撞击坑
诺亚人
角砾岩
成岩作用
地质学
地球化学
水溶液
硫酸盐
浸出(土壤学)
喷气孔
火星探测计划
天体生物学
矿物学
化学
火星人
火山
土壤科学
物理
有机化学
土壤水分
物理化学
作者
R. E. Arvidson,S. W. Squyres,J. F. Bell,Jeffrey G. Catalano,B. C. Clark,L. S. Crumpler,Paulo de Souza,Alberto González Fairén,W. H. Farrand,V. K. Fox,R. Gellert,A. Ghosh,M. P. Golombek,J. P. Grotzinger,E. A. Guinness,K. E. Herkenhoff,B. L. Jolliff,Andrew H. Knoll,R. Li,S. M. McLennan
出处
期刊:Science
[American Association for the Advancement of Science (AAAS)]
日期:2014-01-23
卷期号:343 (6169): 1248097-1248097
被引量:195
标识
DOI:10.1126/science.1248097
摘要
Opportunity has investigated in detail rocks on the rim of the Noachian age Endeavour crater, where orbital spectral reflectance signatures indicate the presence of Fe +3 -rich smectites. The signatures are associated with fine-grained, layered rocks containing spherules of diagenetic or impact origin. The layered rocks are overlain by breccias, and both units are cut by calcium sulfate veins precipitated from fluids that circulated after the Endeavour impact. Compositional data for fractures in the layered rocks suggest formation of Al-rich smectites by aqueous leaching. Evidence is thus preserved for water-rock interactions before and after the impact, with aqueous environments of slightly acidic to circum-neutral pH that would have been more favorable for prebiotic chemistry and microorganisms than those recorded by younger sulfate-rich rocks at Meridiani Planum.
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