. . . . "HD 88133 b"@fr . . . . . "AU"@en . . . . . . . . . . . . "HD 88133 b adalah sebuah planet luar surya yang terletak sekitar 240,61 tahun cahaya dari Bumi. Planet ini ditemukan pada tahun 2004 dengan menggunakan metode kecepatan radial. HD 88133 b memiliki massa sebesar 1,02 massa Jupiter."@in . . "astron"@en . "HD 88133 b \u00E9 um planeta extrassolar que orbita a estrela subgigante de classe G HD 88133, localizada a aproximadamente 270 anos-luz (81 parsecs) da Terra na constela\u00E7\u00E3o de Leo. Foi descoberto em 2004 pelo m\u00E9todo da velocidade radial. \u00C9 um gigante gasoso com uma massa m\u00EDnima de 0,229 vezes a massa de J\u00FApiter, tendo provavelmente uma massa similar \u00E0 de Saturno. Sua \u00F3rbita \u00E9 extremamente curta, tendo um raio m\u00E9dio de apenas 0,0472 UA (4,72% do raio orbital da Terra). O planeta completa uma \u00F3rbita a cada 3,41587 dias."@pt . . . . . . "d"@en . "0"^^ . . "1063402700"^^ . "HD 88133 b"@pt . "HD 88133 b is an extrasolar planet orbiting the star HD 88133. It is probably less massive than Jupiter and even Saturn. It orbits the star in a very tight orbit, completing one revolution around the star in every three and half days or so. Despite the relatively large radius of the star (about 2 times Solar), no transits have been detected. In 2016 the direct detection of the planetary thermal emission spectrum was claimed, but the detection was questioned in 2021."@en . . "HD 88133 b"@en . "" . . . "HD 88133 b"@en . "HD 88133 b"@pl . . "(N2K Consortium)" . . . "4994"^^ . . "HD 88133 b"@ko . . "HD 88133 b (\u0628\u0627\u0644\u0625\u0646\u062C\u0644\u064A\u0632\u064A\u0629: HD 88133 b)\u200F \u0627\u0644\u0630\u064A \u064A\u0631\u0645\u0632 \u0644\u0647 \u0628\u0627\u0644\u0631\u0645\u0632 HD 88133b\u060C \u0647\u0648 \u0643\u0648\u0643\u0628 \u062E\u0627\u0631\u062C \u0627\u0644\u0645\u062C\u0645\u0648\u0639\u0629 \u0627\u0644\u0634\u0645\u0633\u064A\u0629\u060C \u0641\u064A \u0643\u0648\u0643\u0628\u0629 \u0627\u0644\u0623\u0633\u062F\u060C \u064A\u062A\u0628\u0639 \u200F."@ar . . . "Butler et al."@en . . . "HD 88133 b\uB294 \uC5B4\uBA38\uB2C8 \uD56D\uC131 \uC744 \uB3CC\uACE0 \uC788\uB294 \uC678\uACC4 \uD589\uC131\uC774\uB2E4. \uC544\uB9C8\uB3C4 \uC774 \uD589\uC131\uC758 \uC9C8\uB7C9\uC740 \uBAA9\uC131, \uBC0F \uD1A0\uC131\uBCF4\uB2E4\uB3C4 \uAC00\uBCBC\uC6B8 \uAC83\uC73C\uB85C \uBCF4\uC778\uB2E4. \uD56D\uC131\uC73C\uB85C\uBD80\uD130 \uB9E4\uC6B0 \uAC00\uAE4C\uC6B4 \uAC70\uB9AC\uB97C \uB3CC\uACE0 \uC788\uB294\uB370, \uC9C0\uAD6C \uC2DC\uAC04\uC73C\uB85C \uC774 \uD589\uC131\uC758 1\uB144\uC740 3.5\uC77C\uBC16\uC5D0 \uB418\uC9C0 \uC54A\uB294\uB2E4. \uC5B4\uBA38\uB2C8 \uD56D\uC131\uC740 \uD0DC\uC591 \uBC18\uC9C0\uB984\uC758 2\uBC30 \uC815\uB3C4 \uB418\uB294 \uC900\uAC70\uC131\uC778\uB370, \uC544\uC9C1\uAE4C\uC9C0 HD 88133 b\uAC00 \uD56D\uC131 \uD45C\uBA74\uC744 \uC9C0\uB098\uAC00\uB294 \uC7A5\uBA74\uC740 \uD3EC\uCC29\uB418\uC9C0 \uC54A\uC558\uB2E4."@ko . . . "HD 88133 b \u00E9 um planeta extrassolar que orbita a estrela subgigante de classe G HD 88133, localizada a aproximadamente 270 anos-luz (81 parsecs) da Terra na constela\u00E7\u00E3o de Leo. Foi descoberto em 2004 pelo m\u00E9todo da velocidade radial. \u00C9 um gigante gasoso com uma massa m\u00EDnima de 0,229 vezes a massa de J\u00FApiter, tendo provavelmente uma massa similar \u00E0 de Saturno. Sua \u00F3rbita \u00E9 extremamente curta, tendo um raio m\u00E9dio de apenas 0,0472 UA (4,72% do raio orbital da Terra). O planeta completa uma \u00F3rbita a cada 3,41587 dias."@pt . . . "HD 88133 b is an extrasolar planet orbiting the star HD 88133. It is probably less massive than Jupiter and even Saturn. It orbits the star in a very tight orbit, completing one revolution around the star in every three and half days or so. Despite the relatively large radius of the star (about 2 times Solar), no transits have been detected. In 2016 the direct detection of the planetary thermal emission spectrum was claimed, but the detection was questioned in 2021."@en . "2004-09-06"^^ . ""@en . "HD 88133 b"@in . . "HD 88133 b ist ein Exoplanet, der den Unterriesen HD 88133 alle 3,416 Tage umkreist. Er wurde von Debra Fischer et al. im Jahr 2004 mit Hilfe der Radialgeschwindigkeitsmethode entdeckt. Die gro\u00DFe Halbachse der Umlaufbahn des Exoplaneten misst ca. 0,05 Astronomischen Einheiten, ihre Exzentrizit\u00E4t betr\u00E4gt 0,13. Das Objekt hat eine Mindestmasse von ca. 0,29 Jupitermassen (rund 95 Erdmassen)."@de . "HD 88133 b \u2013 planeta typu gor\u0105cy jowisz orbituj\u0105ca wok\u00F3\u0142 gwiazdy HD 88133. Jej masa minimalna jest zbli\u017Cona do masy Saturna. Jeden obieg wok\u00F3\u0142 gwiazdy zajmuje jej tylko oko\u0142o 3,5 dnia."@pl . . . . "HD 88133 b adalah sebuah planet luar surya yang terletak sekitar 240,61 tahun cahaya dari Bumi. Planet ini ditemukan pada tahun 2004 dengan menggunakan metode kecepatan radial. HD 88133 b memiliki massa sebesar 1,02 massa Jupiter."@in . . . "HD 88133 b ist ein Exoplanet, der den Unterriesen HD 88133 alle 3,416 Tage umkreist. Er wurde von Debra Fischer et al. im Jahr 2004 mit Hilfe der Radialgeschwindigkeitsmethode entdeckt. Die gro\u00DFe Halbachse der Umlaufbahn des Exoplaneten misst ca. 0,05 Astronomischen Einheiten, ihre Exzentrizit\u00E4t betr\u00E4gt 0,13. Das Objekt hat eine Mindestmasse von ca. 0,29 Jupitermassen (rund 95 Erdmassen)."@de . . . . "16781402"^^ . . . "Radial velocity" . . "HD 88133 b (\u0628\u0627\u0644\u0625\u0646\u062C\u0644\u064A\u0632\u064A\u0629: HD 88133 b)\u200F \u0627\u0644\u0630\u064A \u064A\u0631\u0645\u0632 \u0644\u0647 \u0628\u0627\u0644\u0631\u0645\u0632 HD 88133b\u060C \u0647\u0648 \u0643\u0648\u0643\u0628 \u062E\u0627\u0631\u062C \u0627\u0644\u0645\u062C\u0645\u0648\u0639\u0629 \u0627\u0644\u0634\u0645\u0633\u064A\u0629\u060C \u0641\u064A \u0643\u0648\u0643\u0628\u0629 \u0627\u0644\u0623\u0633\u062F\u060C \u064A\u062A\u0628\u0639 \u200F."@ar . . "HD 88133 b"@en . . . . "HD 88133 b"@de . . . "HD 88133 b"@ar . . . . "HD 88133 b est une plan\u00E8te extrasolaire en orbite autour de l'\u00E9toile HD 88133. Elle est probablement moins massive que Jupiter et m\u00EAme Saturne. Elle tourne autour de l'\u00E9toile dans une orbite tr\u00E8s serr\u00E9e, op\u00E9rant une r\u00E9volution tous les trois jours et demi environ. Malgr\u00E9 le rayon relativement grand de l'\u00E9toile (environ 2 fois celui du Soleil), aucun transit astronomique n'a \u00E9t\u00E9 mis en \u00E9vidence."@fr . . "HD 88133 b \u2013 planeta typu gor\u0105cy jowisz orbituj\u0105ca wok\u00F3\u0142 gwiazdy HD 88133. Jej masa minimalna jest zbli\u017Cona do masy Saturna. Jeden obieg wok\u00F3\u0142 gwiazdy zajmuje jej tylko oko\u0142o 3,5 dnia."@pl . . . . . "2004-09-06"^^ . . "HD 88133 b est une plan\u00E8te extrasolaire en orbite autour de l'\u00E9toile HD 88133. Elle est probablement moins massive que Jupiter et m\u00EAme Saturne. Elle tourne autour de l'\u00E9toile dans une orbite tr\u00E8s serr\u00E9e, op\u00E9rant une r\u00E9volution tous les trois jours et demi environ. Malgr\u00E9 le rayon relativement grand de l'\u00E9toile (environ 2 fois celui du Soleil), aucun transit astronomique n'a \u00E9t\u00E9 mis en \u00E9vidence."@fr . "HD 88133 b\uB294 \uC5B4\uBA38\uB2C8 \uD56D\uC131 \uC744 \uB3CC\uACE0 \uC788\uB294 \uC678\uACC4 \uD589\uC131\uC774\uB2E4. \uC544\uB9C8\uB3C4 \uC774 \uD589\uC131\uC758 \uC9C8\uB7C9\uC740 \uBAA9\uC131, \uBC0F \uD1A0\uC131\uBCF4\uB2E4\uB3C4 \uAC00\uBCBC\uC6B8 \uAC83\uC73C\uB85C \uBCF4\uC778\uB2E4. \uD56D\uC131\uC73C\uB85C\uBD80\uD130 \uB9E4\uC6B0 \uAC00\uAE4C\uC6B4 \uAC70\uB9AC\uB97C \uB3CC\uACE0 \uC788\uB294\uB370, \uC9C0\uAD6C \uC2DC\uAC04\uC73C\uB85C \uC774 \uD589\uC131\uC758 1\uB144\uC740 3.5\uC77C\uBC16\uC5D0 \uB418\uC9C0 \uC54A\uB294\uB2E4. \uC5B4\uBA38\uB2C8 \uD56D\uC131\uC740 \uD0DC\uC591 \uBC18\uC9C0\uB984\uC758 2\uBC30 \uC815\uB3C4 \uB418\uB294 \uC900\uAC70\uC131\uC778\uB370, \uC544\uC9C1\uAE4C\uC9C0 HD 88133 b\uAC00 \uD56D\uC131 \uD45C\uBA74\uC744 \uC9C0\uB098\uAC00\uB294 \uC7A5\uBA74\uC740 \uD3EC\uCC29\uB418\uC9C0 \uC54A\uC558\uB2E4."@ko . .