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The microstructures and creep and attenuation behaviors of ice-iodine and ice/hydrate eutectic aggregates at planetary conditions.

机译:冰-碘和冰/水合物共晶聚集体在行星条件下的微观结构以及蠕变和衰减行为。

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摘要

The solidification behavior, microstructure and mechanical response of several two-phase aggregates of ice-I + salt hydrates were experimentally and theoretically studied; the binary systems explored were selected based on their potential application to the study of tectonics and heat flow on the Jovian moon Europa. Eutectic solidification of systems H2O-Na 2SO4, H2O-MgSO4, H2O-Na 2CO3, and H2O-H2SO4 was analyzed from a theromodynamic and kinetic perspective and the resulting microstructures by cryogenic scanning electron microscope. Classical eutectic microstructures---fine (mum)-scale intergrowths of ice and hydrate arranged in colonies---are formed in each system, the intergrowth morphology of which can be predicted from the volume fraction of the phase having the highest partial molar entropy of solution and from the magnitude of that entropy. The mechanical testing of ice-I and MgSO4·11H2O ("MS11"; chosen because it has been suggested as a better fit to the near-infrared spectral data of Europa) has shown that the microstructure of the eutectic---in particular the high volume of phase and colony boundaries---endows the aggregate with mechanical properties distinctly different from that of pure ice. In creep, the finely dispersed hydrate, which is distinctly stronger than ice, suppresses significantly the glide of dislocations; the result is a material both stronger and more brittle than pure ice. The eutectic rheology thus opens the possibility for semi-brittle flow in a two-phase, hydrate-ice planetary shell, affecting the tectonic responses. Attenuation in pure polycrystalline ice is effected by diffusional dissipation on low-angle (subgrain) boundaries augmented by non-linear losses wrought by glide of lattice dislocations. Grain boundaries can become significant in the attenuation response under dynamic conditions where a dislocation rheology dictates creep dynamics and the grain size is approximately equal to the subgrain size. In the absence of cracking in the hydrate phase, specifically at modest differential stresses (≤1 MPa) for the materials studied here (colony sizes ≤500 mum; hydrate ice lamellar spacing ≤20 mum), the attenuation response of ice-I/MS11 eutectic aggregates is little different than that of pure polycrystalline ice.
机译:通过实验和理论研究了几种冰-I +盐水合物的两相聚集体的凝固行为,微观结构和力学响应。根据所研究的二元系统在木星欧罗巴构造和热流研究中的潜在应用选择了它们。从热力学和动力学角度分析了H2O-Na 2SO4,H2O-MgSO4,H2O-Na 2CO3和H2O-H2SO4系统的共晶凝固,并通过低温扫描电子显微镜分析了所得的微观结构。在每个系统中都形成了经典的共晶微观结构,即在菌落中排列的冰和水合物的精细(微米)尺度共生体,其共生形态可以通过具有最高部分摩尔熵的相的体积分数来预测解和熵的大小。对Ice-I和MgSO4·11H2O(“ MS11”;之所以选择这种机械测试,是因为它被建议更适合于欧罗巴的近红外光谱数据),它显示了共晶的微观结构,特别是大量的相和菌落边界-赋予了集料与纯冰明显不同的机械性能。在蠕变中,比冰强得多的细分散的水合物可显着抑制位错的滑移。结果是比纯冰更坚固,更脆的材料。因此,共晶流变学为两相水合物冰行星壳中的半脆性流动打开了可能性,从而影响了构造响应。纯多晶冰的衰减受晶格位错滑行造成的非线性损失增加的低角度(亚晶粒)边界上的扩散耗散的影响。在位错流变决定蠕变动力学并且晶粒尺寸大约等于亚晶粒尺寸的动态条件下,晶界在衰减响应中会变得很重要。在水合物相中不存在裂纹的情况下,特别是对于此处研究的材料(菌落尺寸≤500mum;水合物冰层间距≤20mum),在适度的压差(≤1MPa)下,I-MS11的衰减响应共晶聚集体与纯多晶冰几乎没有什么不同。

著录项

  • 作者

    McCarthy, Christine.;

  • 作者单位

    Brown University.;

  • 授予单位 Brown University.;
  • 学科 Geophysics.;Engineering Materials Science.
  • 学位 Ph.D.
  • 年度 2009
  • 页码 224 p.
  • 总页数 224
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

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