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由堤坝上方的地面冰融化引发的火星洪水。

The generation of martian floods by the melting of ground ice above dykes.

作者信息

McKenzie D, Nimmo F

机构信息

Institute of Theoretical Geophysics, Department of Earth Sciences, University of Cambridge, UK.

出版信息

Nature. 1999 Jan 21;397(6716):231-3. doi: 10.1038/16649.

Abstract

The surface of Mars is cut by long linear faults with displacements of metres to kilometres, most of which are thought to have been formed by extension. The surface has also been modified by enormous floods, probably of water, which often flowed out of valleys formed by the largest of these faults. By analogy with structures on Earth, we propose here that the faults are in fact the surface expression of dykes, and not of large-scale tectonic movements. We use a numerical model to show that the intrusion of large dykes can generate structures like Valles Marineris. Such dykes can provide a heat source to melt ground ice, and so provide a source of water for the floods that have been inferred to originate in some of the large valleys.

摘要

火星表面被位移达数米至数公里的长线性断层切割,其中大部分被认为是由伸展作用形成的。火星表面还受到巨大洪水的改造,这些洪水可能是水,它们常常从由这些最大断层形成的山谷中流出。通过与地球上的构造类比,我们在此提出,这些断层实际上是岩脉的地表表现,而非大规模构造运动的表现。我们使用一个数值模型来表明,大型岩脉的侵入可以产生像水手谷这样的构造。这样的岩脉可以提供一个热源来融化地面冰,从而为据推测起源于一些大型山谷的洪水提供水源。

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