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Investigating Weathering of Basaltic Materials in Gale Crater, Mars: A Combined Laboratory, Modeling and Terrestrial Field Approach

机译:研究火星大风火山口中玄武岩材料的风化作用:组合的实验室,建模和陆地野外研究方法

摘要

Recent observations from Gale Crater, Mars document past aqueous alteration both in the formation of the Stimson sandstone unit, as well as in the formation of altered fractures within that unit. Geochemical and mineralogical data from Curiosity also suggest Fe-rich amorphous weathering products are present in most samples measured to date. Here we interpret conditions of possible past weathering in Gale Crater using a combination of field, laboratory, and modeling work. In order to better understand secondary Fe-rich phases on Mars, we are examining formation of weathering products in high Fe and Mg and low Al serpentine soils in the Klamath Mountains, CA. We have isolated potential weathering products from these soils, and are analyzing them using synchrotron XRF and XRD as well as FullPat for a direct comparison to analyses from Gale Crater. In order to interpret the implications of the persistence of potential secondary Fe-containing phases on Mars, we are also measuring the dissolution rates of the secondary weathering products allophane, Fe-rich allophane, and hisingerite. Ongoing dissolution experiments of these materials suggest that they dissolve significantly more rapidly than more crystalline secondary minerals with similar chemical compositions. Finally, to quantify the specific conditions of past aqueous alteration in Gale Crater we are performing reactive transport modeling of a range of possible past environmental conditions. Specifically, we are testing the conditions under which a Stimson unit-like material forms from a parent material similar to Rocknest or Bagnold eolian deposits, and the conditions under which observed altered fracture zones form from a Stimson unit-like parent material. Our modeling results indicate that the formation of the Stimson unit is consistent with leaching of an eolian deposit with a solution of pH = 6-8, and that formation of the altered fracture zones is consistent with leaching with a very acidic (pH = 2-3) high sulfate solution containing Ca. These results suggest circumneutral pH conditions during authigenesis or early diagenesis in the Stimson formation sediments followed by diagenetic alteration by very acidic solutions along fracture zones.
机译:来自火星Gale Crater的最新观测结果记录了在Stimson砂岩单元的形成以及该单元内裂缝的形成中过去的水蚀变化。来自好奇号的地球化学和矿物学数据也表明,迄今为止测量的大多数样品中都存在富铁的非晶态风化产物。在这里,我们结合现场,实验室和建模工作来解释大风火山口过去可能发生的气候条件。为了更好地了解火星上的次生富铁相,我们正在研究加利福尼亚州克拉马斯山的高铁,镁和低铝蛇形土壤中风化产物的形成。我们从这些土壤中分离出了潜在的风化产物,并正在使用同步加速器XRF和XRD以及FullPat对它们进行分析,以便与Gale Crater的分析进行直接比较。为了解释火星上潜在的含铁次生相的持久性的影响,我们还测量了次级风化产物别铝镁石,富铁的别铝镁石和组晶石的溶解速率。正在进行的这些材料的溶解实验表明,它们比具有相似化学组成的更多结晶次生矿物溶解快得多。最后,为了量化Gale Crater中过去水蚀变化的具体条件,我们对一系列可能的过去环境条件进行了反应性输运建模。具体而言,我们正在测试由类似于Rocknest或Bagnold风积物的母体材料形成Stimson单元状材料的条件,以及由Stimson单元状母体材料形成观察到的断裂带变化的条件。我们的模拟结果表明,Stimson单元的形成与在pH = 6-8的溶液中风沙沉积的浸出一致,而改变的裂缝带的形成与在极酸性(pH = 2的溶液)的浸出一致。 3)含Ca的高硫酸盐溶液。这些结果表明,在Stimson地层沉积物的成岩作用或早期成岩过程中,周围环境的pH条件随后是沿断裂带的强酸性溶液成岩作用。

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