What Geology and Mineralogy Tell Us About Water on Mars

What Geology and Mineralogy Tell Us About Water on Mars
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地质学和矿物学告诉我们关于火星上水的信息

DOI:
10.1007/978-981-13-3639-3_21
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发表时间:
2019
期刊:
影响因子:
4.2
通讯作者:
Usui Tomohiro
Usui Tomohiro
中科院分区:
物理与天体物理2区
文献类型:
--
作者:
Lawrence;D. J.;Peplowski;P. N.;Beck;A. W.;Burks;M. T.;Chabot;N. L.;Cully;M. J.;Elphic;R. C.;Ernst;C. M.;Fix;S.;Goldsten;J. O.;Hoffer;E. M.;Kusano;H.;Murchie;S. L.;Schratz;B. C.;Usui;T.;Yokley;Z. W.;Usui Tomohiro

文献摘要

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由于火星作为一个潜在的可居住行星吸引了很多兴趣,因此在任何其他外星天体中,最多的航天器被发送到这颗行星。火星探测为各种与水有关的地质活动提供了证据:河流地貌,古海洋和湖泊,以及表面物质的水蚀变和风化。这些地质观测清楚地表明火星表面存在液态水,而最近的调查发现可能存在地下水(冰)世界,这可能更有利于火星上现存甚至现在的生命。
Since Mars has attracted much interest as a potentially accessible habitable planet, the greatest number of spacecraft has been sent to this planet among any of the other extraterrestrial bodies. The Mars exploration has provided evidence for a variety of water-related geological activities: fluvial landforms, paleo-oceans and lakes, and aqueous alteration and weathering of the surface materials. These geologic observations clearly indicated the existence of liquid water on the surface of Mars, while the most recent investigations have uncovered the possible existence of subsurface water (ice) world, which may be more favorable to extant or even present life on Mars.