作者
Steven W Squyres, Raymond E Arvidson, Steven Ruff, R Gellert, RV Morris, DW Ming, L Crumpler, JD Farmer, DJ Des Marais, A Yen, SM McLennan, W Calvin, James F Bell III, Benton C Clark, A Wang, Timothy J McCoy, ME Schmidt, PA de Souza Jr
发表日期
2008/5/23
期刊
Science
卷号
320
期号
5879
页码范围
1063-1067
出版商
American Association for the Advancement of Science
简介
Mineral deposits on the martian surface can elucidate ancient environmental conditions on the planet. Opaline silica deposits (as much as 91 weight percent SiO2) have been found in association with volcanic materials by the Mars rover Spirit. The deposits are present both as light-toned soils and as bedrock. We interpret these materials to have formed under hydrothermal conditions and therefore to be strong indicators of a former aqueous environment. This discovery is important for understanding the past habitability of Mars because hydrothermal environments on Earth support thriving microbial ecosystems.
引用总数
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学术搜索中的文章
SW Squyres, RE Arvidson, S Ruff, R Gellert, RV Morris… - Science, 2008