The generation of Martian floods by the melting of ground ice above dykes

被引:103
作者
McKenzie, D [1 ]
Nimmo, F [1 ]
机构
[1] Univ Cambridge, Inst Theoret Geophys, Bullard Labs, Dept Earth Sci, Cambridge CB3 0EZ, England
关键词
D O I
10.1038/16649
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
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(1). 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(2). By analogy with structures on Earth(3,4), we propose here that the faults are in fact the surface expression of dykes(5), 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(2).
引用
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页码:231 / 233
页数:3
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