Martian soil-analogue VI-M1 for large-scale geotechnical experiments

IF 1.8 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS
E.N. Slyuta , E.A. Grishakina , V. Yu Makovchuk , A.V. Uvarova , I.A. Agapkin , D.D. Mironov , M.S. Nikitin , E.A. Voznesensky
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Abstract

In the actively evolving research of Mars in recent decades, a special place is occupied by landers and rovers. The diversity of landscapes and soils on Mars, characteristic of terrestrial planets with an atmosphere, makes the development of soil simulators relevant for each new type of terrain in the area of a potential landing site. In the article, based on a comprehensive analysis of the physical and mechanical properties of soils at previous landing sites and a geomorphological analysis of the Oxia Planum plain, the main requirements for the properties of Martian soil analog at the landing site of the ExoMars Rosalind Franklin Mission (RFM) were determined. Readily available technogenic and natural materials have been selected and experimentally justified as components for creating a Martian soil analogue. A methodology for creating the soil analog is presented, and its physical and mechanical properties are measured. The developed Martian soil analog VI-M1 is actively used for large-scale natural experiments, including drop tests of spacecraft in the ExoMars series.

用于大规模岩土工程实验的火星土壤模拟物 VI-M1
在近几十年积极发展的火星研究中,着陆器和漫游车占据了特殊的位置。火星上地貌和土壤的多样性是有大气层的陆地行星所特有的,这使得开发土壤模拟器与潜在着陆点区域的每一种新地形都息息相关。文章根据对以前着陆点土壤物理和机械特性的综合分析以及对 Oxia Planum 平原的地貌分析,确定了 ExoMars 罗莎琳德-富兰克林任务(RFM)着陆点火星土壤模拟特性的主要要求。选择了现成的技术材料和天然材料,并通过实验证明这些材料可作为创建火星模拟土壤的组成部分。介绍了创建模拟土壤的方法,并对其物理和机械性能进行了测量。开发的火星土壤模拟物 VI-M1 正积极用于大规模自然实验,包括 ExoMars 系列航天器的跌落试验。
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来源期刊
Planetary and Space Science
Planetary and Space Science 地学天文-天文与天体物理
CiteScore
5.40
自引率
4.20%
发文量
126
审稿时长
15 weeks
期刊介绍: Planetary and Space Science publishes original articles as well as short communications (letters). Ground-based and space-borne instrumentation and laboratory simulation of solar system processes are included. The following fields of planetary and solar system research are covered: • Celestial mechanics, including dynamical evolution of the solar system, gravitational captures and resonances, relativistic effects, tracking and dynamics • Cosmochemistry and origin, including all aspects of the formation and initial physical and chemical evolution of the solar system • Terrestrial planets and satellites, including the physics of the interiors, geology and morphology of the surfaces, tectonics, mineralogy and dating • Outer planets and satellites, including formation and evolution, remote sensing at all wavelengths and in situ measurements • Planetary atmospheres, including formation and evolution, circulation and meteorology, boundary layers, remote sensing and laboratory simulation • Planetary magnetospheres and ionospheres, including origin of magnetic fields, magnetospheric plasma and radiation belts, and their interaction with the sun, the solar wind and satellites • Small bodies, dust and rings, including asteroids, comets and zodiacal light and their interaction with the solar radiation and the solar wind • Exobiology, including origin of life, detection of planetary ecosystems and pre-biological phenomena in the solar system and laboratory simulations • Extrasolar systems, including the detection and/or the detectability of exoplanets and planetary systems, their formation and evolution, the physical and chemical properties of the exoplanets • History of planetary and space research
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