地质学
火星探测计划
沉积岩
地球化学
海湾
撞击坑
天体生物学
海洋学
物理
作者
S. M. McLennan,R. B. Anderson,J. F. Bell,J. C. Bridges,F. J. Calef,John Campbell,B. C. Clark,S. M. Clegg,P. G. Conrad,A. Cousin,David J. Des Marais,Gilles Dromart,M. D. Dyar,L. A. Edgar,B. L. Ehlmann,C. Fabre,O. Forni,O. Gasnault,R. Gellert,S. Gordon
出处
期刊:Science
[American Association for the Advancement of Science]
日期:2013-12-10
卷期号:343 (6169): 1244734-1244734
被引量:296
标识
DOI:10.1126/science.1244734
摘要
Sedimentary rocks examined by the Curiosity rover at Yellowknife Bay, Mars, were derived from sources that evolved from an approximately average martian crustal composition to one influenced by alkaline basalts. No evidence of chemical weathering is preserved, indicating arid, possibly cold, paleoclimates and rapid erosion and deposition. The absence of predicted geochemical variations indicates that magnetite and phyllosilicates formed by diagenesis under low-temperature, circumneutral pH, rock-dominated aqueous conditions. Analyses of diagenetic features (including concretions, raised ridges, and fractures) at high spatial resolution indicate that they are composed of iron- and halogen-rich components, magnesium-iron-chlorine–rich components, and hydrated calcium sulfates, respectively. Composition of a cross-cutting dike-like feature is consistent with sedimentary intrusion. The geochemistry of these sedimentary rocks provides further evidence for diverse depositional and diagenetic sedimentary environments during the early history of Mars.
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