Geotechnical Properties of Lunar Soil Analogue VI-75 in Dry and Frozen State

IF 0.7 4区 物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS
A. V. Uvarova, E. N. Slyuta, I. A. Agapkin
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引用次数: 0

Abstract

The lunar soil analogue VI-75 fully corresponds to typical lunar regolith in terms of particle morphology, grain-size distribution, and physical-mechanical properties. It is actively used in various experimental studies and tests of space equipment and scientific instruments. This study investigates additional physical and mechanical characteristics of the lunar soil analogue VI-75, such as the angle of repose and the coefficients of subgrade reaction, which are essential for modeling and calculations when planning the placement of infrastructure for a permanent scientific lunar station on the Moon's surface. It is also shown that the water ice content in lunar soil can significantly alter its mechanical properties and greatly increase its strength characteristics. For example, doubling the water ice content in lunar regolith almost doubles its strength properties. The study addresses the rate of water migration due to gravity from the upper layer of the analogue to the lower layer and provides recommendations for preventing undesirable water migration during the preparation of experiments with frozen soil on large-scale test stands.

Abstract Image

月壤VI-75模拟物干冻状态岩土力学特性研究
月壤模拟物VI-75在颗粒形态、粒度分布、物理力学性质等方面与典型月壤完全一致。它积极用于空间设备和科学仪器的各种实验研究和测试。本研究研究了月球土壤模拟物VI-75的其他物理和力学特性,如休止角和路基反应系数,这些对于在月球表面规划永久科学月球站基础设施的位置时建模和计算是必不可少的。结果表明,月壤中水冰含量对月壤力学性能有显著影响,对月壤强度特性有显著提高。例如,月球风化层中的水冰含量增加一倍,几乎使其强度特性增加一倍。该研究解决了由重力引起的水从模拟物上层向下层迁移的速率,并提供了在大型试验台冻土实验准备过程中防止不良水迁移的建议。
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来源期刊
Solar System Research
Solar System Research 地学天文-天文与天体物理
CiteScore
1.60
自引率
33.30%
发文量
32
审稿时长
6-12 weeks
期刊介绍: Solar System Research publishes articles concerning the bodies of the Solar System, i.e., planets and their satellites, asteroids, comets, meteoric substances, and cosmic dust. The articles consider physics, dynamics and composition of these bodies, and techniques of their exploration. The journal addresses the problems of comparative planetology, physics of the planetary atmospheres and interiors, cosmochemistry, as well as planetary plasma environment and heliosphere, specifically those related to solar-planetary interactions. Attention is paid to studies of exoplanets and complex problems of the origin and evolution of planetary systems including the solar system, based on the results of astronomical observations, laboratory studies of meteorites, relevant theoretical approaches and mathematical modeling. Alongside with the original results of experimental and theoretical studies, the journal publishes scientific reviews in the field of planetary exploration, and notes on observational results.
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