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Modeling of regolith structure interaction in extraterrestrial constructed facilities.

机译:地外建筑设施中go石结构相互作用的建模。

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摘要

In the near future, construction on the surface of Earth's Moon is proposed to facilitate space travel and exploration. Construction on the lunar surface will differ most notably from terrestrial-based construction in that designs of lunar constructed facilities will need to be highly exact in order to avoid excessive use of materials and on-site workmanship. This requirement creates a need for a thorough understanding of lunar soil (regolith) properties and behavior and how their variation influences the performance of extraterrestrial structures, where performance reflects the overall strength (stability) as well as the load-settlement characteristics of the foundation.;The lunar landing missions of the 1960's and 1970's (Surveyor, Apollo and Soviet-Luna) have provided a base-level knowledge of lunar regolith mechanical properties. A terrestrial-based lunar soil simulant has been developed to mimic these known properties. This simulant is used in a series of strength and deformation experiments to further investigate the nature of lunar regolith. These experiments include conventional triaxial compression (CTC), unconfined compression, reduced triaxial extension, isotropic compression, direct shear, direct tension, and self-weight unconfined tension. These experiments are used to calibrate a plasticity-based analytical model which was designed particularly for highly-dilatant granular materials under low levels of confining stress. This model, in conjunction with a finite element computer code, is used to predict the behavior of several boundary value problems. The CTC experiment is treated as a soil structure subject to end-displacement conditions, material self-weight body forces, and radially induced membrane confinement. The direct tension experiment is also analyzed as a soil-structure. It is shown that the behavior of this lunar regolith simulant is unusual in that it contains a small amount of cohesion, and markedly smaller levels of tensile strength, in the absence of water, possesses quite high angles of internal friction, and exhibits dilatant behavior for even loose material packings. Furthermore, it is demonstrated that particular care must be taken in constitutive model calibration for ultra-low levels of mean stress where the values of the small, but finite, tensile strength and cohesion become crucial.;A proposed lunar structure, used to house crew and supplies, is studied using geotechnical centrifuge principles and finite element numerical simulations. This structure consists of a very stiff hollow cylinder covered by approximately 2 m of lunar regolith in the form of a regolith-embankment used for radiation shielding. A modeling-of models approach is taken to verify centrifuge scaling relationships. The finite element simulations are found to match experiments well by providing suitable displacement boundary conditions for the bottom of the embankment.
机译:在不久的将来,建议在地球的月球表面进行构造以促进太空旅行和探索。月球表面的建筑与陆地建筑的显着不同之处在于,月球建筑设施的设计需要高度精确,以避免过多使用材料和现场做工。这项要求需要彻底了解月球土壤(重生岩)的特性和行为,以及它们的变化如何影响地外结构的性能,其中性能反映了地基的整体强度(稳定性)以及载荷沉降特性。 ; 1960年代和1970年代的登月任务(测量员,阿波罗和苏维埃-卢纳)提供了有关月球重石力学特性的基础知识。已经开发了一种基于陆地的月球土壤模拟物来模拟这些已知特性。该模拟物用于一系列强度和变形实验,以进一步研究月球巨石的性质。这些实验包括常规三轴压缩(CTC),无侧限压缩,减小的三轴延伸,各向同性压缩,直接剪切,直接拉力和自重无侧限拉力。这些实验用于校准基于可塑性的分析模型,该模型是专为在低水平约束应力下高度膨胀的颗粒材料而设计的。该模型与有限元计算机代码一起用于预测几个边值问题的行为。将CTC实验视为受末端位移条件,材料自重体力和径向诱导膜约束的土壤结构。直接张力试验也被分析为土壤结构。结果表明,这种月球长石模拟物的行为是不寻常的,因为它具有少量的内聚力,并且在没有水的情况下具有显着较小的抗张强度,具有很高的内摩擦角,并且表现出扩张性。甚至松散的材料包装。此外,证明了在本构模型校准中必须特别注意平均应力的超低水平,在这种情况下,很小但有限的抗拉强度和内聚力的值变得至关重要。使用岩土离心机原理和有限元数值模拟研究了物料和物料。这种结构由一个非常坚硬的空心圆柱体组成,上面覆盖着大约2 m的月牙长石,呈月牙石路堤的形式,用于辐射屏蔽。采用模型建模方法来验证离心机的比例关系。通过为路堤底部提供合适的位移边界条件,发现有限元模拟可以很好地匹配实验。

著录项

  • 作者

    Perkins, Steven Will.;

  • 作者单位

    University of Colorado at Boulder.;

  • 授予单位 University of Colorado at Boulder.;
  • 学科 Civil engineering.;Geotechnology.;Aerospace engineering.
  • 学位 Ph.D.
  • 年度 1991
  • 页码 344 p.
  • 总页数 344
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

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