. . . . . . "+0.585"@en . . . "Eta del Bover (\u03B7 Bootis) \u00E9s un estel binari, el tercer estel m\u00E9s brillant a la constel\u00B7laci\u00F3 del Bover despr\u00E9s d'Arcturus (\u03B1 Bootis) i Hissar (\u03B5 Bootis). Amb magnitud aparent +2,68, en el cel apareix molt prop d'Arcturus i de fet ambd\u00F3s estan a una dist\u00E0ncia gaireb\u00E9 id\u00E8ntica de la Terra \u201437 anys llum\u2014, estant separades nom\u00E9s 3,24 anys llum entre si. El nom del component principal Aa, i nom tradicional del sistema, \u00E9s Muphrid."@ca . "-1.6"^^ . "\u03B7 Bo\u00F6tis"@en . . "Mufrid (Eta Bo\u00F6tis / \u03B7 Boo / \u03B7 Bo\u00F6tis) \u00E8 una stella di classe spettrale G0-IV, distante 37 anni luce dal sistema solare, nella costellazione di Boote. Mufrid appare vicina alla stella di spicco di Boote, Arturo (Alpha Bootis) nel cielo della Terra, e Arturo \u00E8 in realt\u00E0 il suo pi\u00F9 prossimo vicino stellare, in quanto entrambe le stelle sono quasi alla stessa distanza dal Sole."@it . . . . "Eta Bootis (\u03B7 Boo / \u03B7 Bootis, \u00CAta Bootis) est une \u00E9toile binaire de la constellation du Bouvier. Elle porte \u00E9galement les noms traditionnels Muphrid ou Mufrid (arabe pour \u00AB solitaire \u00BB) ou Saak, et la d\u00E9signation de Flamsteed 8 Bootis. En astronomie chinoise, elle fait partie de l'ast\u00E9risme Sheti. Le nom de Muphrid a \u00E9t\u00E9 officialis\u00E9 par l'Union astronomique internationale le 12 septembre 2016. D'apr\u00E8s son spectre, Eta Bootis a un large exc\u00E8s d'\u00E9l\u00E9ments plus lourds que l'hydrog\u00E8ne. En fait, son rapport fer sur hydrog\u00E8ne est consid\u00E9r\u00E9 comme proche de la limite sup\u00E9rieure pour les \u00E9toiles naines du disque galactique. Eta Bootis est une binaire spectroscopique suspect\u00E9e avec une p\u00E9riode donn\u00E9e de 494 jours. Cependant, la compagne n'a pu \u00EAtre r\u00E9solue par interf\u00E9rom\u00E9trie des tavelures. Cela implique que si elle existe effectivement, elle doit \u00EAtre un objet de faible masse, de type M7 ou plus tardif encore. L'\u00E9toile appara\u00EEt proche de la brillante Arcturus (Alpha Bootis) dans le ciel, et Arcturus est effectivement sa plus proche voisine. Les deux \u00E9toiles sont distantes d'environ 3,24 ann\u00E9es-lumi\u00E8re, et chacune appara\u00EEtrait brillante dans le ciel de l'autre. Arcturus aurait une magnitude de -5,2 (environ 120 fois plus brillante que vue depuis la Terre, ou pr\u00E8s de deux fois la luminosit\u00E9 de V\u00E9nus) dans le ciel nocturne d'une hypoth\u00E9tique plan\u00E8te en orbite autour de Muphrid, tandis que Muphrid aurait une magnitude de -2,5 dans le ciel d'une hypoth\u00E9tique plan\u00E8te en orbite autour d'Arcturus, soit plus de deux fois la luminosit\u00E9 de Sirius dans notre ciel nocturne."@fr . "Muphrid"@sv . . "Eta Bo\u00F6tis (\u03B7 Boo / \u03B7 Bo\u00F6tis) adalah salah satu bintang di rasi Bo\u00F6tes. Berdasarkan sprktrumnya, Eta Bo\u00F6tis memiliki beberapa kelebihan elemen lebih tinggi daripada hidrogen. Faktanya adalah rasio besi terhadap hidrogen sangat dengan batas limit tertinggi untuk sebuah bintang katai. Bintang ini merupakan bintang ganda dengan period orbitnya adalah 494 hari. Bintang ini memiliki magnitudo 2.68 dan berjarak 37 tahun cahaya."@in . . . . . "Eta Bo\u00F6tis"@in . . . . . . . "\u3046\u3057\u304B\u3044\u5EA7\u30A4\u30FC\u30BF\u661F"@ja . "8.890000000000001"^^ . "Eta del Bover"@ca . . "\u0645\u0641\u0631\u062F \u0627\u0644\u0631\u0627\u0645\u062D (\u0628\u0627\u0644\u0644\u0627\u062A\u064A\u0646\u064A\u0629: \u03B7 Bo\u00F6tis)\u061B (\u0628\u0627\u0644\u0625\u0646\u062C\u0644\u064A\u0632\u064A\u0629: Muphrid)\u200F \u0648\u0647\u0648 \u0646\u062C\u0645 \u0645\u0632\u062F\u0648\u062C \u0634\u0645\u0627\u0644 \u0643\u0648\u0643\u0628\u0629 \u0627\u0644\u0639\u0648\u0627\u0621."@ar . . . . "+0.29 \u00B1\u00A00.07"@en . . . . "6100"^^ . . . . "2903315"^^ . "+0.207"@en . "14532"^^ . . . "\u0645\u0641\u0631\u062F \u0627\u0644\u0631\u0627\u0645\u062D (\u0628\u0627\u0644\u0644\u0627\u062A\u064A\u0646\u064A\u0629: \u03B7 Bo\u00F6tis)\u061B (\u0628\u0627\u0644\u0625\u0646\u062C\u0644\u064A\u0632\u064A\u0629: Muphrid)\u200F \u0648\u0647\u0648 \u0646\u062C\u0645 \u0645\u0632\u062F\u0648\u062C \u0634\u0645\u0627\u0644 \u0643\u0648\u0643\u0628\u0629 \u0627\u0644\u0639\u0648\u0627\u0621."@ar . "2.41"^^ . . "Eta Bo\u00F6tis"@en . "\u53F3\u6444\u63D0\u4E00\uFF08\u03B7 Boo/\u7267\u592B\u5EA7\u03B7\uFF09\uFF0C\u82F1\u6587\u540DMuphrid\uFF0C\u662F\u4E00\u4E2A\u4F4D\u4E8E\u7267\u592B\u5EA7\u7684\u6052\u661F\u3002\u81EA\u4ECE1943\u5E74\uFF0C\u8FD9\u4E2A\u6052\u661F\u7684\u5149\u8C31\u88AB\u4F5C\u4E3A\u5206\u7C7B\u5176\u5B83\u6052\u661F\u7684\u53C2\u8003\u70B9\u4E4B\u4E00\u3002"@zh . . . "1116592119"^^ . . . . "Eta Bo\u00F6tis (\u03B7 Bo\u00F6tis, abbreviated Eta Boo, \u03B7 Boo) is a binary star in the constellation of Bo\u00F6tes. Based on parallax measurements obtained during the Hipparcos mission, it is approximately 37 light-years (11 parsecs) distant from the Sun. Since 1943, the spectrum of this star has served as one of the stable anchor points by which other stars are classified. It forms a double star with the star BD+19 2726."@en . . "Mufrid"@it . . . "Mufrid"@nl . "\uBAA9\uB3D9\uC790\uB9AC \uC5D0\uD0C0\uB294 \uBAA9\uB3D9\uC790\uB9AC\uC5D0 \uC788\uB294 \uD56D\uC131\uC774\uB2E4. \uC774 \uBCC4\uC758 \uACE0\uC720 \uBA85\uCE6D\uC73C\uB85C\uB294 \uBB34\uD504\uB9AC\uB4DC(\uC544\uB78D\uC5B4\uB85C \u2018\uD2B9\uBCC4\uD55C \uC874\uC7AC\u2019\uB77C\uB294 \uC758\uBBF8\uC784) \uB610\uB294 \uC0AC\uC544\uD06C\uAC00 \uC788\uB2E4. \uD50C\uB7A8\uC2A4\uD2F0\uB4DC \uBA85\uBA85\uBC95\uC73C\uB85C\uB294 \uBAA9\uB3D9\uC790\uB9AC 8\uC774\uB77C\uACE0 \uBD80\uB978\uB2E4. \uBD84\uAD11\uD615\uC73C\uB85C \uBBF8\uB8E8\uC5B4 \uBCF4\uC544 \uBAA9\uB3D9\uC790\uB9AC \uC5D0\uD0C0\uB294 \uC218\uC18C\uBCF4\uB2E4 \uBB34\uAC70\uC6B4 \uC6D0\uC18C\uC758 \uD568\uB7C9\uC774 \uB9E4\uC6B0 \uB9CE\uB2E4. \uC2E4\uC81C \uC774 \uBCC4\uC758 \uC218\uC18C\uC5D0 \uB300\uD55C \uCCA0\uC758 \uD568\uB7C9\uC740 \uC5D0 \uC788\uB294 \uC8FC\uACC4\uC5F4\uC131\uB4E4\uC758 \uC0C1\uD55C\uC120\uC5D0 \uAC00\uAE4C\uC6B4 \uAC83\uC73C\uB85C \uBCF4\uC778\uB2E4. \uC774 \uBCC4\uC740 \uBD84\uAD11\uC30D\uC131\uC73C\uB85C\uB3C4 \uAD00\uCE21\uB418\uC5B4 \uC654\uC73C\uBA70, \uAD6C\uC131\uC6D0 \uB458\uC740 \uC11C\uB85C\uC758 \uC9C8\uB7C9\uC911\uC2EC\uC744 494\uC77C \uC8FC\uAE30\uB85C \uB3C8\uB2E4. \uADF8\uB7EC\uB098 \uB97C \uD1B5\uD574 \uC774 \uBCC4\uC758 \uC0C1\uC744 \uB530\uB85C \uAD6C\uD55C \uC801\uC740 \uC5C6\uB2E4. \uBAA9\uB3D9\uC790\uB9AC \uC5D0\uD0C0\uB294 \uC9C0\uAD6C \uBC24\uD558\uB298\uC5D0\uC11C \uC544\uD06C\uD22C\uB974\uC2A4\uC640 \uAC00\uAE4C\uC774 \uC788\uB294 \uAC83\uCC98\uB7FC \uBCF4\uC774\uBA70, \uC2E4\uC81C\uB85C \uB450 \uBCC4\uC740 \uAC00\uC7A5 \uAC00\uAE4C\uC774 \uBD99\uC5B4 \uC788\uB294 \uC874\uC7AC\uC774\uAE30\uB3C4 \uD558\uB2E4. \uB450 \uBCC4\uC758 \uC9C0\uAD6C\uB85C\uBD80\uD130\uC758 \uAC70\uB9AC\uB294 \uAC70\uC758 \uAC19\uC73C\uBA70 \uB458 \uC0AC\uC774\uB294 3.24\uAD11\uB144 \uB5A8\uC5B4\uC838 \uC788\uB2E4.[1] \uC11C\uB85C \uCCD0\uB2E4\uBCF8 \uC0C1\uB300 \uBCC4\uC740 \uBC24\uD558\uB298\uC5D0\uC11C \uB9E4\uC6B0 \uBC1D\uAC8C \uBE5B\uB0A0 \uAC83\uC774\uB2E4. \uC544\uD06C\uD22C\uB974\uC2A4\uB294 \uBAA9\uB3D9\uC790\uB9AC \uC5D0\uD0C0\uC5D0\uC11C \uBCFC \uB54C -5.2 \uB4F1\uAE09\uC73C\uB85C \uBC1D\uAC8C \uBE5B\uB0A0 \uAC83\uC774\uBA70, \uC774\uB294 \uC9C0\uAD6C\uC5D0\uC11C \uBC14\uB77C\uBCF8 \uAE08\uC131 \uBC1D\uAE30\uC758 \uAC70\uC758 \uB450 \uBC30\uC5D0 \uC774\uB978\uB2E4. \uBC18\uB300\uB85C \uC544\uD06C\uD22C\uB974\uC2A4\uC5D0\uC11C \uBB34\uD504\uB9AC\uB4DC\uB294 -2.5 \uB4F1\uAE09\uC73C\uB85C \uBE5B\uB0A0 \uAC83\uC774\uBA70 \uC774\uB294 \uC9C0\uAD6C\uC5D0\uC11C \uBC14\uB77C\uBCF8 \uC2DC\uB9AC\uC6B0\uC2A4 \uBC1D\uAE30\uC758 \uB450 \uBC30\uC5D0 \uC774\uB978\uB2E4."@ko . . "Mufrid (auch Muphrid, aus arabisch \u0645\u0641\u0631\u062F \u0627\u0644\u0631\u0627\u0645\u062D, DMG mufrad ar-r\u0101mi\u1E25 \u201Aeinzelner Lanzentr\u00E4ger\u2018) ist der Eigenname des Sterns \u03B7 Bootis (Eta Bootis) im Sternbild B\u00E4renh\u00FCter. Er stellt den rechten Fu\u00DF der mythologischen Gestalt dar. Mufrid hat eine scheinbare Helligkeit von 2,8 mag, womit er trotz des 7. griechischen Buchstabens \u03B7 der dritthellste Stern im Bootes ist. Er geh\u00F6rt der Spektralklasse G0 an und ist ca. 37 Lichtjahre von der Sonne entfernt (Hipparcos Datenbank). Anderer Name: Saak."@de . "2.68"^^ . "Mufrid (auch Muphrid, aus arabisch \u0645\u0641\u0631\u062F \u0627\u0644\u0631\u0627\u0645\u062D, DMG mufrad ar-r\u0101mi\u1E25 \u201Aeinzelner Lanzentr\u00E4ger\u2018) ist der Eigenname des Sterns \u03B7 Bootis (Eta Bootis) im Sternbild B\u00E4renh\u00FCter. Er stellt den rechten Fu\u00DF der mythologischen Gestalt dar. Mufrid hat eine scheinbare Helligkeit von 2,8 mag, womit er trotz des 7. griechischen Buchstabens \u03B7 der dritthellste Stern im Bootes ist. Er geh\u00F6rt der Spektralklasse G0 an und ist ca. 37 Lichtjahre von der Sonne entfernt (Hipparcos Datenbank). Anderer Name: Saak."@de . . . "Eta Bootis (\u03B7 Boo) \u2013 gwiazda w gwiazdozbiorze Wolarza, b\u0119d\u0105ca podolbrzymem typu widmowego G. Znajduje si\u0119 oko\u0142o 37 lat \u015Bwietlnych od Ziemi."@pl . . . ""@en . . "\u0645\u0641\u0631\u062F \u0627\u0644\u0631\u0627\u0645\u062D (\u0646\u062C\u0645)"@ar . "\u3046\u3057\u304B\u3044\u5EA7\u03B7\u661F\uFF08\u3046\u3057\u304B\u3044\u3056\u30A4\u30FC\u30BF\u305B\u3044\u3001\u03B7 Boo / \u03B7 Bo\u00F6tis\uFF09\u306F\u3001\u3046\u3057\u304B\u3044\u5EA7\u306E\u6052\u661F\u30673\u7B49\u661F\u3002"@ja . . . . . . . . . . . "-356.29"^^ . . "Eta Bootis (\u03B7 Boo / \u03B7 Bootis, \u00CAta Bootis) est une \u00E9toile binaire de la constellation du Bouvier. Elle porte \u00E9galement les noms traditionnels Muphrid ou Mufrid (arabe pour \u00AB solitaire \u00BB) ou Saak, et la d\u00E9signation de Flamsteed 8 Bootis. En astronomie chinoise, elle fait partie de l'ast\u00E9risme Sheti. Le nom de Muphrid a \u00E9t\u00E9 officialis\u00E9 par l'Union astronomique internationale le 12 septembre 2016."@fr . . . "\u53F3\u651D\u63D0\u4E00"@zh . . . . . "Mufrid (eta Bootis) is een heldere ster in het sterrenbeeld Ossenhoeder (Bo\u00F6tes)."@nl . . . . . . . . . . "Mufrid (Eta Bo\u00F6tis / \u03B7 Boo / \u03B7 Bo\u00F6tis) \u00E8 una stella di classe spettrale G0-IV, distante 37 anni luce dal sistema solare, nella costellazione di Boote. Mufrid appare vicina alla stella di spicco di Boote, Arturo (Alpha Bootis) nel cielo della Terra, e Arturo \u00E8 in realt\u00E0 il suo pi\u00F9 prossimo vicino stellare, in quanto entrambe le stelle sono quasi alla stessa distanza dal Sole."@it . "Mufrid"@es . . ""@en . "\u3046\u3057\u304B\u3044\u5EA7\u03B7\u661F\uFF08\u3046\u3057\u304B\u3044\u3056\u30A4\u30FC\u30BF\u305B\u3044\u3001\u03B7 Boo / \u03B7 Bo\u00F6tis\uFF09\u306F\u3001\u3046\u3057\u304B\u3044\u5EA7\u306E\u6052\u661F\u30673\u7B49\u661F\u3002"@ja . . . . . . . . . . . "1.24"^^ . . . . "Eta Bo\u00F6tis (\u03B7 Boo / \u03B7 Bo\u00F6tis) adalah salah satu bintang di rasi Bo\u00F6tes. Berdasarkan sprktrumnya, Eta Bo\u00F6tis memiliki beberapa kelebihan elemen lebih tinggi daripada hidrogen. Faktanya adalah rasio besi terhadap hidrogen sangat dengan batas limit tertinggi untuk sebuah bintang katai. Bintang ini merupakan bintang ganda dengan period orbitnya adalah 494 hari. Bintang ini memiliki magnitudo 2.68 dan berjarak 37 tahun cahaya."@in . . . . . . . ""@en . . "\uBAA9\uB3D9\uC790\uB9AC \uC5D0\uD0C0"@ko . ""@en . "Mufrid o Muphrid (\u03B7 Bootis / \u03B7 Boo / 8 Bootis)\u200B es la tercera estrella m\u00E1s brillante de la constelaci\u00F3n de Bootes despu\u00E9s de Arturo (\u03B1 Bootis) e Izar (\u03B5 Bootis). Con magnitud aparente +2,68, en el cielo aparece muy cerca de Arturo y de hecho ambas est\u00E1n a una distancia casi id\u00E9ntica de la Tierra \u201437 a\u00F1os luz\u2014, estando separadas s\u00F3lo 3,24 a\u00F1os luz entre s\u00ED."@es . . . . . . . "\uBAA9\uB3D9\uC790\uB9AC \uC5D0\uD0C0\uB294 \uBAA9\uB3D9\uC790\uB9AC\uC5D0 \uC788\uB294 \uD56D\uC131\uC774\uB2E4. \uC774 \uBCC4\uC758 \uACE0\uC720 \uBA85\uCE6D\uC73C\uB85C\uB294 \uBB34\uD504\uB9AC\uB4DC(\uC544\uB78D\uC5B4\uB85C \u2018\uD2B9\uBCC4\uD55C \uC874\uC7AC\u2019\uB77C\uB294 \uC758\uBBF8\uC784) \uB610\uB294 \uC0AC\uC544\uD06C\uAC00 \uC788\uB2E4. \uD50C\uB7A8\uC2A4\uD2F0\uB4DC \uBA85\uBA85\uBC95\uC73C\uB85C\uB294 \uBAA9\uB3D9\uC790\uB9AC 8\uC774\uB77C\uACE0 \uBD80\uB978\uB2E4. \uBD84\uAD11\uD615\uC73C\uB85C \uBBF8\uB8E8\uC5B4 \uBCF4\uC544 \uBAA9\uB3D9\uC790\uB9AC \uC5D0\uD0C0\uB294 \uC218\uC18C\uBCF4\uB2E4 \uBB34\uAC70\uC6B4 \uC6D0\uC18C\uC758 \uD568\uB7C9\uC774 \uB9E4\uC6B0 \uB9CE\uB2E4. \uC2E4\uC81C \uC774 \uBCC4\uC758 \uC218\uC18C\uC5D0 \uB300\uD55C \uCCA0\uC758 \uD568\uB7C9\uC740 \uC5D0 \uC788\uB294 \uC8FC\uACC4\uC5F4\uC131\uB4E4\uC758 \uC0C1\uD55C\uC120\uC5D0 \uAC00\uAE4C\uC6B4 \uAC83\uC73C\uB85C \uBCF4\uC778\uB2E4. \uC774 \uBCC4\uC740 \uBD84\uAD11\uC30D\uC131\uC73C\uB85C\uB3C4 \uAD00\uCE21\uB418\uC5B4 \uC654\uC73C\uBA70, \uAD6C\uC131\uC6D0 \uB458\uC740 \uC11C\uB85C\uC758 \uC9C8\uB7C9\uC911\uC2EC\uC744 494\uC77C \uC8FC\uAE30\uB85C \uB3C8\uB2E4. \uADF8\uB7EC\uB098 \uB97C \uD1B5\uD574 \uC774 \uBCC4\uC758 \uC0C1\uC744 \uB530\uB85C \uAD6C\uD55C \uC801\uC740 \uC5C6\uB2E4. \uBAA9\uB3D9\uC790\uB9AC \uC5D0\uD0C0\uB294 \uC9C0\uAD6C \uBC24\uD558\uB298\uC5D0\uC11C \uC544\uD06C\uD22C\uB974\uC2A4\uC640 \uAC00\uAE4C\uC774 \uC788\uB294 \uAC83\uCC98\uB7FC \uBCF4\uC774\uBA70, \uC2E4\uC81C\uB85C \uB450 \uBCC4\uC740 \uAC00\uC7A5 \uAC00\uAE4C\uC774 \uBD99\uC5B4 \uC788\uB294 \uC874\uC7AC\uC774\uAE30\uB3C4 \uD558\uB2E4. \uB450 \uBCC4\uC758 \uC9C0\uAD6C\uB85C\uBD80\uD130\uC758 \uAC70\uB9AC\uB294 \uAC70\uC758 \uAC19\uC73C\uBA70 \uB458 \uC0AC\uC774\uB294 3.24\uAD11\uB144 \uB5A8\uC5B4\uC838 \uC788\uB2E4.[1] \uC11C\uB85C \uCCD0\uB2E4\uBCF8 \uC0C1\uB300 \uBCC4\uC740 \uBC24\uD558\uB298\uC5D0\uC11C \uB9E4\uC6B0 \uBC1D\uAC8C \uBE5B\uB0A0 \uAC83\uC774\uB2E4. \uC544\uD06C\uD22C\uB974\uC2A4\uB294 \uBAA9\uB3D9\uC790\uB9AC \uC5D0\uD0C0\uC5D0\uC11C \uBCFC \uB54C -5.2 \uB4F1\uAE09\uC73C\uB85C \uBC1D\uAC8C \uBE5B\uB0A0 \uAC83\uC774\uBA70, \uC774\uB294 \uC9C0\uAD6C\uC5D0\uC11C \uBC14\uB77C\uBCF8 \uAE08\uC131 \uBC1D\uAE30\uC758 \uAC70\uC758 \uB450 \uBC30\uC5D0 \uC774\uB978\uB2E4. \uBC18\uB300\uB85C \uC544\uD06C\uD22C\uB974\uC2A4\uC5D0\uC11C \uBB34\uD504\uB9AC\uB4DC\uB294 -2.5 \uB4F1\uAE09\uC73C\uB85C \uBE5B\uB0A0 \uAC83\uC774\uBA70 \uC774\uB294 \uC9C0\uAD6C\uC5D0\uC11C \uBC14\uB77C\uBCF8 \uC2DC\uB9AC\uC6B0\uC2A4 \uBC1D\uAE30\uC758 \uB450 \uBC30\uC5D0 \uC774\uB978\uB2E4."@ko . "2.7"^^ . "Mufrid"@de . "1.71"^^ . "\u042D\u0442\u0430 \u0412\u043E\u043B\u043E\u043F\u0430\u0441\u0430 (\u043B\u0430\u0442. \u03B7 Bo\u00F6tis), 8 \u0412\u043E\u043B\u043E\u043F\u0430\u0441\u0430 (\u043B\u0430\u0442. 8 Bo\u00F6tis), HD 121370 \u2014 \u0442\u0440\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\u043F\u0430\u0441\u0430 \u043D\u0430 \u0440\u0430\u0441\u0441\u0442\u043E\u044F\u043D\u0438\u0438 (\u0432\u044B\u0447\u0438\u0441\u043B\u0435\u043D\u043D\u043E\u043C \u0438\u0437 \u0437\u043D\u0430\u0447\u0435\u043D\u0438\u044F \u043F\u0430\u0440\u0430\u043B\u043B\u0430\u043A\u0441\u0430) \u043F\u0440\u0438\u0431\u043B\u0438\u0437\u0438\u0442\u0435\u043B\u044C\u043D\u043E 37,2 \u0441\u0432\u0435\u0442\u043E\u0432\u044B\u0445 \u043B\u0435\u0442 (\u043E\u043A\u043E\u043B\u043E 11,4 \u043F\u0430\u0440\u0441\u0435\u043A\u043E\u0432) \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 2,058 \u043C\u043B\u0440\u0434 \u043B\u0435\u0442."@ru . "2.672"^^ . "Eta Bo\u00F6tis (Muphrid, Ramih al Ramih, Lancea Lanceator, 8 Bo\u00F6tis) \u00E9 uma estrela na dire\u00E7\u00E3o da constela\u00E7\u00E3o de Bo\u00F6tes. Possui uma ascens\u00E3o reta de 13h 54m 41.12s e uma declina\u00E7\u00E3o de +18\u00B0 23\u2032 54.9\u2033. Sua magnitude aparente \u00E9 igual a 2.68. Considerando sua dist\u00E2ncia de 37 anos-luz em rela\u00E7\u00E3o \u00E0 Terra, sua magnitude absoluta \u00E9 igual a 2.41. Pertence \u00E0 classe espectral G0IV."@pt . . . "\u53F3\u6444\u63D0\u4E00\uFF08\u03B7 Boo/\u7267\u592B\u5EA7\u03B7\uFF09\uFF0C\u82F1\u6587\u540DMuphrid\uFF0C\u662F\u4E00\u4E2A\u4F4D\u4E8E\u7267\u592B\u5EA7\u7684\u6052\u661F\u3002\u81EA\u4ECE1943\u5E74\uFF0C\u8FD9\u4E2A\u6052\u661F\u7684\u5149\u8C31\u88AB\u4F5C\u4E3A\u5206\u7C7B\u5176\u5B83\u6052\u661F\u7684\u53C2\u8003\u70B9\u4E4B\u4E00\u3002"@zh . . . "J2000"@en . ""@en . . . . . "\u042D\u0442\u0430 \u0412\u043E\u043B\u043E\u043F\u0430\u0441\u0430"@ru . . . "Eta Bo\u00F6tis"@pt . . . . . "Muphrid eller Eta Bootis (\u03B7 Bootis, f\u00F6rkortat Eta Boo, \u03B7 Boo), som \u00E4r stj\u00E4rnans Bayerbeteckning, \u00E4r en stj\u00E4rna i s\u00F6dra delen av stj\u00E4rnbilden Bj\u00F6rnvaktaren. Sedan 1943 har spektrumet f\u00F6r denna stj\u00E4rna fungerat som en av de stabila referenserna genom vilka andra stj\u00E4rnor klassificeras."@sv . "-60.95"^^ . "Mufrid (eta Bootis) is een heldere ster in het sterrenbeeld Ossenhoeder (Bo\u00F6tes)."@nl . . . "Eta Bootis (\u03B7 Boo) \u2013 gwiazda w gwiazdozbiorze Wolarza, b\u0119d\u0105ca podolbrzymem typu widmowego G. Znajduje si\u0119 oko\u0142o 37 lat \u015Bwietlnych od Ziemi."@pl . . . . . . . "Mufrid o Muphrid (\u03B7 Bootis / \u03B7 Boo / 8 Bootis)\u200B es la tercera estrella m\u00E1s brillante de la constelaci\u00F3n de Bootes despu\u00E9s de Arturo (\u03B1 Bootis) e Izar (\u03B5 Bootis). Con magnitud aparente +2,68, en el cielo aparece muy cerca de Arturo y de hecho ambas est\u00E1n a una distancia casi id\u00E9ntica de la Tierra \u201437 a\u00F1os luz\u2014, estando separadas s\u00F3lo 3,24 a\u00F1os luz entre s\u00ED."@es . . . . . "Eta del Bover (\u03B7 Bootis) \u00E9s un estel binari, el tercer estel m\u00E9s brillant a la constel\u00B7laci\u00F3 del Bover despr\u00E9s d'Arcturus (\u03B1 Bootis) i Hissar (\u03B5 Bootis). Amb magnitud aparent +2,68, en el cel apareix molt prop d'Arcturus i de fet ambd\u00F3s estan a una dist\u00E0ncia gaireb\u00E9 id\u00E8ntica de la Terra \u201437 anys llum\u2014, estant separades nom\u00E9s 3,24 anys llum entre si. El nom del component principal Aa, i nom tradicional del sistema, \u00E9s Muphrid."@ca . . "87.75"^^ . . . . . . "Eta Bo\u00F6tis (Muphrid, Ramih al Ramih, Lancea Lanceator, 8 Bo\u00F6tis) \u00E9 uma estrela na dire\u00E7\u00E3o da constela\u00E7\u00E3o de Bo\u00F6tes. Possui uma ascens\u00E3o reta de 13h 54m 41.12s e uma declina\u00E7\u00E3o de +18\u00B0 23\u2032 54.9\u2033. Sua magnitude aparente \u00E9 igual a 2.68. Considerando sua dist\u00E2ncia de 37 anos-luz em rela\u00E7\u00E3o \u00E0 Terra, sua magnitude absoluta \u00E9 igual a 2.41. Pertence \u00E0 classe espectral G0IV."@pt . . . . . "11.8"^^ . . . . ""@en . . . "\u042D\u0442\u0430 \u0412\u043E\u043B\u043E\u043F\u0430\u0441\u0430 (\u043B\u0430\u0442. \u03B7 Bo\u00F6tis), 8 \u0412\u043E\u043B\u043E\u043F\u0430\u0441\u0430 (\u043B\u0430\u0442. 8 Bo\u00F6tis), HD 121370 \u2014 \u0442\u0440\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\u043F\u0430\u0441\u0430 \u043D\u0430 \u0440\u0430\u0441\u0441\u0442\u043E\u044F\u043D\u0438\u0438 (\u0432\u044B\u0447\u0438\u0441\u043B\u0435\u043D\u043D\u043E\u043C \u0438\u0437 \u0437\u043D\u0430\u0447\u0435\u043D\u0438\u044F \u043F\u0430\u0440\u0430\u043B\u043B\u0430\u043A\u0441\u0430) \u043F\u0440\u0438\u0431\u043B\u0438\u0437\u0438\u0442\u0435\u043B\u044C\u043D\u043E 37,2 \u0441\u0432\u0435\u0442\u043E\u0432\u044B\u0445 \u043B\u0435\u0442 (\u043E\u043A\u043E\u043B\u043E 11,4 \u043F\u0430\u0440\u0441\u0435\u043A\u043E\u0432) \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 2,058 \u043C\u043B\u0440\u0434 \u043B\u0435\u0442."@ru . "Eta Bootis"@fr . . . . . . "G0 IV"@en . . . . "Eta Bo\u00F6tis"@pl . . "3.817"^^ . "Muphrid eller Eta Bootis (\u03B7 Bootis, f\u00F6rkortat Eta Boo, \u03B7 Boo), som \u00E4r stj\u00E4rnans Bayerbeteckning, \u00E4r en stj\u00E4rna i s\u00F6dra delen av stj\u00E4rnbilden Bj\u00F6rnvaktaren. Sedan 1943 har spektrumet f\u00F6r denna stj\u00E4rna fungerat som en av de stabila referenserna genom vilka andra stj\u00E4rnor klassificeras."@sv . . "Eta Bo\u00F6tis (\u03B7 Bo\u00F6tis, abbreviated Eta Boo, \u03B7 Boo) is a binary star in the constellation of Bo\u00F6tes. Based on parallax measurements obtained during the Hipparcos mission, it is approximately 37 light-years (11 parsecs) distant from the Sun. Since 1943, the spectrum of this star has served as one of the stable anchor points by which other stars are classified. It forms a double star with the star BD+19 2726. As a constituent of a double pair, Eta Bo\u00F6tis is also designated WDS J13547+1824A, with its two components being designated Aa (formally named Muphrid /\u02C8mju\u02D0fr\u026Ad/, the traditional name for the entire system) and Ab. (As part of a binary pair, they are also designated Eta Bo\u00F6tis A and B, respectively.) BD +19 2726 is also designated WDS J13547+1824B."@en .