This page describes an image 木卫一(伊奥)
下载文件 ( 图像 789.81 kB)
图片说明
美国国家航空航天局的伽利略号航天器于1999年7月3日获得了木星卫星木卫一的最高分辨率图像。木卫一是伽利略-伽利雷 1610 年发现的四颗卫星之一。木卫一的颜色源于硫化物,是大量火山活动存在的证据。木星和邻近卫星的潮汐力是木卫一火山活动的原因。
滚动查看其他语言的字幕
图片来源
美国宇航局/JPL/亚利桑那大学 来源链接
注释翻译状态: 已由审核人员批准
注释翻译者: Lin Shijie
注释审校者:: Zhang Ruoyi, Wang Yilin
The media file captions presented on the OAE website were written, translated and reviewed by a collective effort from the OAE, the OAE Centers and Nodes, the OAE National Astronomy Education Coordinators (NAECs) and other volunteers. You can find a full list of credits for our translation project here. All media file captions are released under a Creative Commons CC BY-4.0 license and should be credited to "IAU OAE". The media files themselves may have different licenses (see above) and should be credited as listed above under "credit".
If you notice a factual error in this caption or an error in any of its translations then please get in touch.
其他语言版本的图注
图片说明 Die NASA-Raumsonde Galileo hat am 3. Juli 1999 ihre höchstauflösenden Bilder des Jupitermondes Io aufgenommen. Io ist einer der vier Jupitermonde, die von Galileo Galilei im Jahr 1610 entdeckt wurden. Die Farben von Io zeugen von seiner umfangreichen vulkanischen Aktivität, da sie aus schwefelhaltigen Verbindungen resultiert. Die Gezeitenkräfte von Jupiter und den benachbarten Monden sind die Ursache für den Vulkanismus auf Io.
图片来源 NASA/JPL/Universität von Arizona
相关术语表词条: Galileische Satelliten , Io , Monde 注释翻译状态: 尚未由审核人员批准
注释翻译者: Emma Krojanski
图片说明 NASA's Galileo spacecraft acquired its highest resolution images of Jupiter's moon Io on 3 July 1999. Io is one of the four Jovian moons discovered by Galileo Galilei in 1610. Io's colours are witness to its extensive volcanic activity as they stem from sulphuric compounds. Tidal forces from Jupiter and the neighbouring moons are the cause for Io's volcanism.
图片来源 NASA/JPL/University of Arizona
相关术语表词条: Galilean Satellites , Io , Moons
图片说明 Le 3 juillet 1999, la sonde spatiale Galileo de la NASA a acquis les images à la plus haute résolution du satellite de Jupiter Io. Io est l'une des quatre lunes joviennes découvertes par Galilée en 1610. Les couleurs de Io témoignent de son importante activité volcanique, car elles proviennent de composés sulfuriques. Les forces de marée de Jupiter et des satellites voisins sont à l'origine du volcanisme de Io.
图片来源 NASA/JPL/Université d'Arizona
相关术语表词条: Io , Lunes , Satellites galiléens 注释翻译状态: 已由审核人员批准
注释翻译者: Gilles Remy
注释审校者:: Christophe Hermant
图片说明 La sonda Galileo della NASA ha acquisito le immagini a più alta risoluzione della luna di Giove Io il 3 luglio 1999. Io è una delle quattro lune gioviane, scoperte da Galileo Galilei nel 1610. I colori di Io testimoniano la sua vasta attività vulcanica, poiché derivano da composti solforici. Le forze di marea di Giove e delle lune vicine sono la causa del vulcanismo di Io.
图片来源 NASA/JPL/Università dell'Arizona
相关术语表词条: Io , Lune , Satelliti galileiani 注释翻译状态: 已由审核人员批准
注释翻译者: Giuliana Giobbi
注释审校者:: Rosa Valiante, Rodolfo Canestrari



