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首页> 外文会议>Biennial International Conference on Engineering, Science, Construction, and Operations in Challenging Environments >Compressibility Behavior of a Nearside Highland Regolith Simulant
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Compressibility Behavior of a Nearside Highland Regolith Simulant

机译：附近高地表土模拟物的压缩特性

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The surface of the Moon, both highland and mare regions, experiences collisions from meteorites and solar flares constantly. As a result, regolith particles have ever rotating positions, sizes, and angularity that alter the ability of human activity to be possible without understanding the mechanical properties of the regolith structure that will be built upon. Lunar regolith simulants, based on precious samples of the Apollo missions, are necessary for creating a baseline of how lunar regolith will behave under increased activity. The inconsistencies across the lunar surface due to the raw environment make it difficult to accurately plan the built conditions of a permanent structure. Testing compression and settlement of simulants at varying densities provides a better comprehension of what can be expected regarding the foundations for lunar transportation, building infrastructure, and the large machinery that will have a significant presence during the construction phase building these permanent residences on the face of the Moon. This paper assesses the regolith simulant, OPRH2N, recently developed in 2017, with very similar angularity to lunar regolith in the highland regions. Material properties of specific gravity, and compressibility, were performed and void ratio-stress parameters were developed and compared to estimates from other simulants. The compressibility parameters of these simulants agree with those determined from other simulants and with those of returned lunar regolith. Further, testing and analysis are necessary to establish strength parameters for detailed synopsis of settlement and bearing capacities.
机译：月球表面，无论是高地还是马雷地区，都会不断经历陨石和太阳耀斑的碰撞。因此，表土颗粒的旋转位置、大小和角度会改变人类活动的能力，而不需要了解将要建立的表土结构的机械特性。月球表土模拟物基于阿波罗任务的珍贵样本，对于创建月球表土在活动增加时的行为基线是必要的。由于月球表面的原始条件不一致，很难准确地绘制月球表面的结构图。在不同密度下测试模拟物的压缩和沉降，可以更好地理解月球交通基础、建筑基础设施和大型机械的预期情况，这些大型机械将在月球表面建造永久住所的施工阶段发挥重要作用。本文评估了2017年开发的表土模拟物OPRH2N，其角度与高地地区的月球表土非常相似。对材料的比重和压缩性进行了研究，开发了孔隙比应力参数，并与其他模拟物的估算值进行了比较。这些模拟物的压缩性参数与其他模拟物和返回的月球表土的压缩性参数一致。此外，有必要进行测试和分析，以确定沉降和承载力详细概要的强度参数。

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