首页> 外文期刊>Journal of geophysical research. Planets >Uncertainties in the shock devolatilization of hydrated minerals: A nontronite case study
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Uncertainties in the shock devolatilization of hydrated minerals: A nontronite case study

机译:水合矿物质冲击挥发的不确定性:绿脱石案例研究

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摘要

Controlled recovery of hydrated minerals subjected to planar shock loading is challenging because of the large difference in shock impedance between the natural samples and the engineering materials used as the recovery capsules. Significant differences in recovery capsule design confound straightforward interpretation of existing data on shock modification of hydrated minerals. We present X-ray diffraction and infrared spectroscopy results from new shock recovery experiments on nontronite (a smectite clay observed on Mars) and identify major issues in the interpretation of recovered samples. Previous work assumes that the first shock pressure step in a ring-up configuration is the most important factor in the interpretation of shock modification. By comparing the X-ray diffraction and infrared spectroscopy data from experiments with similar first shock steps but significantly different final shock states, we show that one cannot simply interpret the recovered samples based upon the first shock pressure step. This work demonstrates the need for a deeper understanding of the thermodynamics of ring-up experiments in order to be able to interpret the results in terms of an equivalent single shock loading pressure for planetary applications. In this work, we also show that venting of the samples does not matter significantly at low pressures but may be important at high pressures. We have developed a recovery method and validation test that allows us to address the major issues and technical tradeoffs with shock recovery experiments on volatile materials.
机译:由于天然样品与用作回收胶囊的工程材料之间的抗震阻抗差异很大,因此受到平面冲击载荷作用的水合矿物的受控回收具有挑战性。回收胶囊设计的显着差异混淆了对水合矿物质冲击改性的现有数据的直接解释。我们介绍了对新脱石(在火星上观察到的蒙脱石粘土)进行新的冲击恢复实验的X射线衍射和红外光谱结果,并确定了解释回收样品的主要问题。先前的工作假定振铃配置中的第一步冲击压力是解释冲击变化的最重要因素。通过比较来自具有类似第一冲击步骤但显着不同的最终冲击状态的实验的X射线衍射和红外光谱数据,我们表明人们无法根据第一冲击压力步骤简单地解释回收的样品。这项工作表明需要更深入地了解振铃实验的热力学,以便能够以等效的单冲击载荷压力来解释行星应用中的结果。在这项工作中,我们还表明样品的排气在低压下并不重要,但在高压下可能很重要。我们已经开发了一种回收方法和验证测试,使我们能够通过对挥发性材料进行冲击恢复实验来解决主要问题和技术折衷。

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