@prefix foaf:	<http://xmlns.com/foaf/0.1/> .
@prefix wikipedia-en:	<http://en.wikipedia.org/wiki/> .
@prefix dbr:	<http://dbpedia.org/resource/> .
wikipedia-en:Rho_Scorpii	foaf:primaryTopic	dbr:Rho_Scorpii .
@prefix dbo:	<http://dbpedia.org/ontology/> .
dbr:Delta_Scorpii	dbo:wikiPageWikiLink	dbr:Rho_Scorpii .
dbr:Table_of_stars_with_Bayer_designations	dbo:wikiPageWikiLink	dbr:Rho_Scorpii .
dbr:Table_of_stars_with_Flamsteed_designations	dbo:wikiPageWikiLink	dbr:Rho_Scorpii .
dbr:Scorpius_in_Chinese_astronomy	dbo:wikiPageWikiLink	dbr:Rho_Scorpii .
@prefix rdf:	<http://www.w3.org/1999/02/22-rdf-syntax-ns#> .
@prefix yago:	<http://dbpedia.org/class/yago/> .
dbr:Rho_Scorpii	rdf:type	yago:WikicatBayerObjects ,
		yago:Object100002684 .
@prefix schema:	<http://schema.org/> .
dbr:Rho_Scorpii	rdf:type	schema:Place ,
		yago:Whole100003553 ,
		yago:NaturalObject100019128 ,
		yago:Animal100015388 ,
		yago:Organism100004475 ,
		yago:LivingThing100004258 ,
		dbo:Star .
@prefix owl:	<http://www.w3.org/2002/07/owl#> .
dbr:Rho_Scorpii	rdf:type	owl:Thing ,
		yago:CelestialBody109239740 ,
		yago:Giant101323781 ,
		dbo:CelestialBody ,
		yago:WikicatBinaryStars ,
		yago:PhysicalEntity100001930 ,
		dbo:Location ,
		yago:BinaryStar109221070 ,
		yago:WikicatB-typeMain-sequenceStars ,
		yago:WikicatB-typeStars ,
		dbo:Place ,
		yago:WikicatB-typeGiants ,
		yago:WikicatStars ,
		yago:Star109444100 .
@prefix rdfs:	<http://www.w3.org/2000/01/rdf-schema#> .
dbr:Rho_Scorpii	rdfs:label	"Rho Scorpii"@sv ,
		"\u623F\u5BBF\u4E8C"@zh ,
		"Rho Scorpii"@fr ,
		"Rho Scorpii"@pt ,
		"Ro Scorpii"@pl ,
		"Rho Scorpii"@en ,
		"Rho Scorpii"@es ,
		"Rho Scorpii"@it ,
		"Rho de l'Escorpi\u00F3"@ca ,
		"\u3055\u305D\u308A\u5EA7\u30ED\u30FC\u661F"@ja ,
		"\u0420\u043E \u0421\u043A\u043E\u0440\u043F\u0438\u043E\u043D\u0430"@ru ;
	rdfs:comment	"Rho de l'Escorpi\u00F3 (\u03C1 Scorpii) \u00E9s un estel de magnitud aparent +3,86 situat a la constel\u00B7laci\u00F3 de l'Escorpi\u00F3. S'hi troba a 409 anys llum del sistema solar, pertanyent \u2014igual que Antares (\u03B1 Scorpii), o \u2014 a l'Associaci\u00F3 d'Escorpi\u00F3 Superior, subgrup de la gran Associaci\u00F3 estel\u00B7lar d'Escorpi\u00F3-Centaure."@ca ,
		"Ro Scorpii (\u03C1 Sco, Iklil) \u2013 gwiazda w gwiazdozbiorze Skorpiona. Jest odleg\u0142a o oko\u0142o 472 lata \u015Bwietlne od S\u0142o\u0144ca."@pl ,
		"Rho Scorpii (\u03C1 Sco / \u03C1 Scorpii), \u00E9galement nomm\u00E9e Iklil, est une \u00E9toile binaire de la constellation du Scorpion. Elle est \u00E0 environ 410 ann\u00E9es-lumi\u00E8re de la Terre. Rho Scorpii est un syst\u00E8me binaire spectroscopique, dont les deux \u00E9toiles orbitent l'une autour de l'autre avec une p\u00E9riode de quatre jours et avec une excentricit\u00E9 de 0,27. Sa composante visible est une \u00E9toile bleue-blanche de type spectral B2IV-V. Ce syst\u00E8me d'\u00E9toiles a \u00E9t\u00E9 d\u00E9couvert par le projet SETI.[r\u00E9f. n\u00E9cessaire]"@fr ,
		"Rho Scorpii (5 Scorpii) \u00E9 uma estrela na dire\u00E7\u00E3o da constela\u00E7\u00E3o de Scorpius. Possui uma ascens\u00E3o reta de 15h 56m 53.09s e uma declina\u00E7\u00E3o de \u221229\u00B0 12\u2032 50.4\u2033. Sua magnitude aparente \u00E9 igual a 3.87. Considerando sua dist\u00E2ncia de 409 anos-luz em rela\u00E7\u00E3o \u00E0 Terra, sua magnitude absoluta \u00E9 igual a \u22121.62. Pertence \u00E0 classe espectral B2IV/V."@pt ,
		"Rho Scorpii (\u03C1 Scorpii, f\u00F6rkortat Rho Sco, \u03C1 Sco), som \u00E4r stj\u00E4rnans Bayerbeteckning, \u00E4r en dubbelstj\u00E4rna bel\u00E4gen i den v\u00E4stra delen av stj\u00E4rnbilden Skorpionen. Den har en skenbar magnitud p\u00E5 +3,87 och \u00E4r synlig f\u00F6r blotta \u00F6gat. Baserat p\u00E5 parallaxm\u00E4tningar befinner den sig p\u00E5 ett avst\u00E5nd av 472 ljus\u00E5r (ca 145 parsek) fr\u00E5n solen. P\u00E5 det avst\u00E5ndet reduceras stj\u00E4rnans skenbara magnitud med 0,07 p\u00E5 grund av skymning av interstell\u00E4rt stoft."@sv ,
		"\u0420\u043E \u0421\u043A\u043E\u0440\u043F\u0438\u043E\u043D\u0430 (\u0418\u043A\u043B\u0438\u043B\u044C, \u03C1 Scorpii, \u03C1 Sco, Rho Scorpii, Rho Sco) \u2014 \u0437\u0432\u0435\u0437\u0434\u0430 \u0447\u0435\u0442\u0432\u0451\u0440\u0442\u043E\u0439 \u0432\u0435\u043B\u0438\u0447\u0438\u043D\u044B (3m.88) \u043D\u0430\u0445\u043E\u0434\u044F\u0449\u0430\u044F\u0441\u044F \u0432 \u0441\u043E\u0437\u0432\u0435\u0437\u0434\u0438\u0438 \u0421\u043A\u043E\u0440\u043F\u0438\u043E\u043D \u0440\u044F\u0434\u043E\u043C \u0441 \u0435\u0433\u043E \u0433\u043E\u043B\u043E\u0432\u043E\u0439 \u0438 \u043A\u043B\u0435\u0448\u043D\u044F\u043C\u0438. \u0415\u0451 \u043B\u0435\u0433\u043A\u043E \u043D\u0430\u0439\u0442\u0438, \u0441\u043B\u0435\u0434\u0443\u044F \u0432\u0437\u0433\u043B\u044F\u0434\u043E\u043C \u0432\u043D\u0438\u0437 \u043E\u0442 \u044F\u0440\u043A\u043E\u0433\u043E \u0413\u0440\u0430\u0444\u0444\u0438\u0430\u0441\u0430 (\u0411\u0435\u0442\u0430 \u0421\u043A\u043E\u0440\u043F\u0438\u043E\u043D\u0430) \u0447\u0435\u0440\u0435\u0437 \u0414\u0448\u0443\u0431\u0431\u0443 (\u0414\u0435\u043B\u044C\u0442\u0430 \u0421\u043A\u043E\u0440\u043F\u0438\u043E\u043D\u0430) \u0438 \u041F\u0438 \u0421\u043A\u043E\u0440\u043F\u0438\u043E\u043D\u0430: \u0441\u043B\u0435\u0434\u0443\u044E\u0449\u0430\u044F \u043F\u043E \u044F\u0440\u043A\u043E\u0441\u0442\u0438 \u0437\u0432\u0435\u0437\u0434\u0430 \u0431\u0443\u0434\u0435\u0442 \u0420\u043E. \u0418\u043C\u0435\u044F \u0441\u043A\u043B\u043E\u043D\u0435\u043D\u0438\u0435 29\u00B0 \u044E\u0436\u043D\u0435\u0435 \u043D\u0435\u0431\u0435\u0441\u043D\u043E\u0433\u043E \u044D\u043A\u0432\u0430\u0442\u043E\u0440\u0430, \u0420\u043E \u0421\u043A\u043E\u0440\u043F\u0438\u043E\u043D\u0430 \u044F\u0432\u043B\u044F\u0435\u0442\u0441\u044F \u0437\u0432\u0435\u0437\u0434\u043E\u0439 \u044E\u0436\u043D\u043E\u0433\u043E \u043F\u043E\u043B\u0443\u0448\u0430\u0440\u0438\u044F. \u0412 \u0441\u0435\u0432\u0435\u0440\u043D\u043E\u043C \u043F\u043E\u043B\u0443\u0448\u0430\u0440\u0438\u0438 \u0437\u0432\u0435\u0437\u0434\u0430 \u043D\u0430\u0431\u043B\u044E\u0434\u0430\u0435\u0442\u0441\u044F \u0434\u043E 61\u00B0 \u0441\u0435\u0432\u0435\u0440\u043D\u043E\u0439 \u0448\u0438\u0440\u043E\u0442\u044B, \u0442\u043E \u0435\u0441\u0442\u044C \u043F\u0440\u0430\u043A\u0442\u0438\u0447\u0435\u0441\u043A\u0438 \u0432\u043E \u0432\u0441\u0435\u0445 \u0441\u0442\u0440\u0430\u043D\u0430\u0445, \u0437\u0430. \u0438\u0441\u043A\u043B\u044E\u0447\u0435\u043D\u0438\u0435\u043C \u0413\u0440\u0435\u043D\u043B\u0430\u043D\u0434\u0438\u0438, \u0441\u0435\u0432\u0435\u0440\u043D\u044B\u0445 \u0440\u0435\u0433\u0438\u043E\u043D\u043E\u0432 \u041A\u0430\u043D\u0430\u0434\u044B \u0438 \u0420\u043E\u0441\u0441\u0438\u0438, \u0430 \u0442\u0430\u043A\u0436\u0435 \u0418\u0441\u043B\u0430\u043D\u0434\u0438\u0438 \u0438 \u0431\u043E\u043B\u044C\u0448\u0435\u0439 \u0447\u0430\u0441\u0442\u0438 \u0428\u0432\u0435\u0446\u0438\u0438 \u0438 \u041D\u043E\u0440\u0432\u0435\u0433\u0438\u0438. \u041B\u0443\u0447\u0448\u0438\u0435 \u043C\u0435\u0441\u044F\u0446\u044B \u0434\u043B\u044F \u043D\u0430\u0431\u043B\u044E\u0434\u0435\u043D\u0438\u044F \u0437\u0432\u0435\u0437\u0434\u044B \u0441 \u043C\u0430\u044F \u043F\u043E \u0430\u0432\u0433\u0443\u0441\u0442. \u0412 2017 \u0433\u043E\u0434\u0443 \u041C\u0435\u0436\u0434\u0443\u043D\u0430\u0440\u043E\u0434\u043D\u044B\u0439 \u0430\u0441\u0442\u0440\u043E\u043D\u043E\u043C\u0438\u0447\u0435\u0441\u043A\u0438\u0439 \u0441\u043E\u044E\u0437 \u043F\u0440\u0438\u0441\u0432\u043E\u0438\u043B \u043E\u0444\u0438\u0446\u0438\u0430\u043B\u044C\u043D\u043E\u0435 \u0441\u043E\u0431\u0441\u0442\u0432\u0435\u043D\u043D\u043E\u0435 \u0438\u043C\u044F \u0437\u0432\u0435\u0437\u0434\u0435 \u2014 \u0418\u043A\u043B\u0438\u043B\u044C, \u0432 \u0447\u0435\u0441\u0442\u044C \u0438\u0441\u0442\u043E\u0440\u0438"@ru ,
		"\u623F\u5BBF\u4E8C(\u5929\u874E\u5EA7\u03C1)\u662F\u4F4D\u4E8E\u5929\u874E\u5EA7\u7684\u53CC\u661F\u7CFB\u7EDF\uFF0C\u5176\u89C6\u661F\u7B49\u4E3A3.87\u3002"@zh ,
		"Rho Scorpii (\u03C1 Scorpii, abbreviated Rho Sco, \u03C1 Sco) is a double star in the constellation of Scorpius. It has an apparent visual magnitude of +3.87, which is bright enough to be seen with the naked eye. Based upon parallax measurements, it is located approximately 472 light years from the Sun. At that distance, the visual magnitude of the system is reduced by 0.07 due to extinction from interstellar dust. It is a member of the Upper Scorpius OB association."@en ,
		"Rho Scorpii (\u03C1 Sco / \u03C1 Scorpii, detta anche Iklil) \u00E8 una stella di magnitudine +3,87 appartenente alla costellazione dello Scorpione."@it ,
		"\u3055\u305D\u308A\u5EA7\u03C1\u661F\uFF08\u3055\u305D\u308A\u5EA7\u30ED\u30FC\u661F\u3001\u03C1 Sco / \u03C1 Scorpii\uFF09\uFF09\u306F\u3001\u3055\u305D\u308A\u5EA7\u306E\u6052\u661F\u30674\u7B49\u661F\u3002"@ja ,
		"Rho Scorpii (\u03C1 Sco / 5 Scorpii / HD 142669 / HR 5928) es una estrella de magnitud aparente +3,86\u200B situada en la constelaci\u00F3n del Escorpi\u00F3n.Se encuentra a 409 a\u00F1os luz del Sistema Solar, perteneciendo \u2014al igual que Antares (\u03B1 Scorpii), \u03C1 Ophiuchi o 48 Librae\u2014 a la Asociaci\u00F3n Scorpius Superior, subgrupo de la gran Asociaci\u00F3n estelar de Scorpius-Centaurus.\u200B"@es ;
	foaf:name	"\u03C1 Scorpii"@en ;
	foaf:depiction	<http://commons.wikimedia.org/wiki/Special:FilePath/Scorpius_constellation_map.svg> ,
		<http://commons.wikimedia.org/wiki/Special:FilePath/Red_circle.svg> .
@prefix dcterms:	<http://purl.org/dc/terms/> .
@prefix dbc:	<http://dbpedia.org/resource/Category:> .
dbr:Rho_Scorpii	dcterms:subject	dbc:Bayer_objects ,
		<http://dbpedia.org/resource/Category:Scorpius_(constellation)> ,
		dbc:Upper_Scorpius ,
		dbc:Flamsteed_objects ,
		dbc:B-type_subgiants ,
		dbc:Binary_stars ,
		dbc:Henry_Draper_Catalogue_objects ,
		dbc:Bright_Star_Catalogue_objects ,
		dbc:Hipparcos_objects ,
		dbc:Durchmusterung_objects ;
	dbo:abstract	"Rho Scorpii (\u03C1 Scorpii, f\u00F6rkortat Rho Sco, \u03C1 Sco), som \u00E4r stj\u00E4rnans Bayerbeteckning, \u00E4r en dubbelstj\u00E4rna bel\u00E4gen i den v\u00E4stra delen av stj\u00E4rnbilden Skorpionen. Den har en skenbar magnitud p\u00E5 +3,87 och \u00E4r synlig f\u00F6r blotta \u00F6gat. Baserat p\u00E5 parallaxm\u00E4tningar befinner den sig p\u00E5 ett avst\u00E5nd av 472 ljus\u00E5r (ca 145 parsek) fr\u00E5n solen. P\u00E5 det avst\u00E5ndet reduceras stj\u00E4rnans skenbara magnitud med 0,07 p\u00E5 grund av skymning av interstell\u00E4rt stoft."@sv ,
		"Ro Scorpii (\u03C1 Sco, Iklil) \u2013 gwiazda w gwiazdozbiorze Skorpiona. Jest odleg\u0142a o oko\u0142o 472 lata \u015Bwietlne od S\u0142o\u0144ca."@pl ,
		"Rho Scorpii (\u03C1 Scorpii, abbreviated Rho Sco, \u03C1 Sco) is a double star in the constellation of Scorpius. It has an apparent visual magnitude of +3.87, which is bright enough to be seen with the naked eye. Based upon parallax measurements, it is located approximately 472 light years from the Sun. At that distance, the visual magnitude of the system is reduced by 0.07 due to extinction from interstellar dust. It is a member of the Upper Scorpius OB association. It has two components, designated Rho Scorpii A and B. Rho Scorpii A is itself a single-lined spectroscopic binary whose components are designated Rho Scorpii Aa (formally named Iklil /\u02C8\u026Akl\u026Al/, traditionally the name for several neighboring stars) and Ab."@en ,
		"Rho de l'Escorpi\u00F3 (\u03C1 Scorpii) \u00E9s un estel de magnitud aparent +3,86 situat a la constel\u00B7laci\u00F3 de l'Escorpi\u00F3. S'hi troba a 409 anys llum del sistema solar, pertanyent \u2014igual que Antares (\u03B1 Scorpii), o \u2014 a l'Associaci\u00F3 d'Escorpi\u00F3 Superior, subgrup de la gran Associaci\u00F3 estel\u00B7lar d'Escorpi\u00F3-Centaure. Rho de l'Escorpi\u00F3 \u00E9s un estel blau de la seq\u00FC\u00E8ncia principal \u2014tamb\u00E9 catalogat com a possible subgegant\u2014 de tipus espectral B2 la temperatura superficial del qual \u00E9s 21.150 K. Llueix amb una lluminositat 2.540 vegades superior a la del Sol i el seu radi \u00E9s 3,75 vegades m\u00E9s gran que el radi solar. T\u00E9 una edat aproximada de 33 milions d'anys i \u00E9s 7,5 vegades m\u00E9s massiu que el Sol; just per sota del l\u00EDmit per esclatar com a supernova, probablement finalitzar\u00E0 la seva vida com una nana blanca massiva similar a S\u00EDrius B (\u03B1 Canis Majoris B). Gira sobre si mateixa amb una velocitat de rotaci\u00F3 d'almenys 40 km/s, sent el seu per\u00EDodes de rotaci\u00F3 inferior a 1,4 dies. Rho de l'Escorpi\u00F3 \u00E9s una estrella bin\u00E0ria espectrosc\u00F2pica amb un per\u00EDode orbital de 4,003 dies. De l'estrella acompanyant res se sap, tret que s'hi mou en una \u00F2rbita relativament exc\u00E8ntrica (\u03B5 = 0,27). Un t\u00E8nue estel de magnitud +12,8, visualment a 40 segons d'arc, tamb\u00E9 sembla formar part del sistema. Comparteix moviment propi amb Rho Scorpii i, si veritablement est\u00E0 lligada al llumin\u00F3s estel blau, est\u00E0 separada d'ella almenys 4.900 UA, completant una \u00F2rbita en m\u00E9s de 114.000 anys."@ca ,
		"Rho Scorpii (\u03C1 Sco / \u03C1 Scorpii), \u00E9galement nomm\u00E9e Iklil, est une \u00E9toile binaire de la constellation du Scorpion. Elle est \u00E0 environ 410 ann\u00E9es-lumi\u00E8re de la Terre. Rho Scorpii est un syst\u00E8me binaire spectroscopique, dont les deux \u00E9toiles orbitent l'une autour de l'autre avec une p\u00E9riode de quatre jours et avec une excentricit\u00E9 de 0,27. Sa composante visible est une \u00E9toile bleue-blanche de type spectral B2IV-V. Ce syst\u00E8me d'\u00E9toiles a \u00E9t\u00E9 d\u00E9couvert par le projet SETI.[r\u00E9f. n\u00E9cessaire]"@fr ,
		"\u3055\u305D\u308A\u5EA7\u03C1\u661F\uFF08\u3055\u305D\u308A\u5EA7\u30ED\u30FC\u661F\u3001\u03C1 Sco / \u03C1 Scorpii\uFF09\uFF09\u306F\u3001\u3055\u305D\u308A\u5EA7\u306E\u6052\u661F\u30674\u7B49\u661F\u3002"@ja ,
		"\u0420\u043E \u0421\u043A\u043E\u0440\u043F\u0438\u043E\u043D\u0430 (\u0418\u043A\u043B\u0438\u043B\u044C, \u03C1 Scorpii, \u03C1 Sco, Rho Scorpii, Rho Sco) \u2014 \u0437\u0432\u0435\u0437\u0434\u0430 \u0447\u0435\u0442\u0432\u0451\u0440\u0442\u043E\u0439 \u0432\u0435\u043B\u0438\u0447\u0438\u043D\u044B (3m.88) \u043D\u0430\u0445\u043E\u0434\u044F\u0449\u0430\u044F\u0441\u044F \u0432 \u0441\u043E\u0437\u0432\u0435\u0437\u0434\u0438\u0438 \u0421\u043A\u043E\u0440\u043F\u0438\u043E\u043D \u0440\u044F\u0434\u043E\u043C \u0441 \u0435\u0433\u043E \u0433\u043E\u043B\u043E\u0432\u043E\u0439 \u0438 \u043A\u043B\u0435\u0448\u043D\u044F\u043C\u0438. \u0415\u0451 \u043B\u0435\u0433\u043A\u043E \u043D\u0430\u0439\u0442\u0438, \u0441\u043B\u0435\u0434\u0443\u044F \u0432\u0437\u0433\u043B\u044F\u0434\u043E\u043C \u0432\u043D\u0438\u0437 \u043E\u0442 \u044F\u0440\u043A\u043E\u0433\u043E \u0413\u0440\u0430\u0444\u0444\u0438\u0430\u0441\u0430 (\u0411\u0435\u0442\u0430 \u0421\u043A\u043E\u0440\u043F\u0438\u043E\u043D\u0430) \u0447\u0435\u0440\u0435\u0437 \u0414\u0448\u0443\u0431\u0431\u0443 (\u0414\u0435\u043B\u044C\u0442\u0430 \u0421\u043A\u043E\u0440\u043F\u0438\u043E\u043D\u0430) \u0438 \u041F\u0438 \u0421\u043A\u043E\u0440\u043F\u0438\u043E\u043D\u0430: \u0441\u043B\u0435\u0434\u0443\u044E\u0449\u0430\u044F \u043F\u043E \u044F\u0440\u043A\u043E\u0441\u0442\u0438 \u0437\u0432\u0435\u0437\u0434\u0430 \u0431\u0443\u0434\u0435\u0442 \u0420\u043E. \u0418\u043C\u0435\u044F \u0441\u043A\u043B\u043E\u043D\u0435\u043D\u0438\u0435 29\u00B0 \u044E\u0436\u043D\u0435\u0435 \u043D\u0435\u0431\u0435\u0441\u043D\u043E\u0433\u043E \u044D\u043A\u0432\u0430\u0442\u043E\u0440\u0430, \u0420\u043E \u0421\u043A\u043E\u0440\u043F\u0438\u043E\u043D\u0430 \u044F\u0432\u043B\u044F\u0435\u0442\u0441\u044F \u0437\u0432\u0435\u0437\u0434\u043E\u0439 \u044E\u0436\u043D\u043E\u0433\u043E \u043F\u043E\u043B\u0443\u0448\u0430\u0440\u0438\u044F. \u0412 \u0441\u0435\u0432\u0435\u0440\u043D\u043E\u043C \u043F\u043E\u043B\u0443\u0448\u0430\u0440\u0438\u0438 \u0437\u0432\u0435\u0437\u0434\u0430 \u043D\u0430\u0431\u043B\u044E\u0434\u0430\u0435\u0442\u0441\u044F \u0434\u043E 61\u00B0 \u0441\u0435\u0432\u0435\u0440\u043D\u043E\u0439 \u0448\u0438\u0440\u043E\u0442\u044B, \u0442\u043E \u0435\u0441\u0442\u044C \u043F\u0440\u0430\u043A\u0442\u0438\u0447\u0435\u0441\u043A\u0438 \u0432\u043E \u0432\u0441\u0435\u0445 \u0441\u0442\u0440\u0430\u043D\u0430\u0445, \u0437\u0430. \u0438\u0441\u043A\u043B\u044E\u0447\u0435\u043D\u0438\u0435\u043C \u0413\u0440\u0435\u043D\u043B\u0430\u043D\u0434\u0438\u0438, \u0441\u0435\u0432\u0435\u0440\u043D\u044B\u0445 \u0440\u0435\u0433\u0438\u043E\u043D\u043E\u0432 \u041A\u0430\u043D\u0430\u0434\u044B \u0438 \u0420\u043E\u0441\u0441\u0438\u0438, \u0430 \u0442\u0430\u043A\u0436\u0435 \u0418\u0441\u043B\u0430\u043D\u0434\u0438\u0438 \u0438 \u0431\u043E\u043B\u044C\u0448\u0435\u0439 \u0447\u0430\u0441\u0442\u0438 \u0428\u0432\u0435\u0446\u0438\u0438 \u0438 \u041D\u043E\u0440\u0432\u0435\u0433\u0438\u0438. \u041B\u0443\u0447\u0448\u0438\u0435 \u043C\u0435\u0441\u044F\u0446\u044B \u0434\u043B\u044F \u043D\u0430\u0431\u043B\u044E\u0434\u0435\u043D\u0438\u044F \u0437\u0432\u0435\u0437\u0434\u044B \u0441 \u043C\u0430\u044F \u043F\u043E \u0430\u0432\u0433\u0443\u0441\u0442. \u0412 2017 \u0433\u043E\u0434\u0443 \u041C\u0435\u0436\u0434\u0443\u043D\u0430\u0440\u043E\u0434\u043D\u044B\u0439 \u0430\u0441\u0442\u0440\u043E\u043D\u043E\u043C\u0438\u0447\u0435\u0441\u043A\u0438\u0439 \u0441\u043E\u044E\u0437 \u043F\u0440\u0438\u0441\u0432\u043E\u0438\u043B \u043E\u0444\u0438\u0446\u0438\u0430\u043B\u044C\u043D\u043E\u0435 \u0441\u043E\u0431\u0441\u0442\u0432\u0435\u043D\u043D\u043E\u0435 \u0438\u043C\u044F \u0437\u0432\u0435\u0437\u0434\u0435 \u2014 \u0418\u043A\u043B\u0438\u043B\u044C, \u0432 \u0447\u0435\u0441\u0442\u044C \u0438\u0441\u0442\u043E\u0440\u0438\u0447\u0435\u0441\u043A\u043E\u0433\u043E \u0442\u0440\u0443\u0434\u0430 \u00AB\u0410\u043B\u044C-\u0418\u043A\u043B\u0438\u043B\u044C\u00BB, \u043D\u0430\u043F\u0438\u0441\u0430\u043D\u043D\u043E\u0433\u043E \u0430\u0440\u0430\u0431\u0441\u043A\u0438\u043C \u0443\u0447\u0451\u043D\u044B\u043C \u0410\u0431\u0443 \u041C\u0443\u0445\u0430\u043C\u043C\u0430\u0434\u043E\u043C \u0430\u043B\u044C-\u0425\u0430\u043C\u0434\u0430\u043D\u0438."@ru ,
		"\u623F\u5BBF\u4E8C(\u5929\u874E\u5EA7\u03C1)\u662F\u4F4D\u4E8E\u5929\u874E\u5EA7\u7684\u53CC\u661F\u7CFB\u7EDF\uFF0C\u5176\u89C6\u661F\u7B49\u4E3A3.87\u3002"@zh ,
		"Rho Scorpii (5 Scorpii) \u00E9 uma estrela na dire\u00E7\u00E3o da constela\u00E7\u00E3o de Scorpius. Possui uma ascens\u00E3o reta de 15h 56m 53.09s e uma declina\u00E7\u00E3o de \u221229\u00B0 12\u2032 50.4\u2033. Sua magnitude aparente \u00E9 igual a 3.87. Considerando sua dist\u00E2ncia de 409 anos-luz em rela\u00E7\u00E3o \u00E0 Terra, sua magnitude absoluta \u00E9 igual a \u22121.62. Pertence \u00E0 classe espectral B2IV/V."@pt ,
		"Rho Scorpii (\u03C1 Sco / 5 Scorpii / HD 142669 / HR 5928) es una estrella de magnitud aparente +3,86\u200B situada en la constelaci\u00F3n del Escorpi\u00F3n.Se encuentra a 409 a\u00F1os luz del Sistema Solar, perteneciendo \u2014al igual que Antares (\u03B1 Scorpii), \u03C1 Ophiuchi o 48 Librae\u2014 a la Asociaci\u00F3n Scorpius Superior, subgrupo de la gran Asociaci\u00F3n estelar de Scorpius-Centaurus.\u200B Rho Scorpii es una estrella azul de la secuencia principal \u2014tambi\u00E9n catalogada como posible subgigante\u2014\u200B de tipo espectral B2 cuya temperatura superficial es 21.150 K.Brilla con una luminosidad 2540 veces superior a la del Sol y su radio es 3,75 veces m\u00E1s grande que el radio solar.Tiene una edad aproximada de 33 millones de a\u00F1os y es 7,5 veces m\u00E1s masiva que el Sol; justo por debajo del l\u00EDmite para estallar como supernova, probablemente finalizar\u00E1 su vida como una enana blanca masiva similar a Sirio B (\u03B1 Canis Majoris B).Gira sobre s\u00ED misma con una velocidad de rotaci\u00F3n de al menos 40 km/s, siendo su per\u00EDodos de rotaci\u00F3n inferior a 1,4 d\u00EDas.\u200B Rho Scorpii es una binaria espectrosc\u00F3pica con un per\u00EDodo orbital de 4,003 d\u00EDas.De la estrella acompa\u00F1ante nada se sabe, salvo que se mueve en una \u00F3rbita relativamente exc\u00E9ntrica (\u03B5 = 0,27).Una tenue estrella de magnitud +12,8, visualmente a 40 segundos de arco, tambi\u00E9n parece formar parte del sistema. Comparte movimiento propio con Rho Scorpii y, si verdaderamente est\u00E1 ligada a la luminosa estrella azul, est\u00E1 separada de ella al menos 4900 UA, completando una \u00F3rbita en m\u00E1s de 114.000 a\u00F1os.\u200B"@es ,
		"Rho Scorpii (\u03C1 Sco / \u03C1 Scorpii, detta anche Iklil) \u00E8 una stella di magnitudine +3,87 appartenente alla costellazione dello Scorpione."@it ;
	dbo:wikiPageWikiLink	<http://dbpedia.org/resource/Room_(Chinese_constellation)> ,
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@prefix dbp:	<http://dbpedia.org/property/> .
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dbr:List_of_Arabic_star_names	dbo:wikiPageWikiLink	dbr:Rho_Scorpii .
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	dbo:wikiPageRedirects	dbr:Rho_Scorpii .  <script>parent.window.postMessage('ixistenz.url:http://dbpedia.org/data/Rho_Scorpii.ttl', '*'); </script> <div id='browserdiffcontainer' style='position: fixed; right: 10px; top: 10vh; min-width: 60px;  border: 1px solid white; background: rgb(251, 189, 0);; opacity: 0.9; font-family: helvetica, arial, sans serif;  font-size: 12px; z-index: 20001; padding-bottom: 20px;'><div onclick="toggle('browserdiffcontainerlist'); return false;" style='background: rgb(151, 89, 0);; color: white; '><strong>&nbsp; <span class='glyphicon glyphicon-minus'></span> NODES</strong></div><div id='browserdiffcontainerlist' style='padding-left: 10px; padding-right: 5px; max-height: 50vh; overflow: auto; '><div><a href='#diffid883' style='color: white;' onClick="parent.window.postMessage('ixistenz.opendiff:883', '*');; return false;" style='text-decoration: none; '>Association </a> <a style='color: white;' href='#diffid883'><sup>2</sup></a></div><div><a href='#diffid123' style='color: white;' onClick="parent.window.postMessage('ixistenz.opendiff:123', '*');; return false;" style='text-decoration: none; '>INTERN </a> <a style='color: white;' href='#diffid123'><sup>1</sup></a></div></div></div>
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