryTopic dbr:Eta_Sagittarii .
dbo:wikiPageWikiLink dbr:Eta_Sagittarii .
@prefix rdf: .
@prefix yago: .
dbr:Eta_Sagittarii rdf:type yago:Giant101323781 .
@prefix schema: .
dbr:Eta_Sagittarii rdf:type schema:Place ,
yago:WikicatHenryDraperCatalogueObjects ,
yago:Animal100015388 ,
yago:Variable109468959 ,
yago:WikicatVariableStars ,
yago:WikicatM-typeGiants ,
dbo:Location ,
yago:VariableStar109469152 ,
yago:CelestialBody109239740 ,
dbo:Place ,
yago:Object100002684 ,
yago:WikicatF-typeStars ,
yago:Whole100003553 ,
yago:NaturalObject100019128 ,
yago:WikicatF-typeMain-sequenceStars ,
yago:WikicatG-typeMain-sequenceStars .
@prefix owl: .
dbr:Eta_Sagittarii rdf:type owl:Thing ,
yago:WikicatIrregularVariables ,
yago:WikicatHipparcosObjects ,
yago:LivingThing100004258 ,
yago:Thing100002452 ,
yago:Organism100004475 ,
yago:WikicatBayerObjects ,
yago:BinaryStar109221070 ,
yago:WikicatM-typeStars ,
dbo:Star ,
yago:WikicatBinaryStars ,
yago:PhysicalEntity100001930 ,
yago:Star109444100 ,
dbo:CelestialBody ,
yago:WikicatStars .
@prefix rdfs: .
dbr:Eta_Sagittarii rdfs:label "Eta Sagittarii"@it ,
"Eta Sagittarii"@ca ,
"\u0625\u064A\u062A\u0627 \u0627\u0644\u0631\u0627\u0645\u064A"@ar ,
"Eta Sagittarii"@pt ,
"\u042D\u0442\u0430 \u0421\u0442\u0440\u0435\u043B\u044C\u0446\u0430"@ru ,
"\u3044\u3066\u5EA7\u30A4\u30FC\u30BF\u661F"@ja ,
"Eta Sagittarii"@es ,
"Eta Sagittarii"@pl ,
"\uAD81\uC218\uC790\uB9AC \uC5D0\uD0C0"@ko ,
"Eta Sagittarii"@nl ,
"\u7B95\u5BBF\u56DB"@zh ,
"Eta Sagittarii"@fr ,
"Eta Sagittarii"@sv ,
"Eta Sagittarii"@in ,
"Eta Sagittarii"@en ;
rdfs:comment "eta Sagittarii (\u03B7 Sgr) \u2013 gwiazda w gwiazdozbiorze Strzelca, odleg\u0142a o 146 lat \u015Bwietlnych od S\u0142o\u0144ca."@pl ,
"Eta Sagittarii ( Sagittarii) \u00E9 uma estrela na dire\u00E7\u00E3o da constela\u00E7\u00E3o de Sagittarius. Possui uma ascens\u00E3o reta de 18h 17m 37.73s e uma declina\u00E7\u00E3o de \u221236\u00B0 45\u2032 40.6\u2033. Sua magnitude aparente \u00E9 igual a 3.10. Considerando sua dist\u00E2ncia de 149 anos-luz em rela\u00E7\u00E3o \u00E0 Terra, sua magnitude absoluta \u00E9 igual a \u22120.20. Pertence \u00E0 classe espectral M2III. \u00C9 uma estrela vari\u00E1vel irregular."@pt ,
"\u042D\u0442\u0430 \u0421\u0442\u0440\u0435\u043B\u044C\u0446\u0430 (Eta Sagittarii, Eta Sgr, \u03B7 Sagittarii, \u03B7 Sgr) \u2014 \u0434\u0432\u043E\u0439\u043D\u0430\u044F \u0437\u0432\u0435\u0437\u0434\u043D\u0430\u044F \u0441\u0438\u0441\u0442\u0435\u043C\u0430 \u0432 \u044E\u0436\u043D\u043E\u043C \u0437\u043E\u0434\u0438\u0430\u043A\u0430\u043B\u044C\u043D\u043E\u043C \u0441\u043E\u0437\u0432\u0435\u0437\u0434\u0438\u0438 \u0421\u0442\u0440\u0435\u043B\u044C\u0446\u0430. \u041E\u0441\u043D\u043E\u0432\u044B\u0432\u0430\u044F\u0441\u044C \u043D\u0430 \u0438\u0437\u043C\u0435\u0440\u0435\u043D\u0438\u044F\u0445 \u043F\u0430\u0440\u0430\u043B\u043B\u0430\u043A\u0441\u0430, \u043C\u043E\u0436\u043D\u043E \u0432\u044B\u0447\u0438\u0441\u043B\u0438\u0442\u044C, \u0447\u0442\u043E \u043E\u043D\u0430 \u043D\u0430\u0445\u043E\u0434\u0438\u0442\u0441\u044F \u043D\u0430 \u0440\u0430\u0441\u0441\u0442\u043E\u044F\u043D\u0438\u0438 146 \u0441\u0432\u0435\u0442\u043E\u0432\u044B\u0445 \u043B\u0435\u0442 \u043E\u0442 \u0417\u0435\u043C\u043B\u0438. \u041D\u0430 \u0442\u0435\u0440\u0440\u0438\u0442\u043E\u0440\u0438\u0438 \u0420\u043E\u0441\u0441\u0438\u0438 \u0437\u0432\u0435\u0437\u0434\u0430 \u0432\u0438\u0434\u043D\u0430 \u043D\u0430 \u044E\u0433\u0435 \u0441\u0442\u0440\u0430\u043D\u044B \u043D\u0430\u0447\u0438\u043D\u0430\u044F \u0441 \u043E\u0447\u0435\u043D\u044C \u043D\u0438\u0437\u043A\u043E \u043D\u0430\u0434 \u0433\u043E\u0440\u0438\u0437\u043E\u043D\u0442\u043E\u043C. \u041D\u0435\u0437\u0430\u0445\u043E\u0434\u044F\u0449\u0435\u0439 \u0437\u0432\u0435\u0437\u0434\u0430 \u044F\u0432\u043B\u044F\u0435\u0442\u0441\u044F \u043D\u0430 \u0448\u0438\u0440\u043E\u0442\u0430\u0445 \u044E\u0436\u043D\u0435\u0435 , \u0442. \u0435. \u0442\u043E\u043B\u044C\u043A\u043E \u043D\u0430 \u0430\u043D\u0442\u0430\u0440\u043A\u0442\u0438\u0447\u0435\u0441\u043A\u043E\u043C \u043A\u043E\u043D\u0442\u0438\u043D\u0435\u043D\u0442\u0435 \u0438 \u041E\u0433\u043D\u0435\u043D\u043D\u043E\u0439 \u0417\u0435\u043C\u043B\u0435."@ru ,
"\u0625\u064A\u062A\u0627 \u0627\u0644\u0631\u0627\u0645\u064A Eta Sagittarii (Eta Sgr, \u03B7 Sagittarii, \u03B7 Sgr) \u0647\u0648 \u0646\u062C\u0645 \u062B\u0646\u0627\u0626\u064A \u0641\u064A \u0643\u0648\u0643\u0628\u0629 \u0627\u0644\u0631\u0627\u0645\u064A \u0627\u0633\u062A\u0646\u0627\u062F\u0627 \u0625\u0644\u0649 \u0642\u064A\u0627\u0633\u0627\u062A \u0627\u0644\u062A\u0632\u064A\u062D\u060C \u064A\u0642\u0639 \u0647\u0630\u0627 \u0627\u0644\u0646\u062C\u0645 \u0639\u0644\u0649 \u0645\u0633\u0627\u0641\u0629 146 \u0633\u0646\u0629 \u0636\u0648\u0626\u064A\u0629 (45 \u0641\u0631\u0633\u062E \u0641\u0644\u0643\u064A) \u0645\u0646 \u0627\u0644\u0623\u0631\u0636.\u0625\u064A\u062A\u0627 \u0627\u0644\u0631\u0627\u0645\u064A \u0645\u0646 \u0636\u0645\u0646 \u0645\u062C\u0645\u0629 \u0627\u0644\u0646\u0639\u0627\u0645 \u0627\u0644\u0648\u0627\u0631\u062F \u0645\u0639 \u0646\u062C\u0648\u0645 \u0627\u0644\u0646\u0635\u0644 \u0648\u0648\u0633\u0637 \u0627\u0644\u0642\u0648\u0633 \u0648\u0627\u0644\u0642\u0648\u0633 \u0627\u0644\u062C\u0646\u0648\u0628\u064A ."@ar ,
"Eta Sagittarii (\u03B7 Sgr / \u03B7 Sagittarii) adalah sistem bintang yang berada di rasi Sagittarius. Bintang ini berada pada jarak 149 tahun cahaya dari Bumi. Sebelumnya bintang ini diketahui sebagai \"Beta Telescopii\" (\u03B2 Tel). Bintang utama, \u03B7 Sagittarii A, merupakan bintang raksasa merah tipe M3.5. Bintang ini memiliki magnitudo antara +3.08 dan 3.12. Komponen yang paling terang \u03B7 Sagittarii B, merupakan bintang katai tipe F dengan magnitudo +7.77. Bintang ini menyelesaikan orbit selama 1300 tahun dan terpisah dengan jarak 3.6 di langit."@in ,
"\u3044\u3066\u5EA7\u03B7\u661F\u306F\u3001\u3044\u3066\u5EA7\u306E\u6052\u661F\u30673\u7B49\u661F\u3002 2\u7B49\u661F\u306E\u03B5\u661F\u306E\u5357\u5357\u897F2.5\u00B0\u306B\u4F4D\u7F6E\u3057\u3001\u307E\u305F\u6563\u958B\u661F\u56E3M7\u304C\u897F\u5317\u897F4.5\u00B0\u306B\u4F4D\u7F6E\u3057\u3066\u3044\u308B\u3002"@ja ,
"Eta Sagittarii (Sagittarii) \u00E9s una estrella a la constel\u00B7laci\u00F3 del Sagitari. T\u00E9 una ascensi\u00F3 recta de 18h 17m 37.73s i una declinaci\u00F3 de \u221236\u00B0 45\u2032 40.6\u2033. La seua magnitud aparent \u00E9s de 3.10. Considerant la seua dist\u00E0ncia de 149 anys llum en relaci\u00F3 amb la Terra, la seua magnitud absoluta \u00E9s igual a \u22120,20. Pertany a la classe espectral M2III. \u00C9s una estrela variable irregular."@ca ,
"\u00CAta Sagittarii, en abr\u00E9g\u00E9 \u03B7 Sgr, est une \u00E9toile binaire de la constellation du Sagittaire, \u00E0 149 ann\u00E9es-lumi\u00E8re de la Terre. On le connaissait autrefois sous le nom de \u00AB Beta Telescopii \u00BB (\u03B2 Tel). La principale composante, \u03B7 Sagittarii A, est une g\u00E9ante rouge de type spectral M3.5. Il s'agit d'une \u00E9toile variable avec de petites fluctuations de magnitude entre +3,08 et 3,12, et elle est rang\u00E9e parmi les variables irr\u00E9guli\u00E8res."@fr ,
"\u7B95\u5BBF\u56DB\uFF08\u4EBA\u99AC\u5EA7\u03B7\uFF0C\u03B7 Sgr\uFF09\u662F\u4F4D\u4E8E\u4EBA\u99AC\u5EA7\u7684\u4E00\u500B\u6046\u661F\u7CFB\u7D71\uFF0C\u8DDD\u96E2\u5730\u7403149\u5149\u5E74\u3002\u5728\u62DC\u8033\u5206\u7C7B\u6CD5\u4E2D\uFF0C\u4EBA\u99AC\u5EA7\u03B7\u4E5F\u66FE\u7D93\u662F\u201C\u671B\u9060\u93E1\u5EA7\u03B2\u201D\u3002 \u5176\u4E3B\u661F\u4EBA\u99AC\u5EA7\u03B7A\uFF0C\u662F\u4E00\u9846M3.5\u578B\u7D05\u5DE8\u661F\u3002\u5B83\u662F\u4E00\u9846\u8B8A\u661F\uFF0C\u56E0\u6B64\u5B83\u7684\u8996\u661F\u7B49\u6703\u5728+3.08\u548C3.12\u9593\u8B8A\u52D5\uFF0C\u4E26\u4E14\u88AB\u6B78\u70BA\u4E0D\u898F\u5247\u8B8A\u661F\u3002\u4F34\u661F\u4E4B\u4E2D\u4EAE\u7684\u4E00\u9846\u661F\u4EBA\u99AC\u5EA7\u03B7B\u662F\u4E00\u9846F\u578B\u77EE\u661F\uFF0C\u8996\u661F\u7B49\u70BA+7.77\u3002\u5B83\u8DDD\u96E2\u4E3B\u661F165\u5929\u6587\u55AE\u4F4D\uFF0C\u516C\u8F49\u5468\u671F\u70BA\u5927\u7D041300\u5E74\u3002\u5169\u9846\u661F\u5728\u591C\u7A7A\u4E0A\u8DDD\u96E23.6\u89D2\u79D2\u3002\u53E6\u5916\u9084\u6709\u5169\u9846\u8F03\u6697\u7684\u4F34\u661F\uFF1A\u4EBA\u99AC\u5EA7\u03B7C\uFF0C\u8996\u661F\u7B49\u70BA13\uFF0C\u8DDD\u96E2\u4E3B\u661F33\u89D2\u79D2\uFF1B\u4EBA\u99AC\u5EA7\u03B7D\uFF0C\u8996\u661F\u7B49\u70BA10\uFF0C\u8DDD\u96E2\u4E3B\u661F93\u89D2\u79D2\u3002"@zh ,
"Eta Sagittarii (\u03B7 Sgr / HD 167618 / HR 6832) es una estrella en la constelaci\u00F3n de Sagitario de magnitud aparente +3,10. Recibe los nombres, raramente utilizados, de Sephdar, del \u00E1rabe \u0627\u0644\u0635\u0641\u062F\u0631 al-safdar, \u00ABguerrero violento\u00BB, e Ira Furoris, proveniente del lat\u00EDn y cuyo significado es \u00ABira furiosa\u00BB. Antiguamente recibi\u00F3 el nombre de Beta Telescopii (\u03B2 Tel)."@es ,
"Eta Sagittarii (\u03B7 Sagittarii, f\u00F6rkortat Eta Sgr, \u03B7 Sgr) som \u00E4r stj\u00E4rnans Bayerbeteckning, \u00E4r en dubbelstj\u00E4rna bel\u00E4gen i den sydv\u00E4stra delen av stj\u00E4rnbilden Skytten. Den har en skenbar magnitud p\u00E5 3,11 och \u00E4r klart synlig f\u00F6r blotta \u00F6gat. Baserat p\u00E5 parallaxm\u00E4tning inom Hipparcosuppdraget p\u00E5 ca 22,4 mas, ber\u00E4knas den befinna sig p\u00E5 ett avst\u00E5nd av ca 146 ljus\u00E5r (ca 45 parsek) fr\u00E5n solen."@sv ,
"Eta Sigittarii is een tweevoudige dubbelster in het sterrenbeeld Boogschutter. De belangrijkste ster van het systeem is Eta Sigittarii A, die met een spectraalklasse van M2 III een reuzenster.De andere ster in het systeem, Eta Sigittarii B is met een spectraalklasse van F7 V een hoofdreeksster."@nl ,
"Eta Sagittarii (Eta Sgr, \u03B7 Sagittarii, \u03B7 Sgr) is a binary star system in the southern zodiac constellation of Sagittarius. Based upon parallax measurements, it is located at a distance of 146 light-years (45 parsecs) from Earth. It was formerly known as Beta Telescopii (\u03B2 Tel). In India, where part of the constellation of Sagittarius represents an Elephant, this star forms the creature's tail."@en ,
"Eta Sagittarii (Eta Sgr, \u03B7 Sagittarii, \u03B7 Sgr) \u00E8 una stella binaria di magnitudine apparente 3,11 della costellazione del Sagittario. Dista 146 anni luce dal sistema solare. Ha anche altri nomi tradizionali, poco utilizzati, tra i quali Sephdar, dall'arabo \u0627\u0644\u0635\u0641\u062F\u0631 al-safdar (\"guerriero violento\"), e Ira Furoris, proveniente dal latino e che significa \"ira furiosa\". Anticamente ricevette anche il nome di Beta Telescopii (\u03B2 Telescopii)."@it ,
"\uAD81\uC218\uC790\uB9AC \uC5D0\uD0C0(\u03B7 Sgr)\uB294 \uD669\uB3C4\uB300 \uBCC4\uC790\uB9AC\uC778 \uAD81\uC218\uC790\uB9AC \uBC29\uD5A5\uC5D0 \uC788\uB294 \uC30D\uC131\uACC4\uC774\uB2E4. \uC2DC\uCC28 \uC790\uB8CC\uC5D0 \uB530\uB974\uBA74 \uC774 \uBCC4\uC740 \uC9C0\uAD6C\uB85C\uBD80\uD130 \uC57D 146 \uAD11\uB144 (45 \uD30C\uC139) \uB5A8\uC5B4\uC9C4 \uACF3\uC5D0 \uC788\uB2E4."@ko ;
foaf:name "\u03B7 Sagittarii"@en ;
foaf:depiction ,
.
@prefix dct: .
@prefix dbc: .
dbr:Eta_Sagittarii dct:subject dbc:Durchmusterung_objects ,
dbc:Binary_stars ,
dbc:Bayer_objects ,
dbc:Bright_Star_Catalogue_objects ,
dbc:Hipparcos_objects ,
dbc:M-type_giants ,
dbc:F-type_main-sequence_stars ,
dbc:Slow_irregular_variables ,
dbc:Henry_Draper_Catalogue_objects ,
;
dbo:abstract "Eta Sagittarii (Eta Sgr, \u03B7 Sagittarii, \u03B7 Sgr) \u00E8 una stella binaria di magnitudine apparente 3,11 della costellazione del Sagittario. Dista 146 anni luce dal sistema solare. Ha anche altri nomi tradizionali, poco utilizzati, tra i quali Sephdar, dall'arabo \u0627\u0644\u0635\u0641\u062F\u0631 al-safdar (\"guerriero violento\"), e Ira Furoris, proveniente dal latino e che significa \"ira furiosa\". Anticamente ricevette anche il nome di Beta Telescopii (\u03B2 Telescopii)."@it ,
"Eta Sagittarii ( Sagittarii) \u00E9 uma estrela na dire\u00E7\u00E3o da constela\u00E7\u00E3o de Sagittarius. Possui uma ascens\u00E3o reta de 18h 17m 37.73s e uma declina\u00E7\u00E3o de \u221236\u00B0 45\u2032 40.6\u2033. Sua magnitude aparente \u00E9 igual a 3.10. Considerando sua dist\u00E2ncia de 149 anos-luz em rela\u00E7\u00E3o \u00E0 Terra, sua magnitude absoluta \u00E9 igual a \u22120.20. Pertence \u00E0 classe espectral M2III. \u00C9 uma estrela vari\u00E1vel irregular."@pt ,
"\uAD81\uC218\uC790\uB9AC \uC5D0\uD0C0(\u03B7 Sgr)\uB294 \uD669\uB3C4\uB300 \uBCC4\uC790\uB9AC\uC778 \uAD81\uC218\uC790\uB9AC \uBC29\uD5A5\uC5D0 \uC788\uB294 \uC30D\uC131\uACC4\uC774\uB2E4. \uC2DC\uCC28 \uC790\uB8CC\uC5D0 \uB530\uB974\uBA74 \uC774 \uBCC4\uC740 \uC9C0\uAD6C\uB85C\uBD80\uD130 \uC57D 146 \uAD11\uB144 (45 \uD30C\uC139) \uB5A8\uC5B4\uC9C4 \uACF3\uC5D0 \uC788\uB2E4."@ko ,
"eta Sagittarii (\u03B7 Sgr) \u2013 gwiazda w gwiazdozbiorze Strzelca, odleg\u0142a o 146 lat \u015Bwietlnych od S\u0142o\u0144ca."@pl ,
"\u00CAta Sagittarii, en abr\u00E9g\u00E9 \u03B7 Sgr, est une \u00E9toile binaire de la constellation du Sagittaire, \u00E0 149 ann\u00E9es-lumi\u00E8re de la Terre. On le connaissait autrefois sous le nom de \u00AB Beta Telescopii \u00BB (\u03B2 Tel). La principale composante, \u03B7 Sagittarii A, est une g\u00E9ante rouge de type spectral M3.5. Il s'agit d'une \u00E9toile variable avec de petites fluctuations de magnitude entre +3,08 et 3,12, et elle est rang\u00E9e parmi les variables irr\u00E9guli\u00E8res. Son compagnon le plus brillant, \u03B7 Sagittarii B, est une \u00E9toile naine de type spectral F, avec une magnitude apparente de +7,77. Il est \u00E0 une distance de 165 unit\u00E9s astronomiques de \u03B7 Sagittarii A et met environ 1 300 ans pour d\u00E9crire une orbite. Les deux \u00E9toiles sont s\u00E9par\u00E9es sur le ciel par 3,6 secondes angulaires. Il existe \u00E9galement deux compagnons purement optiques recens\u00E9s, qui sont plus lointains et plus faibles, \u03B7 Sagittarii C de 13e magnitude, s\u00E9par\u00E9 de A de 33 secondes angulaires et \u03B7 Sagittarii D, de 10e magnitude, s\u00E9par\u00E9 de A par 93 secondes angulaires."@fr ,
"\u042D\u0442\u0430 \u0421\u0442\u0440\u0435\u043B\u044C\u0446\u0430 (Eta Sagittarii, Eta Sgr, \u03B7 Sagittarii, \u03B7 Sgr) \u2014 \u0434\u0432\u043E\u0439\u043D\u0430\u044F \u0437\u0432\u0435\u0437\u0434\u043D\u0430\u044F \u0441\u0438\u0441\u0442\u0435\u043C\u0430 \u0432 \u044E\u0436\u043D\u043E\u043C \u0437\u043E\u0434\u0438\u0430\u043A\u0430\u043B\u044C\u043D\u043E\u043C \u0441\u043E\u0437\u0432\u0435\u0437\u0434\u0438\u0438 \u0421\u0442\u0440\u0435\u043B\u044C\u0446\u0430. \u041E\u0441\u043D\u043E\u0432\u044B\u0432\u0430\u044F\u0441\u044C \u043D\u0430 \u0438\u0437\u043C\u0435\u0440\u0435\u043D\u0438\u044F\u0445 \u043F\u0430\u0440\u0430\u043B\u043B\u0430\u043A\u0441\u0430, \u043C\u043E\u0436\u043D\u043E \u0432\u044B\u0447\u0438\u0441\u043B\u0438\u0442\u044C, \u0447\u0442\u043E \u043E\u043D\u0430 \u043D\u0430\u0445\u043E\u0434\u0438\u0442\u0441\u044F \u043D\u0430 \u0440\u0430\u0441\u0441\u0442\u043E\u044F\u043D\u0438\u0438 146 \u0441\u0432\u0435\u0442\u043E\u0432\u044B\u0445 \u043B\u0435\u0442 \u043E\u0442 \u0417\u0435\u043C\u043B\u0438. \u041D\u0430 \u0442\u0435\u0440\u0440\u0438\u0442\u043E\u0440\u0438\u0438 \u0420\u043E\u0441\u0441\u0438\u0438 \u0437\u0432\u0435\u0437\u0434\u0430 \u0432\u0438\u0434\u043D\u0430 \u043D\u0430 \u044E\u0433\u0435 \u0441\u0442\u0440\u0430\u043D\u044B \u043D\u0430\u0447\u0438\u043D\u0430\u044F \u0441 \u043E\u0447\u0435\u043D\u044C \u043D\u0438\u0437\u043A\u043E \u043D\u0430\u0434 \u0433\u043E\u0440\u0438\u0437\u043E\u043D\u0442\u043E\u043C. \u041D\u0435\u0437\u0430\u0445\u043E\u0434\u044F\u0449\u0435\u0439 \u0437\u0432\u0435\u0437\u0434\u0430 \u044F\u0432\u043B\u044F\u0435\u0442\u0441\u044F \u043D\u0430 \u0448\u0438\u0440\u043E\u0442\u0430\u0445 \u044E\u0436\u043D\u0435\u0435 , \u0442. \u0435. \u0442\u043E\u043B\u044C\u043A\u043E \u043D\u0430 \u0430\u043D\u0442\u0430\u0440\u043A\u0442\u0438\u0447\u0435\u0441\u043A\u043E\u043C \u043A\u043E\u043D\u0442\u0438\u043D\u0435\u043D\u0442\u0435 \u0438 \u041E\u0433\u043D\u0435\u043D\u043D\u043E\u0439 \u0417\u0435\u043C\u043B\u0435."@ru ,
"Eta Sagittarii (\u03B7 Sgr / \u03B7 Sagittarii) adalah sistem bintang yang berada di rasi Sagittarius. Bintang ini berada pada jarak 149 tahun cahaya dari Bumi. Sebelumnya bintang ini diketahui sebagai \"Beta Telescopii\" (\u03B2 Tel). Bintang utama, \u03B7 Sagittarii A, merupakan bintang raksasa merah tipe M3.5. Bintang ini memiliki magnitudo antara +3.08 dan 3.12. Komponen yang paling terang \u03B7 Sagittarii B, merupakan bintang katai tipe F dengan magnitudo +7.77. Bintang ini menyelesaikan orbit selama 1300 tahun dan terpisah dengan jarak 3.6 di langit. Lebih dari dua bintang sebelumnya, bintang bermagnitudo 13, \u03B7 Sagittarii C, terpisah dari A sekitar 33 arcsecond, dan bintang bermagnitudo 10, \u03B7 Sagittarii D, terpisah 93 arcseconds dari A."@in ,
"\u3044\u3066\u5EA7\u03B7\u661F\u306F\u3001\u3044\u3066\u5EA7\u306E\u6052\u661F\u30673\u7B49\u661F\u3002 2\u7B49\u661F\u306E\u03B5\u661F\u306E\u5357\u5357\u897F2.5\u00B0\u306B\u4F4D\u7F6E\u3057\u3001\u307E\u305F\u6563\u958B\u661F\u56E3M7\u304C\u897F\u5317\u897F4.5\u00B0\u306B\u4F4D\u7F6E\u3057\u3066\u3044\u308B\u3002"@ja ,
"Eta Sigittarii is een tweevoudige dubbelster in het sterrenbeeld Boogschutter. De belangrijkste ster van het systeem is Eta Sigittarii A, die met een spectraalklasse van M2 III een reuzenster.De andere ster in het systeem, Eta Sigittarii B is met een spectraalklasse van F7 V een hoofdreeksster."@nl ,
"Eta Sagittarii (\u03B7 Sgr / HD 167618 / HR 6832) es una estrella en la constelaci\u00F3n de Sagitario de magnitud aparente +3,10. Recibe los nombres, raramente utilizados, de Sephdar, del \u00E1rabe \u0627\u0644\u0635\u0641\u062F\u0631 al-safdar, \u00ABguerrero violento\u00BB, e Ira Furoris, proveniente del lat\u00EDn y cuyo significado es \u00ABira furiosa\u00BB. Antiguamente recibi\u00F3 el nombre de Beta Telescopii (\u03B2 Tel). A diferencia de la mayor parte de las estrellas en la constelaci\u00F3n, que son estrellas azules calientes, Eta Sagittarii es una gigante roja fr\u00EDa de tipo espectral M3.5III. Con una luminosidad \u2014incluida la radiaci\u00F3n emitida en el infrarrojo\u2014 585 veces superior a la del Sol, su radio es 62 veces m\u00E1s grande que el radio solar, equivalente a tres cuartas partes de la distancia entre Mercurio y el Sol. Como otras estrellas similares, Eta Sagittarii es una variable irregular con una variaci\u00F3n en su brillo de 0,07 magnitudes, no perceptible a simple vista. Se encuentra a 149 a\u00F1os luz de distancia del Sistema Solar. Eta Sagittarii forma un sistema binario con una compa\u00F1era de magnitud +7,8 visualmente a 3,6 segundos de arco. A partir de su brillo, se puede deducir que esta \u00FAltima es una estrella blanco-amarilla \u2014probablemente de tipo F7V\u2014 a una distancia real de la estrella gigante de al menos 165 UA. Emplea 1270 a\u00F1os como m\u00EDnimo en completar su \u00F3rbita."@es ,
"Eta Sagittarii (\u03B7 Sagittarii, f\u00F6rkortat Eta Sgr, \u03B7 Sgr) som \u00E4r stj\u00E4rnans Bayerbeteckning, \u00E4r en dubbelstj\u00E4rna bel\u00E4gen i den sydv\u00E4stra delen av stj\u00E4rnbilden Skytten. Den har en skenbar magnitud p\u00E5 3,11 och \u00E4r klart synlig f\u00F6r blotta \u00F6gat. Baserat p\u00E5 parallaxm\u00E4tning inom Hipparcosuppdraget p\u00E5 ca 22,4 mas, ber\u00E4knas den befinna sig p\u00E5 ett avst\u00E5nd av ca 146 ljus\u00E5r (ca 45 parsek) fr\u00E5n solen."@sv ,
"Eta Sagittarii (Eta Sgr, \u03B7 Sagittarii, \u03B7 Sgr) is a binary star system in the southern zodiac constellation of Sagittarius. Based upon parallax measurements, it is located at a distance of 146 light-years (45 parsecs) from Earth. It was formerly known as Beta Telescopii (\u03B2 Tel). In India, where part of the constellation of Sagittarius represents an Elephant, this star forms the creature's tail. The primary component, \u03B7 Sagittarii A, is a red giant star with a stellar classification of M2 III. It is an evolved star that is currently at a stage called the asymptotic giant branch, having exhausted both the hydrogen and the helium at its core. This star is classified as an oxygen-rich irregular variable, as it undergoes small magnitude fluctuations between +3.08 and 3.12. The measured angular diameter of this star is 11.9 \u00B1 2.1 mas. At the estimated distance of Eta Draconis, this yields a physical size of about 57 times the radius of the Sun. The companion, \u03B7 Sagittarii B, was first noted by American astronomer S. W. Burnham in 1879. The two stars share a common proper motion and hence are probably gravitationally bound to each other. The secondary is likely an F-type main sequence star with an apparent magnitude of +7.77. It located at an angular separation of 3.6 arcseconds from the primary, along a position angle of 108\u00B0. This star is at a projected distance of 165 Astronomical Units from the red giant primary and the pair take a minimum of 1,270 years to complete an orbit. Within the context of the Milky Way galaxy, this system is a member of the faint old disk group. Because of proper motion, this star will move into constellation Corona Australis around 6300 CE. Eta Sagittarii has two optical companions that are not physically associated with the system. The first is a 10th magnitude star at an angular separation of 93 arcseconds with a position angle of 303\u00B0. There is a fainter, 13th magnitude star at an angular separation of 33 arcseconds along a position angle of 276\u00B0."@en ,
"\u7B95\u5BBF\u56DB\uFF08\u4EBA\u99AC\u5EA7\u03B7\uFF0C\u03B7 Sgr\uFF09\u662F\u4F4D\u4E8E\u4EBA\u99AC\u5EA7\u7684\u4E00\u500B\u6046\u661F\u7CFB\u7D71\uFF0C\u8DDD\u96E2\u5730\u7403149\u5149\u5E74\u3002\u5728\u62DC\u8033\u5206\u7C7B\u6CD5\u4E2D\uFF0C\u4EBA\u99AC\u5EA7\u03B7\u4E5F\u66FE\u7D93\u662F\u201C\u671B\u9060\u93E1\u5EA7\u03B2\u201D\u3002 \u5176\u4E3B\u661F\u4EBA\u99AC\u5EA7\u03B7A\uFF0C\u662F\u4E00\u9846M3.5\u578B\u7D05\u5DE8\u661F\u3002\u5B83\u662F\u4E00\u9846\u8B8A\u661F\uFF0C\u56E0\u6B64\u5B83\u7684\u8996\u661F\u7B49\u6703\u5728+3.08\u548C3.12\u9593\u8B8A\u52D5\uFF0C\u4E26\u4E14\u88AB\u6B78\u70BA\u4E0D\u898F\u5247\u8B8A\u661F\u3002\u4F34\u661F\u4E4B\u4E2D\u4EAE\u7684\u4E00\u9846\u661F\u4EBA\u99AC\u5EA7\u03B7B\u662F\u4E00\u9846F\u578B\u77EE\u661F\uFF0C\u8996\u661F\u7B49\u70BA+7.77\u3002\u5B83\u8DDD\u96E2\u4E3B\u661F165\u5929\u6587\u55AE\u4F4D\uFF0C\u516C\u8F49\u5468\u671F\u70BA\u5927\u7D041300\u5E74\u3002\u5169\u9846\u661F\u5728\u591C\u7A7A\u4E0A\u8DDD\u96E23.6\u89D2\u79D2\u3002\u53E6\u5916\u9084\u6709\u5169\u9846\u8F03\u6697\u7684\u4F34\u661F\uFF1A\u4EBA\u99AC\u5EA7\u03B7C\uFF0C\u8996\u661F\u7B49\u70BA13\uFF0C\u8DDD\u96E2\u4E3B\u661F33\u89D2\u79D2\uFF1B\u4EBA\u99AC\u5EA7\u03B7D\uFF0C\u8996\u661F\u7B49\u70BA10\uFF0C\u8DDD\u96E2\u4E3B\u661F93\u89D2\u79D2\u3002"@zh ,
"Eta Sagittarii (Sagittarii) \u00E9s una estrella a la constel\u00B7laci\u00F3 del Sagitari. T\u00E9 una ascensi\u00F3 recta de 18h 17m 37.73s i una declinaci\u00F3 de \u221236\u00B0 45\u2032 40.6\u2033. La seua magnitud aparent \u00E9s de 3.10. Considerant la seua dist\u00E0ncia de 149 anys llum en relaci\u00F3 amb la Terra, la seua magnitud absoluta \u00E9s igual a \u22120,20. Pertany a la classe espectral M2III. \u00C9s una estrela variable irregular."@ca ,
"\u0625\u064A\u062A\u0627 \u0627\u0644\u0631\u0627\u0645\u064A Eta Sagittarii (Eta Sgr, \u03B7 Sagittarii, \u03B7 Sgr) \u0647\u0648 \u0646\u062C\u0645 \u062B\u0646\u0627\u0626\u064A \u0641\u064A \u0643\u0648\u0643\u0628\u0629 \u0627\u0644\u0631\u0627\u0645\u064A \u0627\u0633\u062A\u0646\u0627\u062F\u0627 \u0625\u0644\u0649 \u0642\u064A\u0627\u0633\u0627\u062A \u0627\u0644\u062A\u0632\u064A\u062D\u060C \u064A\u0642\u0639 \u0647\u0630\u0627 \u0627\u0644\u0646\u062C\u0645 \u0639\u0644\u0649 \u0645\u0633\u0627\u0641\u0629 146 \u0633\u0646\u0629 \u0636\u0648\u0626\u064A\u0629 (45 \u0641\u0631\u0633\u062E \u0641\u0644\u0643\u064A) \u0645\u0646 \u0627\u0644\u0623\u0631\u0636.\u0625\u064A\u062A\u0627 \u0627\u0644\u0631\u0627\u0645\u064A \u0645\u0646 \u0636\u0645\u0646 \u0645\u062C\u0645\u0629 \u0627\u0644\u0646\u0639\u0627\u0645 \u0627\u0644\u0648\u0627\u0631\u062F \u0645\u0639 \u0646\u062C\u0648\u0645 \u0627\u0644\u0646\u0635\u0644 \u0648\u0648\u0633\u0637 \u0627\u0644\u0642\u0648\u0633 \u0648\u0627\u0644\u0642\u0648\u0633 \u0627\u0644\u062C\u0646\u0648\u0628\u064A ."@ar ;
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dbp:appmagV "+3.11/+7.8"@en ;
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