Advancements in Lunar and Martian Soil Mechanics: Reliability of Simulants and Implications for Design

A special issue of Applied Sciences (ISSN 2076-3417). This special issue belongs to the section "Civil Engineering".

Deadline for manuscript submissions: closed (30 April 2023) | Viewed by 4234

Special Issue Editor


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Guest Editor
Department of Civil, Environmental, Territorial, Building Engineering and Chemistry (DICATECh), Polytechnic University of Bari, Bari, Italy
Interests: soil drying; soil structure degradation; lunar and martian geotechnics; landslides

Special Issue Information

Dear Colleagues,

This Special Issue of Applied Sciences aims at collecting new theoretical, experimental and numerical studies in the field of the lunar soil mechanics. The construction of a human habitat on the Moon, a permanent lunar base, will require increasing research related to the reliability of the lunar simulants when deducing mechanical parameters for the design. It is well known that the main difference between the real lunar soils and the simulants is the formation environment: thermal and dynamic stresses and vacuum on the moon should involve important effects on the regolith mechanical properties, which are difficult to reproduce on Earth. In this respect, a lunar simulant, once created, should be subjected to suitable disturbance in order to acquire a more reliable soil structure and, therefore, to allow good performance of the geotechnical design. The topic is characterized by strong interplay between physics and geotechnics; therefore, relevant contributions for this Special Issue are expected from researchers of both fields.

Prof. Dr. Francesco Cafaro
Guest Editor

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Keywords

  • lunar regolith simulants
  • mechanical behaviour
  • reliability
  • thermal excursions
  • impact loads
  • moonbase

Published Papers (2 papers)

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Research

14 pages, 2595 KiB  
Article
Performance of Lunar Regolith Shield under Meteoroid Impact: Uncertainties of a Numerical Prediction
by Alessia Verdino, Oscar Arena, Osvaldo Bottiglieri, Francesco Cafaro and Enrico Dini
Appl. Sci. 2022, 12(21), 10885; https://doi.org/10.3390/app122110885 - 27 Oct 2022
Cited by 2 | Viewed by 1295
Abstract
The protection of the future lunar base from radiation, thermal stresses and impacts of meteoroids can be achieved by several options, generally consisting in a shielding system, made of either regolith or combined materials. In the present paper, the incidence of two sources [...] Read more.
The protection of the future lunar base from radiation, thermal stresses and impacts of meteoroids can be achieved by several options, generally consisting in a shielding system, made of either regolith or combined materials. In the present paper, the incidence of two sources of uncertainty on the FEM calculation of stress propagation through the covering regolith layer has been assessed. First, the investigation has pointed out, for a given impact and a given constitutive model, the uncertainty in the stress prediction related to the strain interval adopted for the soil stiffness measurement. Thereafter, calculation has been performed, for a given stiffness value, changing the assumed collision duration of one order of magnitude for equal impact momentum, that is, changing the maximum impact force too, correspondingly. The simulation has been performed based on physical and mechanical parameters of DNA-1A lunar simulant. The results provide indication of the relative importance of the calculation assumptions, which could address the design of a regolith shield. Full article
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11 pages, 4029 KiB  
Article
Interface Direct Shear Tests on JEZ-1 Mars Regolith Simulant
by Kexin Yin, Jiangxin Liu, Jiaxing Lin, Andreea-Roxana Vasilescu, Khaoula Othmani and Eugenia Di Filippo
Appl. Sci. 2021, 11(15), 7052; https://doi.org/10.3390/app11157052 - 30 Jul 2021
Cited by 12 | Viewed by 2213
Abstract
The mechanical behaviors of Martian regolith-structure interfaces are of great significance for the design of rover, development of excavation tools, and construction of infrastructure in Mars exploration. This paper presents an experimental investigation on the properties of a Martian regolith simulant (JEZ-1) through [...] Read more.
The mechanical behaviors of Martian regolith-structure interfaces are of great significance for the design of rover, development of excavation tools, and construction of infrastructure in Mars exploration. This paper presents an experimental investigation on the properties of a Martian regolith simulant (JEZ-1) through one-dimensional oedometer test, direct shear test, and interface direct shear tests between JEZ-1 and steel plates with different roughness. Oedometer result reveals that the compression and swelling indexes of the JEZ-1 are quite low, thus it is a less compressible and lower swelling soil. The cohesion and adhesion of JEZ-1 are lower than 5 kPa. The values of the internal friction angle range from 39.7° to 40.6°, and the interface friction angles are 16.7° to 36.2° for the smooth and rough interface. Furthermore, the direct shear and interface direct shear results indicate that the interface friction angles are lower than the internal friction angles of JEZ-1 and increase close to the internal friction angles with increasing interface roughness. Full article
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