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HAT-P-33b is a planet in the orbit of HAT-P-33, which lies 1,310 light years away from Earth. Its discovery was reported in June 2011, although it was suspected to be a planet as early as 2004. The planet is about three-fourths the mass of Jupiter, but is almost eighty percent larger than Jupiter is; this inflation has, as with the discovery of similar planets WASP-17b and HAT-P-32b, raised the question of what (other than temperature) causes these planets to become so large.

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  • HAT-P-33b (ar)
  • HAT-P-33b (en)
  • HAT-P-33 b (fr)
  • HAT-P-33b (pt)
  • HAT-P-33 b (ru)
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  • HAT-P-33b (بالإنجليزية: HAT-P-33b)‏ الذي يرمز له بالرمز HAT-P-33b، هو كوكب خارج المجموعة الشمسية، في كوكبة التوأمان، يتبع ‏. (ar)
  • HAT-P-33 b est une exoplanète orbitant autour de HAT-P-33, une étoile de type spectral F de la séquence principale du diagramme de Hertzsprung-Russell située à environ 1 367 années-lumière (419 pc) du Soleil dans la constellation des Gémeaux. Elle a été détectée au printemps 2011 par la méthode des transits. (fr)
  • HAT-P-33b is a planet in the orbit of HAT-P-33, which lies 1,310 light years away from Earth. Its discovery was reported in June 2011, although it was suspected to be a planet as early as 2004. The planet is about three-fourths the mass of Jupiter, but is almost eighty percent larger than Jupiter is; this inflation has, as with the discovery of similar planets WASP-17b and HAT-P-32b, raised the question of what (other than temperature) causes these planets to become so large. (en)
  • HAT-P-33b é um planeta extrassolar que orbita a estrela de classe F HAT-P-33, localizada a 419 parsecs (1 367 anos-luz) da Terra na constelação de Gemini. Sua descoberta foi anunciada em 2011 no Astrophysical Journal e foi feita pelo projeto HATNet por meio do método de trânsito. HAT-P-33b tem uma inclinação orbital de 86,7º visto da Terra. Sua órbita está, portanto, quase virada de lado para a Terra, o que possibilita a observação da trânsitos. (pt)
  • HAT-P-33 b (GSC 02461-00988 b)— экзопланета, обращающаяся вокруг звезды HAT-P-33, которая находится в созвездии Близнецы на расстоянии около 1367 световых лет от Солнечной системы. Открытие планеты было подтверждено в июне 2011 года. Планета обладает массой в 0,764 юпитерианских, но на 80 % превосходит Юпитер по радиусу; обнаружение аналогичных планет WASP-17 b и HAT-P-32 b, подняло вопрос о причинах их возникновения (в частности, о том, как планета достигла таких размеров). Открытие было совершено транзитным методом. (ru)
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  • HAT-P-33b (en)
name
  • HAT-P-33b (en)
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  • http://commons.wikimedia.org/wiki/Special:FilePath/Kecknasa.jpg
  • http://commons.wikimedia.org/wiki/Special:FilePath/Exoplanet_Comparison_WASP-17_b.png
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