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Analysis of surface morphology of basaltic grains as environmental indicators for Mars

机译:玄武岩谷物作为火星环境指标的表面形态分析

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Analysing the microtextures of grains from different sediments helps to determine their transport medium. This method is well developed in the case of quartz grains, because quartz is usually dominant in sediments on Earth. In this study, basaltic sands from aeolian and fluvial environments from Iceland and from the Azores Islands were analysed, since basaltic rocks have been found on Mars, and paleo-environment reconstruction is an important goal of future missions. Fixed grains were imaged and analysed by a high-resolution electron microscope. Several different surface identification marks were found corresponding to known examples from quartz micro morphologies: conchoidal fractures, steps, and percussion marks, which are connected to fluvial environments; while precipitation features and bulbous edges were identified and connected to the aeolian transport. In these generally very diverse samples some new micromorphologies, which have not previously been found on quartz grains, were also identified. The identification of such features which are not present on quartz is expected, as the sample has a different composition than quartz. These newly identified features were named as: fan-shaped percussion marks; isometric shaped grains with a rough surface (fluvial); "large voids" with abraded surface and cracked surface (aeolian). Based on our results, a further improved version of the method evaluating grain surface micro-morphology could be useful not only for quartz grains, but in the case of the basaltic grains too. Such information could help to identify the settling environments of grains on Mars, we therefore also discuss the spatial resolution and observational conditions required to do so by in-situ Mars missions there. We conclude that a one order of magnitude increase in the spatial resolution (down to about 1 mu m) would greatly support the identification of grain surface features and interpretation of transport methods. This level of resolution is not far beyond that which is currently available.
机译:分析来自不同沉积物的谷物的微调有助于确定其运输培养基。这种方法在石英谷物的情况下发育良好,因为石英通常在地球上的沉积物中显着。在本研究中,分析了来自冰岛和亚速尔群岛岛屿的玄武岩和苏尔群岛的玄武岩,因为在火星上发现了玄武岩岩石,并且古环境重建是未来任务的重要目标。通过高分辨率电子显微镜对固定晶体进行成像并分析。发现几种不同的表面识别标记对应于石英微观形态的已知实施例:与河流环境相连的孔雀体裂缝,步骤和冲击标记;虽然鉴定了沉淀特征和球根状边缘并连接到Aeolian运输。在这些通常不同的样品中,还确定了一些尚未在石英粒上发现的一些新的微晶。预期识别不存在于石英上的这种特征,因为样品具有不同的组成而不是石英。这些新发现的功能被命名为:粉丝形打击乐标记;等距形状的颗粒具有粗糙表面(河流);带磨损表面和裂纹表面(Aeolian)的“大空隙”。基于我们的结果,评估晶粒表面微观形态的方法的进一步改进版本不仅可以用于石英粒,而且在玄武岩颗粒的情况下也是有用的。因此,这些信息有助于确定火星上谷物的沉降环境,因此还讨论了在那里原位火星任务所需的空间分辨率和观测条件。我们得出结论,空间分辨率(下降至约1μm)的一个数量级增加将极大地支持晶粒表面特征和传输方法的解释。这种分辨率水平不远超过目前可用的水平。

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  • 来源
    《Planetary and space science 》 |2021年第11期| 105338.1-105338.17| 共17页
  • 作者单位

    Res Ctr Astron & Earth Sci Inst Geol & Geochem Res Budapest Hungary|Res Ctr Astron & Earth Sci Konkoly Thege Miklos Astron Inst Konkoly Observ Budapest Hungary|Eotvos Lorand Univ Dept Petrol & Geol Budapest Hungary;

    Res Ctr Astron & Earth Sci Konkoly Thege Miklos Astron Inst Konkoly Observ Budapest Hungary|European Astrobiol Inst Strasbourg France;

    Eotvos Lorand Univ Dept Petrol & Geol Budapest Hungary;

    Res Ctr Astron & Earth Sci Geog Inst Budapest Hungary;

    Res Ctr Astron & Earth Sci Geog Inst Budapest Hungary;

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