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K2-33b (also known by its EPIC designation EPIC 205117205.01) is a very young super-Neptune exoplanet, orbiting the pre-main-sequence star K2-33. It was discovered by NASA's Kepler spacecraft on its "Second Light" mission. It is located about 456 light-years (140 parsecs) away from Earth in the constellation of Scorpius. The exoplanet was found by using the transit method, in which the dimming effect that a planet causes as it crosses in front of its star is measured.

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  • K2-33b (es)
  • K2-33b (en)
  • K2-33 b (fr)
  • K2-33 b (ko)
  • K2-33b (zh)
rdfs:comment
  • K2-33b es un exoplaneta extremadamente joven que orbita alrededor de la estrella de enana roja K2-33 aproximadamente 453.36 años luz de la Tierra.​ (es)
  • K2-33 b (également connu sous la désignation EPIC EPIC 205117205.01) est une très jeune exoplanète de type super-Neptune orbitant autour de l'étoile de la pré-séquence principale K2-33. Elle a été découverte par une équipe d'astronomes travaillant à la NASA à l'aide du télescope spatial Kepler. Elle se situe à ~456 années-lumière (~140 parsecs) de la Terre dans la constellation du Scorpion. L'exoplanète a été découverte et confirmée en utilisant la méthode des transits, dans lequel on mesure la variation de la luminosité provoquée par une planète passant devant son étoile. Elle est surtout remarquable par son très jeune âge, estimé à 9,3 millions d'années, puisqu'une seule autre exoplanète est encore plus jeune avec un âge estimé à 2 millions d'années (V830 Tau b). (fr)
  • K2-33B는 주계열성 이전의 K2-33을 공전하는 매우 젊은 슈퍼해왕성인 엑소플라넷의 외계행성이다. 가스행성에 속한다. 그것은 NASA의 케플러 우주선에 의해 "세컨드 라이트" 임무에서 발견되었다. 그것은 전갈자리에 위치하고 있으며 지구에서 약 456광년(140파섹) 떨어져 있다. 이 외행성은 행성이 항성 앞을 가로지르면서 발생하는 조광 효과를 측정하는 트랜짓 방식을 이용해 발견되었다. 알려진 외부 행성들 중에서 K2-33B는 930만 년밖에 되지 않은 아주 어린 것으로 여겨진다. 오직 한 외조류만이 200만년(V830 Tauri B)의 어린 나이로 더 젊다. (ko)
  • K2-33b,或稱為EPIC 205117205.01,是一顆極為年輕的超級海王星型太陽系外行星,母恆星是主序前星。該行星是由美国国家航空航天局的克卜勒太空望遠鏡K2任務(Second Light,「第二道光」)發現,距離地球約472光年(145秒差距),在天球上位於天蠍座。該行星是以觀測行星通過母恆星盤面與地球觀測者之間造成母恆星亮度下降程度的凌日法發現。K2-33b因為年齡只有約930萬年而聞名,並且目前只有一顆系外行星金牛座V830b比它年輕(年齡約200萬年)。 (zh)
  • K2-33b (also known by its EPIC designation EPIC 205117205.01) is a very young super-Neptune exoplanet, orbiting the pre-main-sequence star K2-33. It was discovered by NASA's Kepler spacecraft on its "Second Light" mission. It is located about 456 light-years (140 parsecs) away from Earth in the constellation of Scorpius. The exoplanet was found by using the transit method, in which the dimming effect that a planet causes as it crosses in front of its star is measured. (en)
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  • K2-33b (en)
name
  • K2-33b (en)
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  • http://commons.wikimedia.org/wiki/Special:FilePath/Comparing_K2-33_to_our_Solar_System.jpg
  • http://commons.wikimedia.org/wiki/Special:FilePath/K2-33b.jpg
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