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• Parameter Estimation of Lunar Regolith from Lunar Penetrating Radar Data.
  Parameter estimation of the lunar regolith not only provides important information about the composition but is also critical to quantifying potential resources for lunar exploration and engineering for human outposts. The Lunar Penetrating Radar (LPR) onboard…
  europepmc 2018 置信度 0.80
• Manufacturing Dense Thick Films of Lunar Regolith Simulant EAC-1 at Room Temperature.
  The Aerosol Deposition (AD, also known as gas kinetic spraying or vacuum deposition) method is a rather novel coating process to produce dense thick films directly from dry ceramic (or metal) powders on a variety of substrates without any heat treatment. Becau…
  europepmc 2019 置信度 0.80
• Towards in situ de-risking of lunar granular materials handling: Design, manufacture, and initial testing and initial validation of a rotating drum breadboard suitable for vacuum conditions and eventual lunar gravity parabolic flight
  Abstract As lunar exploration and prospects for commercial exploitation accelerate, understanding regolith behaviour under low gravitational and vacuum conditions is vital for engineering robust In-Situ Resource Utilisation (ISRU) systems. Accurate characteris…
  europepmc 2026 置信度 0.80
• A bioartificial 3D bronchial epithelial airway model to study lunar hay fever on Earth.
  A significant challenge for sustained human presence on the Moon revolves around lunar regolith dust. In the past, Apollo astronauts experienced adverse reactions to lunar dust, reporting allergy-like symptoms after tracking the dust into the lunar module. A 3…
  europepmc 2026 置信度 0.80
• Integrating resource utilization and bioregenerative life support systems for sustainable space exploration.
  The long-term presence of humans in space depends on reducing reliance on Earth's resupply of materials and resources. In situ resource utilization (ISRU) represents a sustainable approach to support human activities in space by converting local materials into…
  europepmc 2026 置信度 0.80
• Feasibility of Real-Time Astronaut Eye-Tracking During Analog Extravehicular Activities.
  Introduction As lunar missions increase in frequency and duration, astronauts will conduct more extravehicular activities (EVAs) under demanding conditions that elevate workload, reduce situational awareness, and heighten the risk of operational errors. Despit…
  europepmc 2026 置信度 0.80
• Exploring differential gene correlations in <i>Arabidopsis thaliana</i> for sustainable space farming.
  The plans for sustained human presence on the Moon have increased interest in understanding the effects of lunar conditions on terrestrial biology. Plants play a vital role in space exploration, as they not only generate oxygen and remove carbon dioxide but al…
  europepmc 2026 置信度 0.80
• Searching for surficial water ice in lunar permanently shaded regions (PSRs) with ShadowCam.
  Airless bodies such as the Moon, Mercury, and Ceres have permanently shaded regions (PSRs) that can cold trap water ice. Mercury and Ceres have substantial ice deposits in their PSRs, but lunar water ice distribution remains uncertain because of sparse detecti…
  europepmc 2026 置信度 0.80
• Lunar and Martian Regolith Simulants Desorb and Weather after Exposure to Bioregenerative Life Support System Effluent.
  The extraction of plant essential nutrients from extraterrestrial regolith will be necessary to ensure the sustainability of lunar and martian agriculture. An essential instrument of these outposts will be bioregenerative life support systems (BLiSS) that atte…
  europepmc Harrison R. Coker, Daniella Saetta, Misle M. Tessema, Jackson L. Smith 等 2026 置信度 0.80 RegolithMartianLife support systemSorptionMartian soil
• Increased small impactor flux on the Moon as inferred from regolith thickness at the Chang'E-5 Region.
  Knowledge of the small impactor flux on the Moon can provide critical insights into lunar geological evolution and the dynamics of the inner solar system. However, it cannot be directly deciphered from the observed populations of small craters due to their rap…
  europepmc 2025 置信度 0.80
• Zero-shot semantic landmark-based visual odometry using foundation models for unstructured planetary exploration.
  Precise autonomous navigation on unstructured planetary surfaces is a critical prerequisite for future exploration missions, particularly in GNSS-denied environments such as the Lunar South Pole or Martian deserts. Traditional Visual Odometry (VO) methods, whi…
  europepmc 2026 置信度 0.80
• Assessing Toxicity and Nuclear and Mitochondrial DNA Damage Caused by Exposure of Mammalian Cells to Lunar Regolith Simulants.
  Previous missions to the lunar surface implicated potential dangers of lunar soil. In future explorations, astronauts may spend weeks or months on the Moon, increasing the risk of inhaling lunar dust. In an effort to understand the biological impact of lunar r…
  europepmc 2018 置信度 0.80
• Moon Regolith Simulant-Based All-3D-Printed Triboelectric Nanogenerator for Effective Mechanical Energy Conversion.
  Sustained human activity on the Moon will require energy systems that can be manufactured directly from lunar materials, avoiding the mass and cost constraints of transporting devices from the Earth. Here, we demonstrate a triboelectric nanogenerator (TENG) fa…
  europepmc 2026 置信度 0.80
• Extraterrestrial regolith is hemostatic and potentially suitable for hemorrhage control in space.
  Background Long-duration space missions beyond low Earth orbit pose increased risks of injuries to astronauts. Traumatic hemorrhage will be a cause of preventable death. Due to payload constraints, in situ production of medical materials is essential. Regolith…
  europepmc Nabil Ali-Mohamad, Ting-Hsuan Wang, Lih Jiin Juang, Nuoya Peng 等 2026 置信度 0.80 RegolithExtraterrestrial lifeAstrobiologySpace (punctuation)Coagulation
• Plasma nitrogen fixation for future lunar agriculture.
  Here, we introduce the potential of plasma technology for future lunar agriculture. The use of discharge plasma to convert nitrogen, oxygen, and water into reactive species for nitrogen fixation is discussed. This study demonstrated the effectiveness of dinitr…
  europepmc 2026 置信度 0.80
• A universal scaling framework for granular asteroid strength and its application to the surface of asteroid Bennu.
  Granular asteroids exhibit surprising structural stability despite low gravity and high spin rates. Understanding the mechanisms behind their strength is essential for predicting their evolution and informing deflection strategies. Using 3D particle-dynamics s…
  europepmc 2026 置信度 0.80
• Regolith-supported biofabrication: 3D bioprinting of living, photosynthetically active structures using Lunar and Martian regolith simulants.
  Bioprinting, a technology with the potential to support long-term space missions, offers medical solutions for human settlements on the Moon and Mars. Moreover, 'green bioprinting' presents a promising approach to address terrestrial environmental challenges. …
  europepmc 2025 置信度 0.80
• KREEP materials recorded in impact glasses of Chang'e-6 regolith returned from the South Pole-Aitken Basin.
  The Chang'e-6 mission achieved the first-ever sample return from the lunar farside. The landing site is located within the South Pole-Aitken (SPA) basin, which is the largest and oldest impact structure on the Moon. In this study, approximately 2360 glass bead…
  europepmc 2026 置信度 0.80
• Emerging Chemical and Biological Materials Technologies in the Extraplanetary Environment.
  Space exploration and manufacturing are of critical importance for scientific advancement, technological innovation, national security, and the acquisition of extraterrestrial resources. In view of this, chemical and biological nano-/micro-/meso-scale manufact…
  europepmc 2026 置信度 0.80
• EAC-1A: A novel large-volume lunar regolith simulant.
  The European Astronaut Centre (EAC) is currently constructing the European Lunar Exploration Laboratory (LUNA), a large training and operations facility to be located adjacent to EAC at the DLR (German Aerospace Centre) campus in Cologne, Germany. With an esti…
  europepmc 2020 置信度 0.80
• Predicting residual friction angle of lunar regolith based on Chang'e-5 lunar samples.
  With the rapid development of human lunar exploration projects, the lunar base establishment and resource utilization are on the way, and hence it is urgent and significant to reasonably predict engineering properties of the lunar regolith, which remains to be…
  europepmc 2023 置信度 0.80
• Plants grown in Apollo lunar regolith present stress-associated transcriptomes that inform prospects for lunar exploration.
  The extent to which plants can enhance human life support on other worlds depends on the ability of plants to thrive in extraterrestrial environments using in-situ resources. Using samples from Apollo 11, 12, and 17, we show that the terrestrial plant Arabidop…
  europepmc Anna‐Lisa Paul, S. M. Elardo, Robert J. Ferl 2022 置信度 0.80 RegolithAstrobiologyLunar soilIcy moonApollo
• Untangling the formation and liberation of water in the lunar regolith.
  The source of water (H 2 O) and hydroxyl radicals (OH), identified on the lunar surface, represents a fundamental, unsolved puzzle. The interaction of solar-wind protons with silicates and oxides has been proposed as a key mechanism, but laboratory experiments…
  europepmc 2019 置信度 0.80
• The lunar regolith - Comparative chemistry of the Apollo sites
  In a grain-size study of various sections of the Apollo 17 drill core conducted by Laul et al. (1978, 1979), it was found that the fine fractions were consistently more enriched in highland material than the coarse fractions. Relative to the coarse fractions, …
  openalex J. C. Laul, J. J. Papike 1980-01-01 置信度 0.72 RegolithLunar soilSoil waterApolloGeology
• Synthesis and characterization of geopolymer from lunar regolith simulant based on natural volcanic scoria
  In this study, a new GVS (Ground Volcanic Scoria) lunar regolith simulant was produced. The similarity between GVS and lunar soil was proved by comparison with Apollo lunar soil samples and other commercial lunar soil simulants. Then, GVS lunar regolith simula…
  openalex Siqi Zhou, Xingyi Zhu, Chenghong Lu, Feng Li 2020-06-27 置信度 0.72 RegolithGeopolymerMaterials scienceCompressive strengthLunar soil
• Sintering of lunar regolith structures fabricated via digital light processing
  openalex Rui Dou, Weizhe Tang, Li Wang, Shan Li 等 2019-05-25 置信度 0.72 RegolithSinteringMaterials scienceMicrostructurePhase (matter)
• Comparison of Dielectric Properties and Structure of Lunar Regolith at Chang'e‐3 and Chang'e‐4 Landing Sites Revealed by Ground‐Penetrating Radar
  Abstract On 3 January 2019, the Chang'e‐4 (CE‐4) touched down on the Von Karman crater located inside the South Pole‐Aitken Basin, providing for the first time the opportunity for in situ measurements of the lunar regolith at the farside of the Moon. The CE‐4 …
  openalex Jialong Lai, Yi Xu, Xiaoping Zhang, Long Xiao 等 2019-10-23 置信度 0.72 RegolithEjectaGeologyImpact craterSpace weathering
• Monte Carlo calculations of lunar Regolith thickness distributions
  openalex V. R. Oberbeck, W. L. Quaide, M. Mahan, Joel A. Paulson 1973-05-01 置信度 0.72 RegolithImpact craterMonte Carlo methodGeologyAstrobiology
• The regolith properties of the Chang'e-5 landing region and the ground drilling experiments using lunar regolith simulants
  openalex Yuqi Qian, Long Xiao, Shen Yin, Ming Zhang 等 2019-11-01 置信度 0.72 RegolithLunar soilLunar mareGeologySpace weathering
• Regolith-based additive manufacturing for sustainable development of lunar infrastructure – An overview
  openalex Maxim Isachenkov, Svyatoslav Chugunov, Iskander Akhatov, Igor Shishkovsky 2021-01-10 置信度 0.72 Regolith3D printingResource (disambiguation)AstrobiologyEarth science
• Some compositional aspects of lunar regolith evolution
  Abstract This paper discusses the compositional aspects of the lunar regolith in terms of regolith dynamics. Emphasis is placed on problems concerning lateral movement and mixing of soil components in response to meteoroid bombardment, and on the source of app…
  openalex J. M. Rhodes 1977-03-31 置信度 0.72 RegolithBasaltGeologyMeteoroidLunar soil
• The technology of lunar regolith environment construction on Earth
  openalex Tao Zhang, Chaoyue Chao, Zhixiao Yao, Kun Xu 等 2020-09-07 置信度 0.72 RegolithAstrobiologyEarth scienceLunar orbitLunar soil
• Laser melting manufacturing of large elements of lunar regolith simulant for paving on the Moon.
  The next steps for the expansion of the human presence in the solar system will be taken on the Moon. However, due to the low lunar gravity, the suspended dust generated when lunar rovers move across the lunar soil is a significant risk for lunar missions as i…
  europepmc 2023 置信度 0.80
• Manufacture of glass and mirrors from lunar regolith simulant
  Future planetary surface missions to the Moon or Mars, for example, can be augmented by the use of local materials, in order to reduce launch mass and expand mission capability. Using lunar regolith simulant and heating it within a susceptor-assisted microwave…
  openalex Juergen Schleppi, J. J. Gibbons, Alexander Groetsch, Jim Buckman 等 2018-11-19 置信度 0.72 RegolithMaterials sciencePolishingLunar mareAstrobiology
• Determining the feasible conditions for processing lunar regolith simulant via laser powder bed fusion
  openalex Leonardo Caprio, Ali Gökhan Demir, Barbara Previtali, Bianca Maria Colosimo 2019-12-31 置信度 0.72 Materials scienceRaw materialRegolithFusionDeposition (geology)
• Global Regolith Thermophysical Properties of the Moon From the Diviner Lunar Radiometer Experiment
  Abstract We used infrared data from the Lunar Reconnaissance Orbiter (LRO) Diviner Lunar Radiometer Experiment to globally map thermophysical properties of the Moon's regolith fines layer. Thermal conductivity varies from 7.4 × 10 −4 W m −1 K −1 at the surface…
  openalex Paul O. Hayne, Joshua L. Bandfield, Matthew A. Siegler, Ashwin R. Vasavada 等 2017-11-01 置信度 0.72 RegolithThermal inertiaImpact craterThermal conductivityRadiometer
• Lunar regolith thermal behavior revealed by Chang'E-1 microwave brightness temperature data
  openalex K. L. Chan, K. T. Tsang, Bruce Kong, Yongchun Zheng 2010-05-11 置信度 0.72 RegolithBrightness temperatureGeologyOrbiterBrightness
• Use of lunar regolith as a substrate for plant growth
  openalex D. W. Ming, D. L. Henninger 1994-11-01 置信度 0.72 RegolithEnvironmental scienceAstrobiologyNutrientSoil water
• Drilling forces model for lunar regolith exploration and experimental validation
  openalex Tao Zhang, Xilun Ding 2016-11-29 置信度 0.72 RegolithDrillLunar soilDrillingTorque
• Parameters and structure of lunar regolith in Chang'E-3 landing area from lunar penetrating radar (LPR) data
  openalex Zehua Dong, Guangyou Fang, Yicai Ji, Yunze Gao 等 2016-09-22 置信度 0.72 RegolithGeologyLunar mareRadarAstrobiology
• Lunar Regolith Simulant User's Guide
  Based on primary characteristics, currently or recently available lunar regolith simulants are discussed from the perspective of potential experimental uses. The characteristics used are inherent properties of the material rather than their responses to behavi…
  openalex Christian Schrader, Alabama D. L. Rickman, Carole McLemore, John Fikes 2010-09-01 置信度 0.72 RegolithAstrobiologyParticle (ecology)Lunar soilPerspective (graphical)
• Preparation of geopolymer based on lunar regolith simulant at in-situ lunar temperature and its durability under lunar high and cryogenic temperature
  openalex Rongrong Zhang, Siqi Zhou, Feng Li 2021-12-11 置信度 0.72 RegolithGeopolymerMaterials scienceCompressive strengthFlexural strength
• Solar wind record in the lunar regolith - Nitrogen and noble gases
  The measured elemental and isotopic abundances of noble gases and nitrogen have been measured in five different samples of lunar regolith material. It was found noble gases liberated by chemical attack on grain surfaces from two of the samples were solar. The …
  openalex U. Frick, R. H. Becker, Robert O. Pepin 1988-01-01 置信度 0.72 RegolithNoble gasAstrobiologyNitrogenSolar wind
• Properties of Lunar Regolith on the Moon's Farside Unveiled by Chang'E‐4 Lunar Penetrating Radar
  Abstract The complex thermal history of the Moon leads to an unequal distribution of volcanic products between the lunar nearside and the farside. So far, no lunar materials have been sampled from the Moon's farside and no detailed properties of lunar regolith…
  openalex Zehua Dong, Guangyou Fang, Bin Zhou, Di Zhao 等 2021-05-22 置信度 0.72 RegolithImpact craterGeologyAstrobiologyRadar
• Lunar surface rock abundance and regolith fines temperatures derived from LRO Diviner Radiometer data
  [1] Surface temperatures derived from thermal infrared measurements provide a means of understanding the physical properties of the lunar surface. The contrasting thermophysical properties between rocks and regolith fines cause multiple temperatures to be pres…
  openalex J. L. Bandfield, R. R. Ghent, A. R. Vasavada, D. A. Paige 等 2011-08-05 置信度 0.72 RegolithAbundance (ecology)GeologyRadiometerAstrobiology
• Long‐term compositional variation in solar corpuscular radiation: Evidence from nitrogen isotopes in the lunar regolith
  Implantation of solar corpuscular radiation into the lunar surface generates a population of solar atoms in the rims of lunar regolith grains. Laboratory analysis of those atoms can yield a measure of solar composition. Nitrogen trapped in the lunar regolith c…
  openalex J. F. Kerridge 1993-11-01 置信度 0.72 RegolithNoble gasSolar energetic particlesAstrobiologySolar System
• Simulation of the Lunar Regolith and Lunar-Penetrating Radar Data Processing
  Lunar-penetrating radar (LPR) was conducted by the “Yutu” rover of China's Chang-E 3 lunar mission to study the shallow subsurface of the Moon. Both regolith modeling and numerical simulation can provide a reliable reference for data processing of the Moon. In…
  openalex Ling Zhang, Zhaofa Zeng, Jing Li, Jingyi Lin 等 2018-01-17 置信度 0.72 RegolithTerrainGeologyRadarMoon landing
• Two‐dimensional distribution of volatiles in the lunar regolith from space weathering simulations
  We present simulations of space weathering effects on ice deposits in regions of permanent shadow on the Moon. These Monte Carlo simulations follow the effects of space weathering processes on the distribution of the volatiles over time. The model output const…
  openalex D. M. Hurley, D. J. Lawrence, D. Benjamin J. Bussey, R. R. Vondrak 等 2012-04-11 置信度 0.72 Space weatheringRegolithGeologyWeatheringIce sheet
• Multispectral polarimetry as a tool to investigate texture and chemistry of lunar regolith particles
  openalex Yuriy Shkuratov, Nikolay Opanasenko, Evgenij Zubko, Yevgen Grynko 等 2006-12-13 置信度 0.72 RegolithPolarization (electrochemistry)PhysicsAsteroidPolarimetry
• JSC-1: A New Lunar Regolith Simulant
  Simulants of lunar rocks and soils with appropriate properties, although difficult to produce in some cases, will be essential to meeting the system requirements for lunar exploration. In order to address this need a new lunar regolith simulant, JSC-1, has bee…
  openalex D. S. McKay, James L. Carter, Walter W. Boles, Carlton C. Allen 等 1993-01-01 置信度 0.72 RegolithLunar soilBasaltGeology of the MoonLunar mare
• Three dimensional shape analysis of JSC-1A simulated lunar regolith particles
  openalex Edward J. Garboczi 2010-10-26 置信度 0.72 Particle (ecology)Materials scienceParticle sizeRegolithSpherical harmonics
• Science from the Moon: The NASA/NLSI Lunar University Network for Astrophysics Research (LUNAR)
  The Moon is a unique platform for fundamental astrophysical measurements of gravitation, the Sun, and the Universe. Lacking a permanent ionosphere and, on the farside, shielded from terrestrial radio emissions, a radio telescope on the Moon will be an unparall…
  arxiv Jack O. Burns, the LUNAR Consortium 2009-09-08T15:40:04Z 置信度 0.78 astro-ph.IMastro-ph.COastro-ph.SR
• Rheological Lunar Regolith Simulants
  Regolith simulants are essential for space research and technology development. Yet, their physical properties often differ from those of true planetary soil, particularly when compared to regolith properties in-situ, that experience notably reduced gravity. W…
  arxiv Léonie Gasteiner, Alyona Glazyrina, Naomi Murdoch, Olfa D'Angelo 2025-10-27T14:04:10Z 置信度 0.78 astro-ph.EPcond-mat.soft
• Experiments Indicate Regolith is Looser in the Lunar Polar Regions than at the Lunar Landing Sites
  Since the Apollo program or earlier it has been widely believed that the lunar regolith was compacted through vibrations including nearby impact events, thermal stress release in the regolith, deep moon quakes, and shallow moon quakes. Experiments have shown t…
  arxiv Philip T. Metzger, Seamus Anderson, Anthony Colaprete 2018-01-17T17:01:35Z 置信度 0.78 astro-ph.EPcond-mat.soft
• Lunar-G2R: Geometry-to-Reflectance Learning for High-Fidelity Lunar BRDF Estimation
  We address the problem of estimating realistic, spatially varying reflectance for complex planetary surfaces such as the lunar regolith, which is critical for high-fidelity rendering and vision-based navigation. Existing lunar rendering pipelines rely on simpl…
  arxiv Clementine Grethen, Nicolas Menga, Roland Brochard, Geraldine Morin 等 2026-01-15T14:39:25Z 置信度 0.78 cs.CV
• An Open Database of Lunar Regolith and Simulants Properties
  Lunar regolith, the layer of unconsolidated material covering the Moon's surface, is central to the science and technology developed for the Moon, notably related to in-situ science investigations, resource utilization, surface infrastructure, and mobility sys…
  arxiv Léonie Gasteiner, Naomi Murdoch, Olfa D'Angelo 2026-02-03T18:44:32Z 置信度 0.78 astro-ph.EPastro-ph.IMphysics.space-ph
• Astrophysics Conducted by the Lunar University Network for Astrophysics Research (LUNAR) and the Center for Lunar Origins (CLOE)
  [Abridged] The Moon is a unique platform from and on which to conduct astrophysical measurements. The Lunar University Network for Astrophysics Research (LUNAR) and the Center for Lunar Origins and Evolution (CLOE) teams within the NASA Lunar Science Institute…
  arxiv Jack O. Burns, T. Joseph W. Lazio, William Bottke 2012-09-11T06:17:38Z 置信度 0.78 astro-ph.COastro-ph.EPastro-ph.IM
• Additive Manufacturing of Lunar Regolith for Reconfigurable Building Blocks toward Lunar Habitation
  Utilizing locally available materials is a crucial step towards sustainable planetary habitation. Lunar regolith has gained tremendous interest in additive manufacturing in the past decades. However, due to the constrained manufacturing facilities and material…
  arxiv Cole McCallum, Youwen Liang, Nahid Tushar, Ben Xu 等 2025-06-05T17:28:31Z 置信度 0.78 astro-ph.IMastro-ph.EPcond-mat.other
• Physicochemical properties of lunar regolith simulant for in situ oxygen production
  Permanent lunar settlements will rely on in situ oxygen production from regolith for life support and propulsion. While oxygen is abundant in lunar materials, it is chemically bound within metal oxides whose extractability depends strongly on regolith composit…
  arxiv Alyssa Ang De Guzman, Anish Mathai Varghese, Saif Alshalloudi, Lance Kosca 等 2026-01-21T07:19:10Z 置信度 0.78 physics.space-phcond-mat.mtrl-sci
• Additive Manufacturing of PEEK/Lunar Regolith Composites for Sustainable Lunar Manufacturing
  As humanity advances toward long-term lunar presence under NASA's Artemis program, the development of lunar-based manufacturing and construction (LBMC) capabilities has become increasingly critical. The high cost of transporting materials from Earth makes in-s…
  arxiv Mohammad Azami, Pierre-Lucas Aubin-Fournier, Mehdi Hojjati, Krzysztof Skonieczny 2025-07-27T16:54:02Z 置信度 0.78 astro-ph.IMastro-ph.EPcond-mat.mtrl-sci
• Lunar neutrinos
  Cosmic rays bombard the lunar surface producing mesons, which attenuate inside the regolith. They get slower and decay weakly into mostly sub-GeV neutrinos leaving the surface. Thus the Moon shines in neutrinos. Here we calculate spectra of low energy neutrino…
  arxiv S. Demidov, D. Gorbunov 2020-12-23T18:37:05Z 置信度 0.78 hep-phastro-ph.HE
• Effect of Sintering Temperature on Microstructure and Mechanical Properties of Molded Martian and Lunar Regolith
  Cylindrical specimens of Martian and Lunar regolith simulants were molded using a salt water binder and sintered at various temperatures for comparing microstructure, mechanical properties and shrinkage. Material microstructure are reported using optical micro…
  arxiv Peter Warren, Nandhini Raju, Hossein Ebrahimi, Milos Krsmanovic 等 2022-05-13T19:00:48Z 置信度 0.78 cond-mat.mtrl-sci
• Lunar Outgassing, Transient Phenomena & the Return to the Moon, II: Predictions and Tests for Outgassing/Regolith Interactions
  We follow Paper I with predictions of how gas leaking through the lunar surface could influence the regolith, as might be observed via optical Transient Lunar Phenomena (TLPs) and related effects. We touch on several processes, but concentrate on low and high …
  arxiv Arlin P. S. Crotts, Cameron Hummels 2009-09-21T18:21:53Z 置信度 0.78 astro-ph.EP
• Lunar Palaeoregolith Deposits as Recorders of the Galactic Environment of the Solar System and Implications for Astrobiology
  One of the principal scientific reasons for wanting to resume in situ exploration of the lunar surface is to gain access to the record it contains of early Solar System history. Part of this record will pertain to the galactic environment of the Solar System, …
  arxiv Ian A. Crawford, Sarah A. Fagents, Katherine H. Joy, M. Elise Rumpf 2010-08-24T12:26:21Z 置信度 0.78 astro-ph.EP
• Lunar Outgassing, Transient Phenomena and The Return to The Moon, II: Predictions for Interactions between Outgassing and Regolith
  We consider the implications from Paper I on how gas leaking through the lunar surface might interact with the regolith, and in what respects this might affect or cause the appearance of optical Transient Lunar Phenomena (TLPs). We consider briefly a range of …
  arxiv Arlin P. S. Crotts, Cameron Hummels 2007-06-27T03:48:47Z 置信度 0.78 astro-ph
• Dielectric properties and stratigraphy of regolith in the lunar South Pole-Aitken basin: Observations from the Lunar Penetrating Radar
  We examine data obtained by the Lunar Penetrating Radar (LPR) onboard the Chang'E-4 (CE-4) mission to study the dielectric properties and stratigraphy of lunar regolith on the far side of the Moon. The data collected from January 2019 to September 2020 were pr…
  arxiv Jianqing Feng, Matthew. A. Siegler, Mackenzie N. White 2022-03-06T00:17:33Z 置信度 0.78 astro-ph.EPphysics.geo-ph
• Cohesion and Shear Strength of Compacted Lunar and Martian Regolith Simulants
  Shear strength and cohesion of granular materials are important geotechnical properties that play a crucial role in the stability and behavior of lunar and Martian regolith, as well as their terrestrial analog materials. To characterize and predict shear stren…
  arxiv B. Dotson, D. Sanchez Valencia, C. Millwater, P. Easter 等 2024-03-16T22:20:03Z 置信度 0.78 physics.space-phastro-ph.EP
• Contribution of cosmic alphas to generation of albedo neutrons and gammas in lunar regolith: A computational study based on GEANT4 simulations
  The lunar surface is constantly and directly exposed to Galactic Cosmic Rays (GCRs) due to the lack of the atmosphere and the magnetic field around it. The high-energetic alpha particles subsequently contribute to the generation of the secondary neutrons throu…
  arxiv Harshala Gaonkar, A. Ilker Topuz 2026-07-15T12:25:36Z 置信度 0.78 physics.ins-detastro-ph.HE
• Thermal Extraction of Volatiles from Lunar and Asteroid Regolith in Axisymmetric Crank-Nicholson Modeling
  A physics-based computer model has been developed to support the development of volatile extraction from regolith of the Moon and asteroids. The model is based upon empirical data sets for extraterrestrial soils and simulants, including thermal conductivity of…
  arxiv Philip T. Metzger, Kris Zacny, Phillip Morrison 2023-06-06T15:33:02Z 置信度 0.78 astro-ph.EPphysics.app-phphysics.space-ph
• Radio astronomy with the Lunar Lander: opening up the last unexplored frequency regime
  The active broadband (1 kHz-100 MHz) tripole antenna now envisaged to be placed on the European Lunar Lander located at the Lunar South Pole allows for sensitive measurements of the exosphere and ionosphere, and their interaction with the Earths magnetosphere,…
  arxiv Marc Klein Wolt, Amin Aminaei, Philippe Zarka, Jan-Rutger Schrader 等 2012-09-13T20:40:21Z 置信度 0.78 astro-ph.IM
• Gardening on the Moon: An Advection-Diffusion Model to Guide the Search for Supernova Debris in the Lunar Regolith
  The vertical redistribution of materials in the lunar regolith - ranging from continuously produced space-weathering products to sporadic pulses of supernova- or kilonova-derived isotopes - remains a fundamental problem in planetary science. We present a unifi…
  arxiv Emily S. Costello, John Ellis, Brian D. Fields, Rebecca Surman 等 2026-04-10T17:44:35Z 置信度 0.78 astro-ph.EPastro-ph.HEastro-ph.IM
• Back to the Moon: The Scientific Rationale for Resuming Lunar Surface Exploration
  The lunar geological record has much to tell us about the earliest history of the Solar System, the origin and evolution of the Earth-Moon system, the geological evolution of rocky planets, and the near-Earth cosmic environment throughout Solar System history.…
  arxiv I. A. Crawford, M. Anand, C. S. Cockell, H. Falcke 等 2012-06-04T20:04:47Z 置信度 0.78 astro-ph.EPastro-ph.IM
• Synthetic space bricks from lunar and martian regolith via sintering
  The prospect of establishing extra-terrestrial habitats using in situ resource utilization (ISRU) constitutes a long-term goal of multiple space agencies around the world. In this work, we investigate sintering as a potential route for making building blocks -…
  arxiv Nitin Gupta, Vineet Dawara, Aloke Kumar, Koushik Viswanathan 2023-08-28T06:19:06Z 置信度 0.78 physics.app-phcond-mat.mtrl-sci
• Comparison of two laser wavelengths for LIBS bioimaging of plants grown in lunar regolith
  The colonisation of extraterrestrial planets requires sustainable food production independent of Earth-based supplies. Due to the high costs and complicated logistics of food transport, in-situ cultivation will be essential. Growing plants directly in regolith…
  arxiv T. Vozár, L. Čechová, J. Buday, M. Füleky 等 2026-04-30T14:41:02Z 置信度 0.78 physics.opticsphysics.app-ph
• A Critical Review of the Lunar Laser Ranging
  This paper provides an overview of the Lunar Laser Ranging (LLR) experiments. The measurement principle is explained and its theory is derived. Both contributions, the direct reflected light from retroreflectors as well as the scattered light from the lunar su…
  arxiv Andreas Märki 2018-05-15T15:54:50Z 置信度 0.78 astro-ph.IM
• Moon's Radiation Environment and Expected Performance of Solar Cells during Future Lunar Missions
  Several lunar missions are planned ahead and there is an increasing demand for efficient photovoltaic power generation in the moon. The knowledge of solar cell operation in the lunar surface obtained during early seventies need to be updated considering curren…
  arxiv T. E Girish, S Aranya 2010-12-03T12:31:41Z 置信度 0.78 physics.gen-ph
• Was the Sun a Slow Rotator? -- Sodium and Potassium Constraints from the Lunar Regolith
  While the Earth and Moon are generally similar in composition, a notable difference between the two is the apparent depletion in moderately volatile elements in lunar samples. This is often attributed to the formation process of the Moon and demonstrates the i…
  arxiv Prabal Saxena, Rosemary M. Killen, Vladimir Airapetian, Noah E. Petro 等 2019-06-13T18:56:37Z 置信度 0.78 astro-ph.EPastro-ph.SR
• Terrestrial atmospheric ion implantation occurred in the nearside lunar regolith during the history of Earth's dynamo
  Light volatile elements in lunar regolith are thought to be a mixture of the solar wind and Earth's atmosphere, the latter sourced in the absence of geomagnetic field. However, the extent to which both the current and primitive geodynamo influence the transpor…
  arxiv Shubhonkar Paramanick, Eric G. Blackman, John A. Tarduno, Jonathan Carroll-Nellenback 2024-11-30T15:58:48Z 置信度 0.78 astro-ph.EPastro-ph.SRphysics.geo-phphysics.space-ph
• Completion of Lunar Magma Ocean Solidification at 4.43 Ga
  Crystallization of the lunar magma ocean yielded a chemically unique liquid residuum named KREEP. This component is expressed as a large patch on the near side of the Moon, and a possible smaller patch in the northwest portion of the Moon's South Pole-Aitken b…
  arxiv Nicolas Dauphas, Zhe J. Zhang, Xi Chen, Mélanie Barboni 等 2025-01-27T16:56:11Z 置信度 0.78 astro-ph.EPphysics.geo-ph
• SELENA: Semi-analytical Integrator for Lunar Artificial Satellites
  The present report summarizes the main theory and implementation steps associated with SELENA (SEmi-anaLytical intEgrator for a luNar Artificial satellite), i.e. the semi-analytical propagator for lunar satellite orbits developed in the framework of the the R&…
  arxiv Christos Efthymiopoulos, Kleomenis Tsiganis, Ioannis Gkolias, Michalis Gaitanas 等 2023-09-21T09:15:54Z 置信度 0.78 astro-ph.EPastro-ph.IM
• Benchmarking Universal Machine Learning Force Fields for Molecular Dynamics of Lunar Regolith Minerals
  Universal machine-learning interatomic potentials provide a promising route for accelerating molecular dynamics simulations of materials, but their transferability to lunar regolith-relevant silicates, oxides, and hydrogen-bearing surface species remains eluci…
  arxiv Ziyu Huang, Ken-ichi Nomura 2026-07-10T00:19:43Z 置信度 0.78 physics.geo-ph
• Characterizing the Radio Quiet Region Behind the Lunar Farside for Low Radio Frequency Experiments
  Low radio frequency experiments performed on Earth are contaminated by both ionospheric effects and radio frequency interference (RFI) from Earth-based sources. The lunar farside provides a unique environment above the ionosphere where RFI is heavily attenuate…
  arxiv Neil Bassett, David Rapetti, Jack O. Burns, Keith Tauscher 等 2020-03-06T23:44:04Z 置信度 0.78 astro-ph.IMastro-ph.EP
• Equilibration in the Aftermath of the Lunar-Forming Giant Impact
  Simulations of the moon-forming impact suggest that most of the lunar material derives from the impactor rather than the Earth. Measurements of lunar samples, however, reveal an oxygen isotope composition that is indistinguishable from terrestrial samples, and…
  arxiv Kaveh Pahlevan, David Stevenson 2010-12-24T00:02:06Z 置信度 0.78 astro-ph.EP
• Is there a semi-molten layer at the base of the lunar mantle?
  Parameterised by the Love number $k_2$ and the tidal quality factor $Q$, and inferred from lunar laser ranging (LLR), tidal dissipation in the Moon follows an unexpected frequency dependence often interpreted as evidence for a highly dissipative, melt-bearing …
  arxiv Michaela Walterová, Marie Běhounková, Michael Efroimsky 2023-01-06T12:22:41Z 置信度 0.78 astro-ph.EP
• Physiological and Transcriptional Responses of Arabidopsis thaliana to Simulated Lunar and Martian Regolith Substrates
  The integration of plant-based bioregenerative life support systems is a central objective in NASA's Moon to Mars strategy. Arabidopsis thaliana, a model organism with extensive genomic resources, serves as a key species to investigate plant resilience in extr…
  arxiv A'nya Buckner, Sarah Lang, Rafael Loureiro 2025-05-19T16:40:43Z 置信度 0.78 q-bio.QM
• Variable Emissivity Modeling for Sustainable Lunar Surface Habitats
  Lunar habitats will be one of the first platforms to enable long-term human presence beyond Low Earth Orbit. These structures act as a stepping stone for exploring our solar system while simultaneously enabling lunar resource utilization, low-energy cryopreser…
  arxiv S. Keller, S. Stewart, S. Taylor, O. Ilic 2026-07-26T14:32:34Z 置信度 0.78 physics.app-phphysics.comp-ph
• Micron-Scale Technosignatures: How a Cubic Metre of Lunar Regolith May Begin to Constrain the Number of Past Technological Civilisations in the Galaxy
  Building on Arkhipov's proposal that technogenic artefacts may survive natural interstellar transport and accumulate on airless Solar System bodies, we examine the prospects for identifying micron-scale engineered particulate material within the lunar regolith…
  arxiv Lewis J. Pinault, Brian C. Lacki, Ian A. Crawford, Andrew P. V. Siemion 2026-06-23T00:07:50Z 置信度 0.78 astro-ph.EP
• Model for Asteroid Regolith to Guide Simulant Development
  When creating asteroid regolith simulant, it is necessary to have a model of asteroid regolith to guide and to evaluate the simulant. We created a model through evaluation and synthesis of the available data sets including (1) the returned sample from Itokawa …
  arxiv Philip T. Metzger, Daniel T. Britt 2019-12-23T04:57:22Z 置信度 0.78 astro-ph.EPastro-ph.IMcond-mat.stat-mech
• Observing the Earth as an exoplanet with LOUPE, the Lunar Observatory for Unresolved Polarimetry of Earth
  The detections of small, rocky exoplanets have surged in recent years and will likely continue to do so. To know whether a rocky exoplanet is habitable, we have to characterise its atmosphere and surface. A promising characterisation method for rocky exoplanet…
  arxiv T. Karalidi, D. M. Stam, F. Snik, S. Bagnulo 等 2012-03-01T15:05:46Z 置信度 0.78 astro-ph.EPastro-ph.IM
• A Lunar Farside Low Radio Frequency Array for Dark Ages 21-cm Cosmology
  An array of low-frequency dipole antennas on the lunar farside surface will probe a unique, unexplored epoch in the early Universe called the Dark Ages. It begins at Recombination when neutral hydrogen atoms formed, first revealed by the cosmic microwave backg…
  arxiv Jack Burns, Gregg Hallinan, Tzu-Ching Chang, Marin Anderson 等 2021-03-15T18:05:17Z 置信度 0.78 astro-ph.IMastro-ph.COhep-ex
• Lunar Imaging and Ionospheric Calibration for the Lunar Cherenkov Technique
  The Lunar Cherenkov technique is a promising method for UHE neutrino and cosmic ray detection which aims to detect nanosecond radio pulses produced during particle interactions in the Lunar regolith. For low frequency experiments, such as NuMoon, the frequency…
  arxiv Rebecca McFadden, Olaf Scholten, Maaijke Mevius 2013-06-03T11:02:00Z 置信度 0.78 astro-ph.IMastro-ph.HE
• The role of breccia lenses in regolith generation from the formation of small, simple craters: Application to the Apollo 15 landing site
  Impact cratering is likely a primary agent of regolith generation on airless bodies. Regolith production via impact cratering has long been a key topic of study since the Apollo era. The evolution of regolith due to impact cratering, however, is not well under…
  arxiv M. Hirabayashi, B. A. Howl, C. I. Fassett, J. M. Soderblom 等 2018-02-10T23:17:04Z 置信度 0.78 astro-ph.EP
• Extremely high reflection of solar wind protons as neutral hydrogen atoms from regolith in space
  We report on measurements of extremely high reflection rates of solar wind particles from regolith-covered lunar surfaces. Measurements by the Sub-keV Atom Reflecting Analyzer (SARA) instrument on the Indian Chandrayaan-1 spacecraft in orbit around the Moon sh…
  arxiv Martin Wieser, Stas Barabash, Yoshifumi Futaana, Mats Holmström 等 2010-12-14T09:31:31Z 置信度 0.78 astro-ph.EPphysics.plasm-phphysics.space-ph
• Formation of Lunar Swirls
  In this paper we show a plausible mechanism that could lead to the formation of the Dark Lanes in Lunar Swirls, and the electromagnetic shielding of the lunar surface that results in the preservation of the white colour of the lunar regolith. We present the re…
  arxiv R. A. Bamford, E. P. Alves, F. Cruz, B. J. Kellett 等 2015-05-23T10:22:15Z 置信度 0.78 astro-ph.EPphysics.space-ph
• Measuring the Fidelity of Asteroid Regolith and Cobble Simulants
  NASA has developed a "Figure of Merit" method to grade the fidelity of lunar simulants for scientific and engineering purposes. Here we extend the method to grade asteroid simulants, both regolith and cobble variety, and we apply the method to the newly develo…
  arxiv Philip T. Metzger, Daniel T. Britt, Stephen Covey, Cody Schultz 等 2019-12-23T05:17:04Z 置信度 0.78 astro-ph.EPastro-ph.IMcond-mat.stat-mech
• The stratification of regolith on celestial objects
  All atmosphere-less planetary bodies are covered with a dust layer, the so-called regolith, which determines the optical, mechanical and thermal properties of their surface. These properties depend on the regolith material, the size distribution of the particl…
  arxiv Rainer Schräpler, Jürgen Blum, Ingo von Borstel, Carsten Güttler 2015-05-12T09:24:22Z 置信度 0.78 astro-ph.EP
• Stick-slip dynamics in penetration experiments on simulated regolith
  The surfaces of many planetary bodies, including asteroids and small moons, are covered with dust to pebble-sized regolith held weakly to the surface by gravity and contact forces. Understanding the reaction of regolith to an external perturbation will allow f…
  arxiv Jack Featherstone, Robert Bullard, Tristan Emm, Anna Jackson 等 2020-11-25T17:14:50Z 置信度 0.78 astro-ph.EPcond-mat.soft
• Laboratory investigations of Lunar ice imaging in permanently shadowed regions using reflected starlight
  A proof of concept for a frost detection imager using reflected starlight is presented; the limitations of this technique are explored experimentally. An ice-covered lunar surface is simulated inside a vacuum chamber, which is then illuminated with a lamp cont…
  arxiv Paul J. Godin, Jacob L. Kloos, Alex Seguin, John E. Moores 2020-03-02T22:33:11Z 置信度 0.78 astro-ph.EPastro-ph.IM
• A new method to determine the grain size of planetary regolith
  Airless planetary bodies are covered by a dusty layer called regolith. The grain size of the regolith determines the temperature and the mechanical strength of the surface layers. Thus, knowledge of the grain size of planetary regolith helps to prepare future …
  arxiv Bastian Gundlach, Jürgen Blum 2012-12-13T10:11:48Z 置信度 0.78 astro-ph.EP
• Prospects of Probing the Radio Emission of Lunar UHECRv Events
  Radio detection of Ultra High Energetic Cosmic Rays and Neutrinos (UHECRv) which hit the Moon has been investigated in recent years. In preparation for near-future lunar science missions, we discuss technical requirements for radio experiments onboard lunar or…
  arxiv Amin Aminaei, Linjie Chen, Hamid R. Pourshaghaghi, Stijn Buitink 等 2018-08-07T10:02:49Z 置信度 0.78 astro-ph.IMastro-ph.HE