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首页> 外文期刊>Earth and Planetary Science Letters: A Letter Journal Devoted to the Development in Time of the Earth and Planetary System >Stratigraphy and sedimentology of a dry to wet eolian depositional system, Burns formation, Meridiani Planum, Mars
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Stratigraphy and sedimentology of a dry to wet eolian depositional system, Burns formation, Meridiani Planum, Mars

机译:干湿风成沉积体系的地层学和沉积学,烧伤形成,梅里迪亚尼普朗姆,火星

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摘要

Outcrop exposures of sedimentary rocks at the Opportunity landing site (Meridiani Planum) form a set of genetically related strata defined here informally as the Burns formation. This formation call be subdivided into lower, middle, and upper units which, respectively, represent eolian dune, eolian sand sheer, and mixed eolian sand sheet and interdune facies associations. Collectively, these three units are at least 7 m thick and define a "wetting-upward" Succession which records a progressive increase in the influence of groundwater and, ultimately, surface water in controlling primary depositional processes.
机译:机会登陆点(Meridiani Planum)的沉积岩露头暴露形成了一组与遗传相关的地层,这里非正式地定义为伯恩斯地层。该地层划分为下层,中层和上层单元,分别代表风沙丘,风沙纯粹以及混合的风沙薄片和中间砂岩相联系。这三个单元的总厚度至少为7 m,并定义为“向上润湿”演替,记录了在控制一次沉积过程中地下水(最终是地表水)的影响逐渐增加的情况。

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