@prefix dbpprop: .
@prefix dbpedia: .
dbpedia:M101_Group dbpprop:brightestMember dbpedia:Pinwheel_Galaxy .
@prefix rdf: .
@prefix ns3: .
dbpedia:Pinwheel_Galaxy rdf:type ns3:MessierObjects ,
ns3:NGCObjects ,
ns3:UGCObjects ,
ns3:PGCObjects ,
ns3:ArpObjects ;
dbpprop:name "Pinwheel Galaxy"@en .
@prefix owl: .
@prefix ns5: .
dbpedia:Pinwheel_Galaxy owl:sameAs ns5:Pinwheel_Galaxy ,
.
@prefix foaf: .
@prefix ns7: .
dbpedia:Pinwheel_Galaxy foaf:page ns7:Pinwheel_Galaxy .
@prefix ns8: .
dbpedia:Pinwheel_Galaxy dbpprop:reference ns8:a ,
,
,
,
.
@prefix rdfs: .
dbpedia:Pinwheel_Galaxy rdfs:label "Vindsnurregalaxen"@sv ,
"Galassia Girandola"@it ,
"F\u0131r\u0131ldak G\u00F6kadas\u0131"@tr ,
"Pinwheel Galaxy"@en ,
"Messier 101"@ro ,
"M101"@ja ,
"Gal\u00E1xia Pinwheel"@pt ,
"Galaxia espiral M101"@es ,
"Messier 101"@hu ,
"Gal\u00E0xia del Molinet"@ca ,
"NGC 5457"@uk ,
"Galaktyka Wiatraczek"@pl ,
"Galaxie V\u011Btrn\u00EDk"@cs ,
"Messier 101"@de ,
"M101"@fr ,
"Windmolenstelsel"@nl ,
"\u0421\u043F\u0438\u0440\u0430\u043B\u044C\u043D\u0430\u044F \u0433\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u0430 M101"@ru ,
"Tuulimyllygalaksi"@fi ,
"\u98A8\u8ECA\u661F\u7CFB"@zh .
@prefix dbpedia-owl: .
dbpedia:Pinwheel_Galaxy dbpedia-owl:thumbnail ;
dbpprop:abstract "NGC 5457 ou M101, popularmente conhecida como Gal\u00E1xia do Catavento, \u00E9 uma gal\u00E1xia espiral localizada a cerca de vinte e sete milh\u00F5es de anos-luz de dist\u00E2ncia na dire\u00E7\u00E3o da constela\u00E7\u00E3o de Ursa Maior. Possui entre cento e setenta e duzentos mil anos-luz de di\u00E2metro, uma magnitude aparente de 7,5, uma magnitude absoluta de -21,6, uma declina\u00E7\u00E3o de +54\u00BA 20' 55\" e uma ascens\u00E3o reta de 14 horas 03 minutos 12,4 segundos. A gal\u00E1xia NGC 5457 foi descoberta em 27 de Mar\u00E7o de 1781 por Pierre M\u00E9chain e faz parte de um grupo de pelo menos nove gal\u00E1xias, o grupo de gal\u00E1xias M101 que inclui as gal\u00E1xias M51, NGC 5195 (companheira de M51), M63, NGC 5474, NGC 5585, NGC 5204, NGC 5238, NGC 5477, UGC 8508, UGC 8837, UGC 9405 e, logicamente, NGC 5457. Nesta gal\u00E1xia foram descobertas tr\u00EAs supernovas: SN 1909A - 26 de Janeiro de 1909 1951H (tipo II) - Setembro de 1951 SN 1970G (tipo II) - 30 de julho de 1970 Astronomia extragal\u00E1ctica Lista de gal\u00E1xias Lista de objetos NGC"@pt ,
"La Gal\u00E0xia del Molinet (Messier 101, M101 o NGC 5457) \u00E9s una gal\u00E0xia espiral vista frontalment situada a la constel\u00B7laci\u00F3 de l'\u00D3ssa Major. Va ser descoberta per Pierre M\u00E9chain el 27 de mar\u00E7 de 1781, qui va comunicar el seu descobriment al seu amic Charles Messier qui va verificar la seva posici\u00F3 i la va afegir al seu cat\u00E0leg."@ca ,
"A Messier 101 (m\u00E1s n\u00E9ven M101, NGC 5457 vagy Sz\u00E9lker\u00E9k-Galaxis) egy spir\u00E1lgalaxis az Ursa Major (Nagy Medve) csillagk\u00E9pben."@hu ,
"The Pinwheel Galaxy (also known as Messier 101 or NGC 5457) is a face-on spiral galaxy about 27 million light-years away in the constellation Ursa Major. It was discovered by Pierre M\u00E9chain on March 27, 1781, and he subsequently communicated his discovery to Charles Messier who verified its position and added it to the Messier Catalogue as one of the final entries. On February 28, 2006, NASA and the ESA released a very detailed image of Pinwheel Galaxy, which was the largest and most detailed image of a galaxy by Hubble Space Telescope at the time. The image was composed from 51 individual exposures, plus some extra ground-based photos."@en ,
"M101 (NGC5457) \u306F\u304A\u304A\u3050\u307E\u5EA7\u306B\u3042\u308B\u6E26\u5DFB\u9280\u6CB3\u3002\u8DDD\u96E2\u7D042700\u4E07\u5149\u5E74\u30021781\u5E74\u306B\u30D4\u30A8\u30FC\u30EB\u30FB\u30E1\u30B7\u30E3\u30F3\u304C\u767A\u898B\u3057\u305F\u3002\u540C\u5E74\u30E1\u30B7\u30A8\u306F\u300C\u661F\u306E\u306A\u3044\u661F\u96F2\u3067\u3001\u975E\u5E38\u306B\u3082\u3046\u308D\u3046\u3068\u3057\u3066\u304D\u308C\u3044\u3002\u5F84\u306F6'\u3042\u308B\u3044\u306F7'\u3002\u3046\u3057\u304B\u3044\u306E\u5DE6\u624B\u3068\u5C3E\u5C0F\u718A\u306E\u5C3E\u306E\u4E2D\u9593\u306B\u3042\u308B\u3002\u8996\u91CE\u306E\u5341\u5B57\u7DDA\u304C\u5149\u3063\u3066\u3044\u308B\u3068\u304D\u306F\u3080\u305A\u304B\u3057\u3044\u300D\u3068\u8A18\u3057\u3066\u3044\u308B\u3002\u30A6\u30A3\u30EA\u30A2\u30E0\u30FB\u30CF\u30FC\u30B7\u30A7\u30EB\u306F\u300C\u307E\u3060\u3089\u306E\u3042\u308B\u661F\u96F2\u72B6\u300D\u30B8\u30E7\u30F3\u30FB\u30CF\u30FC\u30B7\u30A7\u30EB\u306F\u300C\u304B\u306A\u308A\u5927\u304D\u304F\u660E\u308B\u3044\u4E0D\u6B63\u5186\u5F62\u300D\u30B9\u30DF\u30B9\u306F1844\u5E74\u300C\u62E1\u6563\u3057\u305F\u8F1D\u304F\u7269\u8CEA\u304B\u3089\u3067\u304D\u3066\u3044\u308B\u3002\u3068\u3044\u3046\u3088\u308A\u3080\u3057\u308D\u5DE8\u5927\u306A\u661F\u584A\u304B\u3089\u3067\u304D\u305F\u7403\u72B6\u306E\u661F\u56E3\u306E\u3072\u3068\u3064\u3002\u306F\u304B\u308A\u77E5\u308C\u306A\u3044\u307B\u3069\u306E\u8DDD\u96E2\u300D1855\u5E74\u306B\u306F\u300C\u9752\u767D\u3044\u661F\u56E3\u3067\u3001\u6761\u4EF6\u304C\u3088\u3051\u308C\u3070\u5927\u304D\u304F\u3088\u308A\u5E83\u304C\u3063\u3066\u3044\u308B\u3002\u3054\u304F\u5FAE\u304B\u3060\u304C\u4E2D\u5FC3\u90E8\u306F\u3088\u304F\u5149\u3063\u3066\u3044\u308B\u300D\u3068\u3057\u305F\u3002\u30ED\u30B9\u537F\u306F\u300C\u5927\u304D\u304F\u6E26\u72B6\u3002\u5FAE\u304B\u3067\u6570\u500B\u306E\u8155\u304C\u51FA\u3066\u304A\u308A\u3001\u4E2D\u5FC3\u90E8\u306E\u7D50\u3073\u76EE\u306F\u5C11\u306A\u304F\u3068\u3082\u5F8414'\u300D\u3068\u3057\u305F\u3002\u5F7C\u306E\u30B9\u30B1\u30C3\u30C1\u306B\u306F\u306F\u3063\u304D\u308A\u3068\u6E26\u72B6\u306E\u8155\u304C\u63CF\u304B\u308C\u3066\u3044\u308B\u3002 1909\u5E74\u306B\u306F\u8D85\u65B0\u661F\u304C\u51FA\u73FE\u3057\u3001M\u30FB\u30A6\u30A9\u30EB\u30D5\u306B\u3088\u3063\u3066\u767A\u898B\u3055\u308C\u3066\u3044\u308B\u3002\u305D\u306E\u5F8C1950\u5E74\u306B17.5\u7B49\u30011970\u5E748\u6708\u306B\u306F11.7\u7B49\u306E\u5408\u8A083\u500B\u306E\u8D85\u65B0\u661F\u304C\u51FA\u73FE\u3057\u3066\u3044\u308B\u3002 \u53CC\u773C\u93E1\u3067\u306F\u6761\u4EF6\u304C\u826F\u3051\u308C\u3070\u5927\u304D\u304F\u5E83\u304C\u3063\u305F\u5186\u5F62\u3067\u6FC3\u6DE1\u306E\u306A\u3044\u5149\u6591\u3068\u3057\u3066\u898B\u3048\u308B\u3068\u3044\u3046\u3002\u53E3\u5F848cm\u306E\u671B\u9060\u93E1\u306E\u4F4E\u500D\u7387\u3067\u6FC3\u6DE1\u304C\u898B\u3048\u308B\u304C\u3001\u53CC\u773C\u93E1\u306E\u65B9\u304C\u304B\u3048\u3063\u3066\u3088\u304F\u898B\u3048\u308B\u3068\u3059\u308B\u610F\u898B\u3082\u3042\u308B\u3002\u30DE\u30E9\u30B9\u306F\u53E3\u5F8410cm\u306E\u671B\u9060\u93E1\u3067\u89B3\u5BDF\u3057\u3066\u300C\u4F4E\u500D\u7387\u304C\u6709\u52B9\u3002\u4E2D\u5FC3\u90E8\u304C\u30D5\u30EF\u30D5\u30EF\u3068\u9280\u8272\u306B\u8F1D\u304F\u3002\u307E\u308B\u3067\u661F\u96F2\u72B6\u7269\u8CEA\u306B\u3068\u308A\u304B\u3053\u307E\u308C\u3066\u3044\u308B\u300D\u3068\u3057\u305F\u3002\u30B8\u30E7\u30FC\u30F3\u30BA\u306F\u53E3\u5F8420cm\u306E\u671B\u9060\u93E1\u3067\u89B3\u5BDF\u3057\u3066\u300C\u5C0F\u3055\u3044\u304C\u6838\u306F\u306F\u3063\u304D\u308A\u3068\u3059\u308B\u3002\u20261\uFF5E2\u500B\u306E\u660E\u308B\u3044\u500B\u6240\u304C\u3042\u308B\u3002\u897F\u3068\u5357\u897F\u306E\u958B\u3044\u305F\u5206\u5C90\u4E2D\u306E\u3082\u306E\u304B\u3082\u3057\u308C\u306A\u3044\u300D\u3068\u3057\u3066\u3044\u308B\u3002\u30D2\u30E5\u30FC\u30B9\u30C8\u30F3\u306F10\u30A4\u30F3\u30C1(24.5cm)\u671B\u9060\u93E1\u3067\u898B\u3066\u300C\u660E\u308B\u304F\u8F1D\u3044\u3066\u5927\u304D\u306A\u5206\u5C90\u3092\u6697\u793A\u3059\u308B\u304C\u3001\u521D\u3081\u3066\u898B\u308B\u4EBA\u306F\u305D\u3046\u306F\u601D\u308F\u306A\u3044\u3060\u308D\u3046\u300D\u3068\u3057\u305F\u3002\u53E3\u5F8420cm\u3067\u8155\u306E\u90E8\u5206\u306E\u5FAE\u661F\u304C\u89B3\u5BDF\u3067\u304D\u308B\u3068\u3044\u3046\u3002\u53E3\u5F8430cm\u4EE5\u4E0A\u306B\u306A\u308B\u3068\u3001\u8155\u306E\u69CB\u9020\u304C\u308F\u304B\u308A\u3001\u8155\u306E\u90E8\u5206\u3067\u8F1D\u3044\u3066\u3044\u308B\u3068\u3053\u308D\u3092\u89B3\u5BDF\u3067\u304D\u308B\u3002\u3053\u308C\u3089\u306B\u306FNGC\u30CA\u30F3\u30D0\u30FC\u304C\u3075\u3089\u308C\u3066\u3044\u308B\u3082\u306E\u3082\u591A\u3044\u3002NGC5447\u3001NGC5455\u3001NGC5461\u3001NGC5462\u3001NGC5461\u3001NGC5462\u304C\u540C\u8996\u91CE\u306B\u898B\u3048\u3066\u304F\u308B\u3002\u307E\u305F\u5468\u56F2\u306B\u306FNGC5471\u3001NGC5422\u3001NGC5473\u3001NGC5474\u3001NGC5485\u306A\u3069\u306E\u4F34\u9280\u6CB3\u304C\u3042\u308A\u3001\u305D\u308C\u3089\u3082\u898B\u308B\u3053\u3068\u304C\u3067\u304D\u308B\u3002 \u53F3\u306E\u5199\u771F\u3067\u3001\u4E2D\u5FC3\u90E8\u306E\u5DE6\u3084\u3084\u4E0A\u306B\u96E2\u308C\u3066\u3042\u308B\u5149\u6591\u304CNGC5462\u3001\u5DE6\u3084\u3084\u4E0B\u306B\u5C11\u3057\u96E2\u308C\u3066\u3042\u308B\u306E\u304CNGC5461\u3001\u53F3\u4E0B\u306B\u304F\u3063\u3064\u304D\u6C17\u5473\u306B\u3042\u308B\u306E\u304CNGC5455\u3001\u53F3\u4E0B\u306E\u753B\u9762\u7AEF\u306B\u3042\u308B\u306E\u304CNGC5447\u3067\u3042\u308B\u3002\u3053\u308C\u3089\u591A\u304F\u306E\u9280\u6CB3\u306FM101\u9280\u6CB3\u7FA4\u3092\u4F5C\u3063\u3066\u3044\u308B\u3002M101\u306F\u305D\u306E\u4E2D\u6838\u3092\u306A\u3059\u6700\u3082\u660E\u308B\u3044\u9280\u6CB3\u3067\u3042\u308B\u3002"@ja ,
"La Galaxia del Molinete (tambi\u00E9n conocida como Messier 101 o NGC 5457) es una galaxia espiral a unos 27 millones de a\u00F1os luz en la constelaci\u00F3n Osa Mayor. Fue descubierta por Pierre M\u00E9chain el 27 de marzo de 1781, y \u00E9l posteriormente comunic\u00F3 su descubrimiento a Charles Messier que verific\u00F3 su posici\u00F3n y la a\u00F1adi\u00F3 a Cat\u00E1logo Messier como una de las \u00FAltimas entradas. Es una de las galaxias m\u00E1s grandes existentes en la vecindad de la V\u00EDa L\u00E1ctea, con un di\u00E1metro de m\u00E1s del doble que ella, y se caracteriza tanto por su riqueza en gas para formar nuevas estrellas c\u00F3mo por su elevado n\u00FAmero de regiones HII (m\u00E1s de 3000, algunas tan grandes y brillantes que tienen n\u00FAmero NGC propio y que han sido estudiadas por el Telescopio Espacial Hubble, mostrando la presencia de super c\u00FAmulos estelares al menos en algunas de ellas) y de c\u00FAmulos estelares j\u00F3venes (tambi\u00E9n estudiados con dicho telescopio), lo que apunta a una elevada tasa de formaci\u00F3n estelar. Ello junto a la asimetr\u00EDa que muestra en las fotograf\u00EDas (que la ha hecho aparecer en el Atlas de galaxias peculiares de Halton C. Arp c\u00F3mo Arp 26, y definida c\u00F3mo Galaxia espiral con un brazo bien definido) hace pensar que -en t\u00E9rminos astron\u00F3micos- hace relativamente poco otra galaxia estuvo a punto de colisionar con ella, causando ambos fen\u00F3menos. \u00C9sta galaxia tiene un bulbo casi inexistente, y de acuerdo a estudios recientes parece carecer de un agujero negro supermasivo en su centro, a diferencia de por ejemplo nuestra galaxia. M101 est\u00E1 acompa\u00F1ada por cinco galaxias sat\u00E9lite prominentes: NGC 5204, NGC 5474, NGC 5477, NGC 5585, y Holmberg IV, que pueden ser las responsables de su estado actual -de hecho, M101 parece haber distorsionado a la galaxia NGC 5474-."@es ,
"Tuulimyllygalaksi (tunnetaan my\u00F6s nimell\u00E4 Messier 101, M101 ja NGC 5457) on p\u00E4\u00E4lt\u00E4 p\u00E4in n\u00E4kyv\u00E4 kierteisgalaksi Ison karhun t\u00E4hdist\u00F6ss\u00E4. Se on noin 27 miljoonan valovuoden et\u00E4isyydell\u00E4. M101 on kirkkain kohde ss\u00E4. Pierre M\u00E9chain l\u00F6ysi M101:n 27. maaliskuuta 1781 ja h\u00E4n kertoi l\u00F6yd\u00F6st\u00E4\u00E4n Charles Messierille, joka varmisti kohteen sijainnin ja lis\u00E4si sen Messierin luetteloon. 28. helmikuuta 2006 NASA ja ESA julkaisivat yksityiskohtaisen kuvan Tuulimyllygalaksista, suurimman ja tarkimman Hubblen mist\u00E4\u00E4n galaksista ottaman kuvan. Kuva on yhdistetty 51:st\u00E4 eri valotuksesta."@fi ,
"Vindsnurregalaxen (M101, ocks\u00E5 katalogiserad som NGC 5457) \u00E4r en frontalv\u00E4nd spiralgalax bel\u00E4gen omkring 27 miljoner ljus\u00E5r bort i stj\u00E4rnbilden Stora bj\u00F6rnen. M101 \u00E4r en relativt stor galax j\u00E4mf\u00F6rt med Vintergatan. Med en diameter p\u00E5 170 000 ljus\u00E5r \u00E4r den n\u00E4stan dubbelt s\u00E5 stor som v\u00E5r galax. N\u00E5got som utm\u00E4rker M101 \u00E4r att den har ett mycket stort antal H II-regioner, omkring 3 000 stycken \u00E4r synliga p\u00E5 fotografier. HII-regioner \u00E4r omr\u00E5den i galaxer som best\u00E5r av enorma moln av t\u00E4t v\u00E4tgas, i vilka nya stj\u00E4rnor f\u00F6ds. Unga, heta stj\u00E4rnor ger HII-regionerna sitt karakteristiska bl\u00E5a sken. Messier 101 \u00E4r asymmetrisk p\u00E5 en sida, vilket antas bero p\u00E5 att galaxen n\u00E4tt och j\u00E4mnt undgick en kollision med en annan galax men deformerades av de gravitationella krafterna. Vindsnurregalaxen har fem prominenta f\u00F6ljeslagare; galaxerna NGC 5204, NGC 5474, NGC 5477, NGC 5585, och Holmberg IV."@sv ,
"F\u0131r\u0131ldak G\u00F6kadas\u0131 (ayr\u0131ca Messier 101 veya NGC 5457 olarak da bilinir) 27 milyon \u0131\u015F\u0131k y\u0131l\u0131 uzakl\u0131kta B\u00FCy\u00FCk Ay\u0131 y\u00F6n\u00FCnde bulunan tam kar\u015F\u0131dan g\u00F6r\u00FClen sarmal g\u00F6kada. Pierre M\u00E9chain taraf\u0131ndan 27 Mart 1781 tarihinde ke\u015Ffedilmi\u015F ve Charles Messier, konumunu do\u011Frulayarak katalo\u011Funa eklemi\u015Ftir. 28 \u015Eubat 2006'da NASA ve ESA, Hubble Uzay Teleskopuyla bu zamana kadar olan en b\u00FCy\u00FCk ve detayl\u0131 F\u0131r\u0131ldak G\u00F6kadas\u0131 foto\u011Fraflar\u0131n\u0131 yay\u0131mlad\u0131. Foto\u011Fraf, 51 ayr\u0131 pozdan ve ayr\u0131ca yer temelli foto\u011Fraflardan olu\u015Fmaktad\u0131r."@tr ,
"Messier 101 (tak\u00E9 NGC 5457 nebo galaxie V\u011Btrn\u00EDk, anglicky Pinwheel Galaxy je spir\u00E1ln\u00ED galaxie o \u00FAhlov\u00FDch rozm\u011Brech 28,5' x 28,3' a hv\u011Bzdn\u00E9 velikosti o +7,90 mag v souhv\u011Bzd\u00ED Velk\u00E9 medv\u011Bdice. Galaxie V\u011Btrn\u00EDk je od Zem\u011B vzd\u00E1lena 27 mili\u00F3n\u016F sv\u011Bteln\u00FDch let a je nejjasn\u011Bj\u0161\u00EDm \u010Dlenem kupy galaxi\u00ED M 101."@cs ,
"M101 (Messier 101 / NGC 5457), ook wel het Windmolenstelsel genoemd, is een spiraalvormig sterrenstelsel in het sterrenbeeld Grote Beer. M101 heeft een diameter van 170.000 lichtjaar en een absolute magnitude van -21,6. Waarnemingen van Cephe\u00EFde hebben aangetoond dat dit stelsel zo'n 27 miljoen lichtjaar van ons af ligt. Er zijn drie supernova's in M101 waargenomen, in 1909, 1951 en 1970. M101 is het helderste lid van de M101 groep van sterrenstelsels."@nl ,
"\u98A8\u8ECA\u661F\u7CFB\uFF08\u4E5F\u7A31\u70BAM101\u6216NGC 5457\uFF09\u662F\u6B63\u9762\u671D\u5411\u6211\u5011\u7684\u87BA\u65CB\u661F\u7CFB\uFF0C\u4F4D\u65BC\u5927\u718A\u5EA7\uFF0C\u8DDD\u96E2\u5927\u7D042,700\u842C\u5149\u5E74\u3002 \u4ED6\u57281781\u5E743\u670827\u65E5\u88AB\u76AE\u57C3\u723E\u00B7\u6885\u9999\u767C\u73FE\uFF0C\u96A8\u5F8C\u4ED6\u5C07\u6B64\u4E00\u767C\u73FE\u8F49\u9054\u7D66\u6885\u897F\u723E\uFF0C\u6885\u897F\u723E\u5728\u6838\u5C0D\u4E86\u4F4D\u7F6E\u4E4B\u5F8C\u5C07\u4E4B\u767B\u9304\u65BC\u6885\u897F\u723E\u76EE\u9304\u4E2D\uFF0C\u4E26\u4F5C\u70BA\u7D42\u7D50\u7684\u8A18\u9304\u3002 \u57282006\u5E742\u670828\u65E5NASA\u548CESA\u91CB\u653E\u51FA\u4E00\u5F35\u98A8\u8ECA\u661F\u7CFB\u975E\u5E38\u8A73\u7D30\u7684\u7167\u7247\uFF0C\u5728\u7576\u6642\uFF0C\u90A3\u5F35\u7167\u7247\u662F\u54C8\u67CF\u592A\u7A7A\u671B\u9060\u93E1\u6240\u62CD\u6700\u5927\u548C\u6700\u8A73\u7D30\u7684\u661F\u7CFB\u7167\u7247\u3002\u9019\u5F35\u7167\u7247\u662F\u7D93\u753151\u6B21\u7368\u7ACB\u7684\u66DD\u5149\uFF0C\u518D\u52A0\u4E0A\u4E00\u4E9B\u5728\u5730\u9762\u4E0A\u62CD\u651D\u7684\u7167\u7247\u3002"@zh ,
"Messier 101 (auch als NGC 5457, Pinwheel-Galaxie oder Feuerrad-Galaxie bezeichnet) ist eine Spiralgalaxie mit den Abmessungen 28,8' \u00D7 26,9' und der scheinbaren Helligkeit von +7,5 mag im Sternbild Gro\u00DFer B\u00E4r. Ihre Entfernung betr\u00E4gt 27 Millionen Lichtjahre, ihr Durchmesser 170.000 Lj. Am 28. Februar 2006 ver\u00F6ffentlichten NASA und ESA ein sehr eindrucksvolles Bild, das gr\u00F6\u00DFte und detaillierteste Bild einer Galaxie, das mit Hilfe von Hubble angefertigt wurde . Das Bild wurde aus \u00FCber 51 Aufnahmen zusammengesetzt."@de ,
"La Galassia Girandola (nota anche come M 101, o NGC 5457) \u00E8 una galassia a spirale nella costellazione dell'Orsa Maggiore. La galassia fu scoperta nel 1781 da Charles Messier e da Pierre M\u00E9chain. William Herschel fu il primo a osservare delle piccole macchie (che in realt\u00E0 erano dei frammenti dei bracci a spirale) circondare la galassia."@it ,
"M101 (Messier 101, \u041C\u0435\u0441\u0441\u044C\u0435 101, NGC 5457, \u0413\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u0430 \u0426\u0435\u0432\u043E\u0447\u043D\u043E\u0435 \u043A\u043E\u043B\u0435\u0441\u043E)\u00A0\u2014 \u0441\u043F\u0438\u0440\u0430\u043B\u044C\u043D\u0430\u044F \u0433\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u0430 \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. \u041C\u043E\u0436\u043D\u043E \u0432\u0441\u0442\u0440\u0435\u0442\u0438\u0442\u044C \u043F\u043E\u0434 \u043D\u0430\u0437\u0432\u0430\u043D\u0438\u0435\u043C \u0413\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u0430 \u0426\u0435\u0432\u043E\u0447\u043D\u043E\u0435 \u041A\u043E\u043B\u0435\u0441\u043E. \u041E\u0431\u044A\u0435\u043A\u0442 \u0432\u0445\u043E\u0434\u0438\u0442 \u0432 \u0430\u0442\u043B\u0430\u0441 \u043F\u0435\u043A\u0443\u043B\u044F\u0440\u043D\u044B\u0445 \u0433\u0430\u043B\u0430\u043A\u0442\u0438\u043A \u043F\u043E\u0434 \u043D\u0430\u0437\u0432\u0430\u043D\u0438\u0435\u043C Arp 26. \u041E\u0442\u043A\u0440\u044B\u0442\u0438\u0435 \u0431\u044B\u043B\u043E \u0441\u0434\u0435\u043B\u0430\u043D\u043E \u041F\u044C\u0435\u0440\u043E\u043C \u041C\u0435\u0448\u0435\u043D\u043E\u043C 27 \u043C\u0430\u0440\u0442\u0430 1781 \u0433\u043E\u0434\u0430. \u0412\u043F\u043E\u0441\u043B\u0435\u0434\u0441\u0442\u0432\u0438\u0438 \u043E\u043D \u0441\u043E\u043E\u0431\u0449\u0438\u043B \u043E \u043D\u0435\u043C \u0428\u0430\u0440\u043B\u044E \u041C\u0435\u0441\u0441\u044C\u0435. \u041F\u043E\u0441\u043B\u0435\u0434\u043D\u0438\u0439 \u0443\u0442\u043E\u0447\u043D\u0438\u043B \u043C\u0435\u0441\u0442\u043E\u043F\u043E\u043B\u043E\u0436\u0435\u043D\u0438\u0435 \u043E\u0431\u044A\u0435\u043A\u0442\u0430 \u0438 \u0434\u043E\u0431\u0430\u0432\u0438\u043B \u0432 \u0441\u0432\u043E\u0439 \u043A\u0430\u0442\u0430\u043B\u043E\u0433 \u043E\u0434\u043D\u043E\u0439 \u0438\u0437 \u043F\u043E\u0441\u043B\u0435\u0434\u043D\u0438\u0445 \u0437\u0430\u043F\u0438\u0441\u0435\u0439. \u0411\u044B\u043B\u0430 \u043A\u043B\u0430\u0441\u0441\u0438\u0444\u0438\u0446\u0438\u0440\u043E\u0432\u0430\u043D\u0430 \u0425\u0430\u0431\u0431\u043B\u043E\u043C \u043A\u0430\u043A \u043E\u0431\u0440\u0430\u0437\u0435\u0446 \u0433\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u0438 Sc."@ru ,
"M101 est une galaxie spirale situ\u00E9e dans la Grande Ourse et distante de 23 millions d'ann\u00E9es-lumi\u00E8re. M101 est vue exactement du dessus mais ses bras spiraux ne sont visibles qu'avec de grands t\u00E9lescopes. Le diam\u00E8tre de la galaxie (170 000 ann\u00E9es-lumi\u00E8re) est pr\u00E8s de deux fois sup\u00E9rieur \u00E0 celui de la n\u00F4tre (100 000 ann\u00E9es-lumi\u00E8re) et le nombre d'\u00E9toiles est estim\u00E9 \u00E0 entre 100 et 1000 milliards (compar\u00E9 \u00E0 100 milliards pour la n\u00F4tre)."@fr ,
"Galaktyka Wiatraczek (znana r\u00F3wnie\u017C jako Messier 101, M101 lub NGC 5457) \u2013 galaktyka spiralna ze s\u0142abym j\u0105drem i bardzo rozwini\u0119tymi ramionami w gwiazdozbiorze Wielkiej Nied\u017Cwiedzicy. Jej jasno\u015B\u0107 wynosi 7,9, a jej rozmiary na niebie 24,5' \u00D7 23,4'. Masa galaktyki jest w przybli\u017Ceniu r\u00F3wna 180 miliardom mas S\u0142o\u0144ca. Znajduje si\u0119 w odleg\u0142o\u015Bci 27 milion\u00F3w lat \u015Bwietlnych. Razem z innymi s\u0142abszymi galaktykami M101 tworzy grup\u0119 galaktyk."@pl ,
"Messier 101 sau M101 este o galaxie spiral\u0103."@ro ;
rdfs:comment ""@ja ,
"A Messier 101 (m\u00E1s n\u00E9ven M101, NGC 5457 vagy Sz\u00E9lker\u00E9k-Galaxis) egy spir\u00E1lgalaxis az Ursa Major (Nagy Medve) csillagk\u00E9pben."@hu ,
"M101 est une galaxie spirale situ\u00E9e dans la Grande Ourse et distante de 23 millions d'ann\u00E9es-lumi\u00E8re. M101 est vue exactement du dessus mais ses bras spiraux ne sont visibles qu'avec de grands t\u00E9lescopes. Le diam\u00E8tre de la galaxie (170 000 ann\u00E9es-lumi\u00E8re) est pr\u00E8s de deux fois sup\u00E9rieur \u00E0 celui de la n\u00F4tre (100 000 ann\u00E9es-lumi\u00E8re) et le nombre d'\u00E9toiles est estim\u00E9 \u00E0 entre 100 et 1000 milliards (compar\u00E9 \u00E0 100 milliards pour la n\u00F4tre)."@fr ,
"F\u0131r\u0131ldak G\u00F6kadas\u0131 (ayr\u0131ca Messier 101 veya NGC 5457 olarak da bilinir) 27 milyon \u0131\u015F\u0131k y\u0131l\u0131 uzakl\u0131kta B\u00FCy\u00FCk Ay\u0131 y\u00F6n\u00FCnde bulunan tam kar\u015F\u0131dan g\u00F6r\u00FClen sarmal g\u00F6kada. Pierre M\u00E9chain taraf\u0131ndan 27 Mart 1781 tarihinde ke\u015Ffedilmi\u015F ve Charles Messier, konumunu do\u011Frulayarak katalo\u011Funa eklemi\u015Ftir. 28 \u015Eubat 2006'da NASA ve ESA, Hubble Uzay Teleskopuyla bu zamana kadar olan en b\u00FCy\u00FCk ve detayl\u0131 F\u0131r\u0131ldak G\u00F6kadas\u0131 foto\u011Fraflar\u0131n\u0131 yay\u0131mlad\u0131."@tr ,
"M101 (Messier 101 / NGC 5457), ook wel het Windmolenstelsel genoemd, is een spiraalvormig sterrenstelsel in het sterrenbeeld Grote Beer. M101 heeft een diameter van 170.000 lichtjaar en een absolute magnitude van -21,6. Waarnemingen van Cephe\u00EFde hebben aangetoond dat dit stelsel zo'n 27 miljoen lichtjaar van ons af ligt. Er zijn drie supernova's in M101 waargenomen, in 1909, 1951 en 1970. M101 is het helderste lid van de M101 groep van sterrenstelsels."@nl ,
"Messier 101 (auch als NGC 5457, Pinwheel-Galaxie oder Feuerrad-Galaxie bezeichnet) ist eine Spiralgalaxie mit den Abmessungen 28,8' \u00D7 26,9' und der scheinbaren Helligkeit von +7,5 mag im Sternbild Gro\u00DFer B\u00E4r. Ihre Entfernung betr\u00E4gt 27 Millionen Lichtjahre, ihr Durchmesser 170.000 Lj. Am 28. Februar 2006 ver\u00F6ffentlichten NASA und ESA ein sehr eindrucksvolles Bild, das gr\u00F6\u00DFte und detaillierteste Bild einer Galaxie, das mit Hilfe von Hubble angefertigt wurde ."@de ,
"Messier 101 (tak\u00E9 NGC 5457 nebo galaxie V\u011Btrn\u00EDk, anglicky Pinwheel Galaxy je spir\u00E1ln\u00ED galaxie o \u00FAhlov\u00FDch rozm\u011Brech 28,5' x 28,3' a hv\u011Bzdn\u00E9 velikosti o +7,90 mag v souhv\u011Bzd\u00ED Velk\u00E9 medv\u011Bdice. Galaxie V\u011Btrn\u00EDk je od Zem\u011B vzd\u00E1lena 27 mili\u00F3n\u016F sv\u011Bteln\u00FDch let a je nejjasn\u011Bj\u0161\u00EDm \u010Dlenem kupy galaxi\u00ED M 101."@cs ,
"M101 (Messier 101, \u041C\u0435\u0441\u0441\u044C\u0435 101, NGC 5457, \u0413\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u0430 \u0426\u0435\u0432\u043E\u0447\u043D\u043E\u0435 \u043A\u043E\u043B\u0435\u0441\u043E)\u00A0\u2014 \u0441\u043F\u0438\u0440\u0430\u043B\u044C\u043D\u0430\u044F \u0433\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u0430 \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. \u041C\u043E\u0436\u043D\u043E \u0432\u0441\u0442\u0440\u0435\u0442\u0438\u0442\u044C \u043F\u043E\u0434 \u043D\u0430\u0437\u0432\u0430\u043D\u0438\u0435\u043C \u0413\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u0430 \u0426\u0435\u0432\u043E\u0447\u043D\u043E\u0435 \u041A\u043E\u043B\u0435\u0441\u043E. \u041E\u0431\u044A\u0435\u043A\u0442 \u0432\u0445\u043E\u0434\u0438\u0442 \u0432 \u0430\u0442\u043B\u0430\u0441 \u043F\u0435\u043A\u0443\u043B\u044F\u0440\u043D\u044B\u0445 \u0433\u0430\u043B\u0430\u043A\u0442\u0438\u043A \u043F\u043E\u0434 \u043D\u0430\u0437\u0432\u0430\u043D\u0438\u0435\u043C Arp 26."@ru ,
"La Gal\u00E0xia del Molinet (Messier 101, M101 o NGC 5457) \u00E9s una gal\u00E0xia espiral vista frontalment situada a la constel\u00B7laci\u00F3 de l'\u00D3ssa Major. Va ser descoberta per Pierre M\u00E9chain el 27 de mar\u00E7 de 1781, qui va comunicar el seu descobriment al seu amic Charles Messier qui va verificar la seva posici\u00F3 i la va afegir al seu cat\u00E0leg."@ca ,
"La Galaxia del Molinete (tambi\u00E9n conocida como Messier 101 o NGC 5457) es una galaxia espiral a unos 27 millones de a\u00F1os luz en la constelaci\u00F3n Osa Mayor. Fue descubierta por Pierre M\u00E9chain el 27 de marzo de 1781, y \u00E9l posteriormente comunic\u00F3 su descubrimiento a Charles Messier que verific\u00F3 su posici\u00F3n y la a\u00F1adi\u00F3 a Cat\u00E1logo Messier como una de las \u00FAltimas entradas."@es ,
"NGC 5457 ou M101, popularmente conhecida como Gal\u00E1xia do Catavento, \u00E9 uma gal\u00E1xia espiral localizada a cerca de vinte e sete milh\u00F5es de anos-luz de dist\u00E2ncia na dire\u00E7\u00E3o da constela\u00E7\u00E3o de Ursa Maior. Possui entre cento e setenta e duzentos mil anos-luz de di\u00E2metro, uma magnitude aparente de 7,5, uma magnitude absoluta de -21,6, uma declina\u00E7\u00E3o de +54\u00BA 20' 55\" e uma ascens\u00E3o reta de 14 horas 03 minutos 12,4 segundos."@pt ,
"La Galassia Girandola (nota anche come M 101, o NGC 5457) \u00E8 una galassia a spirale nella costellazione dell'Orsa Maggiore. La galassia fu scoperta nel 1781 da Charles Messier e da Pierre M\u00E9chain. William Herschel fu il primo a osservare delle piccole macchie (che in realt\u00E0 erano dei frammenti dei bracci a spirale) circondare la galassia."@it ,
""@zh ,
"The Pinwheel Galaxy (also known as Messier 101 or NGC 5457) is a face-on spiral galaxy about 27 million light-years away in the constellation Ursa Major. It was discovered by Pierre M\u00E9chain on March 27, 1781, and he subsequently communicated his discovery to Charles Messier who verified its position and added it to the Messier Catalogue as one of the final entries."@en ,
"Messier 101 sau M101 este o galaxie spiral\u0103."@ro ,
"Tuulimyllygalaksi (tunnetaan my\u00F6s nimell\u00E4 Messier 101, M101 ja NGC 5457) on p\u00E4\u00E4lt\u00E4 p\u00E4in n\u00E4kyv\u00E4 kierteisgalaksi Ison karhun t\u00E4hdist\u00F6ss\u00E4. Se on noin 27 miljoonan valovuoden et\u00E4isyydell\u00E4. M101 on kirkkain kohde ss\u00E4. Pierre M\u00E9chain l\u00F6ysi M101:n 27. maaliskuuta 1781 ja h\u00E4n kertoi l\u00F6yd\u00F6st\u00E4\u00E4n Charles Messierille, joka varmisti kohteen sijainnin ja lis\u00E4si sen Messierin luetteloon. 28."@fi ,
"Galaktyka Wiatraczek (znana r\u00F3wnie\u017C jako Messier 101, M101 lub NGC 5457) \u2013 galaktyka spiralna ze s\u0142abym j\u0105drem i bardzo rozwini\u0119tymi ramionami w gwiazdozbiorze Wielkiej Nied\u017Cwiedzicy. Jej jasno\u015B\u0107 wynosi 7,9, a jej rozmiary na niebie 24,5' \u00D7 23,4'. Masa galaktyki jest w przybli\u017Ceniu r\u00F3wna 180 miliardom mas S\u0142o\u0144ca. Znajduje si\u0119 w odleg\u0142o\u015Bci 27 milion\u00F3w lat \u015Bwietlnych. Razem z innymi s\u0142abszymi galaktykami M101 tworzy grup\u0119 galaktyk."@pl ,
"Vindsnurregalaxen (M101, ocks\u00E5 katalogiserad som NGC 5457) \u00E4r en frontalv\u00E4nd spiralgalax bel\u00E4gen omkring 27 miljoner ljus\u00E5r bort i stj\u00E4rnbilden Stora bj\u00F6rnen. M101 \u00E4r en relativt stor galax j\u00E4mf\u00F6rt med Vintergatan. Med en diameter p\u00E5 170 000 ljus\u00E5r \u00E4r den n\u00E4stan dubbelt s\u00E5 stor som v\u00E5r galax. N\u00E5got som utm\u00E4rker M101 \u00E4r att den har ett mycket stort antal H II-regioner, omkring 3 000 stycken \u00E4r synliga p\u00E5 fotografier."@sv ;
foaf:depiction .
@prefix skos: .
@prefix ns12: .
dbpedia:Pinwheel_Galaxy skos:subject ns12:Ursa_Major_constellation ,
ns12:M101_Group ,
ns12:Spiral_galaxies ,
ns12:Messier_objects ,
ns12:Intermediate_spiral_galaxies ,
ns12:NGC_objects ,
ns12:UGC_objects ,
ns12:PGC_objects ,
ns12:Arp_objects .
@prefix ns13: .
dbpedia:Pinwheel_Galaxy dbpprop:wikiPageUsesTemplate ns13:sky ,
ns13:commons ,
ns13:infobox_galaxy ;
dbpprop:type "SAB(rs)cd"@en .
@prefix ns14: .
dbpedia:Pinwheel_Galaxy dbpprop:dec ns14:DEC ;
dbpprop:constellationName dbpedia:Ursa_Major ;
dbpprop:z "241 \u00B1 2 km/"@en ;
dbpprop:names dbpedia:Uppsala_General_Catalogue ,
dbpedia:Principal_Galaxies_Catalogue ,
dbpedia:Atlas_of_Peculiar_Galaxies ,
dbpedia:New_General_Catalogue ,
dbpedia:Messier_object ;
dbpprop:epoch dbpedia:J2000 ;
dbpprop:commonsProperty "Pinwheel Galaxy"@en ,
"Messier 101"@en .
@prefix ns15: .
dbpedia:Pinwheel_Galaxy dbpprop:ra ns15:RA ;
dbpprop:skyProperty 14 ,
27000000 ,
"+"@en ,
3 ,
12.6 ,
20 ,
57 ,
54 ;
dbpprop:sizeV "28′.8 × 26′.9"@en ;
dbpprop:caption "The Pinwheel Galaxy. Credit: NASA/\u20AC"@en ;
dbpprop:appmagV 8.3 ;
dbpprop:distLy dbpedia:Light-year ,
.
@prefix ns16: .
dbpedia:Pinwheel_Galaxy dbpprop:hasPhotoCollection ns16:Pinwheel_Galaxy .
dbpedia:PGC_50063 dbpprop:redirect dbpedia:Pinwheel_Galaxy .
dbpedia:Messier_101 dbpprop:redirect dbpedia:Pinwheel_Galaxy .
dbpedia:NGC_5457 dbpprop:redirect dbpedia:Pinwheel_Galaxy .
dbpedia:Arp_26 dbpprop:redirect dbpedia:Pinwheel_Galaxy .
dbpedia:Messier_Object_101 dbpprop:redirect dbpedia:Pinwheel_Galaxy .
dbpedia:Pinwheel_galaxy dbpprop:redirect dbpedia:Pinwheel_Galaxy .
dbpedia:UGC_8981 dbpprop:redirect dbpedia:Pinwheel_Galaxy .
@prefix yago: .
yago:Pinwheel_Galaxy owl:sameAs dbpedia:Pinwheel_Galaxy .