. "Owl Nebula Messier 97"@en . . . . "La nebulosa Civetta (nota anche come Nebulosa Gufo o con le sigle M 97 o NGC 3587) \u00E8 una nebulosa planetaria visibile nella costellazione dell'Orsa Maggiore; \u00E8 stata scoperta da Pierre M\u00E9chain nel 1781. Il nome \"Nebulosa Gufo\" \u00E8 stato invece assegnato da William Parsons nel 1848 a causa delle due macchie scure, che assomigliano agli occhi di un gufo. M97 \u00E8 una delle nebulose planetarie pi\u00F9 complesse. Il suo aspetto \u00E8 stato interpretato come una sfera senza poli, con gli occhi del gufo in corrispondenza delle zone povere di materia ai poli. La sua et\u00E0 \u00E8 stimata in 6.000 anni."@it . "Ugglenebulosan eller Messier 97 (M97) \u00E4ven k\u00E4nd som NGC 3587, \u00E4r en planetarisk nebulosa i stj\u00E4rnbilden Stora Bj\u00F6rnen p\u00E5 ett avst\u00E5nd av ca 2 030 ljus\u00E5r fr\u00E5n solsystemet. Ugglenebulosan \u00E4r klassificerad som en av de mer komplexa av de planetariska nebulosorna. Centralstj\u00E4rnan med en skenbar magnitud p\u00E5 16, har en massa av ca 0,7 solmassor och nebulosan sj\u00E4lv ca 0,15 solmassor. Nebulosan formades f\u00F6r ungef\u00E4r 8 000 \u00E5r sedan. Den har ungef\u00E4r cirkul\u00E4rt tv\u00E4rsnitt med svaga inre strukturer och bildades fr\u00E5n utfl\u00F6det av material fr\u00E5n den centrala stj\u00E4rnans stj\u00E4rnvind n\u00E4r den utvecklades l\u00E4ngs den asymptotiska j\u00E4ttegrenen."@sv . . . . . . . . . "9.9"^^ . . "A Nebulosa da Coruja (tamb\u00E9m conhecida como Messier 97 ou NGC 3587) \u00E9 uma nebulosa planet\u00E1ria localizada na constela\u00E7\u00E3o de Ursa Major. Foi descoberta por Pierre M\u00E9chain em 1781. \u00C9 considerada uma das mais complexas nebulosas planet\u00E1rias. A estrela central de magnitude 16 tem cerca de 0,7 massas solares e a nebulosa em si cerca de 0,15 massas solares. A nebulosa foi formada apenas h\u00E1 cerca de 8000 anos. A Nebulosa da Coruja recebeu o seu nome devido aos seus \"olhos\" parecidos com o de uma coruja quando vista atrav\u00E9s de um telesc\u00F3pio (> 200 mm) grande sob um c\u00E9u escuro com o aux\u00EDlio de um \"filtro de nebulosa\". Os \"olhos\" s\u00E3o tamb\u00E9m facilmente vis\u00EDveis atrav\u00E9s de fotografias tiradas da nebulosa."@pt . . . "\u0422\u0443\u043C\u0430\u0301\u043D\u043D\u043E\u0441\u0442\u044C \u0421\u043E\u0432\u0430\u0301 (\u0430\u043D\u0433\u043B. Messier 97, M 97, NGC 3587, \u0440\u0443\u0441. \u041C\u0435\u0441\u0441\u044C\u0435 97) \u2014 \u043F\u043B\u0430\u043D\u0435\u0442\u0430\u0440\u043D\u0430\u044F \u0442\u0443\u043C\u0430\u043D\u043D\u043E\u0441\u0442\u044C \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. \u041E\u0442\u043A\u0440\u044B\u0442\u0430 \u041F\u044C\u0435\u0440\u043E\u043C \u041C\u0435\u0448\u0435\u043D\u043E\u043C \u0432 1781 \u0433\u043E\u0434\u0443. \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."@ru . "J2000.0"@en . "\u0422\u0443\u043C\u0430\u043D\u043D\u0456\u0441\u0442\u044C \u0421\u043E\u0432\u0430 (M97, NGC 3587) \u2014 \u043F\u043B\u0430\u043D\u0435\u0442\u0430\u0440\u043D\u0430 \u0442\u0443\u043C\u0430\u043D\u043D\u0456\u0441\u0442\u044C \u0442\u0438\u043F\u0443 PN \u0443 \u0441\u0443\u0437\u0456\u0440'\u0457 \u0412\u0435\u043B\u0438\u043A\u0430 \u0412\u0435\u0434\u043C\u0435\u0434\u0438\u0446\u044F.\u0412\u0456\u0434\u043A\u0440\u0438\u0432\u0430\u0447\u0435\u043C \u0446\u044C\u043E\u0433\u043E \u043E\u0431'\u0454\u043A\u0442\u0430 \u0454 \u041C\u0435\u0448\u0430\u043D \u041F'\u0454\u0440 \u0424\u0440\u0430\u043D\u0441\u0443\u0430 \u0410\u043D\u0434\u0440\u0435, \u044F\u043A\u0438\u0439 \u0432\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 16 \u043B\u044E\u0442\u043E\u0433\u043E 1781.\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 (NGC)."@uk . . "Mg\u0142awica Sowa (r\u00F3wnie\u017C Messier 97, M97 lub NGC 3587) \u2013 mg\u0142awica planetarna znajduj\u0105ca si\u0119 w gwiazdozbiorze Wielkiej Nied\u017Awiedzicy. Odkry\u0142 j\u0105 Pierre M\u00E9chain 16 lutego 1781 roku. M97 jest jedn\u0105 z bardziej z\u0142o\u017Conych mg\u0142awic planetarnych. Ma mas\u0119 oko\u0142o 0,15 masy S\u0142o\u0144ca, masa jej gwiazdy centralnej to ok. 0,7 masy S\u0142o\u0144ca. Jasno\u015B\u0107 tej gwiazdy wynosi 16m. Jasno\u015B\u0107 wizualna mg\u0142awicy to 9,9m, a jej fotograficzna jasno\u015B\u0107 wynosi 12m. System powsta\u0142 oko\u0142o 6000 lat temu. Do jej zaobserwowania wystarcza teleskop o \u015Brednicy 10-12 cm, dobre warunki obserwacyjne (brak Ksi\u0119\u017Cyca i \u015Bwiate\u0142 miejskich) oraz nie za du\u017Ce powi\u0119kszenie. Teleskop o \u015Brednicy wi\u0119kszej ni\u017C 15 cm pozwoli zauwa\u017Cy\u0107 w mg\u0142awicy dwie ciemne plamki wygl\u0105daj\u0105ce jak oczy sowy. To w\u0142a\u015Bnie im mg\u0142awica zawdzi\u0119cza swoj\u0105 nazw\u0119."@pl . . . "Sov\u00ED mlhovina (tak\u00E9 M 97 nebo NGC 3587) je planet\u00E1rn\u00ED mlhovina v souhv\u011Bzd\u00ED Velk\u00E9 medv\u011Bdice. Objevil ji Pierre M\u00E9chain 16. \u00FAnora 1781 a Sov\u00ED mlhovinou ji nazval Lord Rosse roku 1848."@cs . . "Owl Nebula"@en . . . . . . . . "La nebulosa del B\u00FAho (tambi\u00E9n conocida como Messier 97 o NGC 3587) es una nebulosa planetaria ubicada en la constelaci\u00F3n de la Osa Mayor. Fue descubierta por Pierre M\u00E9chain en 1781. El nombre de Nebulosa del B\u00FAho fue acu\u00F1ado por Lord Rosse, quien por vez primera lo utiliz\u00F3 en 1848. En 1866, William Huggins reconoci\u00F3 su naturaleza de nebulosa gaseosa a partir de la observaci\u00F3n de su espectro.\u200B Se encuentra a una incierta distancia de 2600 a\u00F1os luz de la Tierra. M97 est\u00E1 considerada como una de las nebulosas planetarias m\u00E1s complejas. Su apariencia ha sido interpretada como una cubierta cil\u00EDndrica t\u00F3rica vista oblicuamente, de forma que los extremos del cilindro se asocian a zonas pobres en material expulsado, correspondiendo a los ojos del b\u00FAho. Esta cubierta se halla envuelta por una nebulosa m\u00E1s tenue y menos ionizada.\u200B La estrella central, de magnitud 16, tiene una masa aproximada de 0,7 masas solares, mientras que la masa de la propia nebulosa se estima en 0,15 masas solares. La nebulosa se form\u00F3 hace unos 6000 a\u00F1os."@es . "De Uilnevel (M97) is een planetaire nevel in het sterrenbeeld Grote Beer (Ursa Major). Het is een van de zwakste objecten uit de lijst van Charles Messier, die het opnam in 1781. De naam \"Uilnevel\" werd in 1848 gegeven door Lord Rosse, omdat hij door twee donkere vlekken wel wat weg heeft van de kop van een Uil. Zoals de meeste planetaire nevels zendt de Uilnevel zijn zichtbare licht voornamelijk in een enkele spectraallijn uit, 500,7 nm. De centrale ster van deze nevel is ongeveer 0,7 maal zo zwaar als onze zon en de nevel is 6000 jaar oud."@nl . . . . . . . "Mg\u0142awica Sowa (r\u00F3wnie\u017C Messier 97, M97 lub NGC 3587) \u2013 mg\u0142awica planetarna znajduj\u0105ca si\u0119 w gwiazdozbiorze Wielkiej Nied\u017Awiedzicy. Odkry\u0142 j\u0105 Pierre M\u00E9chain 16 lutego 1781 roku. M97 jest jedn\u0105 z bardziej z\u0142o\u017Conych mg\u0142awic planetarnych. Ma mas\u0119 oko\u0142o 0,15 masy S\u0142o\u0144ca, masa jej gwiazdy centralnej to ok. 0,7 masy S\u0142o\u0144ca. Jasno\u015B\u0107 tej gwiazdy wynosi 16m. Jasno\u015B\u0107 wizualna mg\u0142awicy to 9,9m, a jej fotograficzna jasno\u015B\u0107 wynosi 12m. System powsta\u0142 oko\u0142o 6000 lat temu."@pl . . "\u0422\u0443\u043C\u0430\u043D\u043D\u0456\u0441\u0442\u044C \u0421\u043E\u0432\u0430"@uk . "M97, NGC 3587, PN G148.4+57.0"@en . . "La nebulosa del B\u00FAho (tambi\u00E9n conocida como Messier 97 o NGC 3587) es una nebulosa planetaria ubicada en la constelaci\u00F3n de la Osa Mayor. Fue descubierta por Pierre M\u00E9chain en 1781. El nombre de Nebulosa del B\u00FAho fue acu\u00F1ado por Lord Rosse, quien por vez primera lo utiliz\u00F3 en 1848. En 1866, William Huggins reconoci\u00F3 su naturaleza de nebulosa gaseosa a partir de la observaci\u00F3n de su espectro.\u200B Se encuentra a una incierta distancia de 2600 a\u00F1os luz de la Tierra."@es . . . "Sov\u00ED mlhovina"@cs . "De Uilnevel (M97) is een planetaire nevel in het sterrenbeeld Grote Beer (Ursa Major). Het is een van de zwakste objecten uit de lijst van Charles Messier, die het opnam in 1781. De naam \"Uilnevel\" werd in 1848 gegeven door Lord Rosse, omdat hij door twee donkere vlekken wel wat weg heeft van de kop van een Uil. Zoals de meeste planetaire nevels zendt de Uilnevel zijn zichtbare licht voornamelijk in een enkele spectraallijn uit, 500,7 nm. De centrale ster van deze nevel is ongeveer 0,7 maal zo zwaar als onze zon en de nevel is 6000 jaar oud."@nl . . . . . . . . . . . . . "Nebula Burung Hantu"@in . "Nebulosa da Coruja"@pt . "The Owl Nebula (also known as Messier 97, M97 or NGC 3587) is a starburst (\"planetary\") nebula approximately 2,030 light years away in the northern constellation Ursa Major. The estimated age of the Owl Nebula is about 8,000 years. It is approximately circular in cross-section with faint internal structure. It was formed from the outflow of material from the stellar wind of the central star as it evolved along the asymptotic giant branch. The nebula is arranged in three concentric shells/envelopes, with the outermost shell being about 20\u201330% larger than the inner shell. A mildly owl-like appearance of the nebula is the result of an inner shell that is not circularly symmetric, but instead forms a barrel-like structure aligned at an angle of 45\u00B0 to the line of sight."@en . . . "1085477459"^^ . . . "\u0633\u062F\u064A\u0645 \u0627\u0644\u0628\u0648\u0645\u0629 \u0623\u0648 \u00AB\u0645\u0633\u064A\u064A\u0647 97\u00BB \u0623\u0648 \u00AB\u0625\u0646 \u062C\u064A \u0633\u064A 3587\u00BB \u0647\u0648 \u0639\u0628\u0627\u0631\u0629 \u0639\u0646 \u0633\u062F\u064A\u0645 \u0643\u0648\u0643\u0628\u064A \u064A\u0642\u0639 \u0641\u064A \u0643\u0648\u0643\u0628\u0629 \u0627\u0644\u062F\u0628 \u0627\u0644\u0623\u0643\u0628\u0631. \u0627\u0643\u062A\u0634\u0641\u0647 \u0627\u0644\u0641\u0644\u0643\u064A \u0628\u064A\u064A\u0631 \u0645\u064A\u0634\u0627\u0646 \u0641\u064A \u0639\u0627\u0645 1781\u0645. \u062A\u0628\u0644\u063A \u0643\u062A\u0644\u0629 \u0627\u0644\u0646\u062C\u0645 \u0627\u0644\u0648\u0627\u0642\u0639 \u0641\u064A \u0648\u0633\u0637 \u0627\u0644\u0633\u062F\u064A\u0645 0.7 \u0643\u062A\u0644\u0629 \u0634\u0645\u0633\u064A\u0629 \u0648\u0642\u062F\u0631\u0647 \u0627\u0644\u0638\u0627\u0647\u0631\u064A \u0647\u0648 16. \u0623\u0645\u0627 \u0627\u0644\u0633\u062F\u064A\u0645 \u0627\u0644\u0643\u0648\u0643\u0628\u064A \u0627\u0644\u0630\u064A \u064A\u062D\u064A\u0637 \u0628\u0647 (\u0648\u0647\u0648 \u0633\u062F\u064A\u0645 \u0627\u0644\u0628\u0648\u0645\u0629) \u0641\u0643\u062A\u0644\u062A\u0647 0.15 \u0643\u062A\u0644\u0629 \u0634\u0645\u0633\u064A\u0629 \u0648\u0642\u062F\u0631\u0647 \u0627\u0644\u0638\u0627\u0647\u0631\u064A 10 \u062A\u0642\u0631\u064A\u0628\u0627\u064B. \u064A\u0628\u0639\u062F \u0647\u0630\u0627 \u0627\u0644\u0633\u062F\u064A\u0645 2600 \u0633\u0646\u0629 \u0636\u0648\u0626\u064A\u0629 \u0639\u0646\u0627 \u0648\u0642\u062F \u062A\u0634\u0643\u0644 \u0642\u0628\u0644 6000 \u0633\u0646\u0629 \u062A\u0642\u0631\u064A\u0628\u0627\u064B \u0648\u0646\u0635\u0641 \u0642\u0637\u0631\u0647 \u064A\u0628\u0644\u063A 1.5 \u0633\u0646\u0629 \u0636\u0648\u0626\u064A\u0629. \u0648\u0642\u062F \u062C\u0627\u0621 \u0627\u0633\u0645 \u0627\u0644\u0633\u062F\u064A\u0645 \u0645\u0646 \u0623\u0646 \u0634\u0643\u0644\u0647 \u064A\u0634\u0628\u0647 \u0634\u0643\u0644 \u0639\u064A\u0646 \u0627\u0644\u0628\u0648\u0645\u0629."@ar . . . "\uC62C\uBE7C\uBBF8 \uC131\uC6B4(\uC601\uC5B4: Owl Nebula, M97, NGC 3587)\uC740 \uD070\uACF0\uC790\uB9AC\uC5D0 \uC788\uB294 \uD589\uC131\uC0C1 \uC131\uC6B4\uC774\uB2E4. \uAC70\uB9AC\uB294 2,600\uAD11\uB144\uC774\uBA70, \uB2E4\uC18C \uD070 \uD3B8\uC778 \uD589\uC131\uC0C1 \uC131\uC6B4\uC774\uC9C0\uB9CC, \uBC1D\uAE30\uAC00 +11.2\uC5D0 \uC548 \uB418\uC5B4\uC11C \uBC1C\uACAC\uD558\uAE30\uAC00 \uC27D\uC9C0 \uC54A\uB2E4. 2\uB4F1\uAE09\uC758 \uD070\uACF0\uC790\uB9AC \uBCA0\uD0C0(\u03B2) \uBCC4\uC5D0\uC11C \uB0A8\uB3D9\uCABD\uC73C\uB85C 2.4\u00B0 \uB5A8\uC5B4\uC838 \uC788\uB294 \uBD81\uB450\uCE60\uC131\uC758 \uAD6D\uC790 \uBAA8\uC591 \uBC11\uBC14\uB2E5\uC5D0 \uC790\uB9AC\uC7A1\uACE0 \uC788\uB294 \uC774 \uD589\uC131\uC0C1\uC131\uC6B4\uC740 1781\uB144 \uC774 \uBC1C\uACAC\uD588\uB2E4. \uD06C\uACE0 \uD76C\uBBF8\uD558\uC5EC \uBB18\uC0AC\uD558\uAE30\uAC00 \uC5B4\uB835\uACE0 \uBCF5\uC7A1\uD55C \uC774 \uC131\uC6B4\uC740, \uC704\uC5D0\uC11C \uB0B4\uB824\uB2E4\uBCF4\uC558\uC744 \uB54C \uBE44\uC2A4\uB4EC\uD55C \uC6D0\uD1B5 \uBAA8\uC591\uC758 \uC6D0\uD615\uCCB4\uCC98\uB7FC \uC0DD\uACBC\uB2E4. \uC774 \uB300\uC0C1\uC744 \uAD00\uCE21\uD558\uC600\uB358 \uD5C8\uC15C(1792~1871)\uC740 M97\uC744 \uBC00\uC9D1\uB41C \uC0B0\uAC1C \uC131\uB2E8\uC73C\uB85C \uC0DD\uAC01\uD588\uB2E4. \uADF8\uB7EC\uB098 \uD6D7\uB0A0 \uC601\uAD6D\uC758 \uB85C\uC2A4(1800~1867)\uAC00 \uC774 \uC131\uC6B4\uC758 \uBCF4\uC774\uB294 \uBAA8\uC2B5\uC774 \uC62C\uBE7C\uBBF8 \uC5BC\uAD74\uC744 \uB2EE\uC558\uB2E4 \uD558\uC5EC \uCC98\uC74C\uC73C\uB85C \uC62C\uBE7C\uBBF8\uC131\uC6B4\uC774\uB77C\uB294 \uC774\uB984\uC774 \uBD99\uC5C8\uB2E4. \uB300\uD615 \uB9DD\uC6D0\uACBD\uC73C\uB85C \uBCF4\uBA74 \uC131\uC6B4 \uAC00\uC6B4\uB370 \uBD80\uBD84\uC5D0 \uB450 \uAC1C\uC758 \uAD6C\uBA4D\uC774 \uBCF4\uC774\uB294\uB370 \uC774\uAC83\uC774 \uC62C\uBE7C\uBBF8\uC758 \uB208\uCC98\uB7FC \uBCF4\uC778\uB2E4. \uC774\uB7EC\uD55C \uC62C\uBE7C\uBBF8\uC758 \uB208\uC740 \uB35C \uC774\uC628\uD654\uB41C \uC131\uC6B4\uC758 \uAC00\uC2A4\uB85C \uB36E\uC5EC \uC788\uB294 \uAC83\uC774\uB2E4. \uC774 \uC131\uC6B4\uC758 \uC911\uC2EC\uBCC4\uC778 \uBC31\uC0C9 \uC65C\uC131\uC758 \uC9C8\uB7C9\uC740 \uD0DC\uC591\uC758 0.15\uBC30 \uC815\uB3C4\uB85C \uCE21\uC815\uB418\uC5C8\uACE0, \uBC1D\uAE30\uB294 +9.9\uB85C \uB2E4\uC18C \uC5B4\uB461\uB2E4. \uC131\uC6B4\uC758 \uC911\uC2EC\uC5D0\uB294 \uC774 \uC131\uC6B4\uC744 \uC0DD\uC131\uD55C +16.0\uB4F1\uC131\uC758 \uBC31\uC0C9 \uC65C\uC131\uC774 \uC788\uB294\uB370 \uC9C8\uB7C9\uC740 \uD0DC\uC591\uC758 0.7\uBC30 \uB418\uB294 \uAC83\uC73C\uB85C \uC54C\uB824\uC838 \uC788\uB2E4. \uC774\uB7EC\uD55C \uC810\uC73C\uB85C \uBBF8\uB8E8\uC5B4\uBCFC \uB54C \uD589\uC131\uC0C1\uC131\uC6B4\uC758 \uD2B9\uC131\uC0C1 \uC62C\uBE7C\uBBF8\uC131\uC6B4\uC740 \uB9D0\uAE30\uC5D0 \uC18D\uD55C\uB2E4. \uC774 \uC131\uC6B4\uC740 \uC57D 6,000\uB144 \uC804\uC5D0 \uC0DD\uC131\uB41C \uAC83\uC73C\uB85C \uCD94\uC815\uB41C\uB2E4. 1844\uB144 \uC70C\uB9AC\uC5C4 \uC2A4\uBBF8\uC2A4 \uC81C\uB3C5\uC774 \uCC98\uC74C\uC73C\uB85C \uC774 \uCC9C\uCCB4\uB97C \uD589\uC131\uC0C1\uC131\uC6B4\uC73C\uB85C \uBD84\uB958\uD558\uC600\uACE0, 1866\uB144 \uC70C\uB9AC\uC5C4 \uD734\uC9C4\uC2A4\uAC00 \uBD84\uAD11\uAD00\uCE21\uC744 \uD1B5\uD574 \uAC00\uC2A4\uC131\uC6B4\uC758 \uD2B9\uC131\uC744 \uD30C\uC545\uD558\uC600\uB2E4. M97\uC740 \uC57D 6,000\uB144 \uC804\uC5D0 \uD0DC\uC591\uAC19\uC740 \uBCC4\uC774 \uC8FD\uC740 \uAC83\uC774\uB2E4. M97\uC758 \uC911\uC2EC\uBCC4\uC758 \uD45C\uBA74\uC628\uB3C4\uB294 123,000 K\uC5D0 \uB2EC\uD558\uBA70, \uC9C8\uB7C9\uC740 0.5-0.6 \uD0DC\uC591 \uC9C8\uB7C9\uC774\uB2E4."@ko . "\u0422\u0443\u043C\u0430\u043D\u043D\u043E\u0441\u0442\u044C \u0421\u043E\u0432\u0430"@ru . . . . . . . . . "\u3075\u304F\u308D\u3046\u661F\u96F2\uFF08\u3075\u304F\u308D\u3046\u305B\u3044\u3046\u3093\u3001Owl Nebula \u3001M97\u3001NGC 3587\uFF09\u306F\u304A\u304A\u3050\u307E\u5EA7\u306B\u3042\u308B\u60D1\u661F\u72B6\u661F\u96F2\u3067\u3042\u308B\u3002"@ja . . . . "Hontzaren Nebulosa (Messier 97 edo NGC 3587 bezala ezaguna) Hartz Handia konstelazioan dagoen nebulosa da. aurkitu zuen 1781ean. Hontzaren Nebulosa izena Lord Rossek sortu zuen, lehen aldiz 1848an erabili zuena. 1866an, William Hugginsek bere nebulosa gaseosa izaera ezagutu zuen bere espektroa behatuz. Lurretik 2.600 argi urte ingurura dago. M97 nebulosa planetario konplexuenetako bat bezala hartzen da. Bere itxura, zeharka ikusitako estalki zilindriko toriko bezala interpretatu da, zilindroaren muturrak, kanporatutako materialetan txiroak diren guneekin lotzen direlarik, hontzaren begiei dagokiona. Estalki hau nebulosa ahulago eta ez hain ionizatu batez bildua dago. Erdiko izarrak, 16 magnitudekoa, 0,7 eguzki masako masa du, nebulosaren beraren masa 0,15 eguzki masatan estimatzen den bitartean. Nebulosa duela 6.000 urte sortu zen."@eu . . "Pri la aliaj signifoj de \"M97\" vidu artikolon M kun nombro. M97 (Messier 97, aliaj indikoj \u2014 NGC 3587, PK 148+57.1) estas planeduma nebulozo en konstelacio Granda Ursino. \u0108i tiu objekto estis jam en la originala versio de NGC-katalogo."@eo . . . . "Nebula Burung Hantu adalah nebula planet terletak sekitar 2.030 tahun cahaya di konstelasi Ursa Mayor. Nebula ini dikenal dengan pengidentifikasi katalog Messier Object 97 (M97) and NGC 3587. Ditemukan pertama kali oleh astronom Prancis Pierre M\u00E9chain pada 16 February 1781. Ketika mengamati nebula tersebut pada tahun 1848, gambar dari ilustrasi tangannya membentuk kepala burung hantu. Kemudian nebula ini mendapatkan julukan sebagai nebula burung hantu."@in . . . . . . "M97 (parfois appel\u00E9e n\u00E9buleuse du Hibou, ou NGC 3587) est une n\u00E9buleuse plan\u00E9taire situ\u00E9e \u00E0 une distance de 729 \u00B1 35 pc (\u223C2 380 a.l.) dans la constellation de la Grande Ourse. Elle s'\u00E9tend sur une distance d'environ 2,35 ann\u00E9es-lumi\u00E8re. Son \u00E2ge est estim\u00E9 \u00E0 6 000 ans. Elle a \u00E9t\u00E9 d\u00E9couverte par Pierre M\u00E9chain le 16 f\u00E9vrier 1781. La masse totale de la n\u00E9buleuse est d'environ 0,15 masse solaire, tandis que l'\u00E9toile centrale, une naine blanche, aurait une masse estim\u00E9e entre 0,55 et 0,6 masse solaire."@fr . . . . . . . . "\u3075\u304F\u308D\u3046\u661F\u96F2"@ja . . "Messier 97 (tamb\u00E9 coneguda com la Nebulosa del mussol, M97 o NGC 3587) \u00E9s una nebulosa planet\u00E0ria situada a la constel\u00B7laci\u00F3 de l'Ossa Major. Va ser descoberta per Pierre M\u00E9chain en 1781. li va donar el nom de Nebulosa del mussol el 1848. El 1866, William Huggins va recon\u00E8ixer la seva naturalesa de nebulosa gasosa a partir de l'observaci\u00F3 del seu espectre. Es troba a una dist\u00E0ncia aproximadament de 2600 anys llum de la Terra."@ca . . . "15485"^^ . . . . . "A Nebulosa da Coruja (tamb\u00E9m conhecida como Messier 97 ou NGC 3587) \u00E9 uma nebulosa planet\u00E1ria localizada na constela\u00E7\u00E3o de Ursa Major. Foi descoberta por Pierre M\u00E9chain em 1781. \u00C9 considerada uma das mais complexas nebulosas planet\u00E1rias. A estrela central de magnitude 16 tem cerca de 0,7 massas solares e a nebulosa em si cerca de 0,15 massas solares. A nebulosa foi formada apenas h\u00E1 cerca de 8000 anos."@pt . "\uC62C\uBE7C\uBBF8 \uC131\uC6B4"@ko . . . "M97"@eo . . . . . . "Nebula Burung Hantu adalah nebula planet terletak sekitar 2.030 tahun cahaya di konstelasi Ursa Mayor. Nebula ini dikenal dengan pengidentifikasi katalog Messier Object 97 (M97) and NGC 3587. Ditemukan pertama kali oleh astronom Prancis Pierre M\u00E9chain pada 16 February 1781. Ketika mengamati nebula tersebut pada tahun 1848, gambar dari ilustrasi tangannya membentuk kepala burung hantu. Kemudian nebula ini mendapatkan julukan sebagai nebula burung hantu. Usia nebula itu diperkirakan mencapai 8000 tahun. Ini berjarak sekitar melingkar di penampang melintang dengan struktur internal sedikit terlihat. Terbentuk dari material yang mengalir dari angin bintang yang berasal dari pusat bintang seraya berkembang di sepanjang cabang raksasa asimtotik. Nebula ini disusun dalam tiga cangkang konsentris, dengan kulit terluar sekitar 20-30% lebih besar dari kulit terdalam. Penampilan dari nebula yang seperti burung hantu itu hasil dari kulit terdalam yang tidak melingkar simetris, melainkan membentuk struktur seperti barrel yang selaras dengan sudut 45\u00B0 terhadap garis pengelihatan. Nebula tersebut menahan materi sekitar 0.13 kali massa matahari, termasuk hidrogen, helium, nitrogen, oksigen, dan belerang; dengan kerapatannya kurang dari 100 partikel per kubik sentimeter. Radius luarnya sekitar 0.91 tahun cahaya (0.28 parsek) dan mengembang dengan kecepatan 27-39 km/s ke dalam medium antarbintang sekitarnya. Besarnya 14 bintang pusat sejak telah mencapai titik balik evolusi akan memadat membentuk katai putih. memiliki sekira 55-60% massa matahari, 41-148 kali lebih cerah dibandingkan matahari, dan suhu efektif 123,000 K. Bintang ini sudah berhasil diselesaikan oleh Teleskop luar angkasa Spitzer sebagai sumber titik yang tidak menunjukkan selisih karakteristik inframerah dari disk melingkar."@in . . "Hontzaren Nebulosa (Messier 97 edo NGC 3587 bezala ezaguna) Hartz Handia konstelazioan dagoen nebulosa da. aurkitu zuen 1781ean. Hontzaren Nebulosa izena Lord Rossek sortu zuen, lehen aldiz 1848an erabili zuena. 1866an, William Hugginsek bere nebulosa gaseosa izaera ezagutu zuen bere espektroa behatuz. Lurretik 2.600 argi urte ingurura dago. Erdiko izarrak, 16 magnitudekoa, 0,7 eguzki masako masa du, nebulosaren beraren masa 0,15 eguzki masatan estimatzen den bitartean. Nebulosa duela 6.000 urte sortu zen."@eu . . "\u0633\u062F\u064A\u0645 \u0627\u0644\u0628\u0648\u0645\u0629"@ar . "\u3075\u304F\u308D\u3046\u661F\u96F2\uFF08\u3075\u304F\u308D\u3046\u305B\u3044\u3046\u3093\u3001Owl Nebula \u3001M97\u3001NGC 3587\uFF09\u306F\u304A\u304A\u3050\u307E\u5EA7\u306B\u3042\u308B\u60D1\u661F\u72B6\u661F\u96F2\u3067\u3042\u308B\u3002"@ja . "Nebulosa del Mussol"@ca . "\uC62C\uBE7C\uBBF8 \uC131\uC6B4(\uC601\uC5B4: Owl Nebula, M97, NGC 3587)\uC740 \uD070\uACF0\uC790\uB9AC\uC5D0 \uC788\uB294 \uD589\uC131\uC0C1 \uC131\uC6B4\uC774\uB2E4. \uAC70\uB9AC\uB294 2,600\uAD11\uB144\uC774\uBA70, \uB2E4\uC18C \uD070 \uD3B8\uC778 \uD589\uC131\uC0C1 \uC131\uC6B4\uC774\uC9C0\uB9CC, \uBC1D\uAE30\uAC00 +11.2\uC5D0 \uC548 \uB418\uC5B4\uC11C \uBC1C\uACAC\uD558\uAE30\uAC00 \uC27D\uC9C0 \uC54A\uB2E4. 2\uB4F1\uAE09\uC758 \uD070\uACF0\uC790\uB9AC \uBCA0\uD0C0(\u03B2) \uBCC4\uC5D0\uC11C \uB0A8\uB3D9\uCABD\uC73C\uB85C 2.4\u00B0 \uB5A8\uC5B4\uC838 \uC788\uB294 \uBD81\uB450\uCE60\uC131\uC758 \uAD6D\uC790 \uBAA8\uC591 \uBC11\uBC14\uB2E5\uC5D0 \uC790\uB9AC\uC7A1\uACE0 \uC788\uB294 \uC774 \uD589\uC131\uC0C1\uC131\uC6B4\uC740 1781\uB144 \uC774 \uBC1C\uACAC\uD588\uB2E4. \uD06C\uACE0 \uD76C\uBBF8\uD558\uC5EC \uBB18\uC0AC\uD558\uAE30\uAC00 \uC5B4\uB835\uACE0 \uBCF5\uC7A1\uD55C \uC774 \uC131\uC6B4\uC740, \uC704\uC5D0\uC11C \uB0B4\uB824\uB2E4\uBCF4\uC558\uC744 \uB54C \uBE44\uC2A4\uB4EC\uD55C \uC6D0\uD1B5 \uBAA8\uC591\uC758 \uC6D0\uD615\uCCB4\uCC98\uB7FC \uC0DD\uACBC\uB2E4. \uC774 \uB300\uC0C1\uC744 \uAD00\uCE21\uD558\uC600\uB358 \uD5C8\uC15C(1792~1871)\uC740 M97\uC744 \uBC00\uC9D1\uB41C \uC0B0\uAC1C \uC131\uB2E8\uC73C\uB85C \uC0DD\uAC01\uD588\uB2E4. 1844\uB144 \uC70C\uB9AC\uC5C4 \uC2A4\uBBF8\uC2A4 \uC81C\uB3C5\uC774 \uCC98\uC74C\uC73C\uB85C \uC774 \uCC9C\uCCB4\uB97C \uD589\uC131\uC0C1\uC131\uC6B4\uC73C\uB85C \uBD84\uB958\uD558\uC600\uACE0, 1866\uB144 \uC70C\uB9AC\uC5C4 \uD734\uC9C4\uC2A4\uAC00 \uBD84\uAD11\uAD00\uCE21\uC744 \uD1B5\uD574 \uAC00\uC2A4\uC131\uC6B4\uC758 \uD2B9\uC131\uC744 \uD30C\uC545\uD558\uC600\uB2E4. M97\uC740 \uC57D 6,000\uB144 \uC804\uC5D0 \uD0DC\uC591\uAC19\uC740 \uBCC4\uC774 \uC8FD\uC740 \uAC83\uC774\uB2E4. M97\uC758 \uC911\uC2EC\uBCC4\uC758 \uD45C\uBA74\uC628\uB3C4\uB294 123,000 K\uC5D0 \uB2EC\uD558\uBA70, \uC9C8\uB7C9\uC740 0.5-0.6 \uD0DC\uC591 \uC9C8\uB7C9\uC774\uB2E4."@ko . . "M97\uFF08\u540C\u6642\u540D\u70BA\u591C\u67AD\u661F\u4E91\u3001\u732B\u5934\u9E70\u661F\u4E91\u6216NGC3587\uFF09\uFF0C\u5B83\u7684\u540D\u5B57\u6765\u81EA\u4E8E\u5B83\u7684\u76D8\u4E0A\u7684\u4E24\u4E2A\u6697\u533A\u3002\u5B83\u662F\u4E00\u4E2A\u884C\u661F\u72B6\u661F\u4E91\uFF0C\u9762\u79EF\u4E3A3.4' x 3.3'\uFF0C\u4EAE\u5EA6\u4E3A+9.9\u7B49\uFF0C\u752812\u82F1\u5BF8\uFF0830\u5398\u7C73\uFF09\u671B\u8FDC\u955C\u53EF\u89C1\u3002 M97\u662F\u6CD5\u56FD\u5929\u6587\u5B66\u5BB6\u76AE\u57C3\u5C14\u00B7\u6885\u9999\uFF08Pierre M\u00E9chain\uFF091781\u5E74\u53D1\u73B0\u7684\u3002\u5B83\u662F\u4E00\u4E2A\u6BD4\u8F83\u590D\u6742\u7684\u884C\u661F\u72B6\u661F\u4E91\uFF0C\u5B83\u7684\u4E2D\u5FC3\u661F\u7EA616\u7B49\u4EAE\uFF0C\u5176\u8D28\u91CF\u4E3A\u592A\u9633\u76840.7\u500D\uFF0C\u661F\u4E91\u672C\u8EAB\u7EA6\u4E3A0.15\u592A\u9633\u8D28\u91CF\u3002\u5B83\u5927\u7EA6\u662F6000\u5E74\u524D\u5F62\u6210\u7684\u3002 M97\u4F4D\u4E8E\u5927\u718A\u5EA7\uFF0C\u5750\u6807\u4E3A\uFF1A \n* \u8D64\u7ECF\uFF1A11h14m48.00s \n* \u8D64\u7EAC\uFF1A+55\u00B001'00.0\""@zh . . . . . ""@en . . "Der Eulennebel (auch als Messier 97 oder NGC 3587 bezeichnet) ist einer der etwa 1600 planetarischen Nebel in unserer Milchstra\u00DFe. Mit den Abmessungen 3,4\u2032 \u00D7 3,3\u2032 und einer scheinbaren Helligkeit von 9,9 mag liegt er im Sternbild Gro\u00DFer B\u00E4r. Die vom Zentralstern ausgesto\u00DFene H\u00FClle hat etwa 2 Lichtjahre Durchmesser und dehnt sich mit etwa 40 km/s im Weltraum aus."@de . "Nebulosa del B\u00FAho"@es . "M97\uFF08\u540C\u6642\u540D\u70BA\u591C\u67AD\u661F\u4E91\u3001\u732B\u5934\u9E70\u661F\u4E91\u6216NGC3587\uFF09\uFF0C\u5B83\u7684\u540D\u5B57\u6765\u81EA\u4E8E\u5B83\u7684\u76D8\u4E0A\u7684\u4E24\u4E2A\u6697\u533A\u3002\u5B83\u662F\u4E00\u4E2A\u884C\u661F\u72B6\u661F\u4E91\uFF0C\u9762\u79EF\u4E3A3.4' x 3.3'\uFF0C\u4EAE\u5EA6\u4E3A+9.9\u7B49\uFF0C\u752812\u82F1\u5BF8\uFF0830\u5398\u7C73\uFF09\u671B\u8FDC\u955C\u53EF\u89C1\u3002 M97\u662F\u6CD5\u56FD\u5929\u6587\u5B66\u5BB6\u76AE\u57C3\u5C14\u00B7\u6885\u9999\uFF08Pierre M\u00E9chain\uFF091781\u5E74\u53D1\u73B0\u7684\u3002\u5B83\u662F\u4E00\u4E2A\u6BD4\u8F83\u590D\u6742\u7684\u884C\u661F\u72B6\u661F\u4E91\uFF0C\u5B83\u7684\u4E2D\u5FC3\u661F\u7EA616\u7B49\u4EAE\uFF0C\u5176\u8D28\u91CF\u4E3A\u592A\u9633\u76840.7\u500D\uFF0C\u661F\u4E91\u672C\u8EAB\u7EA6\u4E3A0.15\u592A\u9633\u8D28\u91CF\u3002\u5B83\u5927\u7EA6\u662F6000\u5E74\u524D\u5F62\u6210\u7684\u3002 M97\u4F4D\u4E8E\u5927\u718A\u5EA7\uFF0C\u5750\u6807\u4E3A\uFF1A \n* \u8D64\u7ECF\uFF1A11h14m48.00s \n* \u8D64\u7EAC\uFF1A+55\u00B001'00.0\""@zh . . . . "Sov\u00ED mlhovina (tak\u00E9 M 97 nebo NGC 3587) je planet\u00E1rn\u00ED mlhovina v souhv\u011Bzd\u00ED Velk\u00E9 medv\u011Bdice. Objevil ji Pierre M\u00E9chain 16. \u00FAnora 1781 a Sov\u00ED mlhovinou ji nazval Lord Rosse roku 1848."@cs . "Ugglenebulosan eller Messier 97 (M97) \u00E4ven k\u00E4nd som NGC 3587, \u00E4r en planetarisk nebulosa i stj\u00E4rnbilden Stora Bj\u00F6rnen p\u00E5 ett avst\u00E5nd av ca 2 030 ljus\u00E5r fr\u00E5n solsystemet. Ugglenebulosan \u00E4r klassificerad som en av de mer komplexa av de planetariska nebulosorna. Centralstj\u00E4rnan med en skenbar magnitud p\u00E5 16, har en massa av ca 0,7 solmassor och nebulosan sj\u00E4lv ca 0,15 solmassor. Nebulosan formades f\u00F6r ungef\u00E4r 8 000 \u00E5r sedan. Den har ungef\u00E4r cirkul\u00E4rt tv\u00E4rsnitt med svaga inre strukturer och bildades fr\u00E5n utfl\u00F6det av material fr\u00E5n den centrala stj\u00E4rnans stj\u00E4rnvind n\u00E4r den utvecklades l\u00E4ngs den asymptotiska j\u00E4ttegrenen."@sv . . "Der Eulennebel (auch als Messier 97 oder NGC 3587 bezeichnet) ist einer der etwa 1600 planetarischen Nebel in unserer Milchstra\u00DFe. Mit den Abmessungen 3,4\u2032 \u00D7 3,3\u2032 und einer scheinbaren Helligkeit von 9,9 mag liegt er im Sternbild Gro\u00DFer B\u00E4r. Die vom Zentralstern ausgesto\u00DFene H\u00FClle hat etwa 2 Lichtjahre Durchmesser und dehnt sich mit etwa 40 km/s im Weltraum aus."@de . "300"^^ . . "Hontzaren Nebulosa"@eu . . "3"^^ . . "\u0633\u062F\u064A\u0645 \u0627\u0644\u0628\u0648\u0645\u0629 \u0623\u0648 \u00AB\u0645\u0633\u064A\u064A\u0647 97\u00BB \u0623\u0648 \u00AB\u0625\u0646 \u062C\u064A \u0633\u064A 3587\u00BB \u0647\u0648 \u0639\u0628\u0627\u0631\u0629 \u0639\u0646 \u0633\u062F\u064A\u0645 \u0643\u0648\u0643\u0628\u064A \u064A\u0642\u0639 \u0641\u064A \u0643\u0648\u0643\u0628\u0629 \u0627\u0644\u062F\u0628 \u0627\u0644\u0623\u0643\u0628\u0631. \u0627\u0643\u062A\u0634\u0641\u0647 \u0627\u0644\u0641\u0644\u0643\u064A \u0628\u064A\u064A\u0631 \u0645\u064A\u0634\u0627\u0646 \u0641\u064A \u0639\u0627\u0645 1781\u0645. \u062A\u0628\u0644\u063A \u0643\u062A\u0644\u0629 \u0627\u0644\u0646\u062C\u0645 \u0627\u0644\u0648\u0627\u0642\u0639 \u0641\u064A \u0648\u0633\u0637 \u0627\u0644\u0633\u062F\u064A\u0645 0.7 \u0643\u062A\u0644\u0629 \u0634\u0645\u0633\u064A\u0629 \u0648\u0642\u062F\u0631\u0647 \u0627\u0644\u0638\u0627\u0647\u0631\u064A \u0647\u0648 16. \u0623\u0645\u0627 \u0627\u0644\u0633\u062F\u064A\u0645 \u0627\u0644\u0643\u0648\u0643\u0628\u064A \u0627\u0644\u0630\u064A \u064A\u062D\u064A\u0637 \u0628\u0647 (\u0648\u0647\u0648 \u0633\u062F\u064A\u0645 \u0627\u0644\u0628\u0648\u0645\u0629) \u0641\u0643\u062A\u0644\u062A\u0647 0.15 \u0643\u062A\u0644\u0629 \u0634\u0645\u0633\u064A\u0629 \u0648\u0642\u062F\u0631\u0647 \u0627\u0644\u0638\u0627\u0647\u0631\u064A 10 \u062A\u0642\u0631\u064A\u0628\u0627\u064B. \u064A\u0628\u0639\u062F \u0647\u0630\u0627 \u0627\u0644\u0633\u062F\u064A\u0645 2600 \u0633\u0646\u0629 \u0636\u0648\u0626\u064A\u0629 \u0639\u0646\u0627 \u0648\u0642\u062F \u062A\u0634\u0643\u0644 \u0642\u0628\u0644 6000 \u0633\u0646\u0629 \u062A\u0642\u0631\u064A\u0628\u0627\u064B \u0648\u0646\u0635\u0641 \u0642\u0637\u0631\u0647 \u064A\u0628\u0644\u063A 1.5 \u0633\u0646\u0629 \u0636\u0648\u0626\u064A\u0629. \u0648\u0642\u062F \u062C\u0627\u0621 \u0627\u0633\u0645 \u0627\u0644\u0633\u062F\u064A\u0645 \u0645\u0646 \u0623\u0646 \u0634\u0643\u0644\u0647 \u064A\u0634\u0628\u0647 \u0634\u0643\u0644 \u0639\u064A\u0646 \u0627\u0644\u0628\u0648\u0645\u0629."@ar . "Nebulosa Civetta"@it . . "Owl-like \"eyes\" visible through larger telescopes"@en . "\u03A4\u03BF \u039C\u03B5\u03C3\u03B9\u03AD 97 (\u03B3\u03BD\u03C9\u03C3\u03C4\u03CC \u03BA\u03B1\u03B9 \u03C9\u03C2 \u03BD\u03B5\u03C6\u03AD\u03BB\u03C9\u03BC\u03B1 \u039A\u03BF\u03C5\u03BA\u03BF\u03C5\u03B2\u03AC\u03B3\u03B9\u03B1 (Owl Nebula), \u039C97 \u03BA\u03B1\u03B9 NGC 3587) \u03B5\u03AF\u03BD\u03B1\u03B9 \u03C0\u03BB\u03B1\u03BD\u03B7\u03C4\u03B9\u03BA\u03CC \u03BD\u03B5\u03C6\u03AD\u03BB\u03C9\u03BC\u03B1 \u03C3\u03B5 \u03B1\u03C0\u03CC\u03C3\u03C4\u03B1\u03C3\u03B7 \u03C0\u03B5\u03C1\u03AF\u03C0\u03BF\u03C5 2.000 \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. \u0391\u03BD\u03B1\u03BA\u03B1\u03BB\u03CD\u03C6\u03B8\u03B7\u03BA\u03B5 \u03B1\u03C0\u03CC \u03C4\u03BF\u03BD \u03A0\u03B9\u03AD\u03C1 \u039C\u03B5\u03C3\u03B1\u03AF\u03BD \u03C4\u03BF 1781. \u03A3\u03C4\u03B7\u03BD \u03C0\u03B5\u03C1\u03B9\u03B3\u03C1\u03B1\u03C6\u03AE \u03C4\u03BF\u03C5 \u03B1\u03BD\u03B1\u03C6\u03AD\u03C1\u03B5\u03B9 \u03B5\u03C0\u03AF\u03C3\u03B7\u03C2 \u03C4\u03BF\u03C5\u03C2 \u039C\u03B5\u03C3\u03B9\u03AD 108 \u03BA\u03B1\u03B9 \u039C\u03B5\u03C3\u03B9\u03AD 109."@el . "\u0422\u0443\u043C\u0430\u0301\u043D\u043D\u043E\u0441\u0442\u044C \u0421\u043E\u0432\u0430\u0301 (\u0430\u043D\u0433\u043B. Messier 97, M 97, NGC 3587, \u0440\u0443\u0441. \u041C\u0435\u0441\u0441\u044C\u0435 97) \u2014 \u043F\u043B\u0430\u043D\u0435\u0442\u0430\u0440\u043D\u0430\u044F \u0442\u0443\u043C\u0430\u043D\u043D\u043E\u0441\u0442\u044C \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. \u041E\u0442\u043A\u0440\u044B\u0442\u0430 \u041F\u044C\u0435\u0440\u043E\u043C \u041C\u0435\u0448\u0435\u043D\u043E\u043C \u0432 1781 \u0433\u043E\u0434\u0443. \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. \u0426\u0435\u043D\u0442\u0440\u0430\u043B\u044C\u043D\u0430\u044F \u0437\u0432\u0435\u0437\u0434\u0430 \u0442\u0443\u043C\u0430\u043D\u043D\u043E\u0441\u0442\u0438 16-\u0439 \u0437\u0432\u0451\u0437\u0434\u043D\u043E\u0439 \u0432\u0435\u043B\u0438\u0447\u0438\u043D\u044B \u0438\u043C\u0435\u0435\u0442 \u043C\u0430\u0441\u0441\u0443, \u0440\u0430\u0432\u043D\u0443\u044E 0,7 \u043C\u0430\u0441\u0441\u044B \u0421\u043E\u043B\u043D\u0446\u0430, \u0430 \u043C\u0430\u0441\u0441\u0430 \u043E\u0441\u0442\u0430\u043B\u044C\u043D\u043E\u0439 \u0447\u0430\u0441\u0442\u0438 \u0442\u0443\u043C\u0430\u043D\u043D\u043E\u0441\u0442\u0438 \u0441\u043E\u0441\u0442\u0430\u0432\u043B\u044F\u0435\u0442 0,15 \u0441\u043E\u043B\u043D\u0435\u0447\u043D\u043E\u0439 \u043C\u0430\u0441\u0441\u044B. \u0422\u0443\u043C\u0430\u043D\u043D\u043E\u0441\u0442\u044C \u0440\u0430\u0441\u043F\u043E\u043B\u043E\u0436\u0435\u043D\u0430 \u043D\u0430 \u0440\u0430\u0441\u0441\u0442\u043E\u044F\u043D\u0438\u0438 \u043F\u0440\u0438\u043C\u0435\u0440\u043D\u043E 621 \u043F\u043A (\u043E\u043A\u043E\u043B\u043E 2025 \u0441\u0432\u0435\u0442\u043E\u0432\u044B\u0445 \u043B\u0435\u0442) \u043E\u0442 \u0421\u043E\u043B\u043D\u0435\u0447\u043D\u043E\u0439 \u0441\u0438\u0441\u0442\u0435\u043C\u044B \u0438 \u043E\u0431\u0440\u0430\u0437\u043E\u0432\u0430\u043B\u0430\u0441\u044C \u043F\u0440\u0438\u043C\u0435\u0440\u043D\u043E 6000 \u043B\u0435\u0442 \u043D\u0430\u0437\u0430\u0434. \u041D\u0430\u0437\u0432\u0430\u043D\u0438\u0435 \u0442\u0443\u043C\u0430\u043D\u043D\u043E\u0441\u0442\u0438 \u0434\u0430\u043D\u043E \u043B\u043E\u0440\u0434\u043E\u043C \u0420\u043E\u0441\u0441\u043E\u043C \u0432 1848 \u0433\u043E\u0434\u0443 \u0438\u0437-\u0437\u0430 \u0441\u0445\u043E\u0434\u0441\u0442\u0432\u0430 \u0434\u0432\u0443\u0445 \u0442\u0451\u043C\u043D\u044B\u0445 \u043F\u044F\u0442\u0435\u043D \u0441 \u0433\u043B\u0430\u0437\u0430\u043C\u0438 \u0441\u043E\u0432\u044B. \u0427\u0442\u043E\u0431\u044B \u043F\u043E\u0434\u0447\u0435\u0440\u043A\u043D\u0443\u0442\u044C \u044D\u0442\u043E \u0441\u0445\u043E\u0434\u0441\u0442\u0432\u043E, \u043E\u043D \u0441\u0434\u0435\u043B\u0430\u043B \u0440\u0438\u0441\u0443\u043D\u043E\u043A."@ru . . . . . "\u0422\u0443\u043C\u0430\u043D\u043D\u0456\u0441\u0442\u044C \u0421\u043E\u0432\u0430 (M97, NGC 3587) \u2014 \u043F\u043B\u0430\u043D\u0435\u0442\u0430\u0440\u043D\u0430 \u0442\u0443\u043C\u0430\u043D\u043D\u0456\u0441\u0442\u044C \u0442\u0438\u043F\u0443 PN \u0443 \u0441\u0443\u0437\u0456\u0440'\u0457 \u0412\u0435\u043B\u0438\u043A\u0430 \u0412\u0435\u0434\u043C\u0435\u0434\u0438\u0446\u044F.\u0412\u0456\u0434\u043A\u0440\u0438\u0432\u0430\u0447\u0435\u043C \u0446\u044C\u043E\u0433\u043E \u043E\u0431'\u0454\u043A\u0442\u0430 \u0454 \u041C\u0435\u0448\u0430\u043D \u041F'\u0454\u0440 \u0424\u0440\u0430\u043D\u0441\u0443\u0430 \u0410\u043D\u0434\u0440\u0435, \u044F\u043A\u0438\u0439 \u0432\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 16 \u043B\u044E\u0442\u043E\u0433\u043E 1781.\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 (NGC)."@uk . . . "Planetary"@en . . . . . . . . . . "Messier 97, Owl Nebula"@en . . "M97 (parfois appel\u00E9e n\u00E9buleuse du Hibou, ou NGC 3587) est une n\u00E9buleuse plan\u00E9taire situ\u00E9e \u00E0 une distance de 729 \u00B1 35 pc (\u223C2 380 a.l.) dans la constellation de la Grande Ourse. Elle s'\u00E9tend sur une distance d'environ 2,35 ann\u00E9es-lumi\u00E8re. Son \u00E2ge est estim\u00E9 \u00E0 6 000 ans. Elle a \u00E9t\u00E9 d\u00E9couverte par Pierre M\u00E9chain le 16 f\u00E9vrier 1781. La masse totale de la n\u00E9buleuse est d'environ 0,15 masse solaire, tandis que l'\u00E9toile centrale, une naine blanche, aurait une masse estim\u00E9e entre 0,55 et 0,6 masse solaire. La n\u00E9buleuse dans son ensemble aurait une forme de \u00AB tore cylindrique \u00BB (un peu comme un globe auquel on aurait retir\u00E9 les p\u00F4les) qui serait vue depuis la Terre de fa\u00E7on oblique. Ainsi, les deux \u00AB trous \u00BB des extr\u00E9mit\u00E9s, qui sont en fait des r\u00E9gions beaucoup plus pauvres en mati\u00E8re, formeraient les \u00AB yeux \u00BB du hibou, par transparence."@fr . . . "\u039C\u03B5\u03C3\u03B9\u03AD 97"@el . "\u03A4\u03BF \u039C\u03B5\u03C3\u03B9\u03AD 97 (\u03B3\u03BD\u03C9\u03C3\u03C4\u03CC \u03BA\u03B1\u03B9 \u03C9\u03C2 \u03BD\u03B5\u03C6\u03AD\u03BB\u03C9\u03BC\u03B1 \u039A\u03BF\u03C5\u03BA\u03BF\u03C5\u03B2\u03AC\u03B3\u03B9\u03B1 (Owl Nebula), \u039C97 \u03BA\u03B1\u03B9 NGC 3587) \u03B5\u03AF\u03BD\u03B1\u03B9 \u03C0\u03BB\u03B1\u03BD\u03B7\u03C4\u03B9\u03BA\u03CC \u03BD\u03B5\u03C6\u03AD\u03BB\u03C9\u03BC\u03B1 \u03C3\u03B5 \u03B1\u03C0\u03CC\u03C3\u03C4\u03B1\u03C3\u03B7 \u03C0\u03B5\u03C1\u03AF\u03C0\u03BF\u03C5 2.000 \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. \u0391\u03BD\u03B1\u03BA\u03B1\u03BB\u03CD\u03C6\u03B8\u03B7\u03BA\u03B5 \u03B1\u03C0\u03CC \u03C4\u03BF\u03BD \u03A0\u03B9\u03AD\u03C1 \u039C\u03B5\u03C3\u03B1\u03AF\u03BD \u03C4\u03BF 1781. \u03A3\u03C4\u03B7\u03BD \u03C0\u03B5\u03C1\u03B9\u03B3\u03C1\u03B1\u03C6\u03AE \u03C4\u03BF\u03C5 \u03B1\u03BD\u03B1\u03C6\u03AD\u03C1\u03B5\u03B9 \u03B5\u03C0\u03AF\u03C3\u03B7\u03C2 \u03C4\u03BF\u03C5\u03C2 \u039C\u03B5\u03C3\u03B9\u03AD 108 \u03BA\u03B1\u03B9 \u039C\u03B5\u03C3\u03B9\u03AD 109."@el . . . . . "Pri la aliaj signifoj de \"M97\" vidu artikolon M kun nombro. M97 (Messier 97, aliaj indikoj \u2014 NGC 3587, PK 148+57.1) estas planeduma nebulozo en konstelacio Granda Ursino. \u0108i tiu objekto estis jam en la originala versio de NGC-katalogo."@eo . . . . . . . "La nebulosa Civetta (nota anche come Nebulosa Gufo o con le sigle M 97 o NGC 3587) \u00E8 una nebulosa planetaria visibile nella costellazione dell'Orsa Maggiore; \u00E8 stata scoperta da Pierre M\u00E9chain nel 1781. Il nome \"Nebulosa Gufo\" \u00E8 stato invece assegnato da William Parsons nel 1848 a causa delle due macchie scure, che assomigliano agli occhi di un gufo. M97 \u00E8 una delle nebulose planetarie pi\u00F9 complesse. Il suo aspetto \u00E8 stato interpretato come una sfera senza poli, con gli occhi del gufo in corrispondenza delle zone povere di materia ai poli. La sua et\u00E0 \u00E8 stimata in 6.000 anni."@it . . . "M97"@zh . . . "Mg\u0142awica Sowa"@pl . . . "Eulennebel"@de . "Messier 97 (tamb\u00E9 coneguda com la Nebulosa del mussol, M97 o NGC 3587) \u00E9s una nebulosa planet\u00E0ria situada a la constel\u00B7laci\u00F3 de l'Ossa Major. Va ser descoberta per Pierre M\u00E9chain en 1781. li va donar el nom de Nebulosa del mussol el 1848. El 1866, William Huggins va recon\u00E8ixer la seva naturalesa de nebulosa gasosa a partir de l'observaci\u00F3 del seu espectre. Es troba a una dist\u00E0ncia aproximadament de 2600 anys llum de la Terra. M97 \u00E9s considerada com una de les nebuloses planet\u00E0ries m\u00E9s complexes. La seva aparen\u00E7a ha estat interpretada com una coberta t\u00F2rica vista obliquament (\u00E9s a dir, com una esfera sense els pols), de manera que els extrems del cilindre es corresponen a zones pobres en material expulsat, la zona corresponent als ulls del mussol. Aquesta coberta es troba embolicada per una nebulosa m\u00E9s t\u00E8nue i menys ionitzada. L'estrella central, de magnitud 16, t\u00E9 una massa aproximada de 0,7 masses solars, mentre que la massa de la mateixa nebulosa s'estima en 0,15 masses solars. La nebulosa es va formar fa uns 6000 anys."@ca . . "Uilnevel"@nl . . "M97 (n\u00E9buleuse plan\u00E9taire)"@fr . "Ugglenebulosan"@sv . . . "The Owl Nebula (also known as Messier 97, M97 or NGC 3587) is a starburst (\"planetary\") nebula approximately 2,030 light years away in the northern constellation Ursa Major. The estimated age of the Owl Nebula is about 8,000 years. It is approximately circular in cross-section with faint internal structure. It was formed from the outflow of material from the stellar wind of the central star as it evolved along the asymptotic giant branch. The nebula is arranged in three concentric shells/envelopes, with the outermost shell being about 20\u201330% larger than the inner shell. A mildly owl-like appearance of the nebula is the result of an inner shell that is not circularly symmetric, but instead forms a barrel-like structure aligned at an angle of 45\u00B0 to the line of sight. The nebula holds about 0.13 solar masses (M\u2609) of matter, including hydrogen, helium, nitrogen, oxygen, and sulfur; all with a density of less than 100 particles per cubic centimeter. Its outer radius is around 0.91 ly (0.28 pc) and it is expanding with velocities in the range of 27\u201339 km/s into the surrounding interstellar medium. The 14th magnitude central star has passed an apex of its evolution so is condensing to form a white dwarf. It has 55% to 60% of solar mass, is 41 to 148 times solar luminosity (L\u2609), and has an effective temperature of 123,000 K. The star has been successfully resolved by the Spitzer Space Telescope as a point source that does not show the infrared excess characteristic of a circumstellar disk."@en . . "974931"^^ . . .