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dbr:Theoretical_astronomy	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
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dbr:David_Dunlap_Observatory_Catalogue	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Dwarf_elliptical_galaxy	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Dark_galaxy	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:High-velocity_cloud	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Beta_Andromedae	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:List_of_largest_nebulae	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Intergalactic_star	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Intergalactic_travel	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:SN_1885A	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
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dbr:Eridanus_II	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Anemic_galaxy	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:PA-99-N2	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:History_of_supernova_observation	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Kamil_Hornoch	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
<http://dbpedia.org/resource/Nicholas_U._Mayall_Telescope>	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Multiwavelength_Atlas_of_Galaxies	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Sufi_Observing_Competition	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Universal_Natural_History_and_Theory_of_the_Heavens	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Supernova_neutrinos	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:NGC_1232	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:NGC_147	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:NGC_185	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy ;
	dbp:notes	dbr:Andromeda_Galaxy .
dbr:NGC_4216	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:NGC_4527	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:NGC_4565	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:NGC_5204	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:NGC_6822	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:NGC_891	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Andromeda_II	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Andromeda_III	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
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dbr:Aquarius_Dwarf	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Maffei_1	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Tucana_Dwarf	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:IC_342	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Messier_110	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Messier_32	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy ;
	dbp:notes	dbr:Andromeda_Galaxy .
dbr:Messier_90	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:List_of_The_Ultraman_characters	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:NGC_3109	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
<http://dbpedia.org/resource/12621_Alsufi>	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:S_Doradus	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
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dbr:Islamic_Golden_Age	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Abd_al-Rahman_al-Sufi	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:List_of_Doctor_Who_universe_creatures_and_aliens	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:May_1923	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Schwarzschild_radius	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:List_of_alien_races_in_DC_Comics	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:List_of_black_holes	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:List_of_fictional_spacecraft	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:List_of_largest_known_stars	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Pegasus_Dwarf_Spheroidal_Galaxy	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:List_of_adjectivals_and_demonyms_of_astronomical_bodies	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Timeline_of_cosmological_theories	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Comet_Holmes	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Mu_Andromedae	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:NGC_206	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:The_Urantia_Book	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
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dbr:Whole_Earth_Catalog	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Isaac_Roberts	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Local_Volume	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:The_Relativity_of_Wrong	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
<http://dbpedia.org/resource/51_Andromedae>	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Ancient_astronauts_in_popular_culture	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Nu_Andromedae	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Dire_Wraith	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:History_of_the_center_of_the_Universe	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Astronomical_naming_conventions	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Space_Cases	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Messier_106	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
<http://dbpedia.org/resource/Once_Upon_a_Time..._Space>	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:The_Galactus_Trilogy	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:List_of_brightest_natural_objects_in_the_sky	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
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@prefix wikipedia-en:	<http://en.wikipedia.org/wiki/> .
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dbr:Jodrell_Bank_Observatory	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Death_Valley_National_Park	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Skrull	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Formation_and_evolution_of_the_Solar_System	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Galactic_tide	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Galactic_year	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Galactic_Center	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
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dbr:Timeline_of_the_far_future	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Universe_Sandbox	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Lloigor	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Xandar	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy ;
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dbr:NGC_7418	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
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dbr:Giovanni_Sostero	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:V1	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
<http://dbpedia.org/resource/Fourteen_(manga)>	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:AE_Andromedae	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
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dbr:Star	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
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dbr:Cosmic_distance_ladder	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Location_of_Earth	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
<http://dbpedia.org/resource/Symbiote_(comics)>	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:World_egg	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
<http://dbpedia.org/resource/Hubble_(film)>	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Cassiopeia_Dwarf	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
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dbr:Future_of_an_expanding_universe	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:House_of_Suns	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:The_Andromeda_Galaxy	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy ;
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dbr:Stellar_kinematics	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
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dbr:Stellar_halo	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Andromeda_Shun	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:List_of_Mass_Effect_characters	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Phantasy_Star_II	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
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dbr:Vatican_Advanced_Technology_Telescope	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
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dbr:Parsec	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
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dbr:List_of_galaxies	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:List_of_the_most_distant_astronomical_objects	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
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dbr:Robert_Hanbury_Brown	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Martin_Mobberley	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Galaxy_Express_999	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
<http://dbpedia.org/resource/Galaxy_Express_999_(film)>	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:War_of_the_Satellites	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:The_First_Three_Minutes	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
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dbr:Lemuel_Roscoe_Cleveland	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:A_for_Andromeda	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
<http://dbpedia.org/resource/Renkin_3-ky\u016B_Magical%3F_Pok\u0101n>	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
<http://dbpedia.org/resource/Characters_of_Blake\u0027s_7>	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Indradhanush	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Henrietta_Hill_Swope	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Titanic_Rising	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
<http://dbpedia.org/resource/Face_Off_(season_8)>	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
<http://dbpedia.org/resource/Red_Rock_Canyon_State_Park_(California)>	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
<http://dbpedia.org/resource/War_of_the_Planets_(1966_film)>	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
<http://dbpedia.org/resource/Fata_Morgana_(1971_film)>	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
<http://dbpedia.org/resource/Ice_Planet_(film)>	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:SkyWeek	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:When_Knowledge_Conquered_Fear	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
<http://dbpedia.org/resource/Geraint_F._Lewis>	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
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<http://dbpedia.org/resource/John_E._Baldwin>	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
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dbr:Great_Andromeda_Nebula	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy ;
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dbr:Pan-Andromeda_Archaeological_Survey	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Mass_Effect	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Galaxy	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Black_hole	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Emil_Artin	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
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dbr:H_II_region	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
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<http://dbpedia.org/resource/Cassiopeia_(constellation)>	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
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dbr:Dark_matter	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:List_of_nearest_galaxies	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Redshift	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
<http://dbpedia.org/resource/Nicholas_U._Mayall>	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
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dbr:Omega_Centauri	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Andromeda_IX	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy ;
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dbr:Large_Magellanic_Cloud	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
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dbr:NGC_2841	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Antennae_Galaxies	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:List_of_largest_galaxies	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Cepheid_variable	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
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@prefix wikidata:	<http://www.wikidata.org/entity/> .
dbr:Andromeda_Galaxy	rdf:type	wikidata:Q318 ,
		yago:PhysicalEntity100001930 ,
		yago:WikicatNGCObjects ,
		yago:WikicatMessierObjects ,
		dbo:CelestialBody ,
		yago:Collection107951464 ,
		dbo:Place ,
		dbo:Location .
@prefix rdfs:	<http://www.w3.org/2000/01/rdf-schema#> .
dbr:Andromeda_Galaxy	rdfs:label	"Gal\u00E1xia de Andr\u00F4meda"@pt ,
		"\u30A2\u30F3\u30C9\u30ED\u30E1\u30C0\u9280\u6CB3"@ja ,
		"Galaxie d'Androm\u00E8de"@fr ,
		"\u0627\u0644\u0645\u0631\u0623\u0629 \u0627\u0644\u0645\u0633\u0644\u0633\u0644\u0629 (\u0645\u062C\u0631\u0629)"@ar ,
		"Galaksi Andromeda"@in ,
		"Andromedagalaxen"@sv ,
		"\uC548\uB4DC\uB85C\uBA54\uB2E4 \uC740\uD558"@ko ,
		"Andromedagalaxie"@de ,
		"Andromedanevel"@nl ,
		"Andromeda galaksio"@eo ,
		"Galaxia de Andr\u00F3meda"@es ,
		"Galaktyka Andromedy"@pl ,
		"\u4ED9\u5973\u5EA7\u661F\u7CFB"@zh ,
		"Andromeda Galaxy"@en ,
		"\u0413\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u0430 \u0410\u043D\u0434\u0440\u043E\u043C\u0435\u0434\u044B"@ru ,
		"Galaxie v Andromed\u011B"@cs ,
		"R\u00E9altra Andraim\u00E9ide"@ga ,
		"Gal\u00E0xia d'Andr\u00F2meda"@ca ,
		"\u0393\u03B1\u03BB\u03B1\u03BE\u03AF\u03B1\u03C2 \u03C4\u03B7\u03C2 \u0391\u03BD\u03B4\u03C1\u03BF\u03BC\u03AD\u03B4\u03B1\u03C2"@el ,
		"\u0413\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u0430 \u0410\u043D\u0434\u0440\u043E\u043C\u0435\u0434\u0438"@uk ,
		"Galassia di Andromeda"@it ,
		"Andromeda galaxia"@eu ;
	rdfs:comment	"La Andromeda Galaksio (M31, Messier 31, aliaj indikoj \u2014 NGC 224, PGC 2557, UGC 454, MCG 7-2-16, ZWG 535.17) estas galaksio en konstelacio Andromedo, la\u016D kiu \u011Di estis nomita. En la astronomia katalogo de Messier \u011Di havas la nomon \"M31\".\u0108i tiu objekto estis jam en la originala versio de NGC-katalogo. \u011Ci situas \u0109irka\u016D 2,52 milionoj da lumjaroj for de ni kaj estas la plej malproksima objekto videbla nudokule de sur Tero. NGC 206 estas parto de Andromeda galaksio."@eo ,
		"\uC548\uB4DC\uB85C\uBA54\uB2E4 \uC740\uD558(\uC601\uC5B4: Andromeda Galaxy)\uB294 \uC9C0\uAD6C\uB85C\uBD80\uD130 \uC57D 780 \uD0AC\uB85C\uD30C\uC139(250\uB9CC \uAD11\uB144) \uB5A8\uC5B4\uC838 \uC788\uB294 \uB098\uC120\uC740\uD558\uC774\uB2E4. \uC774\uB294 \uC6B0\uB9AC\uC740\uD558\uB85C\uBD80\uD130 \uAC00\uC7A5 \uAC00\uAE4C\uC6B4 \uD070 \uC740\uD558(major galaxy)\uC774\uBA70, \uBA54\uC2DC\uC5D0 31(M31) \uB610\uB294 NGC 224\uB85C \uC54C\uB824\uC838 \uC788\uAE30\uB3C4 \uD558\uB2E4. \uC61B \uBB38\uD5CC\uC5D0\uC11C\uB294 \uC885\uC885 \uC548\uB4DC\uB85C\uBA54\uB2E4\uC790\uB9AC \uB300\uC131\uC6B4(Andromeda\u5927\u661F\u96F2)\uC73C\uB85C \uD45C\uD604\uB418\uC5C8\uB2E4. \uC740\uD558\uC758 \uBA85\uCE6D\uC740 \uC740\uD558\uAC00 \uBCF4\uC774\uB294 \uBCC4\uC790\uB9AC, \uC989 \uC548\uB4DC\uB85C\uBA54\uB2E4\uC790\uB9AC\uC758 \uBA85\uCE6D\uC744 \uB530\uC11C \uBD99\uC5EC\uC84C\uB2E4. \uC5EC\uAE30\uC11C \uC548\uB4DC\uB85C\uBA54\uB2E4\uC790\uB9AC\uB294 \uADF8\uB9AC\uC2A4 \uC2E0\uD654\uC758 \uC548\uB4DC\uB85C\uBA54\uB2E4 \uACF5\uC8FC\uC758 \uC774\uB984\uC744 \uB530 \uBD99\uC5EC\uC9C4 \uBCC4\uC790\uB9AC\uC774\uB2E4. \uD3ED\uC774 \uB300\uB7B5 22\uB9CC \uAD11\uB144\uC778 \uC548\uB4DC\uB85C\uBA54\uB2E4 \uC740\uD558\uB294 \uC6B0\uB9AC \uC740\uD558 \uBC0F \uC0BC\uAC01\uD615\uC790\uB9AC \uC740\uD558\uC640 \uB300\uB7B5 44\uAC1C\uC758 \uC791\uC740 \uC740\uD558\uB4E4\uC744 \uD3EC\uD568\uD558\uB294 \uAD6D\uBD80\uC740\uD558\uAD70\uC5D0\uC11C \uAC00\uC7A5 \uD070 \uC740\uD558\uC774\uB2E4. \uCD08\uAE30\uC758 \uD0D0\uC0AC\uB4E4\uC740 \uC6B0\uB9AC\uC740\uD558\uAC00 \uB354 \uB9CE\uC740 \uC554\uD751\uBB3C\uC9C8\uC744 \uD3EC\uD568\uD558\uBA70 \uAD6D\uBD80\uC740\uD558\uAD70\uC5D0\uC11C \uAC00\uC7A5 \uD074 \uAC83\uC774\uB77C\uACE0 \uC2DC\uC0AC\uD558\uC600\uC9C0\uB9CC, 2006\uB144 \uC2A4\uD53C\uCC98 \uC6B0\uC8FC \uB9DD\uC6D0\uACBD\uC744 \uD1B5\uD55C \uAD00\uCE21\uB4E4\uC740 \uC548\uB4DC\uB85C\uBA54\uB2E4 \uC740\uD558\uAC00 2,000~4,000\uC5B5 \uAC1C\uC758 \uBCC4\uB4E4\uC744 \uD3EC\uD568\uD560 \uAC83\uC73C\uB85C \uCD94\uC815\uB418\uB294 \uC6B0\uB9AC\uC740\uD558\uC758 \uC801\uC5B4\uB3C4 \uB450 \uBC30\uC5D0 \uD574\uB2F9\uD558\uB294, 1\uC870 \uAC1C\uC758 \uBCC4\uB4E4\uC744 \uD3EC\uD568\uD558\uB294 \uAC83\uC744 \uBCF4\uC5EC\uC8FC\uC5C8\uB2E4."@ko ,
		"Galaksi Andromeda (nama lain, Messier 31 dan NGC 224) adalah sebuah galaksi spiral yang berjarak kira-kira 2,5 juta tahun cahaya dari bumi. Galaksi ini merupakan salah satu galaksi di luar galaksi Bima Sakti yang dapat dilihat dengan mata telanjang pada malam yang cerah, tanpa bulan, dan tanpa polusi cahaya. Strukturnya mirip dengan galaksi Bima Sakti yaitu berbentuk spiral. Jaraknya sekitar 2,5 juta tahun cahaya. Letaknya di langit adalah di belahan langit utara, sekitar 41 derajat di sebelah utara khatulistiwa langit. Galaksi ini dapat diamati di bulan September, Oktober, dan November."@in ,
		"\u039F \u0393\u03B1\u03BB\u03B1\u03BE\u03AF\u03B1\u03C2 \u03C4\u03B7\u03C2 \u0391\u03BD\u03B4\u03C1\u03BF\u03BC\u03AD\u03B4\u03B1\u03C2 (\u03B3\u03BD\u03C9\u03C3\u03C4\u03CC\u03C2 \u03BA\u03B1\u03B9 \u03C9\u03C2 \u039C\u03B5\u03C3\u03B9\u03AD 31) \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\u03C4\u03BF\u03BD \u03B1\u03C3\u03C4\u03B5\u03C1\u03B9\u03C3\u03BC\u03CC \u0391\u03BD\u03B4\u03C1\u03BF\u03BC\u03AD\u03B4\u03B1, \u03C3\u03C4\u03BF\u03BD \u03BF\u03C0\u03BF\u03AF\u03BF \u03BF\u03C6\u03B5\u03AF\u03BB\u03B5\u03B9 \u03BA\u03B1\u03B9 \u03C4\u03BF \u03CC\u03BD\u03BF\u03BC\u03AC \u03C4\u03BF\u03C5. \u039A\u03B1\u03C4\u03AD\u03C7\u03B5\u03B9 \u03AD\u03BD\u03B1 \u03B1\u03BE\u03B9\u03BF\u03C3\u03B7\u03BC\u03B5\u03AF\u03C9\u03C4\u03BF \u03C1\u03B5\u03BA\u03CC\u03C1: \u03B5\u03AF\u03BD\u03B1\u03B9 \u03C4\u03BF \u03C0\u03B9\u03BF \u03B1\u03C0\u03BF\u03BC\u03B1\u03BA\u03C1\u03C5\u03C3\u03BC\u03AD\u03BD\u03BF \u03B1\u03BD\u03C4\u03B9\u03BA\u03B5\u03AF\u03BC\u03B5\u03BD\u03BF \u03B5\u03CD\u03BA\u03BF\u03BB\u03B1 \u03BF\u03C1\u03B1\u03C4\u03CC \u03BC\u03B5 \u03B3\u03C5\u03BC\u03BD\u03CC \u03BC\u03AC\u03C4\u03B9. \u0392\u03C1\u03AF\u03C3\u03BA\u03B5\u03C4\u03B1\u03B9 \u03C3\u03B5 \u03B1\u03C0\u03CC\u03C3\u03C4\u03B1\u03C3\u03B7 \u03BC\u03CC\u03BB\u03B9\u03C2 2,5 \u03B5\u03BA\u03B1\u03C4\u03BF\u03BC\u03BC\u03C5\u03C1\u03AF\u03C9\u03BD \u03B5\u03C4\u03CE\u03BD \u03C6\u03C9\u03C4\u03CC\u03C2 \u03BA\u03B1\u03B9 \u03BC\u03B1\u03B6\u03AF \u03BC\u03B5 \u03C4\u03BF\u03BD \u0393\u03B1\u03BB\u03B1\u03BE\u03AF\u03B1 \u03BC\u03B1\u03C2 \u03B1\u03C0\u03BF\u03C4\u03B5\u03BB\u03BF\u03CD\u03BD \u03C4\u03BF\u03C5\u03C2 \u03B4\u03CD\u03BF \u03BC\u03B5\u03B3\u03B1\u03BB\u03CD\u03C4\u03B5\u03C1\u03BF\u03C5\u03C2 \u03B3\u03B1\u03BB\u03B1\u03BE\u03AF\u03B5\u03C2 \u03C4\u03B7\u03C2 \u03C4\u03BF\u03C0\u03B9\u03BA\u03AE\u03C2 \u03BF\u03BC\u03AC\u03B4\u03B1\u03C2 \u03B3\u03B1\u03BB\u03B1\u03BE\u03B9\u03CE\u03BD. \u0391\u03BD \u03BA\u03B1\u03B9 \u03B5\u03AF\u03BD\u03B1\u03B9 \u03BC\u03B5\u03B3\u03B1\u03BB\u03CD\u03C4\u03B5\u03C1\u03BF\u03C2 \u03B1\u03C0\u03CC \u03C4\u03BF\u03BD \u0393\u03B1\u03BB\u03B1\u03BE\u03AF\u03B1 \u03BC\u03B1\u03C2 (\u03BF \u03BF\u03C0\u03BF\u03AF\u03BF\u03C2 \u03B5\u03AF\u03BD\u03B1\u03B9 \u03BF \u03B4\u03B5\u03CD\u03C4\u03B5\u03C1\u03BF\u03C2 \u03C3\u03B5 \u03BC\u03AD\u03B3\u03B5\u03B8\u03BF\u03C2 \u03C3\u03C4\u03B7\u03BD \u03C4\u03BF\u03C0\u03B9\u03BA\u03AE \u03BF\u03BC\u03AC\u03B4\u03B1 \u03B3\u03B1\u03BB\u03B1\u03BE\u03B9\u03CE\u03BD), \u03C0\u03B9\u03B8\u03B1\u03BD\u03CC\u03C4\u03B1\u03C4\u03B1 \u03BF \u03B4\u03B9\u03BA\u03CC\u03C2 \u03BC\u03B1\u03C2 \u03C0\u03B5\u03C1\u03B9\u03AD\u03C7\u03B5\u03B9 \u03C0\u03B5\u03C1\u03B9\u03C3\u03C3\u03CC\u03C4\u03B5\u03C1\u03B7 \u03C3\u03BA\u03BF\u03C4\u03B5\u03B9\u03BD\u03AE \u03CD\u03BB\u03B7 \u03BA\u03B1\u03B9 \u03AD\u03C7\u03B5\u03B9 \u03BC\u03B5\u03B3\u03B1\u03BB\u03CD\u03C4\u03B5\u03C1\u03B7 \u03BC\u03AC\u03B6\u03B1. \u039D\u03AD\u03B5\u03C2 \u03C0\u03B1\u03C1\u03B1\u03C4\u03B7\u03C1\u03AE\u03C3\u03B5\u03B9\u03C2 \u03B4\u03B5\u03AF\u03C7\u03BD\u03BF\u03C5\u03BD \u03CC\u03C4\u03B9 \u03B4\u03B9\u03B1\u03B8\u03AD\u03C4\u03B5\u03B9 \u03AD\u03BD\u03B1 \u03C4\u03C1\u03B9\u03C3\u03B5\u03BA\u03B1\u03C4\u03BF\u03BC\u03BC\u03CD\u03C1\u03B9\u03BF \u03AC\u03C3\u03C4\u03C1\u03B1, \u03B4\u03B7\u03BB\u03B1\u03B4\u03AE 2,5 \u03BC\u03B5 5 \u03C6\u03BF\u03C1\u03AD\u03C2 \u03C0\u03B5\u03C1\u03B9\u03C3\u03C3\u03CC\u03C4\u03B5\u03C1\u03B1 \u03B1\u03C0\u03CC \u03C4\u03BF\u03BD \u0393\u03B1\u03BB\u03B1\u03BE\u03AF\u03B1 \u03BC\u03B1\u03C2."@el ,
		"The Andromeda Galaxy (IPA: /\u00E6n\u02C8dr\u0252m\u026Ad\u0259/), also known as Messier 31, M31, or NGC 224 and originally the Andromeda Nebula, is a barred spiral galaxy with the diameter of about 46.56 kiloparsecs (152,000 light-years) approximately 2.5 million light-years (765 kiloparsecs) from Earth and the nearest large galaxy to the Milky Way. The galaxy's name stems from the area of Earth's sky in which it appears, the constellation of Andromeda, which itself is named after the princess who was the wife of Perseus in Greek mythology."@en ,
		"Het Andromedastelsel of de Andromedanevel (M31) is een spiraalvormig sterrenstelsel, in het sterrenbeeld Andromeda. Het stelsel heeft dezelfde vorm als ons eigen sterrenstelsel, de Melkweg, maar is wel een stuk groter. De afstand wordt geschat op ongeveer 2,54 miljoen lichtjaar, de diameter ca. 220.000 lichtjaar. De massa wordt geschat op 300 tot 400 miljard zonsmassa's, de totale massa inclusief de halo op 1,2 biljoen zonsmassa's. Vergeleken met de laatste schattingen van de totale massa van de Melkweg, die 1,9 biljoen zonsmassa's bedraagt, zou dus M31 wat lichter zijn, en veel minder dicht. Samen met de Melkweg en een aantal kleinere sterrenstelsels vormt de Andromedanevel de Lokale Groep."@nl ,
		"Andromeda galaxia, Messier 31, M31 edo NGC 224 bezala ere ezaguna, eta, jatorrian, Andromedaren nebulosa (ikus aurrerago), Lurretik 2,5 milioi argi urtera (770 kiloparsecs) dagoen galaxia espiral barratu bat da, baita Esne Bidetik gertuen dagoen galaxia nagusia ere. Galaxiaren izena, lurreko zerutik dator, non Andromeda konstelazioa agertzen den, aldi berean, greziar mitologian, Perseoren emazte izan zen etiopiar edo feniziar printzesaren izena jasotzen duena."@eu ,
		"Die Andromedagalaxie, auch (veraltet) Andromedanebel oder Gro\u00DFer Andromedanebel, ist die der Milchstra\u00DFe mit rund 2,5 Millionen Lichtjahren Entfernung n\u00E4chstgelegene Spiralgalaxie. Sie befindet sich im namensgebenden Sternbild Andromeda und ist das entfernteste Objekt, das unter guten Bedingungen ohne technische Hilfsmittel mit blo\u00DFem Auge beobachtet werden kann. H\u00E4ufig wird sie auch kurz als M31 bezeichnet nach ihrem Eintrag im Messier-Katalog."@de ,
		"Andromedagalaxen, NGC 224 eller M31, \u00E4r en spiralgalax av typ i Vintergatans n\u00E4romr\u00E5de som \u00E4r svagt synlig med blotta \u00F6gat. Den \u00E5terfinns i stj\u00E4rnbilden Andromeda som givit den dess namn. Andromedagalaxen ligger p\u00E5 ett avst\u00E5nd av 2,5\u20132,9 miljoner ljus\u00E5r fr\u00E5n Vintergatan och \u00E4r den n\u00E4rmaste granngalaxen om man inte r\u00E4knar Vintergatans sm\u00E5 satellitgalaxer. M\u00E4tningar visar att den \u00E4r p\u00E5 kollisionskurs med Vintergatan med en radiell hastighet p\u00E5 cirka 120 km/s och galaxerna kommer sannolikt att krocka om cirka 3 miljarder \u00E5r, beroende p\u00E5 hur stor den ok\u00E4nda transversella hastigheten \u00E4r. Resultatet av denna kollision blir f\u00F6rmodligen att de sm\u00E4lter samman till en stor elliptisk galax."@sv ,
		"La galaxia de Andr\u00F3meda, tambi\u00E9n conocida como Galaxia Espiral M31, Messier 31 o NGC 224, es una galaxia espiral con un di\u00E1metro de doscientos veinte mil a\u00F1os luz (en lo que concierne a su halo gal\u00E1ctico) y de unos ciento cincuenta mil a\u00F1os luz entre los extremos de sus brazos. Es el objeto visible a simple vista m\u00E1s lejano de la Tierra (aunque algunos afirman poder ver a simple vista la galaxia del Tri\u00E1ngulo, que est\u00E1 un poco m\u00E1s lejos). Est\u00E1 a 2,5 millones de a\u00F1os luz\u200B en direcci\u00F3n a la constelaci\u00F3n de Andr\u00F3meda. Es, junto con nuestra propia galaxia, la m\u00E1s grande y brillante de las galaxias del Grupo Local, que consiste en aproximadamente 30 peque\u00F1as galaxias m\u00E1s tres grandes galaxias espirales: Andr\u00F3meda, la V\u00EDa L\u00E1ctea y la galaxia del Tri\u00E1ngulo."@es ,
		"\u0645\u062C\u0631\u0629 \u0627\u0644\u0645\u0631\u0623\u0629 \u0627\u0644\u0645\u0633\u0644\u0633\u0644\u0629 (\u0628\u0627\u0644\u0625\u0646\u062C\u0644\u064A\u0632\u064A\u0629: Andromeda)\u200F (\u062A\u0633\u0645\u0649 \u0623\u064A\u0636\u0627 NGC 224 \u0648M31) \u0647\u064A \u0623\u0642\u0631\u0628 \u0627\u0644\u0645\u062C\u0631\u0627\u062A \u0644\u0645\u062C\u0631\u062A\u0646\u0627 (\u0623\u064A \u0623\u0642\u0631\u0628 \u0645\u062C\u0631\u0629 \u0643\u0628\u064A\u0631\u0629\u060C \u0639\u0644\u0649 \u0627\u0644\u0631\u063A\u0645 \u0645\u0646 \u0643\u0648\u0646 \u0645\u062C\u0631\u0629 \u0643\u0627\u0646\u064A\u0633 \u0645\u064A\u062C\u0648\u0631 \u0627\u0644\u0642\u0632\u0645\u0629 \u0623\u0642\u0631\u0628 \u0645\u062C\u0631\u0629 \u0642\u0632\u0645\u0629 \u0625\u0644\u0649 \u062F\u0631\u0628 \u0627\u0644\u062A\u0628\u0627\u0646\u0629)\u060C \u0648\u064A\u0645\u0643\u0646 \u0645\u0634\u0627\u0647\u062F\u062A\u0647\u0627 \u0628\u0627\u0644\u0639\u064A\u0646 \u0627\u0644\u0645\u062C\u0631\u062F\u0629 \u0628\u062F\u0648\u0646 \u0627\u0633\u062A\u062E\u062F\u0627\u0645 \u0627\u0644\u0645\u0642\u0631\u0627\u0628\u060C \u0648\u0647\u064A \u062A\u0628\u0639\u062F \u0639\u0646\u0627 \u0646\u062D\u0648 2.5 \u0645\u0644\u064A\u0648\u0646 \u0633\u0646\u0629 \u0636\u0648\u0626\u064A\u0629. \u0648\u062A\u062D\u062A\u0648\u0649 \u0639\u0644\u0649 \u0646\u062D\u0648 250 \u0645\u0644\u064A\u0627\u0631 \u0646\u062C\u0645 \u0648\u064A\u0628\u0644\u063A \u0642\u0637\u0631\u0647\u0627 220 \u0623\u0644\u0641 \u0633\u0646\u0629 \u0636\u0648\u0626\u064A\u0629\u060C \u0648\u0647\u064A \u0628\u0630\u0644\u0643 \u0623\u0643\u0628\u0631 \u0645\u0646 \u0645\u062C\u0631\u062A\u0646\u0627 \u0627\u0644\u062A\u064A \u064A\u0642\u062F\u0631 \u0639\u062F\u062F \u0627\u0644\u0646\u062C\u0648\u0645 \u0641\u064A\u0647\u0627 \u0645\u0627 \u0628\u064A\u0646 200-400 \u0645\u0644\u064A\u0627\u0631 \u0645\u0646 \u0627\u0644\u0646\u062C\u0648\u0645. \u062A\u0639\u062A\u0628\u0631 \u0645\u062C\u0631\u0629 \u0627\u0644\u0645\u0631\u0623\u0629 \u0627\u0644\u0645\u0633\u0644\u0633\u0644\u0629 \u0645\u0646 \u0627\u0644\u0645\u062C\u0631\u0627\u062A \u0627\u0644\u062A\u064A \u0643\u062A\u0628 \u0639\u0646\u0647\u0627 \u0627\u0644\u0643\u062B\u064A\u0631 \u0645\u0646 \u0627\u0644\u0643\u062A\u0627\u0628 \u0641\u064A \u0631\u0648\u0627\u064A\u0627\u062A \u0627\u0644\u062E\u064A\u0627\u0644 \u0627\u0644\u0639\u0644\u0645\u064A."@ar ,
		"A gal\u00E1xia de Andr\u00F4meda (portugu\u00EAs brasileiro) ou gal\u00E1xia de Andr\u00F3meda (portugu\u00EAs europeu) (Messier 31, NGC 224) \u00E9 uma gal\u00E1xia espiral localizada a cerca de 2,54 milh\u00F5es de anos-luz de dist\u00E2ncia da Terra, na dire\u00E7\u00E3o da constela\u00E7\u00E3o de Andr\u00F4meda. \u00C9 a gal\u00E1xia espiral mais pr\u00F3xima da Via L\u00E1ctea e seu nome \u00E9 derivado da constela\u00E7\u00E3o onde est\u00E1 situada, que, por sua vez, tem o nome derivado da princesa mitol\u00F3gica Andr\u00F4meda. \u00C9 a maior gal\u00E1xia do Grupo Local, que tamb\u00E9m cont\u00E9m a Via L\u00E1ctea, a gal\u00E1xia do Tri\u00E2ngulo e aproximadamente 30 outras menores. O levantamento feito pelo Telesc\u00F3pio Espacial Spitzer em 2006 determinou que sua massa \u00E9 de aproximadamente ~0,8-1,5 \u00D7 1012 massas solares enquanto a Via L\u00E1ctea tem uma massa estimada em 8,5 \u00D7 1011 massas solares. Sua popula\u00E7\u00E3o estelar atinge aproximadame"@pt ,
		"\u0413\u0430\u043B\u0430\u0301\u043A\u0442\u0438\u043A\u0430 \u0410\u043D\u0434\u0440\u043E\u043C\u0435\u0301\u0434\u044B (\u0422\u0443\u043C\u0430\u0301\u043D\u043D\u043E\u0441\u0442\u044C \u0410\u043D\u0434\u0440\u043E\u043C\u0435\u0301\u0434\u044B, M 31, NGC 224, PGC 2557) \u2014 \u0441\u043F\u0438\u0440\u0430\u043B\u044C\u043D\u0430\u044F \u0433\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u0430, \u043D\u0430\u0431\u043B\u044E\u0434\u0430\u0435\u043C\u0430\u044F \u0432 \u0441\u043E\u0437\u0432\u0435\u0437\u0434\u0438\u0438 \u0410\u043D\u0434\u0440\u043E\u043C\u0435\u0434\u044B. \u0415\u0451 \u0434\u0438\u0430\u043C\u0435\u0442\u0440 \u0441\u043E\u0441\u0442\u0430\u0432\u043B\u044F\u0435\u0442 47 \u043A\u0438\u043B\u043E\u043F\u0430\u0440\u0441\u0435\u043A, \u0447\u0442\u043E \u0431\u043E\u043B\u044C\u0448\u0435, \u0447\u0435\u043C \u0443 \u043D\u0430\u0448\u0435\u0439 \u0413\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u0438, \u0438 \u043E\u043D\u0430 \u0441\u043E\u0434\u0435\u0440\u0436\u0438\u0442 \u0432 \u043D\u0435\u0441\u043A\u043E\u043B\u044C\u043A\u043E \u0440\u0430\u0437 \u0431\u043E\u043B\u044C\u0448\u0435 \u0437\u0432\u0451\u0437\u0434, \u0447\u0435\u043C \u041C\u043B\u0435\u0447\u043D\u044B\u0439 \u041F\u0443\u0442\u044C. \u0420\u0430\u0441\u0441\u0442\u043E\u044F\u043D\u0438\u0435 \u043E\u0442 \u043D\u0430\u0448\u0435\u0439 \u0413\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u0438 \u0434\u043E \u043D\u0435\u0451 \u0441\u043E\u0441\u0442\u0430\u0432\u043B\u044F\u0435\u0442 \u043E\u043A\u043E\u043B\u043E 800 \u043A\u0438\u043B\u043E\u043F\u0430\u0440\u0441\u0435\u043A, \u0447\u0442\u043E \u0434\u0435\u043B\u0430\u0435\u0442 \u0435\u0451 \u0431\u043B\u0438\u0436\u0430\u0439\u0448\u0435\u0439 \u0438\u0437 \u043A\u0440\u0443\u043F\u043D\u044B\u0445 \u0433\u0430\u043B\u0430\u043A\u0442\u0438\u043A, \u0430 \u0442\u0430\u043A\u0436\u0435 \u043A\u0440\u0443\u043F\u043D\u0435\u0439\u0448\u0435\u0439 \u0433\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u043E\u0439 \u041C\u0435\u0441\u0442\u043D\u043E\u0439 \u0433\u0440\u0443\u043F\u043F\u044B. \u0415\u0451 \u043C\u0430\u0441\u0441\u0430 \u043F\u0440\u0438\u0431\u043B\u0438\u0437\u0438\u0442\u0435\u043B\u044C\u043D\u043E \u0440\u0430\u0432\u043D\u0430 \u043C\u0430\u0441\u0441\u0435 \u041C\u043B\u0435\u0447\u043D\u043E\u0433\u043E \u041F\u0443\u0442\u0438 \u0438\u043B\u0438 \u0434\u0430\u0436\u0435 \u043C\u0435\u043D\u044C\u0448\u0435."@ru ,
		"Galaxie v Andromed\u011B je spir\u00E1ln\u00ED galaxie, vzd\u00E1len\u00E1 p\u0159ibli\u017En\u011B 2,5 mili\u00F3nu sv\u011Bteln\u00FDch let (2,4\u00D71019 km) od Zem\u011B, v souhv\u011Bzd\u00ED Andromedy. Je tak\u00E9 zn\u00E1ma pod katalogov\u00FDm ozna\u010Den\u00EDm Messier 31 (M31) a NGC 224, ve star\u0161\u00ED astronomick\u00E9 literatu\u0159e m\u00E1 \u010Dasto ozna\u010Den\u00ED Velk\u00E1 mlhovina v Andromed\u011B. Galaxie v Andromed\u011B je nejbli\u017E\u0161\u00ED spir\u00E1ln\u00ED galaxie od na\u0161\u00ED Ml\u00E9\u010Dn\u00E9 dr\u00E1hy, ale nen\u00ED nejbli\u017E\u0161\u00ED galaxi\u00ED. M\u00E1 jm\u00E9no po oblasti hv\u011Bzdn\u00E9 oblohy, ve kter\u00E9 se nach\u00E1z\u00ED a kter\u00E1 je pojmenov\u00E1na po mytologick\u00E9 princezn\u011B Andromed\u011B. Galaxie v Andromed\u011B je nejv\u011Bt\u0161\u00ED galaxie z M\u00EDstn\u00ED skupiny galaxi\u00ED, kter\u00E1 tak\u00E9 obsahuje na\u0161i Ml\u00E9\u010Dnou dr\u00E1hu, Galaxii v Troj\u00FAheln\u00EDku a p\u0159ibli\u017En\u011B 30 dal\u0161\u00EDch men\u0161\u00EDch galaxi\u00ED. P\u0159esto\u017Ee je nejv\u011Bt\u0161\u00ED, nemus\u00ED b\u00FDt nejhmotn\u011Bj\u0161\u00ED, ned\u00E1vn\u00E1 zji\u0161t\u011Bn\u00ED nazna\u010Duj\u00ED, \u017Ee Ml\u00E9\u010Dn\u00E1 dr\u00E1ha obsahuje v\u00EDce temn\u00E9 hmoty, a proto m\u016F\u017Ee b\u00FDt "@cs ,
		"M31(\nPour les articles homonymes, voir Androm\u00E8de, n\u00E9buleuse d'Androm\u00E8de et M31. ) La galaxie d'Androm\u00E8de, \u00E9galement d\u00E9sign\u00E9e M31 dans le Catalogue de Messier et NGC 224, est une galaxie spirale situ\u00E9e \u00E0 environ 2,55 millions d'ann\u00E9es-lumi\u00E8re du Soleil, dans la constellation d'Androm\u00E8de. La galaxie d'Androm\u00E8de (NGC 224) a \u00E9t\u00E9 utilis\u00E9e par G\u00E9rard de Vaucouleurs comme une galaxie de type morphologique SA(s)b dans son atlas des galaxies."@fr ,
		"\u0413\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u0430 \u0410\u043D\u0434\u0440\u043E\u043C\u0435\u0434\u0438 (\u0422\u0443\u043C\u0430\u043D\u043D\u0456\u0441\u0442\u044C \u0410\u043D\u0434\u0440\u043E\u043C\u0435\u0434\u0438, \u041C\u0435\u0441\u0441\u044C\u0454 31, \u041C31, NGC 224) \u2014\u043D\u0430\u0439\u0431\u043B\u0438\u0436\u0447\u0430 \u0434\u043E \u0427\u0443\u043C\u0430\u0446\u044C\u043A\u043E\u0433\u043E \u0428\u043B\u044F\u0445\u0443 \u0432\u0435\u043B\u0438\u043A\u0430 \u0433\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u0430, \u0440\u043E\u0437\u0442\u0430\u0448\u043E\u0432\u0430\u043D\u0430 \u0432 \u0441\u0443\u0437\u0456\u0440'\u0457 \u0410\u043D\u0434\u0440\u043E\u043C\u0435\u0434\u0438 \u0456 \u0432\u0456\u0434\u0434\u0430\u043B\u0435\u043D\u0430 \u0432\u0456\u0434 \u043D\u0430\u0441, \u0437\u0430 \u043E\u0441\u0442\u0430\u043D\u043D\u0456\u043C\u0438 \u0434\u0430\u043D\u0438\u043C\u0438, \u043D\u0430 \u0432\u0456\u0434\u0441\u0442\u0430\u043D\u044C 772 \u043A\u0456\u043B\u043E\u043F\u0430\u0440\u0441\u0435\u043A (2,52 \u043C\u043B\u043D \u0441\u0432\u0456\u0442\u043B\u043E\u0432\u0438\u0445 \u0440\u043E\u043A\u0456\u0432). \u041F\u043B\u043E\u0449\u0438\u043D\u0430 \u0433\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u0438 \u043D\u0430\u0445\u0438\u043B\u0435\u043D\u0430 \u0434\u043E \u043D\u0430\u0441 \u043F\u0456\u0434 \u043A\u0443\u0442\u043E\u043C 15\u00B0, \u0457\u0457 \u0432\u0438\u0434\u0438\u043C\u0438\u0439 \u0440\u043E\u0437\u043C\u0456\u0440 \u2014 3,2\u00B0\u00D71\u00B0, \u0432\u0438\u0434\u0438\u043C\u0430 \u0437\u043E\u0440\u044F\u043D\u0430 \u0432\u0435\u043B\u0438\u0447\u0438\u043D\u0430 \u2014 +3,4 m ."@uk ,
		"R\u00E9altra b\u00EDseach is ea r\u00E9altra Andraim\u00E9ide, agus \u00E9 le feice\u00E1il i r\u00E9altbhu\u00EDon Andraim\u00E9ide. T\u00E1 an r\u00E9altra seo suite faoi 2.2 milli\u00FAn solasbhliain d\u00EDnn, agus is \u00E9 an r\u00E9altra b\u00EDseach is gaire d\u00FAinn. C\u00E9 is moite de Bhealach na B\u00F3 Finne f\u00E9in, is \u00E9 an t-aon r\u00E9altra b\u00EDseach is f\u00E9idir a aithint ar sp\u00E9ir na ho\u00EDche gan \u00FAs\u00E1id a bhaint as gl\u00E9asra cianradhairc ar n\u00F3s na nd\u00E9sh\u00FAileach n\u00F3 an teileasc\u00F3ip. T\u00E1 Scamall M\u00F3r Magellan agus Scamall Beag Magellan le feice\u00E1il chomh maith, ach n\u00ED r\u00E9altra\u00ED b\u00EDseacha iad. Ceann de r\u00E9altra\u00ED an Ghr\u00FApa \u00C1iti\u00FAil \u00E9. Is \u00E9 an teileasc\u00F3p is fearr a thabharfaidh l\u00E9argas air, sin n\u00F3 prionta\u00ED de ghrianghraif fhadnochta."@ga ,
		"\u30A2\u30F3\u30C9\u30ED\u30E1\u30C0\u9280\u6CB3\uFF08\u30A2\u30F3\u30C9\u30ED\u30E1\u30C0\u304E\u3093\u304C\u3001M31\u3001NGC 224\uFF09\u306F\u3001\u30A2\u30F3\u30C9\u30ED\u30E1\u30C0\u5EA7\u306B\u4F4D\u7F6E\u3059\u308B\u5730\u7403\u304B\u3089\u76EE\u8996\u53EF\u80FD\u306A\u6E26\u5DFB\u9280\u6CB3\u3067\u3042\u308B\u3002\u3055\u3093\u304B\u304F\u5EA7\u9280\u6CB3 (M33) \u3001\u9280\u6CB3\u7CFB\uFF08\u5929\u306E\u5DDD\u9280\u6CB3\uFF09\u3001\u5927\u30DE\u30BC\u30E9\u30F3\u96F2\u3001\u5C0F\u30DE\u30BC\u30E9\u30F3\u96F2\u306A\u3069\u3068\u3068\u3082\u306B\u5C40\u6240\u9280\u6CB3\u7FA4\u3092\u69CB\u6210\u3059\u308B\u3002"@ja ,
		"La gal\u00E0xia d'Andr\u00F2meda, Messier 31, M31 o NGC 224, \u00E9s una gal\u00E0xia espiral gegant catalogada per Charles Messier el 1764. \u00C9s l'objecte visible a ull nu m\u00E9s allunyat de la Terra. \u00C9s a 2,5 milions d'anys llum (775 kpc) en direcci\u00F3 a la constel\u00B7laci\u00F3 d'Andr\u00F2meda. Fa part del grup local de gal\u00E0xies, que inclou una gran quantitat de gal\u00E0xies petites m\u00E9s les tres grans gal\u00E0xies espirals: Andr\u00F2meda, la Via L\u00E0ctia i la Gal\u00E0xia del Triangle."@ca ,
		"Galaktyka Andromedy (zwana r\u00F3wnie\u017C Messier 31, M31 lub NGC 224, a wcze\u015Bniej tak\u017Ce Wielk\u0105 Mg\u0142awic\u0105 w Andromedzie) \u2013 galaktyka spiralna, le\u017C\u0105ca oko\u0142o 2,52 miliona lat \u015Bwietlnych od Ziemi w gwiazdozbiorze Andromedy. Galaktyka Andromedy jest najwi\u0119ksz\u0105 i najja\u015Bniejsz\u0105 galaktyk\u0105 nieba p\u00F3\u0142nocnego. Wida\u0107 j\u0105 nawet przez ma\u0142e lornetki. Obserwacje mo\u017Cna prowadzi\u0107 tak\u017Ce go\u0142ym okiem, niekiedy nawet na przedmie\u015Bciach wi\u0119kszych miast, widoczna jest jako niewielka mgie\u0142ka. Jednak jej ca\u0142kowita \u015Brednica k\u0105towa przewy\u017Csza sze\u015Bciokrotnie k\u0105towe rozmiary Ksi\u0119\u017Cyca."@pl ,
		"\u4ED9\u5973\u5EA7\u661F\u7CFB\uFF08Andromeda Galaxy\uFF0C\u570B\u969B\u97F3\u6A19\u70BA\uFF1A/\u02CCan\u02C8dr\u0252m\u0259d\u0259/\uFF0C\u4E5F\u7A31\u70BA\u6885\u897F\u803631\u3001\u661F\u8868\u7F16\u53F7\u4E3AM31\u548CNGC 224\uFF0C\u5728\u820A\u6587\u737B\u4E2D\u66FE\u7D93\u7A31\u70BA\u4ED9\u5973\u5EA7\u661F\u96F2\uFF0C\u5728\u4E2D\u56FD\u53E4\u4EE3\u88AB\u79F0\u4E3A\u594E\u5BBF\u589E\u5EFF\u4E00\uFF09\u662F\u4E00\u500B\u68D2\u65CB\u661F\u7CFB\uFF0C\u8DDD\u96E2\u5730\u7403\u5927\u7D04250\u842C\u5149\u5E74\uFF0C\u662F\u9664\u9EA6\u54F2\u4F26\u4E91\uFF08\u5730\u7403\u6240\u5728\u7684\u94F6\u6CB3\u7CFB\u7684\u4F34\u661F\u7CFB\uFF09\u4EE5\u5916\u6700\u8FD1\u7684\u661F\u7CFB\u3002 \u4ED9\u5973\u5EA7\u661F\u7CFB\u4F4D\u65BC\u4ED9\u5973\u5EA7\u65B9\u5411\uFF0C\u662F\u4EBA\u985E\u8089\u773C\u53EF\u898B\uFF083.4\u7B49\u661F\uFF09\u6700\u9060\u7684\u6DF1\u7A7A\u5929\u9AD4\u3002\u4ED9\u5973\u5EA7\u661F\u7CFB\u88AB\u76F8\u4FE1\u662F\u672C\u661F\u7CFB\u7FA4\u4E2D\u6700\u5927\u7684\u661F\u7CFB\uFF0C\u76F4\u5F84\u7EA620\u4E07\u5149\u5E74\uFF0C\u5916\u8868\u9887\u4F3C\u94F6\u6CB3\u7CFB\u3002\u672C\u661F\u7CFB\u7FA4\u7684\u6210\u54E1\u6709\u4ED9\u5973\u661F\u7CFB\u3001\u9280\u6CB3\u7CFB\u3001\u4E09\u89D2\u5EA7\u661F\u7CFB\uFF0C\u9084\u6709\u5927\u7D0450\u500B\u5C0F\u661F\u7CFB\u3002\u4F46\u6839\u64DA\u6539\u9032\u7684\u6E2C\u91CF\u6280\u8853\u548C\u4E8C\u5341\u4E00\u4E16\u7D00\u521D\u7814\u7A76\u7684\u6578\u64DA\u7D50\u679C\uFF0C\u79D1\u5B78\u5BB6\u73FE\u5728\u76F8\u4FE1\u9280\u6CB3\u7CFB\u6709\u8A31\u591A\u7684\u6697\u7269\u8CEA\uFF0C\u4E26\u4E14\u53EF\u80FD\u662F\u5728\u9019\u500B\u96C6\u5718\u4E2D\u8CEA\u91CF\u6700\u5927\u7684\u3002\u7136\u800C\uFF0C\u53F2\u5339\u54F2\u592A\u7A7A\u671B\u9060\u93E1\u6700\u8FD1\u7684\u89C0\u6E2C\u986F\u793A\u4ED9\u5973\u5EA7\u661F\u7CFB\u6709\u5C07\u8FD1\u4E00\u5146\uFF081012\uFF09\u9846\u6046\u661F\uFF0C\u6578\u91CF\u9060\u6BD4\u6211\u5011\u7684\u9280\u6CB3\u7CFB\u591A\u3002\u57282006\u5E74\u91CD\u65B0\u4F30\u8A08\u9280\u6CB3\u7CFB\u7684\u8CEA\u91CF\u5927\u7D04\u662F\u4ED9\u5973\u5EA7\u661F\u7CFB\u768450\uFF05\uFF0C\u662F7.1\u00D71011M\u2609.\u4ED9\u5973\u5EA7\u661F\u7CFB\u5728\u9069\u5EA6\u9ED1\u6697\u7684\u5929\u7A7A\u74B0\u5883\u4E0B\u5F88\u5BB9\u6613\u7528\u8089\u773C\u770B\u898B\uFF0C\u4F46\u662F\u5982\u6B64\u7684\u5929\u7A7A\u50C5\u5B58\u5728\u65BC\u5C0F\u93AE\u3001\u88AB\u9694\u7D55\u7684\u5340\u57DF\u3001\u548C\u96E2\u4EBA\u53E3\u96C6\u4E2D\u5340\u57DF\u5F88\u9060\u7684\u5730\u65B9\uFF0C\u53EA\u53D7\u5230\u8F15\u5EA6\u5149\u6C61\u67D3\u7684\u74B0\u5883\u4E0B\u3002\u8089\u773C\u770B\u898B\u7684\u4ED9\u5973\u5EA7\u661F\u7CFB\u975E\u5E38\u5C0F\uFF0C\u56E0\u70BA\u5B83\u53EA\u6709\u4E2D\u5FC3\u4E00\u5C0F\u584A\u7684\u5340\u57DF\u6709\u8DB3\u5920\u7684\u4EAE\u5EA6\uFF0C\u4F46\u662F\u9019\u500B\u661F\u7CFB\u5B8C\u6574\u7684\u89D2\u76F4\u5F91\u6709\u6EFF\u6708\u7684\u4E03\u500D\u5927\u3002"@zh ,
		"La Galassia di Andromeda (nota talvolta anche con il vecchio nome Grande Nebulosa di Andromeda o con le sigle di catalogo M 31 e NGC 224) \u00E8 una galassia a spirale gigante che dista circa 2,538 milioni di anni luce dalla Terra in direzione della costellazione di Andromeda, da cui prende il nome. Si tratta della galassia di grandi dimensioni pi\u00F9 vicina alla nostra, la Via Lattea; \u00E8 visibile anche a occhio nudo ed \u00E8 tra gli oggetti pi\u00F9 lontani visibili senza l'ausilio di strumenti."@it ;
	foaf:name	"M31,NGC224,UGC454,PGC2557,2C56 (Core), CGCG 535-17,MCG+07-02-016,IRAS00400+4059,2MASXJ00424433+4116074, GC 116, h 50, Bode 3, Flamsteed 58, Hevelius 32, Ha 3.3, IRC +40013"@en ,
		"Andromeda Galaxy"@en ;
	foaf:depiction	<http://commons.wikimedia.org/wiki/Special:FilePath/The_Galaxy_Next_Door.jpg> ,
		<http://commons.wikimedia.org/wiki/Special:FilePath/Milky_Way_and_Andromeda_in_space,_to_scale.jpg> ,
		<http://commons.wikimedia.org/wiki/Special:FilePath/M31_09-01-2011.jpg> ,
		<http://commons.wikimedia.org/wiki/Special:FilePath/M31_Core_in_X-rays.jpg> ,
		<http://commons.wikimedia.org/wiki/Special:FilePath/WISE-_Andromeda.jpg> ,
		<http://commons.wikimedia.org/wiki/Special:FilePath/Andromeda_constellation_map.svg> ,
		<http://commons.wikimedia.org/wiki/Special:FilePath/Andromeda_Galaxy_with_DESI_Overlay.jpg> ,
		<http://commons.wikimedia.org/wiki/Special:FilePath/Andromeda_active_core.jpg> ,
		<http://commons.wikimedia.org/wiki/Special:FilePath/Andromeda_Galaxy_560mm_FL.jpg> ,
		<http://commons.wikimedia.org/wiki/Special:FilePath/PIA20061_-_Andromeda_in_High-Energy_X-rays,_Figure_1.jpg> ,
		<http://commons.wikimedia.org/wiki/Special:FilePath/Andromeda_galaxy_Ssc2005-20a1.jpg> ,
		<http://commons.wikimedia.org/wiki/Special:FilePath/Andromeda_galaxy.jpg> ,
		<http://commons.wikimedia.org/wiki/Special:FilePath/Hubble_Finds_Giant_Halo_Around_the_Andromeda_Galaxy.jpg> ,
		<http://commons.wikimedia.org/wiki/Special:FilePath/Pic_iroberts1.jpg> ,
		<http://commons.wikimedia.org/wiki/Special:FilePath/\u041D\u0430\u0434_VLT_\u2013_\u0434\u0432\u0435_\u0433\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u0438,_\u0432\u0438\u0434\u0438\u043C\u044B\u0435_\u043F\u0440\u043E\u0441\u0442\u044B\u043C_\u0433\u043B\u0430\u0437\u043E\u043C.jpg> ,
		<http://commons.wikimedia.org/wiki/Special:FilePath/Star_cluster_in_the_Andromeda_galaxy.jpg> ,
		<http://commons.wikimedia.org/wiki/Special:FilePath/Infraredandromeda.jpg> ,
		<http://commons.wikimedia.org/wiki/Special:FilePath/Moon_over_Andromeda_(rotated).jpg> .
@prefix dcterms:	<http://purl.org/dc/terms/> .
@prefix dbc:	<http://dbpedia.org/resource/Category:> .
dbr:Andromeda_Galaxy	dcterms:subject	dbc:UGC_objects ,
		dbc:Principal_Galaxies_Catalogue_objects ,
		dbc:NGC_objects ,
		dbc:Andromeda_Subgroup ,
		dbc:Barred_spiral_galaxies ,
		dbc:IRAS_catalogue_objects ,
		dbc:Local_Group ,
		dbc:Articles_containing_video_clips ,
		dbc:Andromeda_Galaxy ,
		dbc:MCG_objects ,
		<http://dbpedia.org/resource/Category:Andromeda_(constellation)> ,
		dbc:Messier_objects ,
		dbc:Astronomical_objects_known_since_antiquity ;
	dbo:abstract	"Die Andromedagalaxie, auch (veraltet) Andromedanebel oder Gro\u00DFer Andromedanebel, ist die der Milchstra\u00DFe mit rund 2,5 Millionen Lichtjahren Entfernung n\u00E4chstgelegene Spiralgalaxie. Sie befindet sich im namensgebenden Sternbild Andromeda und ist das entfernteste Objekt, das unter guten Bedingungen ohne technische Hilfsmittel mit blo\u00DFem Auge beobachtet werden kann. H\u00E4ufig wird sie auch kurz als M31 bezeichnet nach ihrem Eintrag im Messier-Katalog. Die Andromedagalaxie \u00E4hnelt der Milchstra\u00DFe. Beide Galaxien beherbergen die gleichen Arten von astronomischen Objekten, aus der \u201E\u00E4u\u00DFeren\u201C Perspektive der Milchstra\u00DFe besteht jedoch eine bessere Sicht auf die Struktur der Galaxie. Es sind dunkle Staubb\u00E4nder, Sternentstehungsgebiete und im Au\u00DFenbereich \u00FCber 200, m\u00F6glicherweise 500 Kugelsternhaufen auszumachen. Auch k\u00F6nnen in immer gr\u00F6\u00DFeren Bereichen ihre einzelnen Sterne beobachtet werden. Die Galaxie weist im Zentrum ein massereiches Schwarzes Loch von etwa 100 Millionen Sonnenmassen auf, Spiralarme erstrecken sich davon bis zu einer Distanz von rund 80.000 Lichtjahren, ihr Halo dehnt sich \u00FCber eine Million Lichtjahre aus. Hinsichtlich des Halos ist die Andromedagalaxie das gr\u00F6\u00DFte Mitglied der Lokalen Gruppe, einer Ansammlung gravitativ gebundener Galaxien. Die Andromedagalaxie und die \u00E4hnlich massereiche Milchstra\u00DFe sind in der Lokalen Gruppe die beiden mit Abstand massereichsten Galaxien und binden jeweils eine Vielzahl von Satellitengalaxien an sich. Die in der j\u00FCngeren Literatur angegebenen Sch\u00E4tzwerte f\u00FCr die Masse der Andromedagalaxie bewegen sich zwischen 0,7 und 2,5 Billionen Sonnenmassen, wovon ihre Sterne etwa 100 Milliarden Sonnenmassen ausmachen. Die Andromedagalaxie wird seit langem wissenschaftlich untersucht. Es gelang allerdings erst Ende des 19. Jahrhunderts, dieses zuvor auch in Teleskopen nur als Nebelfleck erscheinende Objekt als Spiralnebel, gebildet aus Sternen, n\u00E4her zu bestimmen. Anhand der Andromedagalaxie wurde dann in den 1920er Jahren festgestellt, dass Spiralnebel eigenst\u00E4ndige, au\u00DFerhalb der Milchstra\u00DFe gelegene Sternsysteme sind. Damit schritt der Erkenntnisgewinn einher, dass das Weltall neben der Milchstra\u00DFe aus zahlreichen weiteren Galaxien besteht. Abweichungen zwischen berechneter und beobachteter Rotation in der Andromedagalaxie deuteten seit etwa 1940 auf Dunkle Materie oder eine Abweichung zur Newtonschen Dynamik hin. Seit der Jahrtausendwende findet man vermehrt Spuren einer zur\u00FCckliegenden Kollision mit einer anderen Galaxie."@de ,
		"Andromeda galaxia, Messier 31, M31 edo NGC 224 bezala ere ezaguna, eta, jatorrian, Andromedaren nebulosa (ikus aurrerago), Lurretik 2,5 milioi argi urtera (770 kiloparsecs) dagoen galaxia espiral barratu bat da, baita Esne Bidetik gertuen dagoen galaxia nagusia ere. Galaxiaren izena, lurreko zerutik dator, non Andromeda konstelazioa agertzen den, aldi berean, greziar mitologian, Perseoren emazte izan zen etiopiar edo feniziar printzesaren izena jasotzen duena. Andromeda galaxiaren masa biriala Esne Bidearenaren magnitude berdinekoa da, bilioi bat eguzki masarekin (2,0 \u00D7 1042 kilogramo). Bi galaxietako edozeinen masa zehaztasunez estimatzea zaila da, baina denbora luzez Andromeda galaxia Esne Bidea baino masiboagoa zela uste izan zen, %25 eta %50 arteko tarteagatik. Hori zalantzan jarri du 2018ko azterlan batek, Andromeda galaxiaren masari buruzko estimazio baxuagoa aipatu baitzuen, esne-bidearen masa altuagoa zenbatesten duen 2019ko azterlanari buruzko aurretiazko txostenekin konbinatuta. Andromeda galaxiak, 220.000 ly (67 kpc) inguruko diametroa du, hedadurari dagokionez, Talde Lokaleko kide handiena bihurtzen duena. Andromeda galaxiak duen izar kopurua bilioi batean (1 \u00D7 1012) estimatzen da, hau da, Esne Biderako estimatutako kopuruaren bikoitza gutxi gorabehera. Esne Bidearen eta Andromedaren galaxiek 4.000 edo 5.000 milioi urte barru talka egitea espero da, galaxia eliptiko erraldoi bat edo galaxia lentikular handi bat sortzeko bat eginez. 3,4ko itxurazko magnitudearekin, Andromeda galaxia Messier objektu distiratsuenen artean dago, Lurretik begi hutsez ilargirik gabeko gauetan ikusgarri bihurtzen duena, baita argi-kutsadura moderatua duten guneetatik ikusten denean ere."@eu ,
		"\u30A2\u30F3\u30C9\u30ED\u30E1\u30C0\u9280\u6CB3\uFF08\u30A2\u30F3\u30C9\u30ED\u30E1\u30C0\u304E\u3093\u304C\u3001M31\u3001NGC 224\uFF09\u306F\u3001\u30A2\u30F3\u30C9\u30ED\u30E1\u30C0\u5EA7\u306B\u4F4D\u7F6E\u3059\u308B\u5730\u7403\u304B\u3089\u76EE\u8996\u53EF\u80FD\u306A\u6E26\u5DFB\u9280\u6CB3\u3067\u3042\u308B\u3002\u3055\u3093\u304B\u304F\u5EA7\u9280\u6CB3 (M33) \u3001\u9280\u6CB3\u7CFB\uFF08\u5929\u306E\u5DDD\u9280\u6CB3\uFF09\u3001\u5927\u30DE\u30BC\u30E9\u30F3\u96F2\u3001\u5C0F\u30DE\u30BC\u30E9\u30F3\u96F2\u306A\u3069\u3068\u3068\u3082\u306B\u5C40\u6240\u9280\u6CB3\u7FA4\u3092\u69CB\u6210\u3059\u308B\u3002"@ja ,
		"\u4ED9\u5973\u5EA7\u661F\u7CFB\uFF08Andromeda Galaxy\uFF0C\u570B\u969B\u97F3\u6A19\u70BA\uFF1A/\u02CCan\u02C8dr\u0252m\u0259d\u0259/\uFF0C\u4E5F\u7A31\u70BA\u6885\u897F\u803631\u3001\u661F\u8868\u7F16\u53F7\u4E3AM31\u548CNGC 224\uFF0C\u5728\u820A\u6587\u737B\u4E2D\u66FE\u7D93\u7A31\u70BA\u4ED9\u5973\u5EA7\u661F\u96F2\uFF0C\u5728\u4E2D\u56FD\u53E4\u4EE3\u88AB\u79F0\u4E3A\u594E\u5BBF\u589E\u5EFF\u4E00\uFF09\u662F\u4E00\u500B\u68D2\u65CB\u661F\u7CFB\uFF0C\u8DDD\u96E2\u5730\u7403\u5927\u7D04250\u842C\u5149\u5E74\uFF0C\u662F\u9664\u9EA6\u54F2\u4F26\u4E91\uFF08\u5730\u7403\u6240\u5728\u7684\u94F6\u6CB3\u7CFB\u7684\u4F34\u661F\u7CFB\uFF09\u4EE5\u5916\u6700\u8FD1\u7684\u661F\u7CFB\u3002 \u4ED9\u5973\u5EA7\u661F\u7CFB\u4F4D\u65BC\u4ED9\u5973\u5EA7\u65B9\u5411\uFF0C\u662F\u4EBA\u985E\u8089\u773C\u53EF\u898B\uFF083.4\u7B49\u661F\uFF09\u6700\u9060\u7684\u6DF1\u7A7A\u5929\u9AD4\u3002\u4ED9\u5973\u5EA7\u661F\u7CFB\u88AB\u76F8\u4FE1\u662F\u672C\u661F\u7CFB\u7FA4\u4E2D\u6700\u5927\u7684\u661F\u7CFB\uFF0C\u76F4\u5F84\u7EA620\u4E07\u5149\u5E74\uFF0C\u5916\u8868\u9887\u4F3C\u94F6\u6CB3\u7CFB\u3002\u672C\u661F\u7CFB\u7FA4\u7684\u6210\u54E1\u6709\u4ED9\u5973\u661F\u7CFB\u3001\u9280\u6CB3\u7CFB\u3001\u4E09\u89D2\u5EA7\u661F\u7CFB\uFF0C\u9084\u6709\u5927\u7D0450\u500B\u5C0F\u661F\u7CFB\u3002\u4F46\u6839\u64DA\u6539\u9032\u7684\u6E2C\u91CF\u6280\u8853\u548C\u4E8C\u5341\u4E00\u4E16\u7D00\u521D\u7814\u7A76\u7684\u6578\u64DA\u7D50\u679C\uFF0C\u79D1\u5B78\u5BB6\u73FE\u5728\u76F8\u4FE1\u9280\u6CB3\u7CFB\u6709\u8A31\u591A\u7684\u6697\u7269\u8CEA\uFF0C\u4E26\u4E14\u53EF\u80FD\u662F\u5728\u9019\u500B\u96C6\u5718\u4E2D\u8CEA\u91CF\u6700\u5927\u7684\u3002\u7136\u800C\uFF0C\u53F2\u5339\u54F2\u592A\u7A7A\u671B\u9060\u93E1\u6700\u8FD1\u7684\u89C0\u6E2C\u986F\u793A\u4ED9\u5973\u5EA7\u661F\u7CFB\u6709\u5C07\u8FD1\u4E00\u5146\uFF081012\uFF09\u9846\u6046\u661F\uFF0C\u6578\u91CF\u9060\u6BD4\u6211\u5011\u7684\u9280\u6CB3\u7CFB\u591A\u3002\u57282006\u5E74\u91CD\u65B0\u4F30\u8A08\u9280\u6CB3\u7CFB\u7684\u8CEA\u91CF\u5927\u7D04\u662F\u4ED9\u5973\u5EA7\u661F\u7CFB\u768450\uFF05\uFF0C\u662F7.1\u00D71011M\u2609.\u4ED9\u5973\u5EA7\u661F\u7CFB\u5728\u9069\u5EA6\u9ED1\u6697\u7684\u5929\u7A7A\u74B0\u5883\u4E0B\u5F88\u5BB9\u6613\u7528\u8089\u773C\u770B\u898B\uFF0C\u4F46\u662F\u5982\u6B64\u7684\u5929\u7A7A\u50C5\u5B58\u5728\u65BC\u5C0F\u93AE\u3001\u88AB\u9694\u7D55\u7684\u5340\u57DF\u3001\u548C\u96E2\u4EBA\u53E3\u96C6\u4E2D\u5340\u57DF\u5F88\u9060\u7684\u5730\u65B9\uFF0C\u53EA\u53D7\u5230\u8F15\u5EA6\u5149\u6C61\u67D3\u7684\u74B0\u5883\u4E0B\u3002\u8089\u773C\u770B\u898B\u7684\u4ED9\u5973\u5EA7\u661F\u7CFB\u975E\u5E38\u5C0F\uFF0C\u56E0\u70BA\u5B83\u53EA\u6709\u4E2D\u5FC3\u4E00\u5C0F\u584A\u7684\u5340\u57DF\u6709\u8DB3\u5920\u7684\u4EAE\u5EA6\uFF0C\u4F46\u662F\u9019\u500B\u661F\u7CFB\u5B8C\u6574\u7684\u89D2\u76F4\u5F91\u6709\u6EFF\u6708\u7684\u4E03\u500D\u5927\u3002"@zh ,
		"\u0645\u062C\u0631\u0629 \u0627\u0644\u0645\u0631\u0623\u0629 \u0627\u0644\u0645\u0633\u0644\u0633\u0644\u0629 (\u0628\u0627\u0644\u0625\u0646\u062C\u0644\u064A\u0632\u064A\u0629: Andromeda)\u200F (\u062A\u0633\u0645\u0649 \u0623\u064A\u0636\u0627 NGC 224 \u0648M31) \u0647\u064A \u0623\u0642\u0631\u0628 \u0627\u0644\u0645\u062C\u0631\u0627\u062A \u0644\u0645\u062C\u0631\u062A\u0646\u0627 (\u0623\u064A \u0623\u0642\u0631\u0628 \u0645\u062C\u0631\u0629 \u0643\u0628\u064A\u0631\u0629\u060C \u0639\u0644\u0649 \u0627\u0644\u0631\u063A\u0645 \u0645\u0646 \u0643\u0648\u0646 \u0645\u062C\u0631\u0629 \u0643\u0627\u0646\u064A\u0633 \u0645\u064A\u062C\u0648\u0631 \u0627\u0644\u0642\u0632\u0645\u0629 \u0623\u0642\u0631\u0628 \u0645\u062C\u0631\u0629 \u0642\u0632\u0645\u0629 \u0625\u0644\u0649 \u062F\u0631\u0628 \u0627\u0644\u062A\u0628\u0627\u0646\u0629)\u060C \u0648\u064A\u0645\u0643\u0646 \u0645\u0634\u0627\u0647\u062F\u062A\u0647\u0627 \u0628\u0627\u0644\u0639\u064A\u0646 \u0627\u0644\u0645\u062C\u0631\u062F\u0629 \u0628\u062F\u0648\u0646 \u0627\u0633\u062A\u062E\u062F\u0627\u0645 \u0627\u0644\u0645\u0642\u0631\u0627\u0628\u060C \u0648\u0647\u064A \u062A\u0628\u0639\u062F \u0639\u0646\u0627 \u0646\u062D\u0648 2.5 \u0645\u0644\u064A\u0648\u0646 \u0633\u0646\u0629 \u0636\u0648\u0626\u064A\u0629. \u0648\u062A\u062D\u062A\u0648\u0649 \u0639\u0644\u0649 \u0646\u062D\u0648 250 \u0645\u0644\u064A\u0627\u0631 \u0646\u062C\u0645 \u0648\u064A\u0628\u0644\u063A \u0642\u0637\u0631\u0647\u0627 220 \u0623\u0644\u0641 \u0633\u0646\u0629 \u0636\u0648\u0626\u064A\u0629\u060C \u0648\u0647\u064A \u0628\u0630\u0644\u0643 \u0623\u0643\u0628\u0631 \u0645\u0646 \u0645\u062C\u0631\u062A\u0646\u0627 \u0627\u0644\u062A\u064A \u064A\u0642\u062F\u0631 \u0639\u062F\u062F \u0627\u0644\u0646\u062C\u0648\u0645 \u0641\u064A\u0647\u0627 \u0645\u0627 \u0628\u064A\u0646 200-400 \u0645\u0644\u064A\u0627\u0631 \u0645\u0646 \u0627\u0644\u0646\u062C\u0648\u0645. \u062A\u0639\u062A\u0628\u0631 \u0645\u062C\u0631\u0629 \u0627\u0644\u0645\u0631\u0623\u0629 \u0627\u0644\u0645\u0633\u0644\u0633\u0644\u0629 \u0645\u0646 \u0627\u0644\u0645\u062C\u0631\u0627\u062A \u0627\u0644\u062A\u064A \u0643\u062A\u0628 \u0639\u0646\u0647\u0627 \u0627\u0644\u0643\u062B\u064A\u0631 \u0645\u0646 \u0627\u0644\u0643\u062A\u0627\u0628 \u0641\u064A \u0631\u0648\u0627\u064A\u0627\u062A \u0627\u0644\u062E\u064A\u0627\u0644 \u0627\u0644\u0639\u0644\u0645\u064A."@ar ,
		"La Andromeda Galaksio (M31, Messier 31, aliaj indikoj \u2014 NGC 224, PGC 2557, UGC 454, MCG 7-2-16, ZWG 535.17) estas galaksio en konstelacio Andromedo, la\u016D kiu \u011Di estis nomita. En la astronomia katalogo de Messier \u011Di havas la nomon \"M31\".\u0108i tiu objekto estis jam en la originala versio de NGC-katalogo. \u011Ci situas \u0109irka\u016D 2,52 milionoj da lumjaroj for de ni kaj estas la plej malproksima objekto videbla nudokule de sur Tero. \u011Ci estas la plej granda galaksio en la \"loka grupo\" de galaksioj, al kiuj apartenas nia propra galaksio, la Lakta vojo. Tiuj du galaksioj tiom proksimas, ke pro gravito ili proksimi\u011Dadas, kvankam \u011Denerale galaksioj malproksimi\u011Das.Post \u0109irka\u016D tri miliardoj da jaroj la du galaksioj kolizios kaj unui\u011Dos, formante eliptikan galaksion. La Andromeda Galaksio kaj la Magelanaj Nuboj estas la solaj galaksioj videblaj nudokule, la Andromeda Galaksio kiel svaga makuleto iom flanke de la tri la\u016Dvicaj steloj de Andromedo. Sed fakte tiu svaga makuleto ne estas la Galaksio, kiu proksima kiom \u011Di estas de la tero havas angulan diametron sepoblan tiun de la luno. Pro malfortigo de \u011Dia lumo nur la densega centro, tiaforme, videblas. NGC 206 estas parto de Andromeda galaksio."@eo ,
		"\uC548\uB4DC\uB85C\uBA54\uB2E4 \uC740\uD558(\uC601\uC5B4: Andromeda Galaxy)\uB294 \uC9C0\uAD6C\uB85C\uBD80\uD130 \uC57D 780 \uD0AC\uB85C\uD30C\uC139(250\uB9CC \uAD11\uB144) \uB5A8\uC5B4\uC838 \uC788\uB294 \uB098\uC120\uC740\uD558\uC774\uB2E4. \uC774\uB294 \uC6B0\uB9AC\uC740\uD558\uB85C\uBD80\uD130 \uAC00\uC7A5 \uAC00\uAE4C\uC6B4 \uD070 \uC740\uD558(major galaxy)\uC774\uBA70, \uBA54\uC2DC\uC5D0 31(M31) \uB610\uB294 NGC 224\uB85C \uC54C\uB824\uC838 \uC788\uAE30\uB3C4 \uD558\uB2E4. \uC61B \uBB38\uD5CC\uC5D0\uC11C\uB294 \uC885\uC885 \uC548\uB4DC\uB85C\uBA54\uB2E4\uC790\uB9AC \uB300\uC131\uC6B4(Andromeda\u5927\u661F\u96F2)\uC73C\uB85C \uD45C\uD604\uB418\uC5C8\uB2E4. \uC740\uD558\uC758 \uBA85\uCE6D\uC740 \uC740\uD558\uAC00 \uBCF4\uC774\uB294 \uBCC4\uC790\uB9AC, \uC989 \uC548\uB4DC\uB85C\uBA54\uB2E4\uC790\uB9AC\uC758 \uBA85\uCE6D\uC744 \uB530\uC11C \uBD99\uC5EC\uC84C\uB2E4. \uC5EC\uAE30\uC11C \uC548\uB4DC\uB85C\uBA54\uB2E4\uC790\uB9AC\uB294 \uADF8\uB9AC\uC2A4 \uC2E0\uD654\uC758 \uC548\uB4DC\uB85C\uBA54\uB2E4 \uACF5\uC8FC\uC758 \uC774\uB984\uC744 \uB530 \uBD99\uC5EC\uC9C4 \uBCC4\uC790\uB9AC\uC774\uB2E4. \uD3ED\uC774 \uB300\uB7B5 22\uB9CC \uAD11\uB144\uC778 \uC548\uB4DC\uB85C\uBA54\uB2E4 \uC740\uD558\uB294 \uC6B0\uB9AC \uC740\uD558 \uBC0F \uC0BC\uAC01\uD615\uC790\uB9AC \uC740\uD558\uC640 \uB300\uB7B5 44\uAC1C\uC758 \uC791\uC740 \uC740\uD558\uB4E4\uC744 \uD3EC\uD568\uD558\uB294 \uAD6D\uBD80\uC740\uD558\uAD70\uC5D0\uC11C \uAC00\uC7A5 \uD070 \uC740\uD558\uC774\uB2E4. \uCD08\uAE30\uC758 \uD0D0\uC0AC\uB4E4\uC740 \uC6B0\uB9AC\uC740\uD558\uAC00 \uB354 \uB9CE\uC740 \uC554\uD751\uBB3C\uC9C8\uC744 \uD3EC\uD568\uD558\uBA70 \uAD6D\uBD80\uC740\uD558\uAD70\uC5D0\uC11C \uAC00\uC7A5 \uD074 \uAC83\uC774\uB77C\uACE0 \uC2DC\uC0AC\uD558\uC600\uC9C0\uB9CC, 2006\uB144 \uC2A4\uD53C\uCC98 \uC6B0\uC8FC \uB9DD\uC6D0\uACBD\uC744 \uD1B5\uD55C \uAD00\uCE21\uB4E4\uC740 \uC548\uB4DC\uB85C\uBA54\uB2E4 \uC740\uD558\uAC00 2,000~4,000\uC5B5 \uAC1C\uC758 \uBCC4\uB4E4\uC744 \uD3EC\uD568\uD560 \uAC83\uC73C\uB85C \uCD94\uC815\uB418\uB294 \uC6B0\uB9AC\uC740\uD558\uC758 \uC801\uC5B4\uB3C4 \uB450 \uBC30\uC5D0 \uD574\uB2F9\uD558\uB294, 1\uC870 \uAC1C\uC758 \uBCC4\uB4E4\uC744 \uD3EC\uD568\uD558\uB294 \uAC83\uC744 \uBCF4\uC5EC\uC8FC\uC5C8\uB2E4. \uC6B0\uB9AC\uC740\uD558\uC758 \uC9C8\uB7C9\uC774 8.5 \u00D7 1011 \uD0DC\uC591\uC9C8\uB7C9\uC73C\uB85C \uCD94\uC815\uB418\uB294 \uB370 \uBE44\uD574, \uC548\uB4DC\uB85C\uBA54\uB2E4 \uC740\uD558\uC758 \uC9C8\uB7C9\uC740 1.5 \u00D7 1012 \uD0DC\uC591\uC9C8\uB7C9\uC73C\uB85C \uCD94\uC815\uB41C\uB2E4. 2006\uB144\uC758 \uC5F0\uAD6C\uAC00 \uC6B0\uB9AC\uC740\uD558\uC758 \uC9C8\uB7C9\uC774 \uC548\uB4DC\uB85C\uBA54\uB2E4 \uC740\uD558\uC758 \uC9C8\uB7C9\uC758 ~80%\uC784\uC744 \uC81C\uC2DC\uD558\uC600\uC9C0\uB9CC, 2009\uB144\uC758 \uC5F0\uAD6C\uC5D0\uC11C\uB294 \uC6B0\uB9AC\uC740\uD558\uC640 \uC548\uB4DC\uB85C\uBA54\uB2E4 \uC740\uD558\uC758 \uC9C8\uB7C9\uC774 \uAC70\uC758 \uAC19\uC74C\uC744 \uBCF4\uC5EC\uC8FC\uC5C8\uB2E4. \uC6B0\uB9AC\uC740\uD558\uC640 \uC548\uB4DC\uB85C\uBA54\uB2E4 \uC740\uD558\uB294 37\uC5B5 5\uCC9C\uB9CC \uB144 \uD6C4\uC5D0 \uCDA9\uB3CC\uD560 \uAC83\uC73C\uB85C \uC608\uCE21\uB418\uB294\uB370, \uADF8 \uACB0\uACFC \uC11C\uB85C \uBCD1\uD569\uD558\uC5EC \uAC70\uB300\uD0C0\uC6D0\uC740\uD558 \uB610\uB294 \uAC70\uB300 \uC6D0\uBC18\uC740\uD558\uB97C \uD615\uC131\uD560 \uAC83\uC774\uB2E4. \uC548\uB4DC\uB85C\uBA54\uB2E4 \uC740\uD558\uC758 \uAC89\uBCF4\uAE30 \uB4F1\uAE09\uC740 3.4\uB4F1\uAE09\uC73C\uB85C \uBA54\uC2DC\uC5D0 \uCC9C\uCCB4 \uC911\uC5D0\uC11C \uAC00\uC7A5 \uBC1D\uB2E4. \uB54C\uBB38\uC5D0 \uAD11\uACF5\uD574\uAC00 \uC801\uC740 \uC9C0\uC5ED\uC5D0\uC11C \uB2EC\uC774 \uC5C6\uB294 \uBC24\uC5D0 \uB9E8\uB208\uC73C\uB85C \uBCF4\uC77C \uC815\uB3C4\uC774\uB2E4. \uADF8\uB7EC\uB098 \uD070 \uB9DD\uC6D0\uACBD\uC744 \uD1B5\uD574 \uCD2C\uC601\uB418\uB294 \uC548\uB4DC\uB85C\uBA54\uB2E4 \uC740\uD558\uC758 \uBAA8\uC2B5(\uC2DC\uC9C1\uACBD)\uC774 \uBCF4\uB984\uB2EC\uBCF4\uB2E4 \uC5EC\uC12F\uBC30\uB098 \uD06C\uAE30 \uB54C\uBB38\uC5D0 \uD45C\uBA74\uBC1D\uAE30 \uBB38\uC81C\uB85C \uC778\uD574 \uC624\uB85C\uC9C0 \uBC1D\uC740 \uC911\uC2EC \uC601\uC5ED\uB9CC\uC774 \uB9E8\uB208\uC774\uB098 \uC30D\uC548\uACBD, \uC791\uC740 \uCC9C\uCCB4\uB9DD\uC6D0\uACBD\uC744 \uD1B5\uD574 \uBCF4\uC778\uB2E4. \uADF8\uB798\uC11C \uC740\uD558\uB294 \uC2E4\uC81C\uB85C \uBCC4\uACFC \uC720\uC0AC\uD55C \uBAA8\uC2B5\uC73C\uB85C \uBCF4\uC778\uB2E4. \uC608\uC804\uC5D0 \uC548\uB4DC\uB85C\uBA54\uB2E4\uAC00 \uC6B0\uB9AC \uC740\uD558\uC5D0 \uC18D\uD574\uC788\uB294 \uC131\uC6B4\uC774\uB77C\uB294 \uC758\uACAC\uACFC \uC6B0\uB9AC \uC740\uD558 \uBC16\uC5D0 \uC788\uB294 \uB610 \uB2E4\uB978 \uC740\uD558\uB77C\uB294 \uC758\uACAC\uC774 \uC788\uC5C8\uC9C0\uB9CC \uD5C8\uBE14\uC774 \uB610 \uB2E4\uB978 \uC740\uD558\uB77C\uB294 \uC0AC\uC2E4\uC744 \uBC1D\uD600\uB0C8\uB2E4."@ko ,
		"A gal\u00E1xia de Andr\u00F4meda (portugu\u00EAs brasileiro) ou gal\u00E1xia de Andr\u00F3meda (portugu\u00EAs europeu) (Messier 31, NGC 224) \u00E9 uma gal\u00E1xia espiral localizada a cerca de 2,54 milh\u00F5es de anos-luz de dist\u00E2ncia da Terra, na dire\u00E7\u00E3o da constela\u00E7\u00E3o de Andr\u00F4meda. \u00C9 a gal\u00E1xia espiral mais pr\u00F3xima da Via L\u00E1ctea e seu nome \u00E9 derivado da constela\u00E7\u00E3o onde est\u00E1 situada, que, por sua vez, tem o nome derivado da princesa mitol\u00F3gica Andr\u00F4meda. \u00C9 a maior gal\u00E1xia do Grupo Local, que tamb\u00E9m cont\u00E9m a Via L\u00E1ctea, a gal\u00E1xia do Tri\u00E2ngulo e aproximadamente 30 outras menores. O levantamento feito pelo Telesc\u00F3pio Espacial Spitzer em 2006 determinou que sua massa \u00E9 de aproximadamente ~0,8-1,5 \u00D7 1012 massas solares enquanto a Via L\u00E1ctea tem uma massa estimada em 8,5 \u00D7 1011 massas solares. Sua popula\u00E7\u00E3o estelar atinge aproximadamente 1 trilh\u00E3o de estrelas enquanto a Via L\u00E1ctea conta com algo entre 200 a 400 bilh\u00F5es de estrelas. Com uma magnitude aparente de 3,4, \u00E9 um dos objetos astron\u00F4micos mais brilhantes do cat\u00E1logo de objetos do c\u00E9u profundo do astr\u00F4nomo franc\u00EAs Charles Messier, vis\u00EDvel a olho nu na aus\u00EAncia da Lua. Possui entre 180 e 220 mil anos-luz de di\u00E2metro e uma magnitude absoluta de -21,4."@pt ,
		"M31(\nPour les articles homonymes, voir Androm\u00E8de, n\u00E9buleuse d'Androm\u00E8de et M31. ) La galaxie d'Androm\u00E8de, \u00E9galement d\u00E9sign\u00E9e M31 dans le Catalogue de Messier et NGC 224, est une galaxie spirale situ\u00E9e \u00E0 environ 2,55 millions d'ann\u00E9es-lumi\u00E8re du Soleil, dans la constellation d'Androm\u00E8de. La galaxie d'Androm\u00E8de (NGC 224) a \u00E9t\u00E9 utilis\u00E9e par G\u00E9rard de Vaucouleurs comme une galaxie de type morphologique SA(s)b dans son atlas des galaxies. Appel\u00E9e grande n\u00E9buleuse d\u2019Androm\u00E8de jusqu'\u00E0 ce que sa vraie nature ait \u00E9t\u00E9 reconnue dans les ann\u00E9es 1920, la galaxie d'Androm\u00E8de est la galaxie spirale la plus proche de la Voie lact\u00E9e (toutes classes confondues, la galaxie la plus proche est la naine du Grand Chien) et le plus grand membre du Groupe local d'une soixantaine de galaxies individuelles dont toutes deux font partie. D'un diam\u00E8tre d'environ 220 000 ann\u00E9es-lumi\u00E8re, elle contiendrait environ mille milliards d'\u00E9toiles, deux \u00E0 cinq fois plus que notre galaxie. Avec une magnitude visuelle de 3,4, la galaxie d'Androm\u00E8de est l\u2019une des rares galaxies observables \u00E0 l'\u0153il nu depuis la Terre dans l\u2019h\u00E9misph\u00E8re nord. C\u2019est \u00E9galement l'un des objets les plus \u00E9tendus de la vo\u00FBte c\u00E9leste, avec un diam\u00E8tre apparent de 3,18\u00B0, soit plus de six fois le diam\u00E8tre apparent de la Lune observ\u00E9e depuis la Terre."@fr ,
		"Andromedagalaxen, NGC 224 eller M31, \u00E4r en spiralgalax av typ i Vintergatans n\u00E4romr\u00E5de som \u00E4r svagt synlig med blotta \u00F6gat. Den \u00E5terfinns i stj\u00E4rnbilden Andromeda som givit den dess namn. Andromedagalaxen ligger p\u00E5 ett avst\u00E5nd av 2,5\u20132,9 miljoner ljus\u00E5r fr\u00E5n Vintergatan och \u00E4r den n\u00E4rmaste granngalaxen om man inte r\u00E4knar Vintergatans sm\u00E5 satellitgalaxer. M\u00E4tningar visar att den \u00E4r p\u00E5 kollisionskurs med Vintergatan med en radiell hastighet p\u00E5 cirka 120 km/s och galaxerna kommer sannolikt att krocka om cirka 3 miljarder \u00E5r, beroende p\u00E5 hur stor den ok\u00E4nda transversella hastigheten \u00E4r. Resultatet av denna kollision blir f\u00F6rmodligen att de sm\u00E4lter samman till en stor elliptisk galax. Andromedagalaxen \u00E4r med en synlig diameter p\u00E5 165 000\u2013200 000 ljus\u00E5r 1,5\u20132 g\u00E5nger s\u00E5 stor som Vintergatan och \u00E4r den st\u00F6rsta galaxen i den lokala galaxhopen. Dess utstr\u00E4ckning p\u00E5 stj\u00E4rnhimlen \u00E4r cirka 3\u00D71 grader vilket \u00E4r mycket st\u00F6rre \u00E4n m\u00E5nens (cirka 0,5 grad). F\u00F6r blotta \u00F6gat \u00E4r dock storleken mindre eftersom endast den centrala ljusa k\u00E4rnan \u00E4r synlig utan teleskop. Andromedagalaxen \u00E5tf\u00F6ljs av ett 10-tal satellitgalaxer, varav ett par (M32 och M110, se bilden) observerades redan av Messier. M32 tycks ha haft \"n\u00E4rkontakt\" med huvudgalaxen och d\u00E4rvid b\u00E5de st\u00F6rt spiralstrukturen p\u00E5 denna och f\u00F6rlorat en viss del av sitt eget stj\u00E4rnbest\u00E5nd. Endast en g\u00E5ng har en supernova observerats i Andromedagalaxen. Det skedde 1885 och var den f\u00F6rsta supernovan utanf\u00F6r Vintergatan som n\u00E5gonsin observerats."@sv ,
		"Galaxie v Andromed\u011B je spir\u00E1ln\u00ED galaxie, vzd\u00E1len\u00E1 p\u0159ibli\u017En\u011B 2,5 mili\u00F3nu sv\u011Bteln\u00FDch let (2,4\u00D71019 km) od Zem\u011B, v souhv\u011Bzd\u00ED Andromedy. Je tak\u00E9 zn\u00E1ma pod katalogov\u00FDm ozna\u010Den\u00EDm Messier 31 (M31) a NGC 224, ve star\u0161\u00ED astronomick\u00E9 literatu\u0159e m\u00E1 \u010Dasto ozna\u010Den\u00ED Velk\u00E1 mlhovina v Andromed\u011B. Galaxie v Andromed\u011B je nejbli\u017E\u0161\u00ED spir\u00E1ln\u00ED galaxie od na\u0161\u00ED Ml\u00E9\u010Dn\u00E9 dr\u00E1hy, ale nen\u00ED nejbli\u017E\u0161\u00ED galaxi\u00ED. M\u00E1 jm\u00E9no po oblasti hv\u011Bzdn\u00E9 oblohy, ve kter\u00E9 se nach\u00E1z\u00ED a kter\u00E1 je pojmenov\u00E1na po mytologick\u00E9 princezn\u011B Andromed\u011B. Galaxie v Andromed\u011B je nejv\u011Bt\u0161\u00ED galaxie z M\u00EDstn\u00ED skupiny galaxi\u00ED, kter\u00E1 tak\u00E9 obsahuje na\u0161i Ml\u00E9\u010Dnou dr\u00E1hu, Galaxii v Troj\u00FAheln\u00EDku a p\u0159ibli\u017En\u011B 30 dal\u0161\u00EDch men\u0161\u00EDch galaxi\u00ED. P\u0159esto\u017Ee je nejv\u011Bt\u0161\u00ED, nemus\u00ED b\u00FDt nejhmotn\u011Bj\u0161\u00ED, ned\u00E1vn\u00E1 zji\u0161t\u011Bn\u00ED nazna\u010Duj\u00ED, \u017Ee Ml\u00E9\u010Dn\u00E1 dr\u00E1ha obsahuje v\u00EDce temn\u00E9 hmoty, a proto m\u016F\u017Ee b\u00FDt nejhmotn\u011Bj\u0161\u00ED galaxi\u00ED v M\u00EDstn\u00ED skupin\u011B. Pozorov\u00E1n\u00EDm Spitzerova vesm\u00EDrn\u00E9ho dalekohledu bylo zji\u0161t\u011Bno, \u017Ee v galaxii M31 se nach\u00E1z\u00ED bili\u00F3n (1012) hv\u011Bzd, co\u017E je nejm\u00E9n\u011B dvojn\u00E1sobn\u00FD po\u010Det hv\u011Bzd Ml\u00E9\u010Dn\u00E9 dr\u00E1hy, jejich\u017E po\u010Det se odhaduje na 200 a\u017E 400 miliard. Hmotnost Galaxie v Andromed\u011B se odhaduje na 7,1\u00D71011 Slunc\u00ED.Studie z roku 2009 odhadla, \u017Ee Ml\u00E9\u010Dn\u00E1 dr\u00E1ha a M31 maj\u00ED p\u0159ibli\u017En\u011B stejnou hmotnost, jin\u00E1 studie z roku 2006 odhadla hmotnost na\u0161\u00ED galaxie na p\u0159ibli\u017En\u011B 80 % hmotnosti Galaxie v Andromed\u011B. O\u010Dek\u00E1v\u00E1 se, \u017Ee ob\u011B galaxie se za v\u00EDce ne\u017E 4,5 miliardy let za\u010Dnou spojovat a pravd\u011Bpodobn\u011B vytvo\u0159\u00ED ob\u0159\u00ED eliptickou galaxii.Galaxie m\u00E1 zd\u00E1nlivou hv\u011Bzdnou velikost 3,4m, je jedn\u00EDm z nejjasn\u011Bj\u0161\u00EDch objekt\u016F Messierova katalogu, lze ji spat\u0159it pouh\u00FDm okem za bezm\u011Bs\u00ED\u010Dn\u00E9 noci, i p\u0159i pohledu z oblast\u00ED s mal\u00FDm sv\u011Bteln\u00FDm zne\u010Di\u0161t\u011Bn\u00EDm. Na fotografi\u00EDch po\u0159\u00EDzen\u00FDch v\u011Bt\u0161\u00EDm dalekohledem se jev\u00ED \u0161estkr\u00E1t v\u011Bt\u0161\u00ED ne\u017E M\u011Bs\u00EDc v \u00FApl\u0148ku, viditeln\u00E1 pouh\u00FDm okem nebo mal\u00FDm dalekohledem \u010Di triedrem je ale pouze jej\u00ED centr\u00E1ln\u00ED oblast."@cs ,
		"La galaxia de Andr\u00F3meda, tambi\u00E9n conocida como Galaxia Espiral M31, Messier 31 o NGC 224, es una galaxia espiral con un di\u00E1metro de doscientos veinte mil a\u00F1os luz (en lo que concierne a su halo gal\u00E1ctico) y de unos ciento cincuenta mil a\u00F1os luz entre los extremos de sus brazos. Es el objeto visible a simple vista m\u00E1s lejano de la Tierra (aunque algunos afirman poder ver a simple vista la galaxia del Tri\u00E1ngulo, que est\u00E1 un poco m\u00E1s lejos). Est\u00E1 a 2,5 millones de a\u00F1os luz\u200B en direcci\u00F3n a la constelaci\u00F3n de Andr\u00F3meda. Es, junto con nuestra propia galaxia, la m\u00E1s grande y brillante de las galaxias del Grupo Local, que consiste en aproximadamente 30 peque\u00F1as galaxias m\u00E1s tres grandes galaxias espirales: Andr\u00F3meda, la V\u00EDa L\u00E1ctea y la galaxia del Tri\u00E1ngulo. La galaxia se est\u00E1 acercando a nosotros a unos 300 kil\u00F3metros por hora,\u200B y algunos especulan que ambas colisionen en unos 5860 millones de a\u00F1os en el futuro fusion\u00E1ndose en una galaxia mayor,\u200B en el evento conocido como Lact\u00F3meda. Aunque muchos confunden Andr\u00F3meda y Enana del Can Major, por pensar que una de ellas es la m\u00E1s cercana a la V\u00EDa l\u00E1ctea, lo que bien es cierto que Andr\u00F3meda es la galaxia espiral m\u00E1s cercana a la V\u00EDa L\u00E1ctea, la Enana del Can Major es la galaxia m\u00E1s cercana a la nuestra, no obstante la existencia de la cercana galaxia se ha disputado,\u200B en caso de no existir la Enana del Can Mayor, el t\u00EDtulo de la galaxia m\u00E1s cercana corresponder\u00EDa a la Enana El\u00EDptica de Sagitario (v\u00E9ase Anexo:Galaxias m\u00E1s cercanas)."@es ,
		"\u0413\u0430\u043B\u0430\u0301\u043A\u0442\u0438\u043A\u0430 \u0410\u043D\u0434\u0440\u043E\u043C\u0435\u0301\u0434\u044B (\u0422\u0443\u043C\u0430\u0301\u043D\u043D\u043E\u0441\u0442\u044C \u0410\u043D\u0434\u0440\u043E\u043C\u0435\u0301\u0434\u044B, M 31, NGC 224, PGC 2557) \u2014 \u0441\u043F\u0438\u0440\u0430\u043B\u044C\u043D\u0430\u044F \u0433\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u0430, \u043D\u0430\u0431\u043B\u044E\u0434\u0430\u0435\u043C\u0430\u044F \u0432 \u0441\u043E\u0437\u0432\u0435\u0437\u0434\u0438\u0438 \u0410\u043D\u0434\u0440\u043E\u043C\u0435\u0434\u044B. \u0415\u0451 \u0434\u0438\u0430\u043C\u0435\u0442\u0440 \u0441\u043E\u0441\u0442\u0430\u0432\u043B\u044F\u0435\u0442 47 \u043A\u0438\u043B\u043E\u043F\u0430\u0440\u0441\u0435\u043A, \u0447\u0442\u043E \u0431\u043E\u043B\u044C\u0448\u0435, \u0447\u0435\u043C \u0443 \u043D\u0430\u0448\u0435\u0439 \u0413\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u0438, \u0438 \u043E\u043D\u0430 \u0441\u043E\u0434\u0435\u0440\u0436\u0438\u0442 \u0432 \u043D\u0435\u0441\u043A\u043E\u043B\u044C\u043A\u043E \u0440\u0430\u0437 \u0431\u043E\u043B\u044C\u0448\u0435 \u0437\u0432\u0451\u0437\u0434, \u0447\u0435\u043C \u041C\u043B\u0435\u0447\u043D\u044B\u0439 \u041F\u0443\u0442\u044C. \u0420\u0430\u0441\u0441\u0442\u043E\u044F\u043D\u0438\u0435 \u043E\u0442 \u043D\u0430\u0448\u0435\u0439 \u0413\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u0438 \u0434\u043E \u043D\u0435\u0451 \u0441\u043E\u0441\u0442\u0430\u0432\u043B\u044F\u0435\u0442 \u043E\u043A\u043E\u043B\u043E 800 \u043A\u0438\u043B\u043E\u043F\u0430\u0440\u0441\u0435\u043A, \u0447\u0442\u043E \u0434\u0435\u043B\u0430\u0435\u0442 \u0435\u0451 \u0431\u043B\u0438\u0436\u0430\u0439\u0448\u0435\u0439 \u0438\u0437 \u043A\u0440\u0443\u043F\u043D\u044B\u0445 \u0433\u0430\u043B\u0430\u043A\u0442\u0438\u043A, \u0430 \u0442\u0430\u043A\u0436\u0435 \u043A\u0440\u0443\u043F\u043D\u0435\u0439\u0448\u0435\u0439 \u0433\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u043E\u0439 \u041C\u0435\u0441\u0442\u043D\u043E\u0439 \u0433\u0440\u0443\u043F\u043F\u044B. \u0415\u0451 \u043C\u0430\u0441\u0441\u0430 \u043F\u0440\u0438\u0431\u043B\u0438\u0437\u0438\u0442\u0435\u043B\u044C\u043D\u043E \u0440\u0430\u0432\u043D\u0430 \u043C\u0430\u0441\u0441\u0435 \u041C\u043B\u0435\u0447\u043D\u043E\u0433\u043E \u041F\u0443\u0442\u0438 \u0438\u043B\u0438 \u0434\u0430\u0436\u0435 \u043C\u0435\u043D\u044C\u0448\u0435. \u0413\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u0430 \u0410\u043D\u0434\u0440\u043E\u043C\u0435\u0434\u044B \u0438\u043C\u0435\u0435\u0442 \u043A\u0430\u043A \u0432\u044B\u0440\u0430\u0436\u0435\u043D\u043D\u0443\u044E \u0441\u0444\u0435\u0440\u0438\u0447\u0435\u0441\u043A\u0443\u044E \u043F\u043E\u0434\u0441\u0438\u0441\u0442\u0435\u043C\u0443, \u0442\u0430\u043A \u0438 \u0434\u0438\u0441\u043A \u0441 \u0437\u0430\u043C\u0435\u0442\u043D\u044B\u043C\u0438 \u0441\u043F\u0438\u0440\u0430\u043B\u044C\u043D\u044B\u043C\u0438 \u0440\u0443\u043A\u0430\u0432\u0430\u043C\u0438, \u043F\u043E\u044D\u0442\u043E\u043C\u0443 \u043F\u043E \u043A\u043B\u0430\u0441\u0441\u0438\u0444\u0438\u043A\u0430\u0446\u0438\u0438 \u0425\u0430\u0431\u0431\u043B\u0430 \u0435\u0451 \u043E\u0442\u043D\u043E\u0441\u044F\u0442 \u043A \u0442\u0438\u043F\u0443 Sb. \u0414\u0438\u0441\u043A \u0441\u043E\u0434\u0435\u0440\u0436\u0438\u0442 \u0431\u043E\u043B\u0435\u0435 \u043F\u043E\u043B\u043E\u0432\u0438\u043D\u044B \u0437\u0432\u0451\u0437\u0434\u043D\u043E\u0439 \u043C\u0430\u0441\u0441\u044B \u0433\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u0438, \u0438\u043C\u0435\u0435\u0442 \u0438\u0441\u043A\u0440\u0438\u0432\u043B\u0451\u043D\u043D\u0443\u044E \u0444\u043E\u0440\u043C\u0443, \u0432 \u043D\u0451\u043C \u043D\u0430\u0431\u043B\u044E\u0434\u0430\u0435\u0442\u0441\u044F \u043A\u043E\u043B\u044C\u0446\u043E \u0440\u0430\u0434\u0438\u0443\u0441\u043E\u043C 10 \u043A\u0438\u043B\u043E\u043F\u0430\u0440\u0441\u0435\u043A \u0441 \u043F\u043E\u0432\u044B\u0448\u0435\u043D\u043D\u044B\u043C \u0441\u043E\u0434\u0435\u0440\u0436\u0430\u043D\u0438\u0435\u043C \u043E\u0431\u043B\u0430\u0441\u0442\u0435\u0439 H II \u0438 OB-\u0430\u0441\u0441\u043E\u0446\u0438\u0430\u0446\u0438\u0439. \u0411\u0430\u043B\u0434\u0436 \u0438 \u0433\u0430\u043B\u043E \u0441\u043F\u043B\u044E\u0441\u043D\u0443\u0442\u044B, \u0431\u0430\u0440 \u0432 \u0433\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u0435 \u043D\u0430\u043F\u0440\u044F\u043C\u0443\u044E \u043D\u0435 \u043D\u0430\u0431\u043B\u044E\u0434\u0430\u0435\u0442\u0441\u044F, \u043D\u043E \u043D\u0435\u043A\u043E\u0442\u043E\u0440\u044B\u0435 \u043F\u0440\u0438\u0437\u043D\u0430\u043A\u0438 \u0443\u043A\u0430\u0437\u044B\u0432\u0430\u044E\u0442 \u043D\u0430 \u0435\u0433\u043E \u043D\u0430\u043B\u0438\u0447\u0438\u0435. \u0412 \u0446\u0435\u043D\u0442\u0440\u0435 \u0433\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u0438 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\u043D\u0435\u0432\u043E\u043E\u0440\u0443\u0436\u0451\u043D\u043D\u044B\u043C \u0433\u043B\u0430\u0437\u043E\u043C \u0438 \u043F\u043E\u043F\u0443\u043B\u044F\u0440\u043D\u0430 \u043A\u0430\u043A \u043E\u0431\u044A\u0435\u043A\u0442 \u0434\u043B\u044F \u043D\u0430\u0431\u043B\u044E\u0434\u0435\u043D\u0438\u044F \u0441\u0440\u0435\u0434\u0438 \u0430\u0441\u0442\u0440\u043E\u043D\u043E\u043C\u043E\u0432-\u043B\u044E\u0431\u0438\u0442\u0435\u043B\u0435\u0439. \u0413\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u0430 \u044F\u0432\u043B\u044F\u0435\u0442\u0441\u044F \u0440\u0430\u0441\u043F\u0440\u043E\u0441\u0442\u0440\u0430\u043D\u0451\u043D\u043D\u043E\u0439 \u043B\u043E\u043A\u0430\u0446\u0438\u0435\u0439 \u0432 \u043D\u0430\u0443\u0447\u043D\u043E\u0439 \u0444\u0430\u043D\u0442\u0430\u0441\u0442\u0438\u043A\u0435."@ru ,
		"La Galassia di Andromeda (nota talvolta anche con il vecchio nome Grande Nebulosa di Andromeda o con le sigle di catalogo M 31 e NGC 224) \u00E8 una galassia a spirale gigante che dista circa 2,538 milioni di anni luce dalla Terra in direzione della costellazione di Andromeda, da cui prende il nome. Si tratta della galassia di grandi dimensioni pi\u00F9 vicina alla nostra, la Via Lattea; \u00E8 visibile anche a occhio nudo ed \u00E8 tra gli oggetti pi\u00F9 lontani visibili senza l'ausilio di strumenti. La Galassia di Andromeda \u00E8 la pi\u00F9 grande del Gruppo Locale, un gruppo di galassie di cui fanno parte anche la Via Lattea e la Galassia del Triangolo, pi\u00F9 circa cinquanta altre galassie minori, molte delle quali satelliti delle principali. Secondo studi pubblicati negli anni duemila, derivati dalle osservazioni del telescopio spaziale Spitzer, conterrebbe circa un bilione di stelle (mille miliardi), un numero superiore a quello della Via Lattea, stimato tra i 200 e i 400 miliardi di stelle. Sulla massa ci sono tuttavia opinioni discordanti: alcuni studi indicano un valore di massa per la Via Lattea pari all'80% di quello di Andromeda, mentre, secondo altri, le due galassie avrebbero dimensioni di massa simili. Alcuni studi suggeriscono per\u00F2 che la Via Lattea contenga pi\u00F9 materia oscura e potrebbe cos\u00EC essere quella con la massa pi\u00F9 grande. Con una magnitudine apparente pari a 3,4, la Galassia di Andromeda \u00E8 uno degli oggetti pi\u00F9 luminosi del catalogo di Messier."@it ,
		"Galaktyka Andromedy (zwana r\u00F3wnie\u017C Messier 31, M31 lub NGC 224, a wcze\u015Bniej tak\u017Ce Wielk\u0105 Mg\u0142awic\u0105 w Andromedzie) \u2013 galaktyka spiralna, le\u017C\u0105ca oko\u0142o 2,52 miliona lat \u015Bwietlnych od Ziemi w gwiazdozbiorze Andromedy. Do niedawna s\u0105dzono, \u017Ce Galaktyka Andromedy jest najmasywniejsz\u0105 galaktyk\u0105 w Grupie Lokalnej, w sk\u0142ad kt\u00F3rej wchodz\u0105 r\u00F3wnie\u017C Droga Mleczna, Galaktyka Tr\u00F3jk\u0105ta oraz oko\u0142o 50 mniejszych galaktyk. Na podstawie obserwacji w podczerwieni dokonanej z u\u017Cyciem Teleskopu Spitzera w 2006 oszacowano liczb\u0119 gwiazd Andromedy na oko\u0142o bilion, dla por\u00F3wnania liczb\u0119 gwiazd w Drodze Mlecznej szacuje si\u0119 na oko\u0142o 400 miliard\u00F3w. Wirialna masa (masa \u0142\u0105cznie z mas\u0105 ciemnej materii) Galaktyki Andromedy jest tego samego rz\u0119du wielko\u015Bci co Drogi Mlecznej i wynosi oko\u0142o 1 biliona mas S\u0142o\u0144ca. Masa obu galaktyk jest trudna do por\u00F3wnania. W 2018 opublikowano szacunek masy Galaktyki Andromedy na podstawie analizy ruchu galaktyk satelickich, w po\u0142\u0105czeniu ze wst\u0119pnymi raportami z badania z 2019 szacuj\u0105cego wi\u0119ksz\u0105 mas\u0119 Drogi Mlecznej. Galaktyka Andromedy ma \u015Brednic\u0119 oko\u0142o 220 000 ly (67 kpc), co czyni j\u0105 najwi\u0119kszym pod wzgl\u0119dem rozbudowy cz\u0142onkiem Grupy Lokalnej. Galaktyka Andromedy jest najwi\u0119ksz\u0105 i najja\u015Bniejsz\u0105 galaktyk\u0105 nieba p\u00F3\u0142nocnego. Wida\u0107 j\u0105 nawet przez ma\u0142e lornetki. Obserwacje mo\u017Cna prowadzi\u0107 tak\u017Ce go\u0142ym okiem, niekiedy nawet na przedmie\u015Bciach wi\u0119kszych miast, widoczna jest jako niewielka mgie\u0142ka. Jednak jej ca\u0142kowita \u015Brednica k\u0105towa przewy\u017Csza sze\u015Bciokrotnie k\u0105towe rozmiary Ksi\u0119\u017Cyca. Nazwa galaktyki pochodzi od mitologicznej etiopskiej kr\u00F3lewny Andromedy."@pl ,
		"R\u00E9altra b\u00EDseach is ea r\u00E9altra Andraim\u00E9ide, agus \u00E9 le feice\u00E1il i r\u00E9altbhu\u00EDon Andraim\u00E9ide. T\u00E1 an r\u00E9altra seo suite faoi 2.2 milli\u00FAn solasbhliain d\u00EDnn, agus is \u00E9 an r\u00E9altra b\u00EDseach is gaire d\u00FAinn. C\u00E9 is moite de Bhealach na B\u00F3 Finne f\u00E9in, is \u00E9 an t-aon r\u00E9altra b\u00EDseach is f\u00E9idir a aithint ar sp\u00E9ir na ho\u00EDche gan \u00FAs\u00E1id a bhaint as gl\u00E9asra cianradhairc ar n\u00F3s na nd\u00E9sh\u00FAileach n\u00F3 an teileasc\u00F3ip. T\u00E1 Scamall M\u00F3r Magellan agus Scamall Beag Magellan le feice\u00E1il chomh maith, ach n\u00ED r\u00E9altra\u00ED b\u00EDseacha iad. Ceann de r\u00E9altra\u00ED an Ghr\u00FApa \u00C1iti\u00FAil \u00E9. Is \u00E9 an teileasc\u00F3p is fearr a thabharfaidh l\u00E9argas air, sin n\u00F3 prionta\u00ED de ghrianghraif fhadnochta. De ghn\u00E1ch, s\u00EDlimid gurb \u00E9 l\u00E1r an r\u00E9altra seo an r\u00E9altra ar fad, ach le f\u00EDrinne, cumhda\u00EDonn Andraim\u00E9ide seacht leithead na l\u00E1nr\u00E9 d'achar na sp\u00E9ire, agus 300,000 milli\u00FAn r\u00E9alta ann ar fad. T\u00E1 dh\u00E1 r\u00E9altra bheaga shatail\u00EDteacha aige, mar at\u00E1 M 32 agus NCG 205, iad araon infheicthe le teileasc\u00F3p beag. Is \u00E9 R\u00E9altra Andraim\u00E9ide an r\u00E9altra is m\u00F3 sa Ghr\u00FApa \u00C1iti\u00FAil, agus is \u00E9 Bealach na B\u00F3 Finne is t\u00E1naiste d\u00F3. T\u00E1 r\u00E9altra Andraim\u00E9ide ag druidim isteach chugainn agus luas 300 cilim\u00E9adar in aghaidh an tsoicind (186 m\u00EDle/soic.) faoi. Mar sin, t\u00E1 s\u00E9 ar an mbeag\u00E1n r\u00E9altra\u00ED gormaistrithe ar an sp\u00E9ir. M\u00E1 chuirtear gluaiseacht \u00E1r ngrianch\u00F3rais f\u00E9in taobh istigh de Bhealach na B\u00F3 Finn san \u00E1ireamh, gheofar an toradh go bhfuil \u00E1r r\u00E9altra f\u00E9in ag dul i dtreo Andraim\u00E9ide agus luas 100 go 140 cilim\u00E9adar in aghaidh an tsoicind faoi (62\u201387 m\u00EDle/soic.). M\u00E1s \u00E9 an t-imbhualadh at\u00E1 i nd\u00E1n don d\u00E1 r\u00E9altra, titfidh s\u00E9 amach i gceann tr\u00ED mh\u00EDle milliun (109) bliain. Sa ch\u00E1s sin, ceaptar go rachfaidh an d\u00E1 r\u00E9altra le ch\u00E9ile le haon r\u00E9altra m\u00F3r \u00E9ilipseach amh\u00E1in a dh\u00E9anamh. Is minic a tharla\u00EDonn an cine\u00E1l seo eachtra\u00ED idir r\u00E9altra\u00ED at\u00E1 suite sa ghr\u00FApa \u00E1iti\u00FAil ch\u00E9anna le ch\u00E9ile."@ga ,
		"\u0413\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u0430 \u0410\u043D\u0434\u0440\u043E\u043C\u0435\u0434\u0438 (\u0422\u0443\u043C\u0430\u043D\u043D\u0456\u0441\u0442\u044C \u0410\u043D\u0434\u0440\u043E\u043C\u0435\u0434\u0438, \u041C\u0435\u0441\u0441\u044C\u0454 31, \u041C31, NGC 224) \u2014\u043D\u0430\u0439\u0431\u043B\u0438\u0436\u0447\u0430 \u0434\u043E \u0427\u0443\u043C\u0430\u0446\u044C\u043A\u043E\u0433\u043E \u0428\u043B\u044F\u0445\u0443 \u0432\u0435\u043B\u0438\u043A\u0430 \u0433\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u0430, \u0440\u043E\u0437\u0442\u0430\u0448\u043E\u0432\u0430\u043D\u0430 \u0432 \u0441\u0443\u0437\u0456\u0440'\u0457 \u0410\u043D\u0434\u0440\u043E\u043C\u0435\u0434\u0438 \u0456 \u0432\u0456\u0434\u0434\u0430\u043B\u0435\u043D\u0430 \u0432\u0456\u0434 \u043D\u0430\u0441, \u0437\u0430 \u043E\u0441\u0442\u0430\u043D\u043D\u0456\u043C\u0438 \u0434\u0430\u043D\u0438\u043C\u0438, \u043D\u0430 \u0432\u0456\u0434\u0441\u0442\u0430\u043D\u044C 772 \u043A\u0456\u043B\u043E\u043F\u0430\u0440\u0441\u0435\u043A (2,52 \u043C\u043B\u043D \u0441\u0432\u0456\u0442\u043B\u043E\u0432\u0438\u0445 \u0440\u043E\u043A\u0456\u0432). \u041F\u043B\u043E\u0449\u0438\u043D\u0430 \u0433\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u0438 \u043D\u0430\u0445\u0438\u043B\u0435\u043D\u0430 \u0434\u043E \u043D\u0430\u0441 \u043F\u0456\u0434 \u043A\u0443\u0442\u043E\u043C 15\u00B0, \u0457\u0457 \u0432\u0438\u0434\u0438\u043C\u0438\u0439 \u0440\u043E\u0437\u043C\u0456\u0440 \u2014 3,2\u00B0\u00D71\u00B0, \u0432\u0438\u0434\u0438\u043C\u0430 \u0437\u043E\u0440\u044F\u043D\u0430 \u0432\u0435\u043B\u0438\u0447\u0438\u043D\u0430 \u2014 +3,4 m ."@uk ,
		"The Andromeda Galaxy (IPA: /\u00E6n\u02C8dr\u0252m\u026Ad\u0259/), also known as Messier 31, M31, or NGC 224 and originally the Andromeda Nebula, is a barred spiral galaxy with the diameter of about 46.56 kiloparsecs (152,000 light-years) approximately 2.5 million light-years (765 kiloparsecs) from Earth and the nearest large galaxy to the Milky Way. The galaxy's name stems from the area of Earth's sky in which it appears, the constellation of Andromeda, which itself is named after the princess who was the wife of Perseus in Greek mythology. The virial mass of the Andromeda Galaxy is of the same order of magnitude as that of the Milky Way, at 1 trillion solar masses (2.0\u00D71042 kilograms). The mass of either galaxy is difficult to estimate with any accuracy, but it was long thought that the Andromeda Galaxy is more massive than the Milky Way by a margin of some 25% to 50%. This has been called into question by a 2018 study that cited a lower estimate on the mass of the Andromeda Galaxy,combined with preliminary reports on a 2019 study estimating a higher mass of the Milky Way. The Andromeda Galaxy has a diameter of about 46.56 kpc (152,000 ly), making it the largest member of the Local Group in terms of extension. The Milky Way and Andromeda galaxies are expected to collide in around 4\u20135 billion years, merging to potentially form a giant elliptical galaxy or a large lenticular galaxy.With an apparent magnitude of 3.4, the Andromeda Galaxy is among the brightest of the Messier objects, and is visible to the naked eye from Earth on moonless nights, even when viewed from areas with moderate light pollution."@en ,
		"Galaksi Andromeda (nama lain, Messier 31 dan NGC 224) adalah sebuah galaksi spiral yang berjarak kira-kira 2,5 juta tahun cahaya dari bumi. Galaksi ini merupakan salah satu galaksi di luar galaksi Bima Sakti yang dapat dilihat dengan mata telanjang pada malam yang cerah, tanpa bulan, dan tanpa polusi cahaya. Strukturnya mirip dengan galaksi Bima Sakti yaitu berbentuk spiral. Jaraknya sekitar 2,5 juta tahun cahaya. Letaknya di langit adalah di belahan langit utara, sekitar 41 derajat di sebelah utara khatulistiwa langit. Galaksi ini dapat diamati di bulan September, Oktober, dan November. Dengan mata telanjang, galaksi ini tampak seperti kabut tipis kecil di langit utara. Namun, jika diamati dengan teropong yang dapat menampakkan bintang-bintang redup di tepian galaksi Andromeda, ukurannya bisa lebih dari 7 kali diameter sudut bulan. Galaksi ini berisi sekitar 1 triliun bintang dan bergerak mendekati Bima Sakti dengan kecepatan sekitar 300 km/detik."@in ,
		"Het Andromedastelsel of de Andromedanevel (M31) is een spiraalvormig sterrenstelsel, in het sterrenbeeld Andromeda. Het stelsel heeft dezelfde vorm als ons eigen sterrenstelsel, de Melkweg, maar is wel een stuk groter. De afstand wordt geschat op ongeveer 2,54 miljoen lichtjaar, de diameter ca. 220.000 lichtjaar. De massa wordt geschat op 300 tot 400 miljard zonsmassa's, de totale massa inclusief de halo op 1,2 biljoen zonsmassa's. Vergeleken met de laatste schattingen van de totale massa van de Melkweg, die 1,9 biljoen zonsmassa's bedraagt, zou dus M31 wat lichter zijn, en veel minder dicht. Samen met de Melkweg en een aantal kleinere sterrenstelsels vormt de Andromedanevel de Lokale Groep."@nl ,
		"\u039F \u0393\u03B1\u03BB\u03B1\u03BE\u03AF\u03B1\u03C2 \u03C4\u03B7\u03C2 \u0391\u03BD\u03B4\u03C1\u03BF\u03BC\u03AD\u03B4\u03B1\u03C2 (\u03B3\u03BD\u03C9\u03C3\u03C4\u03CC\u03C2 \u03BA\u03B1\u03B9 \u03C9\u03C2 \u039C\u03B5\u03C3\u03B9\u03AD 31) \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\u03C4\u03BF\u03BD \u03B1\u03C3\u03C4\u03B5\u03C1\u03B9\u03C3\u03BC\u03CC \u0391\u03BD\u03B4\u03C1\u03BF\u03BC\u03AD\u03B4\u03B1, \u03C3\u03C4\u03BF\u03BD \u03BF\u03C0\u03BF\u03AF\u03BF \u03BF\u03C6\u03B5\u03AF\u03BB\u03B5\u03B9 \u03BA\u03B1\u03B9 \u03C4\u03BF \u03CC\u03BD\u03BF\u03BC\u03AC \u03C4\u03BF\u03C5. \u039A\u03B1\u03C4\u03AD\u03C7\u03B5\u03B9 \u03AD\u03BD\u03B1 \u03B1\u03BE\u03B9\u03BF\u03C3\u03B7\u03BC\u03B5\u03AF\u03C9\u03C4\u03BF \u03C1\u03B5\u03BA\u03CC\u03C1: \u03B5\u03AF\u03BD\u03B1\u03B9 \u03C4\u03BF \u03C0\u03B9\u03BF \u03B1\u03C0\u03BF\u03BC\u03B1\u03BA\u03C1\u03C5\u03C3\u03BC\u03AD\u03BD\u03BF \u03B1\u03BD\u03C4\u03B9\u03BA\u03B5\u03AF\u03BC\u03B5\u03BD\u03BF \u03B5\u03CD\u03BA\u03BF\u03BB\u03B1 \u03BF\u03C1\u03B1\u03C4\u03CC \u03BC\u03B5 \u03B3\u03C5\u03BC\u03BD\u03CC \u03BC\u03AC\u03C4\u03B9. \u0392\u03C1\u03AF\u03C3\u03BA\u03B5\u03C4\u03B1\u03B9 \u03C3\u03B5 \u03B1\u03C0\u03CC\u03C3\u03C4\u03B1\u03C3\u03B7 \u03BC\u03CC\u03BB\u03B9\u03C2 2,5 \u03B5\u03BA\u03B1\u03C4\u03BF\u03BC\u03BC\u03C5\u03C1\u03AF\u03C9\u03BD \u03B5\u03C4\u03CE\u03BD \u03C6\u03C9\u03C4\u03CC\u03C2 \u03BA\u03B1\u03B9 \u03BC\u03B1\u03B6\u03AF \u03BC\u03B5 \u03C4\u03BF\u03BD \u0393\u03B1\u03BB\u03B1\u03BE\u03AF\u03B1 \u03BC\u03B1\u03C2 \u03B1\u03C0\u03BF\u03C4\u03B5\u03BB\u03BF\u03CD\u03BD \u03C4\u03BF\u03C5\u03C2 \u03B4\u03CD\u03BF \u03BC\u03B5\u03B3\u03B1\u03BB\u03CD\u03C4\u03B5\u03C1\u03BF\u03C5\u03C2 \u03B3\u03B1\u03BB\u03B1\u03BE\u03AF\u03B5\u03C2 \u03C4\u03B7\u03C2 \u03C4\u03BF\u03C0\u03B9\u03BA\u03AE\u03C2 \u03BF\u03BC\u03AC\u03B4\u03B1\u03C2 \u03B3\u03B1\u03BB\u03B1\u03BE\u03B9\u03CE\u03BD. \u0391\u03BD \u03BA\u03B1\u03B9 \u03B5\u03AF\u03BD\u03B1\u03B9 \u03BC\u03B5\u03B3\u03B1\u03BB\u03CD\u03C4\u03B5\u03C1\u03BF\u03C2 \u03B1\u03C0\u03CC \u03C4\u03BF\u03BD \u0393\u03B1\u03BB\u03B1\u03BE\u03AF\u03B1 \u03BC\u03B1\u03C2 (\u03BF \u03BF\u03C0\u03BF\u03AF\u03BF\u03C2 \u03B5\u03AF\u03BD\u03B1\u03B9 \u03BF \u03B4\u03B5\u03CD\u03C4\u03B5\u03C1\u03BF\u03C2 \u03C3\u03B5 \u03BC\u03AD\u03B3\u03B5\u03B8\u03BF\u03C2 \u03C3\u03C4\u03B7\u03BD \u03C4\u03BF\u03C0\u03B9\u03BA\u03AE \u03BF\u03BC\u03AC\u03B4\u03B1 \u03B3\u03B1\u03BB\u03B1\u03BE\u03B9\u03CE\u03BD), \u03C0\u03B9\u03B8\u03B1\u03BD\u03CC\u03C4\u03B1\u03C4\u03B1 \u03BF \u03B4\u03B9\u03BA\u03CC\u03C2 \u03BC\u03B1\u03C2 \u03C0\u03B5\u03C1\u03B9\u03AD\u03C7\u03B5\u03B9 \u03C0\u03B5\u03C1\u03B9\u03C3\u03C3\u03CC\u03C4\u03B5\u03C1\u03B7 \u03C3\u03BA\u03BF\u03C4\u03B5\u03B9\u03BD\u03AE \u03CD\u03BB\u03B7 \u03BA\u03B1\u03B9 \u03AD\u03C7\u03B5\u03B9 \u03BC\u03B5\u03B3\u03B1\u03BB\u03CD\u03C4\u03B5\u03C1\u03B7 \u03BC\u03AC\u03B6\u03B1. \u039D\u03AD\u03B5\u03C2 \u03C0\u03B1\u03C1\u03B1\u03C4\u03B7\u03C1\u03AE\u03C3\u03B5\u03B9\u03C2 \u03B4\u03B5\u03AF\u03C7\u03BD\u03BF\u03C5\u03BD \u03CC\u03C4\u03B9 \u03B4\u03B9\u03B1\u03B8\u03AD\u03C4\u03B5\u03B9 \u03AD\u03BD\u03B1 \u03C4\u03C1\u03B9\u03C3\u03B5\u03BA\u03B1\u03C4\u03BF\u03BC\u03BC\u03CD\u03C1\u03B9\u03BF \u03AC\u03C3\u03C4\u03C1\u03B1, \u03B4\u03B7\u03BB\u03B1\u03B4\u03AE 2,5 \u03BC\u03B5 5 \u03C6\u03BF\u03C1\u03AD\u03C2 \u03C0\u03B5\u03C1\u03B9\u03C3\u03C3\u03CC\u03C4\u03B5\u03C1\u03B1 \u03B1\u03C0\u03CC \u03C4\u03BF\u03BD \u0393\u03B1\u03BB\u03B1\u03BE\u03AF\u03B1 \u03BC\u03B1\u03C2."@el ,
		"La gal\u00E0xia d'Andr\u00F2meda, Messier 31, M31 o NGC 224, \u00E9s una gal\u00E0xia espiral gegant catalogada per Charles Messier el 1764. \u00C9s l'objecte visible a ull nu m\u00E9s allunyat de la Terra. \u00C9s a 2,5 milions d'anys llum (775 kpc) en direcci\u00F3 a la constel\u00B7laci\u00F3 d'Andr\u00F2meda. Fa part del grup local de gal\u00E0xies, que inclou una gran quantitat de gal\u00E0xies petites m\u00E9s les tres grans gal\u00E0xies espirals: Andr\u00F2meda, la Via L\u00E0ctia i la Gal\u00E0xia del Triangle. T\u00E9 una massa calculada d'entre 300.000 i 400.000 milions de masses solars (aproximadament una vegada i mitja la massa de la Via L\u00E0ctia) i un di\u00E0metre d'uns 220.000 anys llum. Dins la classificaci\u00F3 de Hubble es considera del tipus Sb. Amb les millores en els mesuraments i les dades obtingudes, alguns cient\u00EDfics consideren que la Via L\u00E0ctia cont\u00E9 molta m\u00E9s mat\u00E8ria fosca i podria ser m\u00E9s massiva que M31. Tot i aix\u00ED, observacions recents del Telescopi espacial Spitzer van revelar que la M31 cont\u00E9 un bili\u00F3 (1012) d'estels, excedint per molt el nombre d'estels de la nostra gal\u00E0xia. La gal\u00E0xia s'acosta a nosaltres a uns 140 quil\u00F2metres per segon i es creu que d'aqu\u00ED a aproximadament 3.000 milions a 5.000 milions d'anys podria col\u00B7lidir amb la nostra gal\u00E0xia i fusionar-s'hi amb la formaci\u00F3 d'una gal\u00E0xia gegant el\u00B7l\u00EDptica. Andr\u00F2meda t\u00E9 un paper important en els estudis gal\u00E0ctics, ja que \u00E9s la gegant espiral m\u00E9s propera. El 1943 Walter Baade va ser el primer a resoldre estels dintre de la regi\u00F3 central de la gal\u00E0xia. Edwin Hubble hi va identificar per primera vegada en fotografia estels variables Cefeida en aquesta gal\u00E0xia, la qual cosa va permetre de determinar la dist\u00E0ncia de nosaltres. , de l', ha detectat fonts de raigs X en la Gal\u00E0xia d'Andr\u00F2meda emprant observacions de l'observatori orbital XMM-Newton de l'Ag\u00E8ncia Espacial Europea. La seva hip\u00F2tesi \u00E9s que poden ser possibles candidats a forats negres o estels de neutrons, que escalfen el gas entrant a milions de graus, el qual emet raigs X. L'espectre dels estels de neutrons \u00E9s el mateix que el dels suposats forats negres, per\u00F2 es distingeixen per les seves masses. El 1991 la C\u00E0mera Planet\u00E0ria del Telescopi Espacial Hubble va fotografiar el nucli d'Andr\u00F2meda. Va sorprendre a tothom que presenti una doble estructura, amb dos punts nuclears calents separats per uns pocs anys llum. Observacions terrestres posteriors han dut a especular que, a m\u00E9s d'existir dos nuclis, aquests es mouen l'un respecte de l'altre i que un dels nuclis est\u00E0 desfent l'altre, que podria ser el romanent d'una gal\u00E0xia m\u00E9s petita \"empassada\" per M31. Sabem que els nuclis de moltes gal\u00E0xies s\u00F3n llocs bastant violents i sovint es proposa l'exist\u00E8ncia de forats negres supermassius per a explicar-los. Scott Chapman, del Calif\u00F2rnia Institute of Technology, i Rodrigo Ibata, de l'Observatoire Astronomique de Strasbourg a Fran\u00E7a, van anunciar el 2005 les seves observacions amb els telescopis Keck, que mostren que la lluentor t\u00E8nue d'estels que s'est\u00E9n cap a fora de la gal\u00E0xia \u00E9s, en realitat, part del mateix disc. Aix\u00F2 significa que el disc espiral d'estels en Andr\u00F2meda \u00E9s tres vegades m\u00E9s llarg de l'estimat fins ara. \u00C9s una evid\u00E8ncia que hi ha un vast disc estel\u00B7lar que fa que la gal\u00E0xia tingui un di\u00E0metre de m\u00E9s de 220.000 anys llum. Els c\u00E0lculs previs estimaven el di\u00E0metre d'Andr\u00F2meda entre els 70.000 i els 120.000 anys llum. Recents investigacions han demostrat l'exist\u00E8ncia d'una barra en el centre de M 31, la qual cosa la converteix en una gal\u00E0xia espiral barrada igual que la Via L\u00E0ctia. L'any 2020, els cient\u00EDfics que treballen amb el telescopi espacial Hubble van cartografiar l'halo gal\u00E0ctic d'Andr\u00F2meda, un immens embolcall de gas que l'envolta. Els va sorprendre la seva magnitud, aquest halo, molt t\u00E8nue, gaireb\u00E9 invisible, abasta un 1,3 milions d'anys des de la gal\u00E0xia, aproximadament arriba fins a la meitat de la dist\u00E0ncia que hi ha fins a la nostra Via L\u00E0ctia. I en algunes direccions arriba a 2 milions d'anys llum, el que significa que l'halo d'Andr\u00F2meda ja est\u00E0 col\u00B7lidint amb el de la nostra gal\u00E0xia."@ca ;
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		<https://web.archive.org/web/20110722021459/http:/blackholes.stardate.org/directory/factsheet.php%3Fp=M31> ,
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		<http://hubblesite.org/newscenter/archive/releases/2015/02/image/a/format/zoom/> ,
		<http://www.andromedaproject.org/> ,
		<http://astro.neutral.org/imagehtml/20050903_m31.html> ,
		<http://space.com/scienceastronomy/060123_andromeda_plane.html> ,
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		<http://apod.nasa.gov/apod/ap130801.html> ,
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dbr:Virgo_Supercluster	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Wide-field_Infrared_Survey_Explorer	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Pinwheel_Galaxy	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Messier_81	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Globular_cluster	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Mayall_II	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:List_of_spiral_galaxies	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Sculptor_Galaxy	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Toluca	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
dbr:Subnautica	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
<http://dbpedia.org/resource/Reciprocity_(photography)>	dbo:wikiPageWikiLink	dbr:Andromeda_Galaxy .
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	dbo:wikiPageRedirects	dbr:Andromeda_Galaxy .  <script>parent.window.postMessage('ixistenz.url:http://dbpedia.org/data/Andromeda_Galaxy.ttl', '*'); </script> <div id='browserdiffcontainer' style='position: fixed; right: 10px; top: 10vh; min-width: 60px;  border: 1px solid white; background: rgb(251, 189, 0);; opacity: 0.9; font-family: helvetica, arial, sans serif;  font-size: 12px; z-index: 20001; padding-bottom: 20px;'><div onclick="toggle('browserdiffcontainerlist'); return false;" style='background: rgb(151, 89, 0);; color: white; '><strong>&nbsp; <span class='glyphicon glyphicon-minus'></span> NODES</strong></div><div id='browserdiffcontainerlist' style='padding-left: 10px; padding-right: 5px; max-height: 50vh; overflow: auto; '><div><a href='#diffid883' style='color: white;' onClick="parent.window.postMessage('ixistenz.opendiff:883', '*');; return false;" style='text-decoration: none; '>Association </a> <a style='color: white;' href='#diffid883'><sup>1</sup></a></div><div><a href='#diffid117' style='color: white;' onClick="parent.window.postMessage('ixistenz.opendiff:117', '*');; return false;" style='text-decoration: none; '>chat </a> <a style='color: white;' href='#diffid117'><sup>6</sup></a></div><div><a href='#diffid884' style='color: white;' onClick="parent.window.postMessage('ixistenz.opendiff:884', '*');; return false;" style='text-decoration: none; '>Idea </a> <a style='color: white;' href='#diffid884'><sup>4</sup></a></div><div><a href='#diffid119' style='color: white;' onClick="parent.window.postMessage('ixistenz.opendiff:119', '*');; return false;" style='text-decoration: none; '>idea </a> <a style='color: white;' href='#diffid119'><sup>4</sup></a></div><div><a href='#diffid123' style='color: white;' onClick="parent.window.postMessage('ixistenz.opendiff:123', '*');; return false;" style='text-decoration: none; '>INTERN </a> <a style='color: white;' href='#diffid123'><sup>1</sup></a></div><div><a href='#diffid878' style='color: white;' onClick="parent.window.postMessage('ixistenz.opendiff:878', '*');; return false;" style='text-decoration: none; '>Note </a> <a style='color: white;' href='#diffid878'><sup>4</sup></a></div></div></div>
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