首页> 外文学位 >Water on ancient Mars: Forming the phyllosilicates at Mawrth Vallis.
【24h】

Water on ancient Mars: Forming the phyllosilicates at Mawrth Vallis.

机译:古代火星上的水:在莫沃斯·瓦利斯(Mawrth Vallis)形成页硅酸盐。

获取原文
获取原文并翻译 | 示例

摘要

The clay units at Mawrth Vallis are among the most extensive on Mars. Here we characterize the mineralogy and texture of these units through analyses of data from the Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) and High Resolution Imaging Science Experiment (HiRISE) instruments and through laboratory studies of mineral mixtures.Analyzing CRISM data, two main phyllosilicate-bearing units have been identified: a nontronite-bearing unit overlain by an Al-phyllosilicate-bearing unit. This upper unit contains a lower layer containing montmorillonite plus hydrated silica and an upper layer containing kaolinite plus hydrated silica. A ferrous mineral has also been identified near the boundary between and mixed with the nontronite- and Al-phyllosilicate-bearing units and saponite has been identified on a crater floor. These individual minerals are identified and distinguished by features at 1.38--1.42, &sim1.91, and 2.17--2.41 microm.To help determine what type of hydrated silica is mixed with the montmorillonite and kaolinite, spectra of mixtures of kaolinite-opal-A, kaolinite-montmorillonite, montmorillonite-obsidian, montmorillonite-hydrated silica (opal), and glass-illite-smectite (where glass was hydrothermally altered to illite-smectite) were measured and analyzed. The best spectral matches with the Mawrth Vallis data are mixtures of obsidian with 20 to 50 % montmorillonite or mixtures of montmorillonite with 25 to 50 % kaolinite. The spectra of clay mixtures with opal and of hydrothermally altered glass-illite-smectite did not represent as well the Martian spectra observed in this region.Finally, HiRISE data was examined to characterize the textures and morphologies of the Mawrth Vallis clays and determine if there are specific textures that correlate with mineralogy. Nontronite-bearing rocks appear tan in HiRISE COLOR data and exhibit irregular polygons 2--5 m across. Montmorillonite-bearing rocks generally appear blue and exhibit regular polygons 0.5--1.5 m across. Kaolinite-bearing rocks are the brightest clay-bearing rock in HiRISE data and are fractured non-polygonally. Hydrated silica and the ferrous mineral exhibit no consistent textures.The nontronite- and montmorillonite-bearing units are remarkably consistent in both mineralogical and textural stratigraphy across the Mawrth Vallis region, suggesting they were formed by a regional process and exposed to regional environmental conditions post-deposition.
机译:Mawrth Vallis的黏土单位是火星上使用最广泛的黏土。在这里,我们通过分析火星紧凑侦察成像光谱仪(CRISM)和高分辨率成像科学实验(HiRISE)仪器的数据以及矿物混合物的实验室研究来表征这些单元的矿物学和质地。分析CRISM数据是两种主要的页硅酸盐已经确定了含轴承单元:由铝硅酸盐轴承单元覆盖的含白云石的单元。该上部单元包含含有蒙脱土和水合二氧化硅的下层,以及包含高岭土和水合二氧化硅的上层。还发现了含铁的矿物和叶绿素和铝的层状硅酸盐的单元之间的边界并与之混合,并且在火山口的地面上也鉴定了皂石。这些单独的矿物通过1.38--1.42,&sim1.91和2.17--2.41微米的特征进行识别和区分。为了帮助确定哪种类型的水合二氧化硅与蒙脱石和高岭石混合,高岭石-蛋白石-混合物的光谱测量并分析了高岭石-蒙脱石,蒙脱石-黑曜石,蒙脱石水合二氧化硅(蛋白石)和玻璃-伊利石-蒙脱石(其中水热玻璃化为伊利石-蒙脱石)。与Mawrth Vallis数据最匹配的光谱是黑曜石与20%至50%的蒙脱石的混合物或蒙脱石与25%至50%的高岭石的混合物。蛋白石和水热蚀变的玻璃伊利石-蒙脱石的黏土混合物的光谱也不能很好地反映该区域的火星光谱。是与矿物学相关的特定纹理。在HiRISE COLOR数据中,含囊脱石的岩石呈棕褐色,并呈2--5 m的不规则多边形。含蒙脱石的岩石通常呈蓝色,并呈0.5--1.5 m的规则多边形。含高岭石的岩石是HiRISE数据中最亮的含粘土岩石,并且呈非多边形裂缝状。水合二氧化硅和黑色金属矿物没有一致的质地。蒙脱石和蒙脱石的构造在整个Mawrth Vallis地区的矿物学和质地地层中都非常一致,这表明它们是由区域过程形成的,并在暴露后暴露于区域环境条件下沉积。

著录项

  • 作者

    McKeown, Nancy K.;

  • 作者单位

    University of California, Santa Cruz.;

  • 授予单位 University of California, Santa Cruz.;
  • 学科 Geology.Physics Astronomy and Astrophysics.Remote Sensing.
  • 学位 Ph.D.
  • 年度 2010
  • 页码 185 p.
  • 总页数 185
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

相似文献

  • 外文文献
  • 中文文献
  • 专利
获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号