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Geology of Icy Bodies

机译:冰冷的身体地质

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The exploration of the outer solar system in the last decades revealed an exotic icy world with surfaces showing the most diverse geology, sometimes exceptional to these icy bodies due to the peculiar rheology of ice. Each of these icy bodies exhibits unique characteristics and its own fascinating geological history - formed by the competition of external and internal forces. Some satellites are still geologically active today while others appear to be mostly inactive at present time. Geologically old surfaces are heavily cratered. Some projectiles which created large craters or basins were massive enough that they could have destroyed the target body, like in the case of the impact crater Herschel on the Saturnian satellite Mimas. The observed impact crater morphologies are often exclusive to icy bodies like impact craters on the Galilean satellites Ganymede and Callisto. They mirror the target properties at the time of impact and thus help to understand the satellite's geological evolution. They also reflect the external influence of the space environment onto the surface material since the impact occurred, which is of major importance since most of these icy bodies do not exhibit an atmosphere. Tectonic resurfacing can often be observed as widely distributed simple extensional fractures. Satellites that experienced a more intricate tectonic resurfacing also show more complex tectonic features like double ridges on the Jovian satellite Europa, the Saturnian satellite Enceladus as well as Neptun's satellite Triton. Peculiar tectonic features that are restricted to a single satellite include Europa's bands and chaotic terrain as well as Miranda's coronae indicating outstanding geological evolutions of these two bodies. These complex features are far from being fully understood. They are, at least partly, expected to be associated with recent and/or past cryovolcanism. Current volcanism, however, has been detected only on the two satellites Enceladus and Triton, finding its peak in geysers on Enceladus originating from its south pole forming vapor plumes that reach up to 500 km into space.
机译:在过去几十年的太阳系外的探索透露了一个奇异的冰雪世界与表面呈现出最多样的地质,有时特殊这些冰冷的尸体,由于冰的独特的流变。这些冰冷的尸体表现出独特的特点和自己的迷人的地质历史上每一个 - 通过外力和内力的竞争形成。一些卫星仍然地质运动活跃的今天,而其他人似乎是在目前大多无效。从地质学老面极为多坑。这创造了较大的环形山盆地或一些抛射物足够庞大,他们可以在火山口上赫歇尔土星的卫星土卫一的影响的情况下摧毁目标的身体,等等。观察到的撞击坑形态往往是独家像伽利略卫星木卫三和木卫四陨石坑冰冷的尸体。它们在撞击时镜像目标属性,从而有助于了解卫星的地质演化。他们还反映在空间环境上,因为发生冲击表面材料,这是非常重要的,因为大多数这些冰冷的尸体都没有表现出大气的外部影响。构造表面重修经常可以观察到广泛分布的简单拉伸骨折。在经历一个更复杂的构造换肤卫星也表现出更复杂的构造特征像木星卫星木卫二,土星的卫星土卫二,以及海王星的卫星海卫双垄沟。被限制为单个卫星特有的构造特征包括欧洲的乐队和混乱的地形以及米兰达的日冕表明这两个机构的杰出的地质演变。这些复杂的功能还远远没有得到充分的理解。他们,至少部分,预计将在近期和/或过去cryovolcanism相关。目前的火山活动,但是,一直只检测上的两个卫星土卫二和Triton,从南极形成蒸汽羽流可达500公里到空间中找到它在土卫二上的间歇泉始发高峰。

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