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Mars-Relevant Field Experiences in Morocco: The Importance of Spatial Scales and Subsurface Exploration

机译:摩洛哥火星相关的现场经验:空间尺度和地下勘探的重要性

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During field work at the Ibn Battuta Mars analogue sites, two research questions were analyzed: (1) How do we identify sampling sites using remote and local imaging and (2) what kind of information can be gained from shallow subsurface exploration? While remote images help in targeting field activities in general, the connection between observations at different spatial scales for different rocky desert terrain types is not well established; in this, focused comparison of remote in situ images of well-selected analogues would help a great deal. Dried up lake beds as discerned in remotely acquired data may not show signatures of past water activity, while shallow subsurface exploration could reveal the lacustrine period. Acquisition of several satellite images of the same terrain under different geometries would help to support the planning of such in situ work. The selection of appropriate sampling sites in fluvial settings could be improved by analyzing long, meter-high, open-air outcrops that formed during most recent fluvial episodes. Such settings are abundant on Earth and could be present on Mars but may be just below the resolution of available data. By using 20–30-cm-deep excavations, shallow subsurface exploration could reveal the last period of geological history that would have been unattainable by surface observation alone. Aggregates embedded in the original strata or from heavily pulverized samples could not be identified; only weakly fragmented samples viewed right after acquisition showed aggregates, and thus, the Close-Up Imager (CLUPI) on the ExoMover might provide information on cementation-related aggregation on the observing plate before crushing. The mechanical separation of different size grains (mainly clays and attached minerals) would also support the identification of individual components. To maximize context information during subsurface exploration, rover imaging should be accomplished before crushing; however, currently planned imaging may not be ideal for this.
机译:在Ibn Battuta火星类似地点的野外工作期间,分析了两个研究问题:(1)我们如何使用远程和本地成像来确定采样地点;(2)可以从浅层地下勘探中获得什么样的信息?虽然远程图像通常有助于将野外活动作为目标,但对于不同的岩石沙漠地形类型,在不同空间尺度上的观测结果之间的联系尚未建立。在这种情况下,对精选的类似物的远程原位图像进行集中比较将大有帮助。从远程获取的数据中可以看出干的湖床可能没有显示过去水活动的特征,而浅层地下勘探可能揭示了湖相时期。采集具有不同几何形状的相同地形的多个卫星图像将有助于支持这种现场工作的计划。通过分析在最近的河流事件中形成的长,米高,露天露头,可以改善在河流环境中合适的采样地点的选择。这样的设置在地球上很丰富,可能存在于火星上,但可能仅低于可用数据的分辨率。通过使用20–30 cm深的开挖,浅层地下勘探可以揭示仅靠地面观测无法获得的最后一段地质历史。无法识别嵌入原始地层或来自严重粉碎样品的骨料;只有在采集后立即观察到的零散的样品显示聚集,因此,ExoMover上的Close-Up Imager(CLUPI)可能会在压碎之前提供有关观察板上胶结相关聚集的信息。机械分离不同大小的谷物(主要是粘土和附着的矿物质)也将有助于识别单个成分。为了在地下勘探过程中最大化背景信息,应该在压碎之前完成流动站成像。但是,当前计划的成像可能对此并不理想。

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