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"http://www.w3.org/2000/01/rdf-schema#label" : [ { "type" : "literal", "value" : "NGC 3862" , "lang" : "fr" } ,
{ "type" : "literal", "value" : "NGC 3862" , "lang" : "ru" } ,
{ "type" : "literal", "value" : "NGC 3862" , "lang" : "de" } ,
{ "type" : "literal", "value" : "NGC 3862" , "lang" : "eo" } ,
{ "type" : "literal", "value" : "NGC 3862" , "lang" : "uk" } ,
{ "type" : "literal", "value" : "NGC 3862" , "lang" : "en" } ,
{ "type" : "literal", "value" : "NGC 3862" , "lang" : "it" } ,
{ "type" : "literal", "value" : "NGC 3862" , "lang" : "pt" } ,
{ "type" : "literal", "value" : "NGC 3862" , "lang" : "pl" } ,
{ "type" : "literal", "value" : "NGC 3862" , "lang" : "eu" } ,
{ "type" : "literal", "value" : "NGC 3862" , "lang" : "nl" } ] ,
"http://www.w3.org/2000/01/rdf-schema#comment" : [ { "type" : "literal", "value" : "NGC 3862 est une galaxie elliptique situ\u00E9e dans la constellation du Lion \u00E0 environ 297 millions d'ann\u00E9es-lumi\u00E8re de la Voie lact\u00E9e. NGC 3862 a \u00E9t\u00E9 d\u00E9couverte par l'astronome germano-britannique William Herschel en 1785. NGC 3862 une galaxie \u00E0 noyau actif (AGN). C'est une galaxie \u00E0 faible \u00E9mission radio (low-excitation radio galaxy, LERG) et \u00E9galement une galaxie dont le noyau pr\u00E9sente un spectre d'\u00E9mission caract\u00E9ris\u00E9 par de larges raies d'atomes faiblement ionis\u00E9s (LINER)). Selon la base de donn\u00E9es Simbad, NGC 3862 est une galaxie active qui contient un quasar (3C 264.0)." , "lang" : "fr" } ,
{ "type" : "literal", "value" : "NGC 3862 o 3C 264 o 3C 264 (B 1142+198), \u00E8 una galassia ellittica che fa parte dell'ammasso di galassie Abell 1367, anche noto come Ammasso del Leone. Fu scoperta il 27 aprile 1785 da William Herschel. NGC 3862 ha una compagna, la galassia ellittica o lenticolare , che si trova ad una distanza di circa 72000 anni luce. \n* NGC 3862 e IC 2955 (in alto) (SDSS DR14) \n*" , "lang" : "it" } ,
{ "type" : "literal", "value" : "NGC 3862 (r\u00F3wnie\u017C PGC 36606 lub UGC 6723) \u2013 galaktyka eliptyczna (E), znajduj\u0105ca si\u0119 w gwiazdozbiorze Lwa. Odkry\u0142 j\u0105 William Herschel 27 kwietnia 1785 roku. Nale\u017Cy do gromady galaktyk Abell 1367. NGC 3862 to galaktyka z aktywnym j\u0105drem. Jest jedn\u0105 z nielicznych znanych galaktyk aktywnych, w kt\u00F3rych w \u015Bwietle widzialnym wykryto d\u017Cet wydobywaj\u0105cy si\u0119 z supermasywnej czarnej dziury w centrum galaktyki. W d\u017Cecie tym znajduj\u0105 si\u0119 ja\u015Bniejsze obszary, kt\u00F3re wydaj\u0105 si\u0119 porusza\u0107 z pr\u0119dko\u015Bci\u0105 kilkukrotnie wi\u0119ksz\u0105 ni\u017C pr\u0119dko\u015B\u0107 \u015Bwiat\u0142a w pr\u00F3\u017Cni, lecz jest to tylko z\u0142udzenie optyczne, w rzeczywisto\u015Bci materia w d\u017Cecie porusza si\u0119 z pr\u0119dko\u015Bci\u0105 ponad 98% pr\u0119dko\u015Bci \u015Bwiat\u0142a w pr\u00F3\u017Cni. Ponadto w 2014 roku zauwa\u017Cono, \u017Ce jeden z tych ja\u015Bniejszych obszar\u00F3w w d\u017Cecie \u201Edogoni\u0142\u201D drugi i po\u0142\u0105czy\u0142 si\u0119 z nim." , "lang" : "pl" } ,
{ "type" : "literal", "value" : "NGC 3862 \u00E9 uma gal\u00E1xia el\u00EDptica (E) localizada na direc\u00E7\u00E3o da constela\u00E7\u00E3o de Leo. Possui uma declina\u00E7\u00E3o de +19\u00B0 36' 23\" e uma ascens\u00E3o recta de 11 horas, 45 minutos e 05,0 segundos. A gal\u00E1xia NGC 3862 foi descoberta em 27 de Abril de 1785 por William Herschel." , "lang" : "pt" } ,
{ "type" : "literal", "value" : "NGC 3862 ist eine elliptische Radiogalaxie vom Hubble-Typ E0 im Sternbild L\u00F6we an der Ekliptik. Sie ist sch\u00E4tzungsweise 289 Millionen Lichtjahre von der Milchstra\u00DFe entfernt und hat einen Durchmesser von etwa 130.000 Lichtjahren. Sie ist Mitglied des Abell 1367-Galaxienhaufens. Im selben Himmelsareal befinden sich u. a. die Galaxien NGC 3857, NGC 3859, NGC 3868, IC 2955. Das Objekt wurde am 27. April 1785 von dem Astronomen Wilhelm Herschel mit seinem 18,7-Zoll-Spiegelteleskop entdeckt." , "lang" : "de" } ,
{ "type" : "literal", "value" : "NGC 3862 is an elliptical galaxy located 300 million light-years away in the constellation Leo. Discovered by astronomer William Herschel on April 27, 1785, NGC 3862 is an outlying member of the Leo Cluster. The galaxy is classified as a FR I radio galaxy and as a Head-tail radio galaxy. It hosts a supermassive black hole that is blasting a jet of plasma that is moving at 98 percent of the speed of light and is one of the few jets that can be seen in visible light." , "lang" : "en" } ,
{ "type" : "literal", "value" : "NGC 3862 galaxia bat da, konstelazioan. William Herschelek aurkitu zuen 1785eko apirilaren\u202F27an." , "lang" : "eu" } ,
{ "type" : "literal", "value" : "NGC 3862 \u2014 \u0433\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u0430 \u0442\u0438\u043F\u0443 E (\u0435\u043B\u0456\u043F\u0442\u0438\u0447\u043D\u0430 \u0433\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u0430) \u0443 \u0441\u0443\u0437\u0456\u0440'\u0457 \u041B\u0435\u0432. \u0412\u0456\u0434\u043A\u0440\u0438\u0432\u0430\u0447\u0435\u043C \u0446\u044C\u043E\u0433\u043E \u043E\u0431'\u0454\u043A\u0442\u0430 \u0454 \u0424\u0440\u0456\u0434\u0440\u0456\u0445 \u0412\u0456\u043B\u044C\u0433\u0435\u043B\u044C\u043C \u0413\u0435\u0440\u0448\u0435\u043B\u044C, \u044F\u043A\u0438\u0439 \u0443\u043F\u0435\u0440\u0448\u0435 \u0441\u043F\u043E\u0441\u0442\u0435\u0440\u0456\u0433\u0430\u0432 \u0437\u0430 \u043E\u0431'\u0454\u043A\u0442\u043E\u043C 27 \u043A\u0432\u0456\u0442\u043D\u044F 1785. \u0426\u0435\u0439 \u043E\u0431'\u0454\u043A\u0442 \u043C\u0456\u0441\u0442\u0438\u0442\u044C\u0441\u044F \u0432 \u043E\u0440\u0438\u0433\u0456\u043D\u0430\u043B\u044C\u043D\u0456\u0439 \u0440\u0435\u0434\u0430\u043A\u0446\u0456\u0457 \u041D\u043E\u0432\u043E\u0433\u043E \u0437\u0430\u0433\u0430\u043B\u044C\u043D\u043E\u0433\u043E \u043A\u0430\u0442\u0430\u043B\u043E\u0433\u0443." , "lang" : "uk" } ,
{ "type" : "literal", "value" : "NGC 3862 (aliaj indikoj \u2014 UGC 6723, MCG 3-30-95, ZWG 97.127, 3C 264, PGC 36606) estas galaksio en konstelacio Leono. \u0108i tiu objekto estis jam en la originala versio de NGC-katalogo." , "lang" : "eo" } ,
{ "type" : "literal", "value" : "NGC 3862 (\u0434\u0440\u0443\u0433\u0438\u0435 \u043E\u0431\u043E\u0437\u043D\u0430\u0447\u0435\u043D\u0438\u044F \u2014 UGC 6723, MCG 3-30-95, ZWG 97.127, 3C 264, PGC 36606) \u2014 \u044D\u043B\u043B\u0438\u043F\u0442\u0438\u0447\u0435\u0441\u043A\u0430\u044F \u0433\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u0430 (E) \u0432 \u0441\u043E\u0437\u0432\u0435\u0437\u0434\u0438\u0438 \u041B\u0435\u0432. \u042D\u0442\u043E\u0442 \u043E\u0431\u044A\u0435\u043A\u0442 \u0432\u0445\u043E\u0434\u0438\u0442 \u0432 \u0447\u0438\u0441\u043B\u043E \u043F\u0435\u0440\u0435\u0447\u0438\u0441\u043B\u0435\u043D\u043D\u044B\u0445 \u0432 \u043E\u0440\u0438\u0433\u0438\u043D\u0430\u043B\u044C\u043D\u043E\u0439 \u0440\u0435\u0434\u0430\u043A\u0446\u0438\u0438 \u00AB\u041D\u043E\u0432\u043E\u0433\u043E \u043E\u0431\u0449\u0435\u0433\u043E \u043A\u0430\u0442\u0430\u043B\u043E\u0433\u0430\u00BB. \u0413\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u0430 NGC 3862 \u0432\u0445\u043E\u0434\u0438\u0442 \u0432 \u0441\u043E\u0441\u0442\u0430\u0432 \u0433\u0440\u0443\u043F\u043F\u044B \u0433\u0430\u043B\u0430\u043A\u0442\u0438\u043A NGC 3842. \u041F\u043E\u043C\u0438\u043C\u043E NGC 3862 \u0432 \u0433\u0440\u0443\u043F\u043F\u0443 \u0442\u0430\u043A\u0436\u0435 \u0432\u0445\u043E\u0434\u044F\u0442 \u0435\u0449\u0451 17 \u0433\u0430\u043B\u0430\u043A\u0442\u0438\u043A. \u0412 \u0441\u0432\u043E\u044E \u043E\u0447\u0435\u0440\u0435\u0434\u044C \u0433\u0440\u0443\u043F\u043F\u0430 \u043E\u0442\u043D\u043E\u0441\u0438\u0442\u044C\u0441\u044F \u043A \u0431\u043E\u043B\u044C\u0448\u043E\u043C\u0443 \u0441\u043A\u043E\u043F\u043B\u0435\u043D\u0438\u044E \u041B\u044C\u0432\u0430. NGC 3862 \u0438\u043C\u0435\u0435\u0442 \u044D\u043B\u043B\u0438\u043F\u0442\u0438\u0447\u0435\u0441\u043A\u0443\u044E \u0438\u043B\u0438 \u043B\u0438\u043D\u0437\u043E\u0432\u0438\u0434\u043D\u0443\u044E \u0433\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u0443-\u043A\u043E\u043C\u043F\u0430\u043D\u044C\u043E\u043D, \u0438\u0437\u0432\u0435\u0441\u0442\u043D\u0443\u044E \u043A\u0430\u043A IC 2955. \u0418\u0441\u0442\u043E\u0447\u043D\u0438\u043A\u043E\u043C \u0434\u0436\u0435\u0442\u043E\u0432 \u044F\u0432\u043B\u044F\u0435\u0442\u0441\u044F \u0441\u0432\u0435\u0440\u0445\u043C\u0430\u0441\u0441\u0438\u0432\u043D\u0430\u044F \u0447\u0451\u0440\u043D\u0430\u044F \u0434\u044B\u0440\u0430 \u0441 \u043F\u0440\u0435\u0434\u043F\u043E\u043B\u0430\u0433\u0430\u0435\u043C\u043E\u0439 \u043C\u0430\u0441\u0441\u043E\u0439 4,7 \u00D7 10 8 M\u2609 ." , "lang" : "ru" } ,
{ "type" : "literal", "value" : "NGC 3862 is een elliptisch sterrenstelsel in het sterrenbeeld Leeuw. Het hemelobject werd op 27 april 1785 ontdekt door de Duits-Britse astronoom William Herschel." , "lang" : "nl" } ] ,
"http://xmlns.com/foaf/0.1/name" : [ { "type" : "literal", "value" : "NGC3862" , "lang" : "en" } ,
{ "type" : "literal", "value" : "UGC06723,PGC036606,MCG+03-30-095, CGCG 097-127, 3C 264, 4C +19.40, PKS 1142+19" , "lang" : "en" } ] ,
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{ "type" : "uri", "value" : "http://commons.wikimedia.org/wiki/Special:FilePath/Hs-2015-19-a-small_web.jpg" } ] ,
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{ "type" : "uri", "value" : "http://dbpedia.org/resource/Category:NGC_objects" } ,
{ "type" : "uri", "value" : "http://dbpedia.org/resource/Category:Leo_(constellation)" } ,
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"http://dbpedia.org/ontology/abstract" : [ { "type" : "literal", "value" : "NGC 3862 is een elliptisch sterrenstelsel in het sterrenbeeld Leeuw. Het hemelobject werd op 27 april 1785 ontdekt door de Duits-Britse astronoom William Herschel." , "lang" : "nl" } ,
{ "type" : "literal", "value" : "NGC 3862 is an elliptical galaxy located 300 million light-years away in the constellation Leo. Discovered by astronomer William Herschel on April 27, 1785, NGC 3862 is an outlying member of the Leo Cluster. The galaxy is classified as a FR I radio galaxy and as a Head-tail radio galaxy. It hosts a supermassive black hole that is blasting a jet of plasma that is moving at 98 percent of the speed of light and is one of the few jets that can be seen in visible light." , "lang" : "en" } ,
{ "type" : "literal", "value" : "NGC 3862 \u2014 \u0433\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u0430 \u0442\u0438\u043F\u0443 E (\u0435\u043B\u0456\u043F\u0442\u0438\u0447\u043D\u0430 \u0433\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u0430) \u0443 \u0441\u0443\u0437\u0456\u0440'\u0457 \u041B\u0435\u0432. \u0412\u0456\u0434\u043A\u0440\u0438\u0432\u0430\u0447\u0435\u043C \u0446\u044C\u043E\u0433\u043E \u043E\u0431'\u0454\u043A\u0442\u0430 \u0454 \u0424\u0440\u0456\u0434\u0440\u0456\u0445 \u0412\u0456\u043B\u044C\u0433\u0435\u043B\u044C\u043C \u0413\u0435\u0440\u0448\u0435\u043B\u044C, \u044F\u043A\u0438\u0439 \u0443\u043F\u0435\u0440\u0448\u0435 \u0441\u043F\u043E\u0441\u0442\u0435\u0440\u0456\u0433\u0430\u0432 \u0437\u0430 \u043E\u0431'\u0454\u043A\u0442\u043E\u043C 27 \u043A\u0432\u0456\u0442\u043D\u044F 1785. \u0426\u0435\u0439 \u043E\u0431'\u0454\u043A\u0442 \u043C\u0456\u0441\u0442\u0438\u0442\u044C\u0441\u044F \u0432 \u043E\u0440\u0438\u0433\u0456\u043D\u0430\u043B\u044C\u043D\u0456\u0439 \u0440\u0435\u0434\u0430\u043A\u0446\u0456\u0457 \u041D\u043E\u0432\u043E\u0433\u043E \u0437\u0430\u0433\u0430\u043B\u044C\u043D\u043E\u0433\u043E \u043A\u0430\u0442\u0430\u043B\u043E\u0433\u0443." , "lang" : "uk" } ,
{ "type" : "literal", "value" : "NGC 3862 o 3C 264 o 3C 264 (B 1142+198), \u00E8 una galassia ellittica che fa parte dell'ammasso di galassie Abell 1367, anche noto come Ammasso del Leone. Fu scoperta il 27 aprile 1785 da William Herschel. \u00C8 considerata la sesta pi\u00F9 brillante galassia tra quelle attive dell'ammasso, i cui getti sono individuabili anche nella luce visibile a causa della presenza al centro di una luminosa sorgente di raggi X e onde radio.NGC 3862 \u00E8 stata ampiamente studiata nel corso degli scorsi decenni (1992, 1994, 1996, 2002), mettendo in evidenza la presenza di un jet di particelle originantesi dal nucleo galattico, che si estende per una lunghezza di 750 anni luce, apparendo nettamente pi\u00F9 luminoso nello studio nella banda dell'ultravioletto, il che risulta piuttosto inusuale. Nel 2014 sono state riprese nuove immagini ad alta risoluzione dal telescopio Hubble e confrontate con i dati precedentemente acquisiti. In particolare si \u00E8 potuto rilevare che all'interno del getto, emesso dal centro galattico, parte della materia si aggrega in forma di \u201Cgrumi\u201D di plasma che, viaggiando a diverse velocit\u00E0, finiscono per scontrarsi generando un'onda d'urto. Un fenomeno simile non era mai stato osservato e le immagini rilevate a distanza di anni lo hanno messo chiaramente in evidenza. NGC 3862 ha una compagna, la galassia ellittica o lenticolare , che si trova ad una distanza di circa 72000 anni luce. \n* NGC 3862 e IC 2955 (in alto) (SDSS DR14) \n*" , "lang" : "it" } ,
{ "type" : "literal", "value" : "NGC 3862 (aliaj indikoj \u2014 UGC 6723, MCG 3-30-95, ZWG 97.127, 3C 264, PGC 36606) estas galaksio en konstelacio Leono. \u0108i tiu objekto estis jam en la originala versio de NGC-katalogo." , "lang" : "eo" } ,
{ "type" : "literal", "value" : "NGC 3862 (\u0434\u0440\u0443\u0433\u0438\u0435 \u043E\u0431\u043E\u0437\u043D\u0430\u0447\u0435\u043D\u0438\u044F \u2014 UGC 6723, MCG 3-30-95, ZWG 97.127, 3C 264, PGC 36606) \u2014 \u044D\u043B\u043B\u0438\u043F\u0442\u0438\u0447\u0435\u0441\u043A\u0430\u044F \u0433\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u0430 (E) \u0432 \u0441\u043E\u0437\u0432\u0435\u0437\u0434\u0438\u0438 \u041B\u0435\u0432. \u042D\u0442\u043E\u0442 \u043E\u0431\u044A\u0435\u043A\u0442 \u0432\u0445\u043E\u0434\u0438\u0442 \u0432 \u0447\u0438\u0441\u043B\u043E \u043F\u0435\u0440\u0435\u0447\u0438\u0441\u043B\u0435\u043D\u043D\u044B\u0445 \u0432 \u043E\u0440\u0438\u0433\u0438\u043D\u0430\u043B\u044C\u043D\u043E\u0439 \u0440\u0435\u0434\u0430\u043A\u0446\u0438\u0438 \u00AB\u041D\u043E\u0432\u043E\u0433\u043E \u043E\u0431\u0449\u0435\u0433\u043E \u043A\u0430\u0442\u0430\u043B\u043E\u0433\u0430\u00BB. \u0413\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u0430 NGC 3862 \u0432\u0445\u043E\u0434\u0438\u0442 \u0432 \u0441\u043E\u0441\u0442\u0430\u0432 \u0433\u0440\u0443\u043F\u043F\u044B \u0433\u0430\u043B\u0430\u043A\u0442\u0438\u043A NGC 3842. \u041F\u043E\u043C\u0438\u043C\u043E NGC 3862 \u0432 \u0433\u0440\u0443\u043F\u043F\u0443 \u0442\u0430\u043A\u0436\u0435 \u0432\u0445\u043E\u0434\u044F\u0442 \u0435\u0449\u0451 17 \u0433\u0430\u043B\u0430\u043A\u0442\u0438\u043A. \u0412 \u0441\u0432\u043E\u044E \u043E\u0447\u0435\u0440\u0435\u0434\u044C \u0433\u0440\u0443\u043F\u043F\u0430 \u043E\u0442\u043D\u043E\u0441\u0438\u0442\u044C\u0441\u044F \u043A \u0431\u043E\u043B\u044C\u0448\u043E\u043C\u0443 \u0441\u043A\u043E\u043F\u043B\u0435\u043D\u0438\u044E \u041B\u044C\u0432\u0430. 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\u0436\u0435\u043C\u0447\u0443\u0433\u0430. \u0418\u0441\u0442\u043E\u0447\u043D\u0438\u043A\u043E\u043C \u0434\u0436\u0435\u0442\u043E\u0432 \u044F\u0432\u043B\u044F\u0435\u0442\u0441\u044F \u0441\u0432\u0435\u0440\u0445\u043C\u0430\u0441\u0441\u0438\u0432\u043D\u0430\u044F \u0447\u0451\u0440\u043D\u0430\u044F \u0434\u044B\u0440\u0430 \u0441 \u043F\u0440\u0435\u0434\u043F\u043E\u043B\u0430\u0433\u0430\u0435\u043C\u043E\u0439 \u043C\u0430\u0441\u0441\u043E\u0439 4,7 \u00D7 10 8 M\u2609 ." , "lang" : "ru" } ,
{ "type" : "literal", "value" : "NGC 3862 est une galaxie elliptique situ\u00E9e dans la constellation du Lion \u00E0 environ 297 millions d'ann\u00E9es-lumi\u00E8re de la Voie lact\u00E9e. NGC 3862 a \u00E9t\u00E9 d\u00E9couverte par l'astronome germano-britannique William Herschel en 1785. NGC 3862 une galaxie \u00E0 noyau actif (AGN). C'est une galaxie \u00E0 faible \u00E9mission radio (low-excitation radio galaxy, LERG) et \u00E9galement une galaxie dont le noyau pr\u00E9sente un spectre d'\u00E9mission caract\u00E9ris\u00E9 par de larges raies d'atomes faiblement ionis\u00E9s (LINER)). Selon la base de donn\u00E9es Simbad, NGC 3862 est une galaxie active qui contient un quasar (3C 264.0). De nombreuses mesures non bas\u00E9es sur le d\u00E9calage vers le rouge (redshift) donnent une distance de 93,442 \u00B1 18,735 Mpc (\u223C305 millions d'a.l.), ce qui est \u00E0 l'int\u00E9rieur des distances calcul\u00E9es en employant la valeur du d\u00E9calage." , "lang" : "fr" } ,
{ "type" : "literal", "value" : "NGC 3862 \u00E9 uma gal\u00E1xia el\u00EDptica (E) localizada na direc\u00E7\u00E3o da constela\u00E7\u00E3o de Leo. Possui uma declina\u00E7\u00E3o de +19\u00B0 36' 23\" e uma ascens\u00E3o recta de 11 horas, 45 minutos e 05,0 segundos. A gal\u00E1xia NGC 3862 foi descoberta em 27 de Abril de 1785 por William Herschel." , "lang" : "pt" } ,
{ "type" : "literal", "value" : "NGC 3862 (r\u00F3wnie\u017C PGC 36606 lub UGC 6723) \u2013 galaktyka eliptyczna (E), znajduj\u0105ca si\u0119 w gwiazdozbiorze Lwa. Odkry\u0142 j\u0105 William Herschel 27 kwietnia 1785 roku. Nale\u017Cy do gromady galaktyk Abell 1367. NGC 3862 to galaktyka z aktywnym j\u0105drem. Jest jedn\u0105 z nielicznych znanych galaktyk aktywnych, w kt\u00F3rych w \u015Bwietle widzialnym wykryto d\u017Cet wydobywaj\u0105cy si\u0119 z supermasywnej czarnej dziury w centrum galaktyki. W d\u017Cecie tym znajduj\u0105 si\u0119 ja\u015Bniejsze obszary, kt\u00F3re wydaj\u0105 si\u0119 porusza\u0107 z pr\u0119dko\u015Bci\u0105 kilkukrotnie wi\u0119ksz\u0105 ni\u017C pr\u0119dko\u015B\u0107 \u015Bwiat\u0142a w pr\u00F3\u017Cni, lecz jest to tylko z\u0142udzenie optyczne, w rzeczywisto\u015Bci materia w d\u017Cecie porusza si\u0119 z pr\u0119dko\u015Bci\u0105 ponad 98% pr\u0119dko\u015Bci \u015Bwiat\u0142a w pr\u00F3\u017Cni. Ponadto w 2014 roku zauwa\u017Cono, \u017Ce jeden z tych ja\u015Bniejszych obszar\u00F3w w d\u017Cecie \u201Edogoni\u0142\u201D drugi i po\u0142\u0105czy\u0142 si\u0119 z nim." , "lang" : "pl" } ,
{ "type" : "literal", "value" : "NGC 3862 galaxia bat da, konstelazioan. William Herschelek aurkitu zuen 1785eko apirilaren\u202F27an." , "lang" : "eu" } ,
{ "type" : "literal", "value" : "NGC 3862 ist eine elliptische Radiogalaxie vom Hubble-Typ E0 im Sternbild L\u00F6we an der Ekliptik. Sie ist sch\u00E4tzungsweise 289 Millionen Lichtjahre von der Milchstra\u00DFe entfernt und hat einen Durchmesser von etwa 130.000 Lichtjahren. Sie ist Mitglied des Abell 1367-Galaxienhaufens. Im selben Himmelsareal befinden sich u. a. die Galaxien NGC 3857, NGC 3859, NGC 3868, IC 2955. Das Objekt wurde am 27. April 1785 von dem Astronomen Wilhelm Herschel mit seinem 18,7-Zoll-Spiegelteleskop entdeckt. Aufnahmen des Hubble-Weltraumteleskops zeigen, dass die Galaxie in ihrem Zentrum eine Akkretionsscheibe und davon ausgehend einen 900 Parsec (rund 3000 Lichtjahre) langen, sich ver\u00E4ndernden Jet hat, welcher Forschungsgegenstand zahlreicher Arbeiten ist." , "lang" : "de" } ] ,
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