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火星马沃斯谷揭示的页硅酸盐多样性与过去的水活动

Phyllosilicate diversity and past aqueous activity revealed at Mawrth Vallis, Mars.

作者信息

Bishop Janice L, Dobrea Eldar Z Noe, McKeown Nancy K, Parente Mario, Ehlmann Bethany L, Michalski Joseph R, Milliken Ralph E, Poulet Francois, Swayze Gregg A, Mustard John F, Murchie Scott L, Bibring Jean-Pierre

机构信息

SETI Institute and NASA Ames Research Center, Mountain View, CA 94043, USA.

出版信息

Science. 2008 Aug 8;321(5890):830-3. doi: 10.1126/science.1159699.

Abstract

Observations by the Mars Reconnaissance Orbiter/Compact Reconnaissance Imaging Spectrometer for Mars in the Mawrth Vallis region show several phyllosilicate species, indicating a wide range of past aqueous activity. Iron/magnesium (Fe/Mg)-smectite is observed in light-toned outcrops that probably formed via aqueous alteration of basalt of the ancient cratered terrain. This unit is overlain by rocks rich in hydrated silica, montmorillonite, and kaolinite that may have formed via subsequent leaching of Fe and Mg through extended aqueous events or a change in aqueous chemistry. A spectral feature attributed to an Fe2+ phase is present in many locations in the Mawrth Vallis region at the transition from Fe/Mg-smectite to aluminum/silicon (Al/Si)-rich units. Fe2+-bearing materials in terrestrial sediments are typically associated with microorganisms or changes in pH or cations and could be explained here by hydrothermal activity. The stratigraphy of Fe/Mg-smectite overlain by a ferrous phase, hydrated silica, and then Al-phyllosilicates implies a complex aqueous history.

摘要

火星勘测轨道飞行器/火星紧凑型侦察成像光谱仪对莫尔特瓦利斯地区的观测显示了几种层状硅酸盐矿物,这表明过去存在广泛的水活动。在浅色露头中观测到铁/镁(Fe/Mg)蒙脱石,这些露头可能是由古老撞击坑地形的玄武岩经水蚀变形成的。该单元之上覆盖着富含水合二氧化硅、蒙脱石和高岭石的岩石,这些岩石可能是通过长时间水活动对铁和镁的后续淋滤或水化学变化形成的。在莫尔特瓦利斯地区从Fe/Mg蒙脱石向富铝/硅(Al/Si)单元过渡的许多位置都存在一个归因于Fe2+相的光谱特征。陆地沉积物中含Fe2+的物质通常与微生物或pH值或阳离子的变化有关,在这里可能是由热液活动造成的。Fe/Mg蒙脱石之上依次为亚铁相、水合二氧化硅,然后是铝层状硅酸盐,这意味着其水历史复杂。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/268f/7007808/3232e0f27013/nihms-1048613-f0001.jpg

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