Structure and Formation Mechanism of Lunar Regolith
Lunar regolith is a thin layer of weakly cohesive detrital materials covering the lunar surface. Studies on returned lunar samples have revealed that the lunar regolith mainly consists of fragments of rocks, minerals, breccia, glasses, and agglutinates ...
Liping Qin +7 more
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Regolith history of lunar meteorites [PDF]
The regolith evolution of the lunar meteorites Dhofar (Dho) 081, Northwest Africa (NWA) 032, NWA 482, NWA 773, Sayh al Uhaymir (SaU) 169, and Yamato (Y-) 981031 was investigated by measuring the light noble gases He, Ne, and Ar. The presence of trapped solar neon in Dho 081, NWA 773, and Y-981031 indicates an exposure at the lunar surface. A neon three-
S. Lorenzetti, H. Busemann, O. Eugster
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Massive Water Production from Cryogenic Icy Lunar Regolith by a Microwave Heating Method [PDF]
Water extraction from lunar regolith is one of the critical techniques for in situ resource utilization on the Moon. Traditional conductive heating methods show low efficiencies for massive water production from lunar regolith due to the low heat ...
Qinggong Wang +5 more
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Telomere dynamics and oxidative stress in Arabidopsis grown in lunar regolith simulant [PDF]
NASA envisions a future where humans establish a thriving colony on the Moon by 2050. Plants will be essential for this endeavor, but little is known about their adaptation to extraterrestrial bodies.
Borja Barbero Barcenilla +10 more
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Thermal conductivity of high latitude lunar regolith measured by Chandra’s Surface Thermophysical Experiment (ChaSTE) onboard Chandrayaan 3 lander [PDF]
The thermal conductivity of the lunar regolith is an essential parameter in studying the thermal behavior of the Moon and in planning future lunar exploration.
Nizy Mathew +35 more
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Use of orbiting reflectors to decrease the technological challenges of surviving the lunar night [PDF]
In this paper the feasibility of using lunar reflectors to decrease the technological challenges of surviving the lunar night is investigated. This is achieved by attempting to find orbits in the two-body problem where the argument of periapsis is ...
Bewick, Russell +2 more
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Deducing Lunar Regolith Porosity From Energetic Neutral Atom Emission [PDF]
The porosity of the upper layers of regolith is key to the interaction of an airless planetary body with precipitating radiation, but it remains difficult to characterize.
A. Galli +19 more
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Lunar meteorite regolith breccias: an in situ study of impact melt composition using LA-ICP-MS with implications for the composition of the lunar crust [PDF]
Dar al Gani (DaG) 400, Meteorite Hills (MET) 01210, Pecora Escarpment (PCA) 02007, and MacAlpine Hills (MAC) 88104/88105 are lunar regolith breccia meteorites that provide sampling of the lunar surface from regions of the Moon that were not visited by ...
Crawford, Ian A. +13 more
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A lunar long duration method which utilizes a characteristic of a very low thermal conductivity of lunar regolith has been proposed. The principle of this method is to put heater in desired depth of the regolith and heat up the regolith layer during ...
Ryota NOTSU +2 more
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Physical and Chemical Evolution of Lunar Mare Regolith
The lunar landscape evolves both physically and chemically over time due to impact cratering and energetic processes collectively known as space weathering.
Byrne, S. +3 more
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