. "J2000"@en . . . . "2900862"^^ . . "Beta Comae Berenices"@pt . . "Beta Comae Berenices"@de . . . . . "\u5468\u9F0E\u4E00 \uFF08\u03B2 Com / \u540E\u53D1\u5EA7\u03B2\uFF09\u662F\u540E\u53D1\u5EA7\u7684\u4E00\u9897\u4E3B\u5E8F\u77EE\u661F\uFF0C\u8DDD\u79BB\u5730\u7403\u7EA630\u5149\u5E74\u3002\u5E0C\u81D8\u5B57\u6BCD\u7684\u03B2\u901A\u5E38\u6A19\u793A\u661F\u5EA7\u4E2D\u8996\u661F\u7B49\u7B2C\u4E8C\u4EAE\u7684\u661F\uFF0C\u4F46\u662F\u5468\u9F0E\u4E00\u6BD4\u540E\u9AEE\u5EA7\u03B1\uFF08+5.22\u7B49\uFF09\u9084\u4EAE\u3002 \u9019\u9846\u6046\u661F\u8207\u6211\u5011\u7684\u592A\u967D\u76F8\u4F3C\uFF0C\u53EA\u662F\u9084\u7A0D\u5FAE\u5927\u4E00\u9EDE\uFF0C\u7D55\u5C0D\u661F\u7B49\u4EAE\u4E00\u9EDE\u3002\u89C0\u5BDF\u8272\u7403\u6D3B\u52D5\u7684\u77ED\u671F\u8B8A\u5316\uFF0C\u8A8D\u70BA\u9019\u9846\u6046\u661F\u7D93\u6B77\u8457\u4E0D\u540C\u7684\u81EA\u8F49\uFF0C\u5468\u671F\u5927\u7D04\u572811\u201313\u5929\u3002\u9019\u9846\u6046\u661F\u8868\u9762\u7684\u6D3B\u52D5\u9031\u671F\u662F16.6\u5E74\uFF0C\u76F8\u8F03\u65BC\u592A\u967D\u768411\u5E74\u4E5F\u8F03\u9577\u4E9B\uFF0C\u4F46\u5B83\u53EF\u80FD\u4E5F\u67099.6\u5E74\u7684\u7B2C\u4E8C\u500B\u6D3B\u52D5\u9031\u671F\u3002\u66FE\u7D93\u4E00\u5EA6\u8A8D\u70BA\u9019\u9846\u6046\u661F\u6709\u9846\u5149\u8B5C\u4F34\u661F\uFF0C\u4F46\u662F\u7CBE\u6E96\u7684\u5F91\u5411\u901F\u5EA6\u6E2C\u91CF\u6392\u9664\u4E86\u9019\u500B\u53EF\u80FD\uFF0C\u4E0D\u50C5\u6C92\u6709\u5075\u6E2C\u5230\u884C\u661F\u74B0\u7E5E\u8457\u5B83\uFF0C\u4E5F\u6C92\u6709\u8B49\u64DA\u986F\u793A\u6709\u5875\u57C3\u76E4\u7684\u5B58\u5728\u3002"@zh . . . . . . . . . . . "Beta Comae Berenices"@sv . . . "Beta Comae Berenices (\u03B2 Com / \u03B2 Comae Berenices / Beta Comae Berenices) \u00E8 una stella appartenente alla sequenza principale che si trova a 29,9 anni luce di distanza dal Sistema solare, nella costellazione della Chioma di Berenice. \u00C8 una stella di classe spettrale G0-V e attualmente, nonostante sia designata con la lettera beta, \u00E8 leggermente pi\u00F9 brillante di Alfa Comae Berenices. Beta Comae Berenices \u00E8 molto simile al nostro Sole. La superficie della stella ha un ciclo di attivit\u00E0 che \u00E8 stato misurato essere di 16,6 anni (quello del Sole \u00E8 di 11 anni), ma potrebbe avere anche un secondo ciclo di 9,6 anni. Nella seconda met\u00E0 del XX secolo si pens\u00F2 che questa stella avesse una compagna spettroscopica, idea per\u00F2 recentemente scartata per via di pi\u00F9 accurate misure sulla velocit\u00E0 radiale di Beta Comae Berenices. Intorno a questa stella non sono stati scoperti pianeti e non vi \u00E8 alcuna prova di un disco di accrescimento."@it . . . "Beta Comae Berenices (\u03B2 Com) \u2013 najja\u015Bniejsza gwiazda w gwiazdozbiorze Warkocza Bereniki. Mimo \u017Ce w oznaczeniu Bayera grecka litera Beta (\u03B2) zwykle oznacza drug\u0105 co do jasno\u015Bci gwiazd\u0119 w gwiazdozbiorze, w tym przypadku ta gwiazda jest nieznacznie ja\u015Bniejsza od Alfa Comae Berenices."@pl . . "\uBA38\uB9AC\uD138\uC790\uB9AC \uBCA0\uD0C0(\u03B2 Com)\uB294 \uBA38\uB9AC\uD138\uC790\uB9AC\uC5D0 \uC788\uB294 \uD669\uC0C9 \uC65C\uC131\uC73C\uB85C \uC9C0\uAD6C\uC5D0\uC11C 29.78 \uAD11\uB144 \uB5A8\uC5B4\uC838 \uC788\uB2E4. \uC774 \uBCC4\uC758 \uBC14\uC774\uC5B4 \uAE30\uD638 \uBCA0\uD0C0(\u03B2)\uB294 \uBCC4\uC790\uB9AC\uC5D0\uC11C \uB450\uBC88\uC9F8\uB85C \uBC1D\uB2E4\uB294 \uC758\uBBF8\uC774\uB098, \uC2E4\uC81C\uB85C \uBA38\uB9AC\uD138\uC790\uB9AC \uBCA0\uD0C0\uC758 \uAC89\uBCF4\uAE30 \uB4F1\uAE09\uC740 4.3\uC73C\uB85C \uBCF4\uB2E4 \uADFC\uC18C\uD558\uAC8C \uBC1D\uB2E4. \uB9E8\uB208\uC73C\uB85C \uBCFC \uC218 \uC788\uB294 \uBC1D\uAE30\uC774\uC9C0\uB9CC \uB3C4\uC2EC\uC9C0\uC5D0\uC11C \uAD11\uACF5\uD574\uC758 \uC601\uD5A5\uC744 \uBC1B\uC744 \uACBD\uC6B0 \uB9E8\uB208 \uAD00\uCE21\uC774 \uD798\uB4E4 \uAC83\uC774\uB2E4. \uC774 \uBCC4\uC740 \uD0DC\uC591\uACFC \uBE44\uC2B7\uD558\uBA70 \uC57D\uAC04 \uB354 \uBC1D\uACE0 \uD45C\uBA74 \uC628\uB3C4\uB3C4 \uC57D\uAC04 \uB354 \uB728\uAC81\uB2E4. \uBD84\uAD11\uD615\uC740 G0 V\uC774\uB2E4. \uBCA0\uD0C0\uC758 \uD45C\uBA74 \uC628\uB3C4\uB294 5936 \uCF08\uBE48\uC73C\uB85C \uC774 \uC628\uB3C4\uC5D0\uC11C \uD56D\uC131\uC740 G\uD615 \uC8FC\uACC4\uC5F4\uC758 \uB178\uB780 \uAD11\uAD6C\uC0C9\uC744 \uBCF4\uC5EC\uC900\uB2E4. \uBCA0\uD0C0\uC758 \uB098\uC774\uB294 \uD0DC\uC591\uBCF4\uB2E4 \uC80A\uC740 \uAC83\uC73C\uB85C \uCD94\uCE21\uB418\uBA70 \uC57D 30\uC5B5 \uB144\uC774\uB2E4(\uD0DC\uC591\uC740 46\uC5B5 \uB144)."@ko . "Beta Comae Berenices"@in . "\u5468\u9F0E\u4E00"@zh . ""@en . . . . . . "Beta Comae Berenices (\u03B2 Com / \u03B2 Comae Berenices / Beta Comae Berenices) \u00E8 una stella appartenente alla sequenza principale che si trova a 29,9 anni luce di distanza dal Sistema solare, nella costellazione della Chioma di Berenice. \u00C8 una stella di classe spettrale G0-V e attualmente, nonostante sia designata con la lettera beta, \u00E8 leggermente pi\u00F9 brillante di Alfa Comae Berenices."@it . "108.8951"^^ . "Beta Comae Berenices (\u03B2 Comae Berenices / \u03B2 Com) est l'\u00E9toile la plus brillante de la constellation de la Chevelure de B\u00E9r\u00E9nice. La lettre grecque b\u00EAta (\u03B2) indique normalement que l'\u00E9toile poss\u00E8de la deuxi\u00E8me plus faible magnitude apparente de la constellation. En r\u00E9alit\u00E9, elle est l\u00E9g\u00E8rement plus brillante que \u03B1 Comae Berenices. C'est une \u00E9toile naine de la s\u00E9quence principale semblable au Soleil, \u00E9tant l\u00E9g\u00E8rement plus grande et brillante en magnitude absolue. La surface de cette \u00E9toile a un cycle d'activit\u00E9 de 16,6 ann\u00E9es (\u00E0 comparer \u00E0 un cycle de 11 ans pour le Soleil). Elle pourrait \u00E9galement avoir un cycle d'activit\u00E9 secondaire de 9,6 ans. \u00C0 une \u00E9poque, on a pens\u00E9 que cette \u00E9toile pouvait avoir une compagne spectroscopique. Cependant, cette hypoth\u00E8se a \u00E9t\u00E9 \u00E9cart\u00E9e au moyen de mesures de vitesse radiale plus pr\u00E9cises. Aucune plan\u00E8te n'a encore \u00E9t\u00E9 d\u00E9tect\u00E9e autour de cette \u00E9toile et il n'y a pas de disque de poussi\u00E8res."@fr . . "Beta Comae Berenices"@pl . "Beta Comae Berenices (43 Comae Berenices) \u00E9 uma estrela na dire\u00E7\u00E3o da Coma Berenices. Possui uma ascens\u00E3o reta de 13h 11m 52.92s e uma declina\u00E7\u00E3o de +27\u00B0 52\u2032 33.7\u2033. Sua magnitude aparente \u00E9 igual a 4.23. Considerando sua dist\u00E2ncia de 30 anos-luz em rela\u00E7\u00E3o \u00E0 Terra, sua magnitude absoluta \u00E9 igual a 4.42. Pertence \u00E0 classe espectral G0V."@pt . . . . . "+0.58"@en . . . . . "\uBA38\uB9AC\uD138\uC790\uB9AC \uBCA0\uD0C0(\u03B2 Com)\uB294 \uBA38\uB9AC\uD138\uC790\uB9AC\uC5D0 \uC788\uB294 \uD669\uC0C9 \uC65C\uC131\uC73C\uB85C \uC9C0\uAD6C\uC5D0\uC11C 29.78 \uAD11\uB144 \uB5A8\uC5B4\uC838 \uC788\uB2E4. \uC774 \uBCC4\uC758 \uBC14\uC774\uC5B4 \uAE30\uD638 \uBCA0\uD0C0(\u03B2)\uB294 \uBCC4\uC790\uB9AC\uC5D0\uC11C \uB450\uBC88\uC9F8\uB85C \uBC1D\uB2E4\uB294 \uC758\uBBF8\uC774\uB098, \uC2E4\uC81C\uB85C \uBA38\uB9AC\uD138\uC790\uB9AC \uBCA0\uD0C0\uC758 \uAC89\uBCF4\uAE30 \uB4F1\uAE09\uC740 4.3\uC73C\uB85C \uBCF4\uB2E4 \uADFC\uC18C\uD558\uAC8C \uBC1D\uB2E4. \uB9E8\uB208\uC73C\uB85C \uBCFC \uC218 \uC788\uB294 \uBC1D\uAE30\uC774\uC9C0\uB9CC \uB3C4\uC2EC\uC9C0\uC5D0\uC11C \uAD11\uACF5\uD574\uC758 \uC601\uD5A5\uC744 \uBC1B\uC744 \uACBD\uC6B0 \uB9E8\uB208 \uAD00\uCE21\uC774 \uD798\uB4E4 \uAC83\uC774\uB2E4. \uC774 \uBCC4\uC740 \uD0DC\uC591\uACFC \uBE44\uC2B7\uD558\uBA70 \uC57D\uAC04 \uB354 \uBC1D\uACE0 \uD45C\uBA74 \uC628\uB3C4\uB3C4 \uC57D\uAC04 \uB354 \uB728\uAC81\uB2E4. \uBD84\uAD11\uD615\uC740 G0 V\uC774\uB2E4. \uBCA0\uD0C0\uC758 \uD45C\uBA74 \uC628\uB3C4\uB294 5936 \uCF08\uBE48\uC73C\uB85C \uC774 \uC628\uB3C4\uC5D0\uC11C \uD56D\uC131\uC740 G\uD615 \uC8FC\uACC4\uC5F4\uC758 \uB178\uB780 \uAD11\uAD6C\uC0C9\uC744 \uBCF4\uC5EC\uC900\uB2E4. \uBCA0\uD0C0\uC758 \uB098\uC774\uB294 \uD0DC\uC591\uBCF4\uB2E4 \uC80A\uC740 \uAC83\uC73C\uB85C \uCD94\uCE21\uB418\uBA70 \uC57D 30\uC5B5 \uB144\uC774\uB2E4(\uD0DC\uC591\uC740 46\uC5B5 \uB144). \uC774 \uBCC4\uC758 \uB2E8\uC8FC\uAE30 \uBC1D\uAE30 \uBCC0\uD654\uB97C \uAD00\uCE21\uD55C \uACB0\uACFC \uBCA0\uD0C0\uB294 \uC704\uB3C4\uC5D0 \uB530\uB77C \uC790\uC804\uC18D\uB3C4\uC5D0 \uCC28\uC774\uAC00 \uC788\uC5C8\uB294\uB370 \uADF8 \uBC94\uC704\uB294 \uCD5C\uC18C 11\uC77C\uC5D0\uC11C \uCD5C\uB300 13\uC77C \uC0AC\uC774\uC774\uB2E4. \uC774 \uBCC4\uC758 \uD751\uC810 \uD65C\uB3D9 \uC8FC\uAE30\uB294 \uD0DC\uC591\uC758 11\uB144\uBCF4\uB2E4 \uC880 \uB354 \uAE34 16\uB144\uC774\uBA70, 9.6\uB144\uC758 \uD65C\uB3D9 \uC8FC\uAE30\uAC00 \uBCC4\uB3C4\uB85C \uC788\uB294 \uAC83\uC73C\uB85C \uBC1D\uD600\uC84C\uB2E4. \uD55C \uB54C \uBA38\uB9AC\uD138\uC790\uB9AC \uBCA0\uD0C0\uAC00 \uB3D9\uBC18\uC131\uC744 \uAC70\uB290\uB9AC\uACE0 \uC788\uB294 \uAC83\uC73C\uB85C \uCD94\uCE21\uD558\uAE30\uB3C4 \uD588\uC73C\uB098, \uC815\uAD50\uD55C \uC2DC\uC120\uC18D\uB3C4 \uAD00\uCE21\uACB0\uACFC \uC9DD\uBCC4\uC740 \uC5C6\uB294 \uAC83\uC73C\uB85C \uBC1D\uD600\uC84C\uB2E4. \uBCA0\uD0C0\uBCC4 \uC8FC\uC704\uC5D0\uB294 \uBA3C\uC9C0 \uC6D0\uBC18\uC774 \uC5C6\uC73C\uBA70, \uC678\uACC4 \uD589\uC131\uC758 \uC874\uC7AC\uB3C4 \uC544\uC9C1 \uD655\uC778\uB418\uC9C0 \uC54A\uACE0 \uC788\uB2E4."@ko . "\uBA38\uB9AC\uD138\uC790\uB9AC \uBCA0\uD0C0"@ko . . "Beta Comae Berenices"@it . . "Beta Comae Berenices (43 Comae Berenices) \u00E9 uma estrela na dire\u00E7\u00E3o da Coma Berenices. Possui uma ascens\u00E3o reta de 13h 11m 52.92s e uma declina\u00E7\u00E3o de +27\u00B0 52\u2032 33.7\u2033. Sua magnitude aparente \u00E9 igual a 4.23. Considerando sua dist\u00E2ncia de 30 anos-luz em rela\u00E7\u00E3o \u00E0 Terra, sua magnitude absoluta \u00E9 igual a 4.42. Pertence \u00E0 classe espectral G0V."@pt . . . . . "Beta Comae Berenices (\u03B2 Comae Berenices / \u03B2 Com) est l'\u00E9toile la plus brillante de la constellation de la Chevelure de B\u00E9r\u00E9nice. La lettre grecque b\u00EAta (\u03B2) indique normalement que l'\u00E9toile poss\u00E8de la deuxi\u00E8me plus faible magnitude apparente de la constellation. En r\u00E9alit\u00E9, elle est l\u00E9g\u00E8rement plus brillante que \u03B1 Comae Berenices."@fr . . . . "Beta Comae Berenices (\u03B2 Com / 43 Com / HD 114710) es la estrella m\u00E1s brillante de la constelaci\u00F3n de Cabellera de Berenice, con magnitud aparente +4,23. Relativamente pr\u00F3xima al Sistema Solar, se encuentra a solo 29,9 a\u00F1os luz de distancia.La estrella conocida m\u00E1s cercana a ella es , distante 4,5 a\u00F1os luz.\u200B Beta Comae Berenices es una enana amarilla no muy distinta del Sol cuyo tipo espectral es G0V.\u200B Con una temperatura efectiva de 6000 K, es unos 280 K m\u00E1s caliente que el Sol, siendo un 37% m\u00E1s luminosa que este. Su par\u00E1metros de masa y di\u00E1metro son un 10% mayores que los del Sol. Su metalicidad \u2014medida por el contenido de hierro en relaci\u00F3n con el de hidr\u00F3geno\u2014 parece ser mayor que la solar, en torno a un 7%.\u200B Con una velocidad de rotaci\u00F3n doble que la del Sol, presenta tambi\u00E9n actividad magn\u00E9tica, incluyendo erupciones y manchas estelares, en un ciclo de 16,6 a\u00F1os y un posible ciclo secundario de 9,6 a\u00F1os. Aunque m\u00E1s joven que el Sol, no hay acuerdo sobre su edad, que seg\u00FAn la fuente consultada puede ser de 1700, 4100 o 4400 millones de a\u00F1os.\u200B Beta Comae Berenices puede tener una compa\u00F1era estelar pr\u00F3xima, detectada solo por espectroscopia, que no ha sido confirmada.\u200B\u200B Estudios llevados a cabo mediante la t\u00E9cnica de velocidad radial no han detectado planetas a su alrededor.\u200B"@es . "1.15"^^ . "Beta Comae Berenices"@es . . "Beta de la Cabellera de Berenice"@ca . "\u0411\u0435\u0442\u0430 \u0412\u043E\u043B\u043E\u0441 \u0412\u0435\u0440\u043E\u043D\u0438\u043A\u0438"@ru . "4.38"^^ . . . . . . . . . . "-803.372"^^ . . . "0.3487"^^ . "+6.1"@en . "\u0411\u0435\u0442\u0430 \u0412\u043E\u043B\u043E\u0441 \u0412\u0435\u0440\u043E\u043D\u0438\u043A\u0438 (\u043B\u0430\u0442. \u03B2 Comae Berenices), 43 \u0412\u043E\u043B\u043E\u0441 \u0412\u0435\u0440\u043E\u043D\u0438\u043A\u0438 (\u043B\u0430\u0442. 43 Comae Berenices), HD 114710 \u2014 \u0434\u0432\u043E\u0439\u043D\u0430\u044F \u0437\u0432\u0435\u0437\u0434\u0430 \u0432 \u0441\u043E\u0437\u0432\u0435\u0437\u0434\u0438\u0438 \u0412\u043E\u043B\u043E\u0441\u044B \u0412\u0435\u0440\u043E\u043D\u0438\u043A\u0438 \u043D\u0430 \u0440\u0430\u0441\u0441\u0442\u043E\u044F\u043D\u0438\u0438 \u043F\u0440\u0438\u0431\u043B\u0438\u0437\u0438\u0442\u0435\u043B\u044C\u043D\u043E 30 \u0441\u0432\u0435\u0442\u043E\u0432\u044B\u0445 \u043B\u0435\u0442 (\u043E\u043A\u043E\u043B\u043E 9,2 \u043F\u0430\u0440\u0441\u0435\u043A\u0430) \u043E\u0442 \u0421\u043E\u043B\u043D\u0446\u0430. \u0412\u043E\u0437\u0440\u0430\u0441\u0442 \u0437\u0432\u0435\u0437\u0434\u044B \u043E\u043F\u0440\u0435\u0434\u0435\u043B\u0451\u043D \u043A\u0430\u043A \u043E\u043A\u043E\u043B\u043E 1,7 \u043C\u043B\u0440\u0434 \u043B\u0435\u0442."@ru . . "G0 V"@en . "4.1"^^ . "Beta Comae Berenices"@en . . . . . "Beta Comae Berenices (\u03B2 Comae Berenices, \u03B2 Com) \u00E4r stj\u00E4rnans Bayerbeteckning och den ing\u00E5r i den norra delen av stj\u00E4rnbilden Berenikes h\u00E5r. Den befinner sig p\u00E5 ett avst\u00E5nd av cirka 29,78 ljus\u00E5r (9,13 parsecs ) fr\u00E5n solen. Den grekiska bokstaven beta (\u03B2) indikerar vanligtvis att stj\u00E4rnan har stj\u00E4rnbildens n\u00E4st h\u00F6gsta skenbara magnitud. Med en skenbar magnitud p\u00E5 4,3 \u00E4r emellertid denna stj\u00E4rna faktiskt n\u00E5got ljusare \u00E4n \u03B1 Comae Berenices. Den kan ses med blotta \u00F6gat, men kan vara f\u00F6r svag f\u00F6r att ses fr\u00E5n ett t\u00E4tortssomr\u00E5de med ljusf\u00F6roreningar."@sv . . . "Beta Comae Berenices"@nl . . "Beta Comae Berenices (\u03B2 Comae Berenices, \u03B2 Com) ist ein Hauptreihenstern im Sternbild Haar der Berenike, der etwa 29,78 Lichtjahre von der Sonne entfernt ist. Die Bayer-Bezeichnung \"Beta\" (\u03B2) legt dabei auf den ersten Blick nahe, dass es sich um den zweithellsten Stern im Sternbild handelt. Tats\u00E4chlich ist seine scheinbare Helligkeit jedoch etwas h\u00F6her als die von Alpha Comae Berenices. \u03B2 Com kann mit dem blo\u00DFen Auge beobachtet werden, ist jedoch in st\u00E4dtischen Gebieten mit hoher Lichtverschmutzung kaum zu erkennen."@de . "\u304B\u307F\u306E\u3051\u5EA7\u03B2\u661F (\u03B2 Comae Berenices / \u03B2 Com) \u306F\u3001\u304B\u307F\u306E\u3051\u5EA7\u3067\u6700\u3082\u660E\u308B\u3044\u6052\u661F\u3002 \u30D0\u30A4\u30A8\u30EB\u7B26\u53F7\u306E\u03B2\uFF08\u30D9\u30FC\u30BF\uFF09\u306F\u3001\u901A\u5E38\u306F\u305D\u306E\u661F\u5EA7\u3067\u5B9F\u8996\u7B49\u7D1A\u304C2\u756A\u76EE\u306B\u660E\u308B\u3044\u6052\u661F\u306B\u4E0E\u3048\u3089\u308C\u308B\u304C\u3001\u3053\u306E\u6052\u661F\u306F\u304B\u307F\u306E\u3051\u5EA7\u03B1\u661F\u3088\u308A\u660E\u308B\u3044\u3002 \u3053\u306E\u6052\u661F\u306F\u8584\u9EC4\u8272\u306E\u4E3B\u7CFB\u5217\u661F\u3067\u3042\u308B\u3002\u592A\u967D\u3068\u4F3C\u3066\u3044\u3066\u3001\u5C11\u3057\u5927\u304D\u304F\uFF08\u7D76\u5BFE\u7B49\u7D1A\u304C\uFF09\u660E\u308B\u3044\u3060\u3051\u3067\u3042\u308B\u3002\u6052\u661F\u8868\u9762\u306E\u6D3B\u52D5\u30B5\u30A4\u30AF\u30EB\u306F16.6\u5E74\uFF08\u592A\u967D\u306F11\u5E74\uFF09\u3067\u30019.6\u5E74\u306E\u7B2C2\u6B21\u6D3B\u52D5\u30B5\u30A4\u30AF\u30EB\u3082\u3042\u308B\u3002\u304B\u3064\u3066\u306F\u5206\u5149\u9023\u661F\u306E\u53EF\u80FD\u6027\u304C\u6307\u6458\u3055\u308C\u305F\u304C\u3001\u8996\u7DDA\u901F\u5EA6\u6E2C\u5B9A\u306E\u7CBE\u5EA6\u304C\u5411\u4E0A\u3057\u305F\u3053\u3068\u3067\u5426\u5B9A\u3055\u308C\u305F\u3002\u3053\u306E\u6052\u661F\u3092\u5DE1\u308B\u60D1\u661F\u304A\u3088\u3073\u539F\u59CB\u60D1\u661F\u7CFB\u5186\u76E4\u306F\u89B3\u6E2C\u3055\u308C\u3066\u3044\u306A\u3044\u3002"@ja . . "\u5468\u9F0E\u4E00 \uFF08\u03B2 Com / \u540E\u53D1\u5EA7\u03B2\uFF09\u662F\u540E\u53D1\u5EA7\u7684\u4E00\u9897\u4E3B\u5E8F\u77EE\u661F\uFF0C\u8DDD\u79BB\u5730\u7403\u7EA630\u5149\u5E74\u3002\u5E0C\u81D8\u5B57\u6BCD\u7684\u03B2\u901A\u5E38\u6A19\u793A\u661F\u5EA7\u4E2D\u8996\u661F\u7B49\u7B2C\u4E8C\u4EAE\u7684\u661F\uFF0C\u4F46\u662F\u5468\u9F0E\u4E00\u6BD4\u540E\u9AEE\u5EA7\u03B1\uFF08+5.22\u7B49\uFF09\u9084\u4EAE\u3002 \u9019\u9846\u6046\u661F\u8207\u6211\u5011\u7684\u592A\u967D\u76F8\u4F3C\uFF0C\u53EA\u662F\u9084\u7A0D\u5FAE\u5927\u4E00\u9EDE\uFF0C\u7D55\u5C0D\u661F\u7B49\u4EAE\u4E00\u9EDE\u3002\u89C0\u5BDF\u8272\u7403\u6D3B\u52D5\u7684\u77ED\u671F\u8B8A\u5316\uFF0C\u8A8D\u70BA\u9019\u9846\u6046\u661F\u7D93\u6B77\u8457\u4E0D\u540C\u7684\u81EA\u8F49\uFF0C\u5468\u671F\u5927\u7D04\u572811\u201313\u5929\u3002\u9019\u9846\u6046\u661F\u8868\u9762\u7684\u6D3B\u52D5\u9031\u671F\u662F16.6\u5E74\uFF0C\u76F8\u8F03\u65BC\u592A\u967D\u768411\u5E74\u4E5F\u8F03\u9577\u4E9B\uFF0C\u4F46\u5B83\u53EF\u80FD\u4E5F\u67099.6\u5E74\u7684\u7B2C\u4E8C\u500B\u6D3B\u52D5\u9031\u671F\u3002\u66FE\u7D93\u4E00\u5EA6\u8A8D\u70BA\u9019\u9846\u6046\u661F\u6709\u9846\u5149\u8B5C\u4F34\u661F\uFF0C\u4F46\u662F\u7CBE\u6E96\u7684\u5F91\u5411\u901F\u5EA6\u6E2C\u91CF\u6392\u9664\u4E86\u9019\u500B\u53EF\u80FD\uFF0C\u4E0D\u50C5\u6C92\u6709\u5075\u6E2C\u5230\u884C\u661F\u74B0\u7E5E\u8457\u5B83\uFF0C\u4E5F\u6C92\u6709\u8B49\u64DA\u986F\u793A\u6709\u5875\u57C3\u76E4\u7684\u5B58\u5728\u3002"@zh . . . . . . . ""@en . . . . . . . ""@en . . . "Beta Coma Berenices (\u03B2 Comae Berenices, \u03B2 Com) adalah bintang katai di rasi Coma Berenices. Bintang ini berada pada jarak 30 tahun cahaya. Meskipun dinamakan beta, tetapi kenyataaannya bintang ini lebih terang daripada \u03B1 Com, yaitu bermagnitudo 4.23"@in . "+882.512 \u00B1 0.526"@en . . "Beta Coma Berenices (\u03B2 Comae Berenices, \u03B2 Com) adalah bintang katai di rasi Coma Berenices. Bintang ini berada pada jarak 30 tahun cahaya. Meskipun dinamakan beta, tetapi kenyataaannya bintang ini lebih terang daripada \u03B1 Com, yaitu bermagnitudo 4.23"@in . . . . . "1.5"^^ . "Beta Comae Berenices is een gele dwerg met een spectraalklasse van G0.V. De ster bevindt zich 30,0 lichtjaar van de zon."@nl . . . "5936"^^ . . "11458"^^ . . . "Beta Comae Berenices (\u03B2 Comae Berenices, \u03B2 Com) ist ein Hauptreihenstern im Sternbild Haar der Berenike, der etwa 29,78 Lichtjahre von der Sonne entfernt ist. Die Bayer-Bezeichnung \"Beta\" (\u03B2) legt dabei auf den ersten Blick nahe, dass es sich um den zweithellsten Stern im Sternbild handelt. Tats\u00E4chlich ist seine scheinbare Helligkeit jedoch etwas h\u00F6her als die von Alpha Comae Berenices. \u03B2 Com kann mit dem blo\u00DFen Auge beobachtet werden, ist jedoch in st\u00E4dtischen Gebieten mit hoher Lichtverschmutzung kaum zu erkennen. Der Stern ist der Sonne \u00E4hnlich, aber etwas gr\u00F6\u00DFer und heller in Bezug auf seine absolute Helligkeit. Seine Spektralklasse wird mit F9.5V angegeben, teilweise auch mit G0V. Die effektive Temperatur seiner Oberfl\u00E4che betr\u00E4gt 5.936 Kelvin. Mit einem Alter von etwa 3 Milliarden Jahren ist \u03B2 Com j\u00FCnger als die Sonne. Beobachtungen legen eine Rotationsperiode von ann\u00E4hernd 11 bis 13 Tagen nahe. Seine Oberfl\u00E4che hat einen Aktivit\u00E4tszyklus von 16,6 Jahren, verglichen mit dem 11-j\u00E4hrigen Zyklus der Sonne. M\u00F6glicherweise hat \u03B2 Com auch einen sekund\u00E4ren Aktivit\u00E4tszyklus von 9,6 Jahren. Zeitweise wurde vermutet, dass er einen spektroskopischen Begleiter besitzt. Dies wurde jedoch durch genauere Messungen seiner Radialgeschwindigkeit ausgeschlossen. Ebenso gibt es bisher keine Hinweise auf einen Exoplaneten oder eine Tr\u00FCmmerscheibe um \u03B2 Com. Die habitable Zone von \u03B2 Com und damit die Region, wo auf einem erd\u00E4hnlichen Planeten fl\u00FCssiges Wasser existieren k\u00F6nnte, erstreckt sich zwischen 0,981 und 1,042 AE Abstand von dem Stern."@de . "Beta Comae Berenices (\u03B2 Comae Berenices, \u03B2 Com) is a main sequence dwarf star in the northern constellation of Coma Berenices. It is located at a distance of about 29.95 light-years (9.18 parsecs) from Earth. The Greek letter beta (\u03B2) usually indicates that the star has the second highest visual magnitude in the constellation. However, with an apparent visual magnitude of 4.3, this star is actually slightly brighter than \u03B1 Comae Berenices. It can be seen with the naked eye, but may be too dim to be viewed from a built-up urban area."@en . . "Beta de la Cabellera de Berenice (\u03B2 Comae Berenices) \u00E9s l'estel m\u00E9s brillant a la constel\u00B7laci\u00F3 de la Cabellera de Berenice, amb magnitud aparent +4,23. Relativament propera al sistema solar, s'hi troba a nom\u00E9s 29,9 anys llum de dist\u00E0ncia. L'estel conegut m\u00E9s proper a ell \u00E9s , distant 4,5 anys llum. Beta de la Cabellera de Berenice pot tenir un company estel\u00B7lar proper, detectat nom\u00E9s per espectrosc\u00F2pia, que no ha estat confirmat. Estudis duts a terme mitjan\u00E7ant la t\u00E8cnica de velocitat radial no han detectat planetes al seu voltant."@ca . "4.26"^^ . "\u0411\u0435\u0442\u0430 \u0412\u043E\u043B\u043E\u0441 \u0412\u0435\u0440\u043E\u043D\u0438\u043A\u0438 (\u043B\u0430\u0442. \u03B2 Comae Berenices), 43 \u0412\u043E\u043B\u043E\u0441 \u0412\u0435\u0440\u043E\u043D\u0438\u043A\u0438 (\u043B\u0430\u0442. 43 Comae Berenices), HD 114710 \u2014 \u0434\u0432\u043E\u0439\u043D\u0430\u044F \u0437\u0432\u0435\u0437\u0434\u0430 \u0432 \u0441\u043E\u0437\u0432\u0435\u0437\u0434\u0438\u0438 \u0412\u043E\u043B\u043E\u0441\u044B \u0412\u0435\u0440\u043E\u043D\u0438\u043A\u0438 \u043D\u0430 \u0440\u0430\u0441\u0441\u0442\u043E\u044F\u043D\u0438\u0438 \u043F\u0440\u0438\u0431\u043B\u0438\u0437\u0438\u0442\u0435\u043B\u044C\u043D\u043E 30 \u0441\u0432\u0435\u0442\u043E\u0432\u044B\u0445 \u043B\u0435\u0442 (\u043E\u043A\u043E\u043B\u043E 9,2 \u043F\u0430\u0440\u0441\u0435\u043A\u0430) \u043E\u0442 \u0421\u043E\u043B\u043D\u0446\u0430. \u0412\u043E\u0437\u0440\u0430\u0441\u0442 \u0437\u0432\u0435\u0437\u0434\u044B \u043E\u043F\u0440\u0435\u0434\u0435\u043B\u0451\u043D \u043A\u0430\u043A \u043E\u043A\u043E\u043B\u043E 1,7 \u043C\u043B\u0440\u0434 \u043B\u0435\u0442."@ru . . . "1.357"^^ . "+0.07"@en . . . ""@en . . "\u304B\u307F\u306E\u3051\u5EA7\u30D9\u30FC\u30BF\u661F"@ja . "1.106"^^ . . "Beta Comae Berenices (\u03B2 Com) \u2013 najja\u015Bniejsza gwiazda w gwiazdozbiorze Warkocza Bereniki. Mimo \u017Ce w oznaczeniu Bayera grecka litera Beta (\u03B2) zwykle oznacza drug\u0105 co do jasno\u015Bci gwiazd\u0119 w gwiazdozbiorze, w tym przypadku ta gwiazda jest nieznacznie ja\u015Bniejsza od Alfa Comae Berenices."@pl . . "Beta Comae Berenices"@en . . . "1079517428"^^ . . . . "Beta de la Cabellera de Berenice (\u03B2 Comae Berenices) \u00E9s l'estel m\u00E9s brillant a la constel\u00B7laci\u00F3 de la Cabellera de Berenice, amb magnitud aparent +4,23. Relativament propera al sistema solar, s'hi troba a nom\u00E9s 29,9 anys llum de dist\u00E0ncia. L'estel conegut m\u00E9s proper a ell \u00E9s , distant 4,5 anys llum. Beta de la Cabellera de Berenice \u00E9s un nan groc no gaire diferent del Sol amb un tipus espectral G0V. Amb una temperatura efectiva de 6.000 K, \u00E9s uns 280 K m\u00E9s calenta que el Sol, i \u00E9s un 37% m\u00E9s lluminosa que aquest. El seu par\u00E0metres de massa i di\u00E0metre s\u00F3n un 10% majors que els de el Sol. La seva metal\u00B7licitat \u2014mesurada pel contingut de ferro en relaci\u00F3 al d'hidrogen\u2014 sembla major que la solar, al voltant d'un 7%. Amb una velocitat de rotaci\u00F3 doble que la del Sol, presenta tamb\u00E9 activitat magn\u00E8tica, incloent-hi erupcions i taques estel\u00B7lars, en un cicle de 16,6 anys i un possible cicle secundari de 9,6 anys. Encara que m\u00E9s jove que el Sol, no hi ha acord sobre la seva edat, que segons la font consultada pot ser de 1.700, 4.100 \u00F3 4.400 milions d'anys. Beta de la Cabellera de Berenice pot tenir un company estel\u00B7lar proper, detectat nom\u00E9s per espectrosc\u00F2pia, que no ha estat confirmat. Estudis duts a terme mitjan\u00E7ant la t\u00E8cnica de velocitat radial no han detectat planetes al seu voltant."@ca . "Beta Comae Berenices (\u03B2 Comae Berenices, \u03B2 Com) is a main sequence dwarf star in the northern constellation of Coma Berenices. It is located at a distance of about 29.95 light-years (9.18 parsecs) from Earth. The Greek letter beta (\u03B2) usually indicates that the star has the second highest visual magnitude in the constellation. However, with an apparent visual magnitude of 4.3, this star is actually slightly brighter than \u03B1 Comae Berenices. It can be seen with the naked eye, but may be too dim to be viewed from a built-up urban area. The star is similar to the Sun, being only slightly larger and brighter in absolute magnitude. It has a stellar classification of G0 V, compared to G2 V for the Sun. The effective temperature of the outer envelope is 5,936 K, giving it a yellow hue of a G-type star. In terms of age it is younger than the Sun, being about 3 billion years old. Observations of short term variations in the chromatic activity suggest that the star undergoes differential rotation, with a rotation period of about 11\u201313 days. Its surface has a measured activity cycle of 16.6 years, compared to 11 years on the Sun. It may also have a secondary activity cycle of 9.6 years. At one time it was thought that this star might have a spectroscopic companion. However, this was ruled out by means of more accurate radial velocity measurements. No planets have yet been detected around it, and there is no evidence of a dusty disk. The habitable zone for this star, defined as the locations where liquid water could be present on an Earth-like planet, is 0.918\u20131.96 AU, where 1 AU is the average distance from the Earth to the Sun."@en . "Beta Comae Berenices is een gele dwerg met een spectraalklasse van G0.V. De ster bevindt zich 30,0 lichtjaar van de zon."@nl . "Beta Comae Berenices (\u03B2 Comae Berenices, \u03B2 Com) \u00E4r stj\u00E4rnans Bayerbeteckning och den ing\u00E5r i den norra delen av stj\u00E4rnbilden Berenikes h\u00E5r. Den befinner sig p\u00E5 ett avst\u00E5nd av cirka 29,78 ljus\u00E5r (9,13 parsecs ) fr\u00E5n solen. Den grekiska bokstaven beta (\u03B2) indikerar vanligtvis att stj\u00E4rnan har stj\u00E4rnbildens n\u00E4st h\u00F6gsta skenbara magnitud. Med en skenbar magnitud p\u00E5 4,3 \u00E4r emellertid denna stj\u00E4rna faktiskt n\u00E5got ljusare \u00E4n \u03B1 Comae Berenices. Den kan ses med blotta \u00F6gat, men kan vara f\u00F6r svag f\u00F6r att ses fr\u00E5n ett t\u00E4tortssomr\u00E5de med ljusf\u00F6roreningar."@sv . "4.46"^^ . "+0.08"@en . . . "Beta Comae Berenices (\u03B2 Com / 43 Com / HD 114710) es la estrella m\u00E1s brillante de la constelaci\u00F3n de Cabellera de Berenice, con magnitud aparente +4,23. Relativamente pr\u00F3xima al Sistema Solar, se encuentra a solo 29,9 a\u00F1os luz de distancia.La estrella conocida m\u00E1s cercana a ella es , distante 4,5 a\u00F1os luz.\u200B Beta Comae Berenices puede tener una compa\u00F1era estelar pr\u00F3xima, detectada solo por espectroscopia, que no ha sido confirmada.\u200B\u200B Estudios llevados a cabo mediante la t\u00E9cnica de velocidad radial no han detectado planetas a su alrededor.\u200B"@es . . . . "Beta Comae Berenices"@fr . . . . "\u304B\u307F\u306E\u3051\u5EA7\u03B2\u661F (\u03B2 Comae Berenices / \u03B2 Com) \u306F\u3001\u304B\u307F\u306E\u3051\u5EA7\u3067\u6700\u3082\u660E\u308B\u3044\u6052\u661F\u3002 \u30D0\u30A4\u30A8\u30EB\u7B26\u53F7\u306E\u03B2\uFF08\u30D9\u30FC\u30BF\uFF09\u306F\u3001\u901A\u5E38\u306F\u305D\u306E\u661F\u5EA7\u3067\u5B9F\u8996\u7B49\u7D1A\u304C2\u756A\u76EE\u306B\u660E\u308B\u3044\u6052\u661F\u306B\u4E0E\u3048\u3089\u308C\u308B\u304C\u3001\u3053\u306E\u6052\u661F\u306F\u304B\u307F\u306E\u3051\u5EA7\u03B1\u661F\u3088\u308A\u660E\u308B\u3044\u3002 \u3053\u306E\u6052\u661F\u306F\u8584\u9EC4\u8272\u306E\u4E3B\u7CFB\u5217\u661F\u3067\u3042\u308B\u3002\u592A\u967D\u3068\u4F3C\u3066\u3044\u3066\u3001\u5C11\u3057\u5927\u304D\u304F\uFF08\u7D76\u5BFE\u7B49\u7D1A\u304C\uFF09\u660E\u308B\u3044\u3060\u3051\u3067\u3042\u308B\u3002\u6052\u661F\u8868\u9762\u306E\u6D3B\u52D5\u30B5\u30A4\u30AF\u30EB\u306F16.6\u5E74\uFF08\u592A\u967D\u306F11\u5E74\uFF09\u3067\u30019.6\u5E74\u306E\u7B2C2\u6B21\u6D3B\u52D5\u30B5\u30A4\u30AF\u30EB\u3082\u3042\u308B\u3002\u304B\u3064\u3066\u306F\u5206\u5149\u9023\u661F\u306E\u53EF\u80FD\u6027\u304C\u6307\u6458\u3055\u308C\u305F\u304C\u3001\u8996\u7DDA\u901F\u5EA6\u6E2C\u5B9A\u306E\u7CBE\u5EA6\u304C\u5411\u4E0A\u3057\u305F\u3053\u3068\u3067\u5426\u5B9A\u3055\u308C\u305F\u3002\u3053\u306E\u6052\u661F\u3092\u5DE1\u308B\u60D1\u661F\u304A\u3088\u3073\u539F\u59CB\u60D1\u661F\u7CFB\u5186\u76E4\u306F\u89B3\u6E2C\u3055\u308C\u3066\u3044\u306A\u3044\u3002"@ja . . .