@prefix rdf: . @prefix dbr: . @prefix wikidata: . dbr:Messier_108 rdf:type wikidata:Q318 . @prefix yago: . dbr:Messier_108 rdf:type yago:WikicatPGCObjects , yago:WikicatMessierObjects , yago:WikicatUGCObjects , yago:Object100002684 . @prefix dbo: . dbr:Messier_108 rdf:type dbo:Location , yago:WikicatNGCObjects , dbo:Place , dbo:CelestialBody , dbo:Galaxy . @prefix schema: . dbr:Messier_108 rdf:type schema:Place . @prefix owl: . dbr:Messier_108 rdf:type owl:Thing , yago:PhysicalEntity100001930 , yago:WikicatAstronomicalObjectsDiscoveredIn1781 . @prefix rdfs: . dbr:Messier_108 rdfs:label "Messier 108"@in , "Messier 108"@nl , "Messier 108"@de , "Messier 108"@en , "M108"@eo , "\u0645\u0633\u064A\u064A\u0647 108"@ar , "Messier 108"@sv , "M108 (astronomia)"@it , "Messier 108"@ca , "\u039C\u03B5\u03C3\u03B9\u03AD 108"@el , "M108 (\u5929\u4F53)"@ja , "Messier 108"@eu , "M 108 (\u0433\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u0430)"@ru , "Messier 108"@pl , "Messier 108"@pt , "\u041C\u0435\u0441\u0441\u044C\u0454 108"@uk , "Messier 108"@cs , "M108"@fr , "M108"@zh , "\uBA54\uC2DC\uC5D0 108"@ko , "Galaxia espiral M108"@es ; rdfs:comment "M 108 (conosciuto anche come NGC 3556 o anche con il suggestivo nome di Galassia Surfboard ) \u00E8 una galassia a spirale a circa 45 milioni di anni luce, nella costellazione dell'Orsa Maggiore, scoperta da Pierre M\u00E9chain nel 1781. Nel 2005, Scott D. Davis sugger\u00EC il nome, Galassia Surfboard, per il fatto che la sua forma ricorda quello di una tavola da surf."@it , "Messier 108, tamb\u00E9m conhecida como NGC 3556 \u00E9 uma gal\u00E1xia espiral situada perto da estrela Beta da Ursa Maior, foi descoberta por Pierre M\u00E9chain em 1781."@pt , "M108\uFF08NGC 3556\uFF09\u662F\u4E00\u4E2A\u4F4D\u4E8E\u5927\u718A\u5EA7\u7684\u6D4B\u5411\u5730\u7403\u7684\u6F29\u6DA1\u661F\u7CFB\u3002\u5176\u661F\u7B49\uFF1A+10"@zh , "Messier 108 (r\u00F3wnie\u017C M108 lub NGC 3556) \u2013 galaktyka spiralna znajduj\u0105ca si\u0119 w gwiazdozbiorze Wielkiej Nied\u017Awiedzicy. Niekt\u00F3re \u017Ar\u00F3d\u0142a klasyfikuj\u0105 j\u0105 jako spiraln\u0105 z poprzeczk\u0105."@pl , "\u041C\u0435\u0441\u0441\u044C\u0454 108 (\u041C108, \u0456\u043D\u0448\u0456 \u043F\u043E\u0437\u043D\u0430\u0447\u0435\u043D\u043D\u044F -NGC 3556,IRAS11085 +5556,UGC 6225,ZWG 267.48,MCG 9-18-98,ZWG 268.1,KARA 469,PGC 34030) \u2014 \u0433\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u0430 (Sc) \u0432 \u0441\u0443\u0437\u0456\u0440'\u0457 \u0412\u0435\u043B\u0438\u043A\u0430 \u0412\u0435\u0434\u043C\u0435\u0434\u0438\u0446\u044F. \u0426\u0435\u0439 \u043E\u0431'\u0454\u043A\u0442 \u0432\u0445\u043E\u0434\u0438\u0442\u044C \u0443 \u0447\u0438\u0441\u043B\u043E \u043F\u0435\u0440\u0435\u0440\u0430\u0445\u043E\u0432\u0430\u043D\u0438\u0445 \u0432 \u043E\u0440\u0438\u0433\u0456\u043D\u0430\u043B\u044C\u043D\u0456\u0439 \u0440\u0435\u0434\u0430\u043A\u0446\u0456\u0457 \u043D\u043E\u0432\u043E\u0433\u043E \u0437\u0430\u0433\u0430\u043B\u044C\u043D\u043E\u0433\u043E \u043A\u0430\u0442\u0430\u043B\u043E\u0433\u0443."@uk , "Messier 108 galaxia espiral bat da, Hartz Handia konstelazioan. aurkitu zuen 1781eko otsailaren\u202F19an."@eu , "Messier 108 (auch als NGC 3556 bezeichnet) ist eine Spiralgalaxie vom Hubble-Typ Sc mit den Abmessungen 8,6\u2032 \u00D7 2,4\u2032 und der scheinbaren Helligkeit von 9,9 mag im Sternbild Gro\u00DFer B\u00E4r. Die Galaxie ist nach bisherigen Messungen etwa 34 Mio. Lichtjahre von der Milchstra\u00DFe entfernt und hat somit einen Durchmesser in der Gr\u00F6\u00DFenordnung von 100.000 Lichtjahren. Am 6. Februar 1969 wurde in dieser Galaxie eine Supernova entdeckt, welche eine Helligkeit von 16 mag erreichte. M108 wurde am 16. Februar 1781 vom franz\u00F6sischen Astronomen Pierre M\u00E9chain entdeckt."@de , "M108 (ou NGC 3556), \u00E9galement appel\u00E9e par plusieurs astronomes amateurs la galaxie de la Planche de Surf, est une galaxie spirale barr\u00E9e vue par la tranche et situ\u00E9e dans le constellation de la Grande Ourse."@fr , "Messier 108 (M108) \u00E4ven k\u00E4nd som NGC 3556, \u00E4r en spiralgalax i stj\u00E4rnbilden Stora bj\u00F6rnen. Den uppt\u00E4cktes av Pierre M\u00E9chain 1781 eller 1782. I siktlinjen fr\u00E5n jorden ses den n\u00E4stan fr\u00E5n kanten."@sv , "M108 (NGC 3556) \u306F\u3001\u304A\u304A\u3050\u307E\u5EA7\u306B\u3042\u308B\u6E26\u5DFB\u9280\u6CB3\u3067\u3042\u308B\u3002"@ja , "Messier 108 (tak\u00E9 M108 nebo NGC 3556) je z boku vid\u011Bn\u00E1 spir\u00E1ln\u00ED galaxie v souhv\u011Bzd\u00ED Velk\u00E9 medv\u011Bdice. Objevil ji Pierre M\u00E9chain 19. \u00FAnora 1781. Od Zem\u011B je vzd\u00E1len\u00E1 p\u0159ibli\u017En\u011B 31 milion\u016F sv\u011Bteln\u00FDch leta je osam\u011Bl\u00FDm \u010Dlenemskupiny galaxi\u00ED Velk\u00E1 medv\u011Bdice, kter\u00E1 je sou\u010D\u00E1st\u00ED M\u00EDstn\u00ED nadkupy galaxi\u00ED."@cs , "Messier 108 (also known as NGC 3556, nicknamed the Surfboard Galaxy) is a barred spiral galaxy about 28 million light-years away from Earth in the northern constellation Ursa Major. It was discovered by Pierre M\u00E9chain in 1781 or 1782. From the Earth, this galaxy is seen almost edge-on. In January 1969, a type II supernova designated as SN 1969B was discovered in Messier 108. It reached a brightness of 13.9 mag."@en , "Messier 108 (juga dikenal sebagai NGC 3556) adalah galaksi spiral berpalang yang terletak di konstelasi Ursa Major. Objek ini ditemukan oleh Pierre M\u00E9chain pada tahun 1781 atau 1782. Dari perspektif Bumi, galaksi ini terlihat hampir di ujung."@in , "\u039F \u039C\u03B5\u03C3\u03B9\u03AD 108 (\u03B3\u03BD\u03C9\u03C3\u03C4\u03CC\u03C2 \u03BA\u03B1\u03B9 \u03C9\u03C2 \u039C108 \u03BA\u03B1\u03B9 NGC 3556) \u03B5\u03AF\u03BD\u03B1\u03B9 \u03C3\u03C0\u03B5\u03B9\u03C1\u03BF\u03B5\u03B9\u03B4\u03AE\u03C2 \u03B3\u03B1\u03BB\u03B1\u03BE\u03AF\u03B1\u03C2 \u03C3\u03B5 \u03B1\u03C0\u03CC\u03C3\u03C4\u03B1\u03C3\u03B7 \u03C0\u03B5\u03C1\u03AF\u03C0\u03BF\u03C5 50 \u03B5\u03BA\u03B1\u03C4\u03BF\u03BC\u03BC\u03C5\u03C1\u03AF\u03C9\u03BD \u03B5\u03C4\u03CE\u03BD \u03C6\u03C9\u03C4\u03CC\u03C2 \u03C3\u03C4\u03BF\u03BD \u03B1\u03C3\u03C4\u03B5\u03C1\u03B9\u03C3\u03BC\u03CC \u039C\u03B5\u03B3\u03AC\u03BB\u03B7 \u0386\u03C1\u03BA\u03C4\u03BF\u03C2. \u0395\u03AF\u03BD\u03B1\u03B9 \u03AD\u03BD\u03B1 \u03B1\u03C0\u03BF\u03BA\u03BF\u03BC\u03BC\u03AD\u03BD\u03BF \u03BC\u03AD\u03BB\u03BF\u03C2 \u03C4\u03BF\u03C5 . \u039F \u039C\u03B5\u03C3\u03B9\u03AD 108 \u03B1\u03C1\u03C7\u03B9\u03BA\u03AC \u03B4\u03B5\u03BD \u03C3\u03C5\u03BC\u03C0\u03B5\u03C1\u03B9\u03BB\u03B1\u03BC\u03B2\u03B1\u03BD\u03CC\u03C4\u03B1\u03BD \u03C3\u03C4\u03B1 \u03B1\u03BD\u03C4\u03B9\u03BA\u03B5\u03AF\u03BC\u03B5\u03BD\u03B1 \u039C\u03B5\u03C3\u03B9\u03AD, \u03B1\u03BB\u03BB\u03AC \u03C0\u03C1\u03BF\u03C3\u03C4\u03AD\u03B8\u03B7\u03BA\u03B5 \u03B1\u03C1\u03B3\u03CC\u03C4\u03B5\u03C1\u03B1."@el , "\uBA54\uC2DC\uC5D0 M108\uC740 \uD070\uACF0\uC790\uB9AC\uC5D0 \uC704\uCE58\uD55C \uB098\uC120 \uC740\uD558\uC774\uB2E4."@ko , "De acuerdo con el manuscrito preliminar de Charles Messier y versi\u00F3n no publicada de su cat\u00E1logo, M108, al igual que M109, fue descubierta por Pierre M\u00E9chain poco despu\u00E9s de M97 (la cual se encontr\u00F3 el 16 de febrero de 1781): M\u00E9chain descubri\u00F3 M108 3 d\u00EDas m\u00E1s tarde de M97 el 19 de febrero de 1781, y M109 el 12 de marzo de 1781. Ambos objetos parece que fueron tambi\u00E9n observados por Charles Messier cuando media la posici\u00F3n de M97 (14 de marzo de 1781), pero aparentemente no encontr\u00F3 el momento propicio para obtener la posici\u00F3n de esos objetos en aquel momento. Messier list\u00F3 este objeto, M108, bajo el n\u00FAmero '98' en su manuscrito, versi\u00F3n preliminar de su cat\u00E1logo, sin asignarle una posici\u00F3n. De acuerdo con Owen Gingerich, midi\u00F3 una posici\u00F3n precisa un tiempo m\u00E1s tarde la cual fue a\u00F1adida ma"@es , "Messier 108 (M108 o NGC 3556) \u00E9s una gal\u00E0xia espiral situada a la constel\u00B7laci\u00F3 de l'Ossa Major. Va ser descoberta per Pierre M\u00E9chain el 19 de febrer de 1781, posteriorment va ser observada per Charles Messier el 24 de mar\u00E7 del mateix any, per\u00F2 no va ser inclosa al seu cat\u00E0leg en la seva \u00E8poca. Va ser descoberta independentment per William Herschel el 1789. Va ser afegida finalment al cat\u00E0leg Messier per el 1953."@ca , "\u0645\u0633\u064A\u064A\u0647 108 \u0623\u0648 \u0625\u0646 \u062C\u064A \u0633\u064A 3556 \u0647\u064A \u0639\u0628\u0627\u0631\u0629 \u0639\u0646 \u0645\u062C\u0631\u0629 \u062D\u0644\u0632\u0648\u0646\u064A\u0629 \u0642\u0636\u064A\u0628\u064A\u0629 \u062A\u0642\u0639 \u0641\u064A \u0643\u0648\u0643\u0628\u0629 \u0627\u0644\u062F\u0628 \u0627\u0644\u0623\u0643\u0628\u0631. \u062A\u0628\u0639\u062F \u0639\u0646\u0627 33.5 \u0645\u0644\u064A\u0648\u0646 \u0633\u0646\u0629 \u0636\u0648\u0626\u064A\u0629 \u062A\u0642\u0631\u064A\u0628\u0627\u064B \u0648\u064A\u0628\u0644\u063A \u0642\u062F\u0631\u0647\u0627 \u0627\u0644\u0638\u0627\u0647\u0631\u064A 10.7. \u0627\u0643\u062A\u0634\u0641\u0647\u0627 \u0627\u0644\u0641\u0644\u0643\u064A \u0628\u064A\u064A\u0631 \u0645\u064A\u0634\u0627\u0646 \u0641\u064A \u0639\u0627\u0645\u064A 1781 \u06481782\u0645. \u0648\u0645\u0646 \u0645\u0646\u0638\u0648\u0631\u0646\u0627 \u0645\u0646 \u0627\u0644\u0623\u0631\u0636 \u0646\u062D\u0646 \u0646\u0631\u0649 \u0647\u0630\u0647 \u0627\u0644\u0645\u062C\u0631\u0629 \u0643\u0639\u0645\u0648\u062F \u0645\u0646 \u0627\u0644\u063A\u0628\u0627\u0631 \u0628\u0633\u0628\u0628 \u0623\u0646\u0646\u0627 \u0646\u0631\u0627\u0647\u0627 \u0645\u0646 \u062C\u0627\u0646\u0628\u0647\u0627 \u0648\u0644\u064A\u0633 \u0645\u0646 \u0623\u0645\u0627\u0645\u0647\u0627\u060C \u0623\u0645\u0627 \u0644\u0648 \u0643\u0646\u0627 \u0646\u0631\u0627\u0647\u0627 \u0645\u0646 \u0623\u0645\u0627\u0645\u0647\u0627 \u0641\u0643\u0646\u0627 \u0633\u0648\u0641 \u0646\u0631\u0649 \u0623\u0630\u0631\u0639\u0647\u0627 \u0627\u0644\u062D\u0644\u0632\u0648\u0646\u064A\u0629. \u0647\u0630\u0647 \u0627\u0644\u0645\u062C\u0631\u0629 \u0645\u0639\u0632\u0648\u0644\u0629 \u0628\u062D\u064A\u062B \u0623\u0646\u0647\u0627 \u0644\u0627 \u062A\u0646\u062A\u0645\u064A \u0625\u0644\u0649 \u0645\u062C\u0645\u0648\u0639\u0629 \u0645\u062C\u0631\u064A\u0629 \u0644\u0643\u0646\u0647\u0627 \u062C\u0632\u0621 \u0645\u0646 \u0627\u0644\u0630\u064A \u0647\u0648 \u0628\u062F\u0648\u0631\u0647 \u062C\u0632\u0621 \u0645\u0646 (\u0623\u064A \u0643\u0646\u062C\u0645 \u064A\u0633\u0628\u062D \u0628\u064A\u0646 \u0627\u0644\u0645\u062C\u0631\u0627\u062A \u0644\u0627 \u064A\u0646\u062A\u0645\u064A \u0625\u0644\u0649 \u0645\u062C\u0631\u0629 \u0645\u0639\u064A\u0646\u0629 \u0641\u0647\u0630\u0647 \u0644\u0627 \u062A\u0646\u062A\u0645\u064A \u0625\u0644\u0649 \u0645\u062C\u0645\u0648\u0639\u0629 \u0645\u0639\u064A\u0646\u0629). \u064A\u064F\u0642\u062F\u0631 \u0627\u0644\u0639\u0644\u0645\u0627\u0621 \u0643\u062A\u0644\u0629 \u0647\u0630\u0647 \u0627\u0644\u0645\u062C\u0631\u0629 \u0628\u0640125 \u0645\u0644\u064A\u0627\u0631 \u0643\u062A\u0644\u0629 \u0634\u0645\u0633\u064A\u0629. \u0648\u0642\u062F \u0623\u0638\u0647\u0631\u062A \u0627\u0644\u062F\u0631\u0627\u0633\u0627\u062A \u0623\u0646\u0647 \u064A\u0648\u062C\u062F \u062B\u0642\u0628 \u0623\u0633\u0648\u062F \u0641\u0627\u0626\u0642 \u0627\u0644\u0636\u062E\u0627\u0645\u0629 \u0641\u064A \u0646\u0648\u0627\u0629 \u0647\u0630\u0647 \u0627\u0644\u0645\u062C\u0631\u0629."@ar , "Messier 108 is een sterrenstelsel in het sterrenbeeld Grote Beer (Ursa Major). Het is in 1781 ontdekt door Pierre M\u00E9chain en zonder veel verdere gegevens als nummer 98 door Charles Messier in zijn catalogus opgenomen. Pas in 1953 is door Owen Gingerich M108 definitief onder nummer 108 in de Messiercatalogus opgenomen. M108 wordt vanaf de kant gezien en is met een kleine telescoop al beter te zien dan de lage helderheid doet vermoeden. Op minder dan een booggraad afstand staat de Uilnevel (M97), een aanmerkelijk zwakker object."@nl , "Messier 108 (\u0430\u043D\u0433\u043B. M 108, NGC 3556, \u0440\u0443\u0441. \u041C\u0435\u0441\u0441\u044C\u0435 108, \u0434\u0440\u0443\u0433\u0438\u0435 \u043E\u0431\u043E\u0437\u043D\u0430\u0447\u0435\u043D\u0438\u044F \u2014 IRAS11085+5556, UGC 6225, ZWG 267.48, MCG 9-18-98, ZWG 268.1, KARA 469, PGC 34030) \u2014 \u0441\u043F\u0438\u0440\u0430\u043B\u044C\u043D\u0430\u044F \u0433\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u0430 (Sc) \u0432 \u0441\u043E\u0437\u0432\u0435\u0437\u0434\u0438\u0438 \u0411\u043E\u043B\u044C\u0448\u0430\u044F \u041C\u0435\u0434\u0432\u0435\u0434\u0438\u0446\u0430. \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. \u0412 \u0433\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u0435 \u0432\u0441\u043F\u044B\u0445\u043D\u0443\u043B\u0430 \u0441\u0432\u0435\u0440\u0445\u043D\u043E\u0432\u0430\u044F SN 1969B. \u0415\u0451 \u043F\u0438\u043A\u043E\u0432\u0430\u044F \u0432\u0438\u0434\u0438\u043C\u0430\u044F \u0437\u0432\u0451\u0437\u0434\u043D\u0430\u044F \u0432\u0435\u043B\u0438\u0447\u0438\u043D\u0430 \u0441\u043E\u0441\u0442\u0430\u0432\u0438\u043B\u0430 16."@ru , "Pri la aliaj signifoj de \"M108\" vidu artikolon M kun nombro. M108 (Messier 108, aliaj indikoj \u2014 NGC 3556, IRAS11085+5556, UGC 6225, ZWG 267.48, MCG 9-18-98, ZWG 268.1, KARA 469, PGC 34030) estas galaksio en konstelacio Granda Ursino. \u0108i tiu objekto estis jam en la originala versio de NGC-katalogo."@eo . @prefix foaf: . dbr:Messier_108 foaf:name "NGC3556,PGC34030,UGC6225"@en , "Messier108"@en . @prefix dbp: . dbr:Messier_108 dbp:name "Messier 108"@en ; foaf:depiction , . @prefix dcterms: . @prefix dbc: . dbr:Messier_108 dcterms:subject dbc:Messier_objects , , dbc:UGC_objects , dbc:Astronomical_objects_discovered_in_1781 , dbc:Barred_spiral_galaxies , , dbc:NGC_objects , dbc:Ursa_Major_Cluster , dbc:Principal_Galaxies_Catalogue_objects ; dbo:wikiPageID 975035 ; dbo:wikiPageRevisionID 1107724536 ; dbo:wikiPageWikiLink dbr:Celestial_hemisphere , dbc:Messier_objects , dbr:Principal_Galaxies_Catalogue , dbr:Ursa_Major , dbr:Arcminute , dbr:Arcminutes , dbr:Infrared_light , dbr:Type_II_supernova , , dbr:NGC_2403 , dbr:Uppsala_General_Catalogue , dbr:Light-years , dbr:J2000 , dbc:Astronomical_objects_discovered_in_1781 , dbc:UGC_objects , dbr:Active_galactic_nucleus , , dbr:New_General_Catalogue , , dbr:Chandra_X-ray_Observatory , dbr:Ursa_Major_Cluster , dbr:Dark_matter , dbr:Messier_object , dbr:Supermassive_black_hole , , dbr:Megaparsec , dbr:Solar_mass , dbr:NGC_4631 , dbr:List_of_Messier_objects , dbr:Dust_lane , dbr:Sloan_Digital_Sky_Survey , dbr:Galaxy_morphological_classification , dbr:X-ray , dbr:NGC_7793 , dbc:Barred_spiral_galaxies , dbr:Apparent_magnitude , dbr:Globular_cluster , , dbr:Barred_spiral_galaxy , , dbr:Intermediate-mass_black_hole , dbr:Kiloparsec , dbr:Second , dbr:Angular_size , dbr:Intergalactic_medium , dbc:NGC_objects , dbc:Ursa_Major_Cluster , dbr:Spitzer_Space_Telescope , dbr:Constellation , dbc:Principal_Galaxies_Catalogue_objects , dbr:Virgo_supercluster ; dbo:wikiPageExternalLink . @prefix ns12: . dbr:Messier_108 dbo:wikiPageExternalLink ns12:abstract , . @prefix dbpedia-de: . dbr:Messier_108 owl:sameAs dbpedia-de:Messier_108 , , . @prefix dbpedia-sv: . dbr:Messier_108 owl:sameAs dbpedia-sv:Messier_108 , , . @prefix ns15: . dbr:Messier_108 owl:sameAs ns15:Messier_108 . @prefix ns16: . dbr:Messier_108 owl:sameAs ns16:NGC_3556 , , wikidata:Q4751 , . @prefix dbpedia-hu: . dbr:Messier_108 owl:sameAs dbpedia-hu:Messier_108 . @prefix dbpedia-es: . dbr:Messier_108 owl:sameAs dbpedia-es:Galaxia_espiral_M108 . @prefix yago-res: . dbr:Messier_108 owl:sameAs yago-res:Messier_108 . @prefix dbpedia-bg: . dbr:Messier_108 owl:sameAs dbpedia-bg:M108 . @prefix dbpedia-af: . dbr:Messier_108 owl:sameAs dbpedia-af:Messier_108 . @prefix dbpedia-et: . dbr:Messier_108 owl:sameAs dbpedia-et:Messier_108 . @prefix dbpedia-ro: . dbr:Messier_108 owl:sameAs dbpedia-ro:Messier_108 , . @prefix dbpedia-he: . dbr:Messier_108 owl:sameAs dbpedia-he:M108 . @prefix dbpedia-id: . dbr:Messier_108 owl:sameAs dbpedia-id:Messier_108 , . @prefix dbpedia-cs: . dbr:Messier_108 owl:sameAs dbpedia-cs:Messier_108 . @prefix dbpedia-fi: . dbr:Messier_108 owl:sameAs dbpedia-fi:Messier_108 , , . @prefix dbpedia-zh: . dbr:Messier_108 owl:sameAs dbpedia-zh:M108 . @prefix ns29: . dbr:Messier_108 owl:sameAs ns29:NGC_3556 , . @prefix dbpedia-sh: . dbr:Messier_108 owl:sameAs dbpedia-sh:Messier_108 . @prefix dbpedia-lb: . dbr:Messier_108 owl:sameAs dbpedia-lb:Messier_108 . @prefix ns32: . dbr:Messier_108 owl:sameAs ns32:Messier_108 . @prefix dbpedia-fr: . dbr:Messier_108 owl:sameAs dbpedia-fr:M108 , . @prefix dbpedia-pl: . dbr:Messier_108 owl:sameAs dbpedia-pl:Messier_108 . @prefix dbpedia-pt: . dbr:Messier_108 owl:sameAs dbpedia-pt:Messier_108 . @prefix dbpedia-vi: . dbr:Messier_108 owl:sameAs dbpedia-vi:Messier_108 . @prefix dbpedia-az: . dbr:Messier_108 owl:sameAs dbpedia-az:NGC_3556 , . @prefix dbpedia-hr: . dbr:Messier_108 owl:sameAs dbpedia-hr:Messier_108 . @prefix dbpedia-eo: . dbr:Messier_108 owl:sameAs dbpedia-eo:M108 , . @prefix dbpedia-no: . dbr:Messier_108 owl:sameAs dbpedia-no:Messier_108 . @prefix dbpedia-sk: . dbr:Messier_108 owl:sameAs dbpedia-sk:Messier_108 . @prefix dbpedia-tr: . dbr:Messier_108 owl:sameAs dbpedia-tr:Messier_108 . @prefix dbpedia-nl: . dbr:Messier_108 owl:sameAs dbpedia-nl:Messier_108 . @prefix dbpedia-eu: . dbr:Messier_108 owl:sameAs dbpedia-eu:Messier_108 , . @prefix dbpedia-ca: . dbr:Messier_108 owl:sameAs dbpedia-ca:Messier_108 . @prefix dbpedia-commons: . dbr:Messier_108 owl:sameAs dbpedia-commons:Messier_108 ; dbp:sizeV 8 . @prefix xsd: . dbr:Messier_108 dbp:z "696.1"^^xsd:double . @prefix dbt: . dbr:Messier_108 dbp:wikiPageUsesTemplate dbt:Ngc40 , dbt:RA , dbt:Sky , dbt:WikiSky , dbt:Messier_objects , dbt:Reflist , dbt:Refn , dbt:Infobox_Galaxy , dbt:DEC , dbt:Short_description , dbt:Commons_category , dbt:Solar_mass , dbt:Portal_bar ; dbo:thumbnail ; dbp:distLy "8.800000000000001"^^xsd:double ; dbp:appmagV 10 ; dbp:caption "A Sloan Digital Sky Survey image of M108."@en ; dbp:epoch dbr:J2000 ; dbp:imageSize 250 ; dbp:names "NGC 3556, PGC 34030, UGC 6225"@en ; dbp:type "SBcd"@en ; dbo:abstract "Messier 108, tamb\u00E9m conhecida como NGC 3556 \u00E9 uma gal\u00E1xia espiral situada perto da estrela Beta da Ursa Maior, foi descoberta por Pierre M\u00E9chain em 1781."@pt , "Messier 108 (tak\u00E9 M108 nebo NGC 3556) je z boku vid\u011Bn\u00E1 spir\u00E1ln\u00ED galaxie v souhv\u011Bzd\u00ED Velk\u00E9 medv\u011Bdice. Objevil ji Pierre M\u00E9chain 19. \u00FAnora 1781. Od Zem\u011B je vzd\u00E1len\u00E1 p\u0159ibli\u017En\u011B 31 milion\u016F sv\u011Bteln\u00FDch leta je osam\u011Bl\u00FDm \u010Dlenemskupiny galaxi\u00ED Velk\u00E1 medv\u011Bdice, kter\u00E1 je sou\u010D\u00E1st\u00ED M\u00EDstn\u00ED nadkupy galaxi\u00ED."@cs , "Messier 108 (M108) \u00E4ven k\u00E4nd som NGC 3556, \u00E4r en spiralgalax i stj\u00E4rnbilden Stora bj\u00F6rnen. Den uppt\u00E4cktes av Pierre M\u00E9chain 1781 eller 1782. I siktlinjen fr\u00E5n jorden ses den n\u00E4stan fr\u00E5n kanten."@sv , "\u041C\u0435\u0441\u0441\u044C\u0454 108 (\u041C108, \u0456\u043D\u0448\u0456 \u043F\u043E\u0437\u043D\u0430\u0447\u0435\u043D\u043D\u044F -NGC 3556,IRAS11085 +5556,UGC 6225,ZWG 267.48,MCG 9-18-98,ZWG 268.1,KARA 469,PGC 34030) \u2014 \u0433\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u0430 (Sc) \u0432 \u0441\u0443\u0437\u0456\u0440'\u0457 \u0412\u0435\u043B\u0438\u043A\u0430 \u0412\u0435\u0434\u043C\u0435\u0434\u0438\u0446\u044F. \u0426\u0435\u0439 \u043E\u0431'\u0454\u043A\u0442 \u0432\u0445\u043E\u0434\u0438\u0442\u044C \u0443 \u0447\u0438\u0441\u043B\u043E \u043F\u0435\u0440\u0435\u0440\u0430\u0445\u043E\u0432\u0430\u043D\u0438\u0445 \u0432 \u043E\u0440\u0438\u0433\u0456\u043D\u0430\u043B\u044C\u043D\u0456\u0439 \u0440\u0435\u0434\u0430\u043A\u0446\u0456\u0457 \u043D\u043E\u0432\u043E\u0433\u043E \u0437\u0430\u0433\u0430\u043B\u044C\u043D\u043E\u0433\u043E \u043A\u0430\u0442\u0430\u043B\u043E\u0433\u0443."@uk , "Messier 108 (\u0430\u043D\u0433\u043B. M 108, NGC 3556, \u0440\u0443\u0441. \u041C\u0435\u0441\u0441\u044C\u0435 108, \u0434\u0440\u0443\u0433\u0438\u0435 \u043E\u0431\u043E\u0437\u043D\u0430\u0447\u0435\u043D\u0438\u044F \u2014 IRAS11085+5556, UGC 6225, ZWG 267.48, MCG 9-18-98, ZWG 268.1, KARA 469, PGC 34030) \u2014 \u0441\u043F\u0438\u0440\u0430\u043B\u044C\u043D\u0430\u044F \u0433\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u0430 (Sc) \u0432 \u0441\u043E\u0437\u0432\u0435\u0437\u0434\u0438\u0438 \u0411\u043E\u043B\u044C\u0448\u0430\u044F \u041C\u0435\u0434\u0432\u0435\u0434\u0438\u0446\u0430. \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. \u0412 \u0433\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u0435 \u0432\u0441\u043F\u044B\u0445\u043D\u0443\u043B\u0430 \u0441\u0432\u0435\u0440\u0445\u043D\u043E\u0432\u0430\u044F SN 1969B. \u0415\u0451 \u043F\u0438\u043A\u043E\u0432\u0430\u044F \u0432\u0438\u0434\u0438\u043C\u0430\u044F \u0437\u0432\u0451\u0437\u0434\u043D\u0430\u044F \u0432\u0435\u043B\u0438\u0447\u0438\u043D\u0430 \u0441\u043E\u0441\u0442\u0430\u0432\u0438\u043B\u0430 16."@ru , "M 108 (conosciuto anche come NGC 3556 o anche con il suggestivo nome di Galassia Surfboard ) \u00E8 una galassia a spirale a circa 45 milioni di anni luce, nella costellazione dell'Orsa Maggiore, scoperta da Pierre M\u00E9chain nel 1781. Nel 2005, Scott D. Davis sugger\u00EC il nome, Galassia Surfboard, per il fatto che la sua forma ricorda quello di una tavola da surf."@it , "Messier 108 (juga dikenal sebagai NGC 3556) adalah galaksi spiral berpalang yang terletak di konstelasi Ursa Major. Objek ini ditemukan oleh Pierre M\u00E9chain pada tahun 1781 atau 1782. Dari perspektif Bumi, galaksi ini terlihat hampir di ujung. Galaksi ini adalah anggota yang terpisah dari gugus galaksi Ursa Major di supergugus Virgo. Galaksi ini memiliki klasifikasi morfologi tipe SBbc dalam sistem de Vaucouleurs, yang berarti galaksi ini merupakan galaksi spiral berpalang dengan lengan yang agak longgar. Maksimum ukuran sudut galasi pada pita optik adalah 11'.1 \u00D7 4'.6, dan cenderung 75\u00B0 dengan garis pandang."@in , "M108\uFF08NGC 3556\uFF09\u662F\u4E00\u4E2A\u4F4D\u4E8E\u5927\u718A\u5EA7\u7684\u6D4B\u5411\u5730\u7403\u7684\u6F29\u6DA1\u661F\u7CFB\u3002\u5176\u661F\u7B49\uFF1A+10"@zh , "Messier 108 (M108 o NGC 3556) \u00E9s una gal\u00E0xia espiral situada a la constel\u00B7laci\u00F3 de l'Ossa Major. Va ser descoberta per Pierre M\u00E9chain el 19 de febrer de 1781, posteriorment va ser observada per Charles Messier el 24 de mar\u00E7 del mateix any, per\u00F2 no va ser inclosa al seu cat\u00E0leg en la seva \u00E8poca. Va ser descoberta independentment per William Herschel el 1789. Va ser afegida finalment al cat\u00E0leg Messier per el 1953. M108 est\u00E0 classificada com de tipus Sc a la seq\u00FC\u00E8ncia de Hubble. Des de la Terra aquesta gal\u00E0xia es mostra de costat, i presenta per tant una forma fina i molt allargada (8x1 minuts d'arc), sembla no tenir ni bulb ni nucli; \u00E9s per la seva forma que Scott D. Davis va suggerir el nom de gal\u00E0xia planxa de surf (surfboard galaxy en angl\u00E8s). Est\u00E0 situada a uns 45 milions d'anys llum del sistema solar, del qual s'allunya a una velocitat de 772 km/s."@ca , "Messier 108 (also known as NGC 3556, nicknamed the Surfboard Galaxy) is a barred spiral galaxy about 28 million light-years away from Earth in the northern constellation Ursa Major. It was discovered by Pierre M\u00E9chain in 1781 or 1782. From the Earth, this galaxy is seen almost edge-on. This galaxy is an isolated member of the Ursa Major Cluster of galaxies in the local supercluster. It has a morphological classification of type SBbc in the de Vaucouleurs system, which means it is a barred spiral galaxy with somewhat loosely wound arms. The maximum angular size of the galaxy in the optical band is 11\u2032.1 \u00D7 4\u2032.6, and it is inclined 75\u00B0 to the line of sight. This galaxy has an estimated mass of 125 billion solar masses (M\u2609) and bears about 290 \u00B1 80 globular clusters. Examination of the distribution of neutral hydrogen in this galaxy shows discrete shells of expanding gas extending for several kiloparsecs, known as H1 supershells. These may be driven by currents of dark matter, dust and gas contributing to large star formation, having caused supernovae explosions. Alternatively they may result from an infall from the intergalactic medium or arise from radio jets. Observations with the Chandra X-ray Observatory have identified 83 X-ray sources, including a source at the nucleus. The brightest of these is consistent with an intermediate-mass black hole accreting matter. The galaxy is also emitting a diffuse soft X-ray radiation within 2.6 arcminutes of the optical galaxy. The spectrum of the source at the core is consistent with an active galactic nucleus, but an examination with the Spitzer Space Telescope showed no indication of activity. The supermassive black hole at the core has an estimated mass of 24 million solar masses (M\u2609). In January 1969, a type II supernova designated as SN 1969B was discovered in Messier 108. It reached a brightness of 13.9 mag. SPIRITS 16tn, another supernova in Messier 108, was discovered by the Spitzer Space Telescope in August 2016. The supernova was only visible in infrared light, because it was heavily obscured by dust. Its extinction was estimated to be 8\u20139 mag, making it one of the most heavily obscured supernovae ever observed."@en , "Messier 108 (auch als NGC 3556 bezeichnet) ist eine Spiralgalaxie vom Hubble-Typ Sc mit den Abmessungen 8,6\u2032 \u00D7 2,4\u2032 und der scheinbaren Helligkeit von 9,9 mag im Sternbild Gro\u00DFer B\u00E4r. Die Galaxie ist nach bisherigen Messungen etwa 34 Mio. Lichtjahre von der Milchstra\u00DFe entfernt und hat somit einen Durchmesser in der Gr\u00F6\u00DFenordnung von 100.000 Lichtjahren. Mit dem R\u00F6ntgenteleskop Chandra fanden sich in der Galaxie viele Starburst-Regionen, in denen auf engem Raum eine gro\u00DFe Anzahl von Sternen gleichzeitig entstehen. Sie sind umgeben von hei\u00DFen Gasblasen, die von den extrem starken Sternwinden massereicher Wolf-Rayet-Sterne und von Supernova-Explosionen erhitzt und aus der galaktischen Scheibe herausgetrieben werden. Die Gasblasen leuchten diffus im R\u00F6ntgenlicht. Am 6. Februar 1969 wurde in dieser Galaxie eine Supernova entdeckt, welche eine Helligkeit von 16 mag erreichte. M108 wurde am 16. Februar 1781 vom franz\u00F6sischen Astronomen Pierre M\u00E9chain entdeckt."@de , "De acuerdo con el manuscrito preliminar de Charles Messier y versi\u00F3n no publicada de su cat\u00E1logo, M108, al igual que M109, fue descubierta por Pierre M\u00E9chain poco despu\u00E9s de M97 (la cual se encontr\u00F3 el 16 de febrero de 1781): M\u00E9chain descubri\u00F3 M108 3 d\u00EDas m\u00E1s tarde de M97 el 19 de febrero de 1781, y M109 el 12 de marzo de 1781. Ambos objetos parece que fueron tambi\u00E9n observados por Charles Messier cuando media la posici\u00F3n de M97 (14 de marzo de 1781), pero aparentemente no encontr\u00F3 el momento propicio para obtener la posici\u00F3n de esos objetos en aquel momento. Messier list\u00F3 este objeto, M108, bajo el n\u00FAmero '98' en su manuscrito, versi\u00F3n preliminar de su cat\u00E1logo, sin asignarle una posici\u00F3n. De acuerdo con Owen Gingerich, midi\u00F3 una posici\u00F3n precisa un tiempo m\u00E1s tarde la cual fue a\u00F1adida manualmente en su copia personal del cat\u00E1logo. Ambos objetos, M108 y M109 tambi\u00E9n son mencionados en la carta de Pierre M\u00E9chain del 6 de mayo de 1783, la cual apoya la sospecha de que probablemente quer\u00EDa a\u00F1adirlas en una edici\u00F3n posterior del cat\u00E1logo de Messier. El objeto M108 fue a\u00F1adido finalmente al cat\u00E1logo de Messier por Owen Gingerich en 1953. Como el descubrimiento de M108 no hab\u00EDa sido publicado, William Herschel redescubri\u00F3 independientemente este objeto el 17 de abril de 1789, y lo catalog\u00F3 como H V.46. El borde cercano de la galaxia M108 parece no tener ninguna protuberancia ni ning\u00FAn n\u00FAcleo pronunciado, es solo un disco moteado rico en detalles con un gran oscurecimiento a lo largo del eje mayor, con unas pocas regiones H II y c\u00FAmulos de estrellas j\u00F3venes expuestos contra el fondo ca\u00F3tico -- en una palabra: 'Muy Sucio'. Hay peque\u00F1as evidencias de un patr\u00F3n espiral bien definido es esta galaxia de tipo Sc, la cual se aleja a 772 km/s. De acuerdo con Brent Tully, est\u00E1 a unos 45 millones de a\u00F1os luz de distancia, y es miembro de la nube de la Osa Mayor, una disperso racimo de galaxias. Tully clasifica esta galaxia como SBcd, es decir Sc muy tard\u00EDa y barrada; el presente autor no puede encontrar evidencias sobre esto a partir de las im\u00E1genes conocidas. Es tambi\u00E9n una galaxia de brote estelar La supernova de tipo II 1969B tuvo lugar en M108 y alcanz\u00F3 la magnitud 13,9 el 23 de enero de 1969. M 108 es bastante sencilla para los aficionados, m\u00E1s sencillo de lo que implican los valores publicados de su brillo (excepci\u00F3n: Don Machholz' estima una mag 9,4). La descripci\u00F3n m\u00E1s acertada es quiz\u00E1 la de : 'una belleza blanca plateada, con forma de plato y muy bien definida' con algo de brillo e irregularidades en la regi\u00F3n central, rodeada por 'ligeros y oscuros n\u00F3dulos'. Es un objeto muy alargado con una dimensi\u00F3n angular de 8x1'. \u00A1Es en realidad sorprendente la cantidad de detalles que pueden verse en esta galaxia con un peque\u00F1o instrumento! Las fotograf\u00EDas a color muestran un aspecto incluso m\u00E1s visible de lo que deber\u00EDa, la cual a veces aparece en fotograf\u00EDas de campo abierto del espacio profundo junto a la nebulosa Owl M97, la cual se encuentra a solo 48' al Sureste. Nota: texto reproducido con la autorizaci\u00F3n del autor AstroSeti"@es , "Messier 108 is een sterrenstelsel in het sterrenbeeld Grote Beer (Ursa Major). Het is in 1781 ontdekt door Pierre M\u00E9chain en zonder veel verdere gegevens als nummer 98 door Charles Messier in zijn catalogus opgenomen. Pas in 1953 is door Owen Gingerich M108 definitief onder nummer 108 in de Messiercatalogus opgenomen. M108 wordt vanaf de kant gezien en is met een kleine telescoop al beter te zien dan de lage helderheid doet vermoeden. Op minder dan een booggraad afstand staat de Uilnevel (M97), een aanmerkelijk zwakker object."@nl , "\u039F \u039C\u03B5\u03C3\u03B9\u03AD 108 (\u03B3\u03BD\u03C9\u03C3\u03C4\u03CC\u03C2 \u03BA\u03B1\u03B9 \u03C9\u03C2 \u039C108 \u03BA\u03B1\u03B9 NGC 3556) \u03B5\u03AF\u03BD\u03B1\u03B9 \u03C3\u03C0\u03B5\u03B9\u03C1\u03BF\u03B5\u03B9\u03B4\u03AE\u03C2 \u03B3\u03B1\u03BB\u03B1\u03BE\u03AF\u03B1\u03C2 \u03C3\u03B5 \u03B1\u03C0\u03CC\u03C3\u03C4\u03B1\u03C3\u03B7 \u03C0\u03B5\u03C1\u03AF\u03C0\u03BF\u03C5 50 \u03B5\u03BA\u03B1\u03C4\u03BF\u03BC\u03BC\u03C5\u03C1\u03AF\u03C9\u03BD \u03B5\u03C4\u03CE\u03BD \u03C6\u03C9\u03C4\u03CC\u03C2 \u03C3\u03C4\u03BF\u03BD \u03B1\u03C3\u03C4\u03B5\u03C1\u03B9\u03C3\u03BC\u03CC \u039C\u03B5\u03B3\u03AC\u03BB\u03B7 \u0386\u03C1\u03BA\u03C4\u03BF\u03C2. \u0395\u03AF\u03BD\u03B1\u03B9 \u03AD\u03BD\u03B1 \u03B1\u03C0\u03BF\u03BA\u03BF\u03BC\u03BC\u03AD\u03BD\u03BF \u03BC\u03AD\u03BB\u03BF\u03C2 \u03C4\u03BF\u03C5 . \u039F \u039C\u03B5\u03C3\u03B9\u03AD 108 \u03B1\u03C1\u03C7\u03B9\u03BA\u03AC \u03B4\u03B5\u03BD \u03C3\u03C5\u03BC\u03C0\u03B5\u03C1\u03B9\u03BB\u03B1\u03BC\u03B2\u03B1\u03BD\u03CC\u03C4\u03B1\u03BD \u03C3\u03C4\u03B1 \u03B1\u03BD\u03C4\u03B9\u03BA\u03B5\u03AF\u03BC\u03B5\u03BD\u03B1 \u039C\u03B5\u03C3\u03B9\u03AD, \u03B1\u03BB\u03BB\u03AC \u03C0\u03C1\u03BF\u03C3\u03C4\u03AD\u03B8\u03B7\u03BA\u03B5 \u03B1\u03C1\u03B3\u03CC\u03C4\u03B5\u03C1\u03B1."@el , "M108 (NGC 3556) \u306F\u3001\u304A\u304A\u3050\u307E\u5EA7\u306B\u3042\u308B\u6E26\u5DFB\u9280\u6CB3\u3067\u3042\u308B\u3002"@ja , "Pri la aliaj signifoj de \"M108\" vidu artikolon M kun nombro. M108 (Messier 108, aliaj indikoj \u2014 NGC 3556, IRAS11085+5556, UGC 6225, ZWG 267.48, MCG 9-18-98, ZWG 268.1, KARA 469, PGC 34030) estas galaksio en konstelacio Granda Ursino. \u0108i tiu objekto estis jam en la originala versio de NGC-katalogo."@eo , "Messier 108 galaxia espiral bat da, Hartz Handia konstelazioan. aurkitu zuen 1781eko otsailaren\u202F19an."@eu , "\u0645\u0633\u064A\u064A\u0647 108 \u0623\u0648 \u0625\u0646 \u062C\u064A \u0633\u064A 3556 \u0647\u064A \u0639\u0628\u0627\u0631\u0629 \u0639\u0646 \u0645\u062C\u0631\u0629 \u062D\u0644\u0632\u0648\u0646\u064A\u0629 \u0642\u0636\u064A\u0628\u064A\u0629 \u062A\u0642\u0639 \u0641\u064A \u0643\u0648\u0643\u0628\u0629 \u0627\u0644\u062F\u0628 \u0627\u0644\u0623\u0643\u0628\u0631. \u062A\u0628\u0639\u062F \u0639\u0646\u0627 33.5 \u0645\u0644\u064A\u0648\u0646 \u0633\u0646\u0629 \u0636\u0648\u0626\u064A\u0629 \u062A\u0642\u0631\u064A\u0628\u0627\u064B \u0648\u064A\u0628\u0644\u063A \u0642\u062F\u0631\u0647\u0627 \u0627\u0644\u0638\u0627\u0647\u0631\u064A 10.7. \u0627\u0643\u062A\u0634\u0641\u0647\u0627 \u0627\u0644\u0641\u0644\u0643\u064A \u0628\u064A\u064A\u0631 \u0645\u064A\u0634\u0627\u0646 \u0641\u064A \u0639\u0627\u0645\u064A 1781 \u06481782\u0645. \u0648\u0645\u0646 \u0645\u0646\u0638\u0648\u0631\u0646\u0627 \u0645\u0646 \u0627\u0644\u0623\u0631\u0636 \u0646\u062D\u0646 \u0646\u0631\u0649 \u0647\u0630\u0647 \u0627\u0644\u0645\u062C\u0631\u0629 \u0643\u0639\u0645\u0648\u062F \u0645\u0646 \u0627\u0644\u063A\u0628\u0627\u0631 \u0628\u0633\u0628\u0628 \u0623\u0646\u0646\u0627 \u0646\u0631\u0627\u0647\u0627 \u0645\u0646 \u062C\u0627\u0646\u0628\u0647\u0627 \u0648\u0644\u064A\u0633 \u0645\u0646 \u0623\u0645\u0627\u0645\u0647\u0627\u060C \u0623\u0645\u0627 \u0644\u0648 \u0643\u0646\u0627 \u0646\u0631\u0627\u0647\u0627 \u0645\u0646 \u0623\u0645\u0627\u0645\u0647\u0627 \u0641\u0643\u0646\u0627 \u0633\u0648\u0641 \u0646\u0631\u0649 \u0623\u0630\u0631\u0639\u0647\u0627 \u0627\u0644\u062D\u0644\u0632\u0648\u0646\u064A\u0629. \u0647\u0630\u0647 \u0627\u0644\u0645\u062C\u0631\u0629 \u0645\u0639\u0632\u0648\u0644\u0629 \u0628\u062D\u064A\u062B \u0623\u0646\u0647\u0627 \u0644\u0627 \u062A\u0646\u062A\u0645\u064A \u0625\u0644\u0649 \u0645\u062C\u0645\u0648\u0639\u0629 \u0645\u062C\u0631\u064A\u0629 \u0644\u0643\u0646\u0647\u0627 \u062C\u0632\u0621 \u0645\u0646 \u0627\u0644\u0630\u064A \u0647\u0648 \u0628\u062F\u0648\u0631\u0647 \u062C\u0632\u0621 \u0645\u0646 (\u0623\u064A \u0643\u0646\u062C\u0645 \u064A\u0633\u0628\u062D \u0628\u064A\u0646 \u0627\u0644\u0645\u062C\u0631\u0627\u062A \u0644\u0627 \u064A\u0646\u062A\u0645\u064A \u0625\u0644\u0649 \u0645\u062C\u0631\u0629 \u0645\u0639\u064A\u0646\u0629 \u0641\u0647\u0630\u0647 \u0644\u0627 \u062A\u0646\u062A\u0645\u064A \u0625\u0644\u0649 \u0645\u062C\u0645\u0648\u0639\u0629 \u0645\u0639\u064A\u0646\u0629). \u064A\u064F\u0642\u062F\u0631 \u0627\u0644\u0639\u0644\u0645\u0627\u0621 \u0643\u062A\u0644\u0629 \u0647\u0630\u0647 \u0627\u0644\u0645\u062C\u0631\u0629 \u0628\u0640125 \u0645\u0644\u064A\u0627\u0631 \u0643\u062A\u0644\u0629 \u0634\u0645\u0633\u064A\u0629. \u0648\u0642\u062F \u0623\u0638\u0647\u0631\u062A \u0627\u0644\u062F\u0631\u0627\u0633\u0627\u062A \u0623\u0646\u0647 \u064A\u0648\u062C\u062F \u062B\u0642\u0628 \u0623\u0633\u0648\u062F \u0641\u0627\u0626\u0642 \u0627\u0644\u0636\u062E\u0627\u0645\u0629 \u0641\u064A \u0646\u0648\u0627\u0629 \u0647\u0630\u0647 \u0627\u0644\u0645\u062C\u0631\u0629."@ar , "Messier 108 (r\u00F3wnie\u017C M108 lub NGC 3556) \u2013 galaktyka spiralna znajduj\u0105ca si\u0119 w gwiazdozbiorze Wielkiej Nied\u017Awiedzicy. Niekt\u00F3re \u017Ar\u00F3d\u0142a klasyfikuj\u0105 j\u0105 jako spiraln\u0105 z poprzeczk\u0105."@pl , "M108 (ou NGC 3556), \u00E9galement appel\u00E9e par plusieurs astronomes amateurs la galaxie de la Planche de Surf, est une galaxie spirale barr\u00E9e vue par la tranche et situ\u00E9e dans le constellation de la Grande Ourse."@fr , "\uBA54\uC2DC\uC5D0 M108\uC740 \uD070\uACF0\uC790\uB9AC\uC5D0 \uC704\uCE58\uD55C \uB098\uC120 \uC740\uD558\uC774\uB2E4."@ko ; dbp:constellationName dbr:Ursa_Major . @prefix gold: . dbr:Messier_108 gold:hypernym dbr:Galaxy . @prefix prov: . dbr:Messier_108 prov:wasDerivedFrom ; dbo:wikiPageLength "8768"^^xsd:nonNegativeInteger . @prefix wikipedia-en: . dbr:Messier_108 foaf:isPrimaryTopicOf wikipedia-en:Messier_108 .