. . "1121642321"^^ . . . . . . . . "Turni\u011Danta nigra truo estas nigra truo kiu havas ne nulan angulan movokvanton. Nigra truo povas nur havi tri fundamentajn propra\u0135ojn: mason M, elektran \u015Dargon Q kaj angulan movokvanton (spinon) J. Turni\u011Dantaj nigraj truoj estas formita en la gravita kolapso de pezaj spinantaj, steloj a\u016D de kolapso de kolekto de steloj kun avera\u011Da ne-nula angula movokvanto. \u0108ar plejparto de steloj turni\u011Das oni atendas ke plejparto de nigraj truoj en naturo estas turni\u011Dantaj nigraj truoj. En komenco de 2006, astronomiistoj raportis pri reala spino de nigraj truoj en . Nigra truo en la Lakta vojo povas turni\u011Di je rapido de 1150 turnoj en sekundo, proksimi\u011Dante la teorian supran limigon."@eo . . "Rotierendes Schwarzes Loch"@de . . "Buraco negro em rota\u00E7\u00E3o"@pt . . "\uCEE4 \uBE14\uB799\uD640"@ko . . . "En astrophysique, un trou noir de Kerrcol. 2''s.v.''trou_noir_de_Kerr_1-0\" class=\"reference\">, ainsi d\u00E9sign\u00E9 en l'honneur du math\u00E9maticien n\u00E9oz\u00E9landais Roy Kerr, est, par d\u00E9finition, un trou noir : \n* de masse strictement positive : ; \n* dont le moment cin\u00E9tique n'est pas nul : , c'est-\u00E0-dire qui est en rotation axiale ; \n* dont la charge \u00E9lectrique est nulle . D'apr\u00E8s la conjecture de calvitie, propos\u00E9e par John Wheeler, il est un des quatre types th\u00E9oriques de trous noirs. Il est d\u00E9crit, dans le cadre de la relativit\u00E9 g\u00E9n\u00E9rale, par la m\u00E9trique de Kerr, une solution exacte, stationnaire et \u00E0 sym\u00E9trieaxiale, de l'\u00E9quation d'Einstein du champ de gravitation dans le vide, d\u00E9couverte par Roy Kerr en 1963col. 1''s.v.''trou_noir_de_Kerr_4-0\" class=\"reference\"> ; elle ne d\u00E9pend que des deux param\u00E8tres et \u00A7 31.15_6-0\" class=\"reference\">, c'est-\u00E0-dire la masse et le moment cin\u00E9tique \u00A7 31.15_6-1\" class=\"reference\">\u00A7 3,_a)_7-0\" class=\"reference\">. La m\u00E9trique de Kerr ne d\u00E9crit un trou noir qu'avec \u00A7 31.15_6-2\" class=\"reference\">. La m\u00E9trique de Schwarzschild correspond au cas particulier de celle de Kerr\u00A7 2,_(2)_8-0\" class=\"reference\">. Le trou noir extr\u00E9mal que celle-ci d\u00E9crit correspond au cas limite \u00A7 31.15_6-3\" class=\"reference\"> ; la temp\u00E9rature de Hawking d'un tel trou noir est nulle\u00A7 31.15_6-4\" class=\"reference\">. Avec , la m\u00E9trique de Kerr pr\u00E9dit l'existence de singularit\u00E9s nues\u00A7 31.15_6-5\" class=\"reference\">, c'est-\u00E0-dire de singularit\u00E9s gravitationnelles qui, contrairement \u00E0 celles des trous noirs sans rotation, ne seraient pas vraiment occult\u00E9es par un horizon des \u00E9v\u00E8nements, hypoth\u00E8se \u00E0 laquelle s'oppose la conjecture de censure cosmique, propos\u00E9e par Roger Penrose. La m\u00E9trique de Minkowski correspond au cas particulier de celle de Kerr\u00A7 2,_(1)_10-0\" class=\"reference\">."@fr . . "Buco nero rotante"@it . . "\u30AB\u30FC\u30FB\u30D6\u30E9\u30C3\u30AF\u30DB\u30FC\u30EB"@ja . . . . "En astrophysique, un trou noir de Kerrcol. 2''s.v.''trou_noir_de_Kerr_1-0\" class=\"reference\">, ainsi d\u00E9sign\u00E9 en l'honneur du math\u00E9maticien n\u00E9oz\u00E9landais Roy Kerr, est, par d\u00E9finition, un trou noir : \n* de masse strictement positive : ; \n* dont le moment cin\u00E9tique n'est pas nul : , c'est-\u00E0-dire qui est en rotation axiale ; \n* dont la charge \u00E9lectrique est nulle . D'apr\u00E8s la conjecture de calvitie, propos\u00E9e par John Wheeler, il est un des quatre types th\u00E9oriques de trous noirs."@fr . "\uCEE4 \uBE14\uB799\uD640(Kerr Black Hole) \uB610\uB294 \uD68C\uC804 \uBE14\uB799\uD640(Rotating black hole)\uC740 \uD68C\uC804\uD558\uACE0 \uC788\uB294 \uBE14\uB799\uD640\uC744 \uB9D0\uD55C\uB2E4. \uBE14\uB799\uD640\uC774 \uAC16\uB294 \uBB3C\uB9AC\uB7C9\uC740 \uC9C8\uB7C9, \uAC01\uC6B4\uB3D9\uB7C9, \uC804\uD558 \uC138 \uAC00\uC9C0\uB2E4. \uBCF4\uD1B5 \uBE14\uB799\uD640\uC744 \uB9D0\uD560 \uB54C\uB294 \uC9C8\uB7C9\uB9CC\uC744 \uAC16\uB294 \uC288\uBC14\uB974\uCE20\uC2E4\uD2B8 \uBE14\uB799\uD640\uC744 \uAC00\uB9AC\uD0A4\uB294 \uAC83\uC774 \uBCF4\uD1B5\uC774\uB098, \uAC01\uC6B4\uB3D9\uB7C9\uC744 \uAC00\uC9C4, \uC989 \uD68C\uC804\uD558\uB294 \uBE14\uB799\uD640\uC774 \uC874\uC7AC\uD558\uBA70 \uC774\uAC83\uC744 \uD68C\uC804 \uBE14\uB799\uD640\uC774\uB77C \uCE6D\uD55C\uB2E4. \uB610\uD55C \uC804\uD558\uB97C \uAC00\uC9C4, \uC989 \uB300\uC804\uB41C \uBE14\uB799\uD640\uC744 \uB300\uC804 \uBE14\uB799\uD640(\uB77C\uC774\uC2A4\uB108-\uB178\uB4DC\uC2A4\uD1B0 \uBE14\uB799\uD640)\uC774\uB77C \uBD80\uB978\uB2E4. \uCD5C\uADFC \uC0C9\uAE54\uC774 \uC788\uB294 \uBE14\uB799\uD640\uC774 \uC874\uC7AC\uD55C\uB2E4\uACE0 \uBC1C\uD45C\uB418\uC5C8\uC9C0\uB9CC, \uBAA8\uB4E0 \uBE14\uB799\uD640\uC740 \uC288\uBC14\uB974\uCE20\uC2E4\uD2B8 \uBE14\uB799\uD640\uC774\uB098 \uD68C\uC804 \uBE14\uB799\uD640\uB85C \uBCC0\uD654\uD55C\uB2E4. \uD68C\uC804 \uBE14\uB799\uD640\uC758 \uD2B9\uC774\uC810\uC740 \uACE0\uB9AC\uBAA8\uC591\uC774\uB2E4."@ko . . . . . . . . . . . . . . . . "12984"^^ . "Um buraco negro em rota\u00E7\u00E3o (buraco negro de Kerr ou buraco negro de Kerr-Newman) \u00E9 um buraco negro que possui momento angular. \u00C9 um dos quatro poss\u00EDveis tipos de buracos negros que podem existir na teoria da gravita\u00E7\u00E3o denominada Relatividade Geral. Buracos negros podem ser caracterizados por tr\u00EAs (e somente tr\u00EAs) grandezas M, J e Q, respectivamente: \n* massa M, (buraco negro de Schwarzschild se J=0 and Q=0) \n* momento angular J (buraco negro de Kerr se J diferente de zero e Q=0) \n* carga el\u00E9trica Q (buraco negro carregado ou buraco negro de Reissner-Nordstr\u00F6m se Q diferente de zero e J=0; ou um buraco negro de Kerr-Newman se tanto J e Q diferentes de zero). Buracos negros em rota\u00E7\u00E3o s\u00E3o formados no colapso gravitacional de uma estrela massiva em rota\u00E7\u00E3o ou do colapso de um conjunto de estrelas com uma m\u00E9dia n\u00E3o nula de momento angular. Como muitas estrelas rodam \u00E9 esperado que a maioria dos buracos negros na natureza s\u00E3o buracos negros em rota\u00E7\u00E3o. Em 2006, astr\u00F4nomos relataram atuais taxas de rota\u00E7\u00E3o de buracos negros no Astrophysical Journal. Um buraco negro na Via L\u00E1ctea, , deve ter rota\u00E7\u00E3o de 1150 vezes por segundo, aproximando-se do limite te\u00F3rico superior. Outras detec\u00E7\u00F5es t\u00EAm sido apresentadas na literatura supostamente sendo de tais fontes. Um buraco negro em rota\u00E7\u00E3o pode produzir grandes quantidades de energia no disp\u00EAndio de sua energia rotacional. No caso um buraco negro em rota\u00E7\u00E3o reduzir-se-\u00E1 a um buraco negro de Schwarzschild, a configura\u00E7\u00E3o m\u00EDnima da qual nenhuma energia adicional pode ser extra\u00EDda. A forma\u00E7\u00E3o de um buraco negro em rota\u00E7\u00E3o por uma collapsar (estrela em colapso) \u00E9 talvez observada como as emiss\u00F5es de erup\u00E7\u00F5es de raios gama."@pt . . . . . . . . . . "A rotating black hole is a black hole that possesses angular momentum. In particular, it rotates about one of its axes of symmetry. All celestial objects \u2013 planets, stars (Sun), galaxies, black holes \u2013 spin."@en . . . . . "Per buco nero rotante s'intende un buco nero che possieda momento angolare."@it . . . . . . "\u0412\u0440\u0430\u0449\u0430\u044E\u0449\u0430\u044F\u0441\u044F \u0447\u0451\u0440\u043D\u0430\u044F \u0434\u044B\u0440\u0430 \u2014 \u0447\u0451\u0440\u043D\u0430\u044F \u0434\u044B\u0440\u0430, \u043A\u043E\u0442\u043E\u0440\u0430\u044F \u043E\u0431\u043B\u0430\u0434\u0430\u0435\u0442 \u043C\u043E\u043C\u0435\u043D\u0442\u043E\u043C \u0438\u043C\u043F\u0443\u043B\u044C\u0441\u0430, \u0442\u043E \u0435\u0441\u0442\u044C \u0432\u0440\u0430\u0449\u0430\u0435\u0442\u0441\u044F \u0432\u043E\u043A\u0440\u0443\u0433 \u043E\u0434\u043D\u043E\u0439 \u0438\u0437 \u0441\u0432\u043E\u0438\u0445 \u043E\u0441\u0435\u0439 \u0441\u0438\u043C\u043C\u0435\u0442\u0440\u0438\u0438."@ru . "Lubang hitam yang berotasi adalah lubang hitam yang memiliki momentum sudut."@in . . . . . . . . "Rotating black hole"@en . . "Um buraco negro em rota\u00E7\u00E3o (buraco negro de Kerr ou buraco negro de Kerr-Newman) \u00E9 um buraco negro que possui momento angular. \u00C9 um dos quatro poss\u00EDveis tipos de buracos negros que podem existir na teoria da gravita\u00E7\u00E3o denominada Relatividade Geral. Buracos negros podem ser caracterizados por tr\u00EAs (e somente tr\u00EAs) grandezas M, J e Q, respectivamente:"@pt . . . . . "Lubang hitam yang berotasi"@in . . "\u30AB\u30FC\u30FB\u30D6\u30E9\u30C3\u30AF\u30DB\u30FC\u30EB\uFF08Kerr Black Hole\uFF09\u3068\u306F\u3001\u81EA\u8EE2\u3057\u3066\u3044\u308B\u30D6\u30E9\u30C3\u30AF\u30DB\u30FC\u30EB\u306E\u3053\u3068\u3092\u3044\u3046\u3002\u767A\u898B\u8005\u3067\u3042\u308B\u30ED\u30A4\u30FB\u30AB\u30FC\u306E\u540D\u3092\u51A0\u3057\u3066\u3053\u3046\u547C\u3076\u3002 \u30D6\u30E9\u30C3\u30AF\u30DB\u30FC\u30EB\u304C\u6301\u3061\u3046\u308B\u7269\u7406\u91CF\u306F\u4E09\u3064\u3060\u3051\u3067\u3042\u308A\u3001\u4E00\u3064\u306F\u8CEA\u91CF\u3001\u4E00\u3064\u306F\u89D2\u904B\u52D5\u91CF\u3001\u3082\u3046\u4E00\u3064\u306F\u96FB\u8377\u3067\u3042\u308B\u3002\u8CEA\u91CF\u30FB\u56DE\u8EE2\u30FB\u96FB\u8377\u306E\u4E09\u3064\u306E\u6027\u8CEA\u304C\u3042\u308A\u3001\u3053\u308C\u3092\u300C\u30D6\u30E9\u30C3\u30AF\u30DB\u30FC\u30EB\u306B\u6BDB\u304C\u4E09\u672C\u300D\u3068\u8868\u73FE\u3059\u308B\u3053\u3068\u304C\u3042\u308B\u3002\u901A\u5E38\u30D6\u30E9\u30C3\u30AF\u30DB\u30FC\u30EB\u3068\u3044\u3048\u3070\u3001\u4E09\u3064\u306E\u7269\u7406\u91CF\u306E\u3046\u3061\u8CEA\u91CF\u306E\u307F\u3092\u3082\u3064\u30B7\u30E5\u30F4\u30A1\u30EB\u30C4\u30B7\u30EB\u30C8\u30FB\u30D6\u30E9\u30C3\u30AF\u30DB\u30FC\u30EB\u3092\u6307\u3059\u306E\u304C\u666E\u901A\u3067\u3042\u308B\u304C\u3001\u8CEA\u91CF\u306B\u52A0\u3048\u89D2\u904B\u52D5\u91CF\u3092\u6301\u3064\u3001\u3064\u307E\u308A\u56DE\u8EE2\u3057\u3066\u3044\u308B\u30D6\u30E9\u30C3\u30AF\u30DB\u30FC\u30EB\u3082\u5B58\u5728\u3057\u3001\u3053\u308C\u3092\u30AB\u30FC\u30FB\u30D6\u30E9\u30C3\u30AF\u30DB\u30FC\u30EB\u3068\u547C\u3076\u3002\u306A\u304A\u8CEA\u91CF\u306B\u52A0\u3048\u3066\u96FB\u8377\u3092\u6301\u3064\u3001\u3064\u307E\u308A\u5E2F\u96FB\u3057\u3066\u3044\u308B\u30D6\u30E9\u30C3\u30AF\u30DB\u30FC\u30EB\u306F\u3001\u30E9\u30A4\u30B9\u30CA\u30FC\u30FB\u30CE\u30EB\u30C9\u30B7\u30E5\u30C8\u30EB\u30E0\u30FB\u30D6\u30E9\u30C3\u30AF\u30DB\u30FC\u30EB\u3068\u547C\u3076\u3002 \u8FD1\u5E74\u30AB\u30E9\u30FC\uFF08\u8272\u8377\uFF09\u3092\u6301\u3064\u30D6\u30E9\u30C3\u30AF\u30DB\u30FC\u30EB\u3082\u5B58\u5728\u3059\u308B\u3068\u767A\u8868\u3055\u308C\u305F\u304C\u3001\u5168\u3066\u306E\u30D6\u30E9\u30C3\u30AF\u30DB\u30FC\u30EB\u306F\u3044\u305A\u308C\u30B7\u30E5\u30F4\u30A1\u30EB\u30C4\u30B7\u30EB\u30C8\u30FB\u30D6\u30E9\u30C3\u30AF\u30DB\u30FC\u30EB\u304B\u30AB\u30FC\u30FB\u30D6\u30E9\u30C3\u30AF\u30DB\u30FC\u30EB\u306B\u5909\u5316\u3059\u308B\u3002 \u30AB\u30FC\u30FB\u30D6\u30E9\u30C3\u30AF\u30DB\u30FC\u30EB\u306E\u7279\u7570\u70B9\u306F\u30EA\u30F3\u30B0\u72B6\uFF08\u74B0\u72B6\uFF09\u306B\u306A\u3063\u3066\u3044\u308B\u3002"@ja . "\u30AB\u30FC\u30FB\u30D6\u30E9\u30C3\u30AF\u30DB\u30FC\u30EB\uFF08Kerr Black Hole\uFF09\u3068\u306F\u3001\u81EA\u8EE2\u3057\u3066\u3044\u308B\u30D6\u30E9\u30C3\u30AF\u30DB\u30FC\u30EB\u306E\u3053\u3068\u3092\u3044\u3046\u3002\u767A\u898B\u8005\u3067\u3042\u308B\u30ED\u30A4\u30FB\u30AB\u30FC\u306E\u540D\u3092\u51A0\u3057\u3066\u3053\u3046\u547C\u3076\u3002 \u30D6\u30E9\u30C3\u30AF\u30DB\u30FC\u30EB\u304C\u6301\u3061\u3046\u308B\u7269\u7406\u91CF\u306F\u4E09\u3064\u3060\u3051\u3067\u3042\u308A\u3001\u4E00\u3064\u306F\u8CEA\u91CF\u3001\u4E00\u3064\u306F\u89D2\u904B\u52D5\u91CF\u3001\u3082\u3046\u4E00\u3064\u306F\u96FB\u8377\u3067\u3042\u308B\u3002\u8CEA\u91CF\u30FB\u56DE\u8EE2\u30FB\u96FB\u8377\u306E\u4E09\u3064\u306E\u6027\u8CEA\u304C\u3042\u308A\u3001\u3053\u308C\u3092\u300C\u30D6\u30E9\u30C3\u30AF\u30DB\u30FC\u30EB\u306B\u6BDB\u304C\u4E09\u672C\u300D\u3068\u8868\u73FE\u3059\u308B\u3053\u3068\u304C\u3042\u308B\u3002\u901A\u5E38\u30D6\u30E9\u30C3\u30AF\u30DB\u30FC\u30EB\u3068\u3044\u3048\u3070\u3001\u4E09\u3064\u306E\u7269\u7406\u91CF\u306E\u3046\u3061\u8CEA\u91CF\u306E\u307F\u3092\u3082\u3064\u30B7\u30E5\u30F4\u30A1\u30EB\u30C4\u30B7\u30EB\u30C8\u30FB\u30D6\u30E9\u30C3\u30AF\u30DB\u30FC\u30EB\u3092\u6307\u3059\u306E\u304C\u666E\u901A\u3067\u3042\u308B\u304C\u3001\u8CEA\u91CF\u306B\u52A0\u3048\u89D2\u904B\u52D5\u91CF\u3092\u6301\u3064\u3001\u3064\u307E\u308A\u56DE\u8EE2\u3057\u3066\u3044\u308B\u30D6\u30E9\u30C3\u30AF\u30DB\u30FC\u30EB\u3082\u5B58\u5728\u3057\u3001\u3053\u308C\u3092\u30AB\u30FC\u30FB\u30D6\u30E9\u30C3\u30AF\u30DB\u30FC\u30EB\u3068\u547C\u3076\u3002\u306A\u304A\u8CEA\u91CF\u306B\u52A0\u3048\u3066\u96FB\u8377\u3092\u6301\u3064\u3001\u3064\u307E\u308A\u5E2F\u96FB\u3057\u3066\u3044\u308B\u30D6\u30E9\u30C3\u30AF\u30DB\u30FC\u30EB\u306F\u3001\u30E9\u30A4\u30B9\u30CA\u30FC\u30FB\u30CE\u30EB\u30C9\u30B7\u30E5\u30C8\u30EB\u30E0\u30FB\u30D6\u30E9\u30C3\u30AF\u30DB\u30FC\u30EB\u3068\u547C\u3076\u3002 \u8FD1\u5E74\u30AB\u30E9\u30FC\uFF08\u8272\u8377\uFF09\u3092\u6301\u3064\u30D6\u30E9\u30C3\u30AF\u30DB\u30FC\u30EB\u3082\u5B58\u5728\u3059\u308B\u3068\u767A\u8868\u3055\u308C\u305F\u304C\u3001\u5168\u3066\u306E\u30D6\u30E9\u30C3\u30AF\u30DB\u30FC\u30EB\u306F\u3044\u305A\u308C\u30B7\u30E5\u30F4\u30A1\u30EB\u30C4\u30B7\u30EB\u30C8\u30FB\u30D6\u30E9\u30C3\u30AF\u30DB\u30FC\u30EB\u304B\u30AB\u30FC\u30FB\u30D6\u30E9\u30C3\u30AF\u30DB\u30FC\u30EB\u306B\u5909\u5316\u3059\u308B\u3002 \u30AB\u30FC\u30FB\u30D6\u30E9\u30C3\u30AF\u30DB\u30FC\u30EB\u306E\u7279\u7570\u70B9\u306F\u30EA\u30F3\u30B0\u72B6\uFF08\u74B0\u72B6\uFF09\u306B\u306A\u3063\u3066\u3044\u308B\u3002"@ja . . "\u062B\u0642\u0628 \u0623\u0633\u0648\u062F \u062F\u0648\u0627\u0631"@ar . "\u8F49\u52D5\u7684\u9ED1\u6D1E\u662F\u64C1\u6709\u89D2\u52D5\u91CF\u7684\u9ED1\u6D1E\u3002"@zh . . . . . . . "Trou noir de Kerr"@fr . . . . "\uCEE4 \uBE14\uB799\uD640(Kerr Black Hole) \uB610\uB294 \uD68C\uC804 \uBE14\uB799\uD640(Rotating black hole)\uC740 \uD68C\uC804\uD558\uACE0 \uC788\uB294 \uBE14\uB799\uD640\uC744 \uB9D0\uD55C\uB2E4. \uBE14\uB799\uD640\uC774 \uAC16\uB294 \uBB3C\uB9AC\uB7C9\uC740 \uC9C8\uB7C9, \uAC01\uC6B4\uB3D9\uB7C9, \uC804\uD558 \uC138 \uAC00\uC9C0\uB2E4. \uBCF4\uD1B5 \uBE14\uB799\uD640\uC744 \uB9D0\uD560 \uB54C\uB294 \uC9C8\uB7C9\uB9CC\uC744 \uAC16\uB294 \uC288\uBC14\uB974\uCE20\uC2E4\uD2B8 \uBE14\uB799\uD640\uC744 \uAC00\uB9AC\uD0A4\uB294 \uAC83\uC774 \uBCF4\uD1B5\uC774\uB098, \uAC01\uC6B4\uB3D9\uB7C9\uC744 \uAC00\uC9C4, \uC989 \uD68C\uC804\uD558\uB294 \uBE14\uB799\uD640\uC774 \uC874\uC7AC\uD558\uBA70 \uC774\uAC83\uC744 \uD68C\uC804 \uBE14\uB799\uD640\uC774\uB77C \uCE6D\uD55C\uB2E4. \uB610\uD55C \uC804\uD558\uB97C \uAC00\uC9C4, \uC989 \uB300\uC804\uB41C \uBE14\uB799\uD640\uC744 \uB300\uC804 \uBE14\uB799\uD640(\uB77C\uC774\uC2A4\uB108-\uB178\uB4DC\uC2A4\uD1B0 \uBE14\uB799\uD640)\uC774\uB77C \uBD80\uB978\uB2E4. \uCD5C\uADFC \uC0C9\uAE54\uC774 \uC788\uB294 \uBE14\uB799\uD640\uC774 \uC874\uC7AC\uD55C\uB2E4\uACE0 \uBC1C\uD45C\uB418\uC5C8\uC9C0\uB9CC, \uBAA8\uB4E0 \uBE14\uB799\uD640\uC740 \uC288\uBC14\uB974\uCE20\uC2E4\uD2B8 \uBE14\uB799\uD640\uC774\uB098 \uD68C\uC804 \uBE14\uB799\uD640\uB85C \uBCC0\uD654\uD55C\uB2E4. \uD68C\uC804 \uBE14\uB799\uD640\uC758 \uD2B9\uC774\uC810\uC740 \uACE0\uB9AC\uBAA8\uC591\uC774\uB2E4."@ko . "\u8F49\u52D5\u7684\u9ED1\u6D1E"@zh . "\u0627\u0644\u062B\u0642\u0628 \u0627\u0644\u0623\u0633\u0648\u062F \u0627\u0644\u062F\u0648\u0627\u0631 \u0647\u0648 \u062B\u0642\u0628 \u0623\u0633\u0648\u062F \u064A\u0645\u0644\u0643 \u0632\u062E\u0645 \u0632\u0627\u0648\u064A \u0623\u064A \u062F\u0648\u0631\u0627\u0646 \u062D\u0648\u0644 \u0646\u0641\u0633\u0647\u060C \u0648\u0628\u0634\u0643\u0644 \u0623\u062F\u0642 \u0641\u0647\u0648 \u064A\u062F\u0648\u0631 \u062D\u0648\u0644 \u0623\u062D\u062F \u0645\u062D\u0627\u0648\u0631\u0647 \u0627\u0644\u062A\u0646\u0627\u0638\u0631\u064A\u0629."@ar . "Turni\u011Danta nigra truo estas nigra truo kiu havas ne nulan angulan movokvanton. Nigra truo povas nur havi tri fundamentajn propra\u0135ojn: mason M, elektran \u015Dargon Q kaj angulan movokvanton (spinon) J. Turni\u011Dantaj nigraj truoj estas formita en la gravita kolapso de pezaj spinantaj, steloj a\u016D de kolapso de kolekto de steloj kun avera\u011Da ne-nula angula movokvanto. \u0108ar plejparto de steloj turni\u011Das oni atendas ke plejparto de nigraj truoj en naturo estas turni\u011Dantaj nigraj truoj. En komenco de 2006, astronomiistoj raportis pri reala spino de nigraj truoj en . Nigra truo en la Lakta vojo povas turni\u011Di je rapido de 1150 turnoj en sekundo, proksimi\u011Dante la teorian supran limigon. Turni\u011Danta nigra truo povas eligi grandan kvanton de energio elspezante sian turnan energion. Tiel turni\u011Danta nigra truo pomalmulte i\u011Das neturni\u011Dantan nigran truon de Schwarzschild, la minimuman konfiguron de kiu plu ne eblas eligi energion (krom )."@eo . "\u8F49\u52D5\u7684\u9ED1\u6D1E\u662F\u64C1\u6709\u89D2\u52D5\u91CF\u7684\u9ED1\u6D1E\u3002"@zh . . . . "Lubang hitam yang berotasi adalah lubang hitam yang memiliki momentum sudut."@in . . . "701158"^^ . . "\u0412\u0440\u0430\u0449\u0430\u044E\u0449\u0430\u044F\u0441\u044F \u0447\u0451\u0440\u043D\u0430\u044F \u0434\u044B\u0440\u0430"@ru . . . . . . "A rotating black hole is a black hole that possesses angular momentum. In particular, it rotates about one of its axes of symmetry. All celestial objects \u2013 planets, stars (Sun), galaxies, black holes \u2013 spin."@en . . "\u0412\u0440\u0430\u0449\u0430\u044E\u0449\u0430\u044F\u0441\u044F \u0447\u0451\u0440\u043D\u0430\u044F \u0434\u044B\u0440\u0430 \u2014 \u0447\u0451\u0440\u043D\u0430\u044F \u0434\u044B\u0440\u0430, \u043A\u043E\u0442\u043E\u0440\u0430\u044F \u043E\u0431\u043B\u0430\u0434\u0430\u0435\u0442 \u043C\u043E\u043C\u0435\u043D\u0442\u043E\u043C \u0438\u043C\u043F\u0443\u043B\u044C\u0441\u0430, \u0442\u043E \u0435\u0441\u0442\u044C \u0432\u0440\u0430\u0449\u0430\u0435\u0442\u0441\u044F \u0432\u043E\u043A\u0440\u0443\u0433 \u043E\u0434\u043D\u043E\u0439 \u0438\u0437 \u0441\u0432\u043E\u0438\u0445 \u043E\u0441\u0435\u0439 \u0441\u0438\u043C\u043C\u0435\u0442\u0440\u0438\u0438."@ru . . . . . . . . "Per buco nero rotante s'intende un buco nero che possieda momento angolare."@it . . . . . "\u0627\u0644\u062B\u0642\u0628 \u0627\u0644\u0623\u0633\u0648\u062F \u0627\u0644\u062F\u0648\u0627\u0631 \u0647\u0648 \u062B\u0642\u0628 \u0623\u0633\u0648\u062F \u064A\u0645\u0644\u0643 \u0632\u062E\u0645 \u0632\u0627\u0648\u064A \u0623\u064A \u062F\u0648\u0631\u0627\u0646 \u062D\u0648\u0644 \u0646\u0641\u0633\u0647\u060C \u0648\u0628\u0634\u0643\u0644 \u0623\u062F\u0642 \u0641\u0647\u0648 \u064A\u062F\u0648\u0631 \u062D\u0648\u0644 \u0623\u062D\u062F \u0645\u062D\u0627\u0648\u0631\u0647 \u0627\u0644\u062A\u0646\u0627\u0638\u0631\u064A\u0629."@ar . . . . "Turni\u011Danta nigra truo"@eo . . .