Showman A P, Malhotra R
Department of Mechanical Engineering, University of Louisville, 215 Sackett Hall, Louisville, KY 40292, USA.
Science. 1999 Oct 1;286(5437):77-84. doi: 10.1126/science.286.5437.77.
NASA's Galileo mission to Jupiter and improved Earth-based observing capabilities have allowed major advances in our understanding of Jupiter's moons Io, Europa, Ganymede, and Callisto over the past few years. Particularly exciting findings include the evidence for internal liquid water oceans in Callisto and Europa, detection of a strong intrinsic magnetic field within Ganymede, discovery of high-temperature silicate volcanism on Io, discovery of tenuous oxygen atmospheres at Europa and Ganymede and a tenuous carbon dioxide atmosphere at Callisto, and detection of condensed oxygen on Ganymede. Modeling of landforms seen at resolutions up to 100 times as high as those of Voyager supports the suggestion that tidal heating has played an important role for Io and Europa.
美国国家航空航天局(NASA)的木星探测任务“伽利略号”以及地基观测能力的提升,使得过去几年我们在了解木星的卫星木卫一、木卫二、木卫三及木卫四方面取得了重大进展。特别令人兴奋的发现包括:木卫四和木卫二存在内部液态水海洋的证据;木卫三内部存在强固有磁场;木卫一上发现高温硅酸盐火山活动;木卫二和木卫三存在稀薄的氧气大气层,木卫四存在稀薄的二氧化碳大气层;在木卫三上检测到凝聚态氧。对分辨率比“旅行者号”高100倍的地貌进行建模,支持了潮汐加热对木卫一和木卫二起重要作用这一观点。