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Diagenetic silica enrichment and late-stage groundwater activity in Gale crater, Mars

机译:火星大风火山口的成岩二氧化硅富集和后期地下水活动

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摘要

Diagenetic silica enrichment in fracture-associated halos that crosscut lacustrine and unconformably overlying aeolian sedimentary bedrock is observed on the lower north slope of Aeolis Mons in Gale crater, Mars. The diagenetic silica enrichment is colocated with detrital silica enrichment observed in the lacustrine bedrock yet extends into a considerably younger, unconformably draping aeolian sandstone, implying that diagenetic silica enrichment postdates the detrital silica enrichment. A causal connection between the detrital and diagenetic silica enrichment implies that water was present in the subsurface of Gale crater long after deposition of the lacustrine sediments and that it mobilized detrital amorphous silica and precipitated it along fractures in the overlying bedrock. Although absolute timing is uncertain, the observed diagenesis likely represents some of the most recent groundwater activity in Gale crater and suggests that the timescale of potential habitability extended considerably beyond the time that the lacustrine sediments of Aeolis Mons were deposited.
机译:在火星大风火山口Aeolis Mons的北下斜坡,发现了与裂缝相关的晕圈中的成岩二氧化硅富集,该晕圈横切了湖相并在风口沉积基岩上形成了不整合的现象。成岩二氧化硅富集与在湖相基岩中观察到的碎屑二氧化硅富集共存,但延伸到相当年轻的,不整合的垂悬风沙岩中,这意味着成岩二氧化硅富集晚于碎屑二氧化硅富集。碎屑和成岩二氧化硅富集之间的因果关系意味着,在湖沉积物沉积后很长一段时间内,Gale火山口的地下存在水,并且它动员了碎屑无定形二氧化硅并使之沿着上覆基岩的裂缝沉淀。尽管绝对时间不确定,但观察到的成岩作用可能代表了大风火山口的一些最新地下水活动,并表明潜在宜居性的时间尺度大大超出了风神蒙斯湖相沉积物的沉积时间。

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