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首页> 外文期刊>Journal of geophysical research. Planets >Field reconnaissance geologic mapping of the Columbia Hills, Mars, based on Mars Exploration Rover Spirit and MRO HiRISE observations
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Field reconnaissance geologic mapping of the Columbia Hills, Mars, based on Mars Exploration Rover Spirit and MRO HiRISE observations

机译:基于火星探索漫游者精神和MRO HiRISE观测的火星哥伦比亚山野外侦查地质图

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Chemical, mineralogic, and lithologic ground truth was acquired for the first time on Mars in terrain units mapped using orbital Mars Reconnaissance Orbiter’s High Resolution Imaging Science Experiment (MRO HiRISE) image data. Examination of several dozen outcrops shows that Mars is geologically complex at meter length scales, the record of its geologic history is well exposed, stratigraphic units may be identified and correlated across significant areas on the ground, and outcrops and geologic relationships between materials may be analyzed with techniques commonly employed in terrestrial field geology. Despite their burial during the course of Martian geologic time by widespread epiclastic materials, mobile fines, and fall deposits, the selective exhumation of deep and well‐preserved geologic units has exposed undisturbed outcrops, stratigraphic sections, and structural information much as they are preserved and exposed on Earth. A rich geologic record awaits skilled future field investigators on Mars. The correlation of ground observations and orbital images enables construction of a corresponding geologic reconnaissance map. Most of the outcrops visited are interpreted to be pyroclastic, impactite, and epiclastic deposits overlying an unexposed substrate, probably related to a modified Gusev crater central peak. Fluids have altered chemistry and mineralogy of these protoliths in degrees that vary substantially within the same map unit. Examination of the rocks exposed above and below the major unconformity between the plains lavas and the Columbia Hills directly confirms the general conclusion from remote sensing in previous studies over past years that the early history of Mars was a time of more intense deposition and modification of the surface. Although the availability of fluids and the chemical and mineral activity declined from this early period, significant later volcanism and fluid convection enabled additional, if localized, chemical activity.
机译:化学,矿物学和岩性地面真相是在火星上首次获得的,其地形单位是使用轨道火星侦察轨道器的高分辨率成像科学实验(MRO HiRISE)图像数据进行绘制的。对几十个露头的检查表明,火星在米长的尺度上地质复杂,其地质历史记录被很好地暴露,可以识别地层单位并将其与地面上的重要区域相关联,并且可以分析露头和物质之间的地质关系。与陆地野外地质常用的技术。尽管在火星地质时期被大量的表层碎屑物,流动粉尘和秋季沉积物掩埋,但深埋和保存完好的地质单元的选择性掘出工作暴露了未受干扰的露头,地层剖面和结构信息,这与它们的保存和保存有关。暴露在地球上。丰富的地质记录正在等待火星上有经验的未来现场调查员。地面观测和轨道图像的相关性使得能够构造相应的地质勘测图。到访的大多数露头被认为是火山碎屑岩,冲积岩和表层碎屑沉积,覆盖在未暴露的基底上,这可能与修饰的Gusev火山口中心峰有关。流体已经改变了这些原石的化学和矿物学,其程度在同一地图单元内发生了很大变化。对平原熔岩和哥伦比亚山之间的主要不整合面之上和之下暴露的岩石进行的检查直接证实了过去几年中的遥感研究得出的一般结论,即火星的早期历史是一个更激烈的沉积和变质时期。表面。尽管从这一早期开始流体的供应以及化学和矿物活动的下降,但是后期大量的火山活动和流体对流使更多的化学活动(如果是局部的)成为可能。

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