Results 41 to 50 of about 391 (168)
Abstract The lunar surface is heterogeneous in grain size and metallic iron abundance due to diverse histories of space weathering. The spectral and polarimetric properties of the lunar regolith are strongly affected by both grain size and metallic iron particles.
Eunjin Cho +10 more
wiley +1 more source
Morphological and Spectral Characterization of Lunar Regolith Breakdown due to Water Ice
Remote sensing observations of the Moon suggest that the lunar polar regolith environment is affected by several natural processes that may cause the regolith in these regions to become more porous and fine particulate.
A. Shackelford +3 more
doaj +1 more source
Abstract Silicate melt viscosity plays a pivotal role in the evolution of rocky bodies within the Solar System, exerting first‐order control on mantle differentiation and stratification, while dictating the metal‐silicate separation and the subsequent volcanic activity.
Fabrizio Di Fiore, Michele Cassetta
wiley +1 more source
Spark Plasma Sintering and Optical Characterization of Lunar Regolith Simulant
Regolith-covered surfaces exist in several planetological environments, including the Moon, Mars, NEAs, etc, some of which have been identified as first targets for future colonization outposts. Clearly, the development of advanced technologies in the framework of ISRU concept is a key asset to boost human space explorations on these celestial bodies ...
Roberta Licheri +4 more
openaire +2 more sources
Constructing lunar pavements is of great significance for improving the transportation efficiency of materials and personnel transfer at lunar bases. Utilizing lunar regolith for the in-situ preparation of geopolymer is an effective means of supplying ...
Lichong Chen +3 more
doaj +1 more source
Since the landing on the lunar surface, the lunar regolith has begun to interact in different ways with landed elements, such as the wheels of a rover, astronaut suits, drills, and plants for extracting oxygen or manufacturing objects.
Giovanni Zanotti +3 more
doaj +1 more source
Abstract Accumulation of dust on the Lunar and Martian surfaces plays a critical role in both surface evolution and human exploration efforts, limiting equipment lifetimes and obscuring optical surfaces. Yet, the underlying physics of surface soiling is still poorly understood.
G. Griffin +3 more
wiley +1 more source
Experimental Evaluation of Lunar Regolith Settlement Caused by Ice Extraction
Water resources are essential to human exploration in deep space or the establishment of long-term lunar habitation. Ice discovered on the Moon may be useful in future missions to the lunar surface, necessitating the consideration of in situ resource ...
Zheng Gong +8 more
doaj +1 more source
New High Precision Measurements of Apollo Samples: 0.3–5 GHz Complex Refractive Indices
Abstract Active and passive radar techniques provide information on the subsurface structure and history of planetary bodies. However, interpretations of radar data are limited by our understanding of the complex dielectric permittivity and magnetic permeability of the surface material.
P. Linton +15 more
wiley +1 more source
Verification of a virtual lunar regolith simulant
Introduction: Physical regolith simulants are valuable tools for developing In-Situ Resource Utilisation hardware. However, using virtual models of regolith instead can reduce costs, limit exposure to hazardous materials, and offer a practical method of testing the effects of reduced gravity.Methods: We verify a virtual model of regolith as ...
Louca, Joe +3 more
openaire +2 more sources

