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• Lunar Ice Cube: first generation deep space CubeSat with compact broadband IR spectrometer development story
  Lunar Ice Cube (LIC) is one of 13 6U cubesats that will be deployed by EM1 in cislunar space. LIC along with Lunar Flashlight and LunaH-Map, all focused on the search for volatiles but with very different payloads, will be the first deep space cubesats designe…
  openalex P. E. Clark, B. Malphrus, Kevin Brown, Nathan Fite 等 2019-08-30 置信度 0.72 CubeSatBroadbandCube (algebra)SpectrometerNASA Deep Space Network
• Current Theories of Lunar Ice
  The classical theory of cold-trapped ice on the Moon and some modern theories are reviewed and compared with observational constraints. The "standard model" for lunar ice posits that ice has accumulated in polar cold traps after the spin axis orientation becam…
  arxiv Norbert Schorghofer 2025-02-09T22:24:40Z 置信度 0.78 astro-ph.EP
• A new perspective on interiors of ice-rich planets: Ice-rock mixture instead of ice on top of rock
  Ice-rich planets are formed exterior to the water ice-line and thus are expected to contain a substantial amount of ices. The high ice content leads to unique conditions in the interior, under which the structure of a planet is affected by ice interaction with…
  arxiv Allona Vazan, Re'em Sari, Ronit Kessel 2020-11-01T19:06:37Z 置信度 0.78 astro-ph.EPphysics.geo-ph
• Life in solid ice
  Some microbes appear to be able to metabolize in glacial ice or permafrost. The rate depends on temperature, nutrient level, and bioelement availability, among other factors. I have developed a plausible argument that they do this while confined in veins fille…
  arxiv P. Buford Price 2005-07-02T20:44:39Z 置信度 0.78 q-bio.PEq-bio.CB
• The Effect of Hole Ice on the Propagation and Detection of Light in IceCube
  IceCube is a neutrino observatory at Earth's South Pole that uses glacial ice as detector medium. Secondary particles from neutrino interactions produce Cherenkov light, which is detected by an array of photo detectors deployed within the ice. In distinction f…
  arxiv Sebastian Fiedlschuster 2019-04-17T16:22:36Z 置信度 0.78 physics.ins-dethep-ex
• Modelling the atomic structure of very high-density amorphous ice
  The structure of very high-density amorphous (VHDA) ice has been modelled by positionally disordering three crystalline phases, namely ice IV, VI and XII. These phases were chosen because only they are stable or metastable in the region of the ice phase diagra…
  arxiv J. K. Christie, M. Guthrie, C. A. Tulk, C. J. Benmore 等 2004-12-21T15:17:18Z 置信度 0.78 cond-mat.mtrl-scicond-mat.dis-nn
• Sea Ice Brightness Temperature as a Function of Ice Thickness, Part II: Computed curves for thermodynamically modelled ice profiles
  Ice thickness is an important variable for climate scientists and is still difficult to accurately determine from microwave radiometer measurements. There has been some success detecting the thickness of thin ice and with this in mind this study attempts to mo…
  arxiv Peter Mills 2012-02-29T15:07:38Z 置信度 0.78 physics.ao-ph
• A two layer model for wave dissipation in sea ice
  Sea ice is highly complex due to the inhomogeneity of the physical properties (e.g. temperature and salinity) as well as the permeability and mixture of water and a matrix of sea ice and/or sea ice crystals. Such complexity has proven itself to be difficult to…
  arxiv Graig Sutherland, Jean Rabault, Kai H. Christensen, Atle Jensen 2018-05-03T06:30:42Z 置信度 0.78 physics.ao-ph
• ICE: Intrinsic Concept Extraction from a Single Image via Diffusion Models
  The inherent ambiguity in defining visual concepts poses significant challenges for modern generative models, such as the diffusion-based Text-to-Image (T2I) models, in accurately learning concepts from a single image. Existing methods lack a systematic way to…
  arxiv Fernando Julio Cendra, Kai Han 2025-03-25T17:58:29Z 置信度 0.78 cs.CV
• A comparison of wave observations in the Arctic marginal ice zone with spectral models
  Increased economic activity and research interest in the Arctic raise the need for better wave forecasts in the marginal ice zone (MIZ). Mathematical and numerical models of wave propagation in sea ice would benefit from more in situ data for validation. This …
  arxiv Trygve K. Løken, Jean Rabault, Erin E. Thomas, Malte Müller 等 2020-03-20T19:20:33Z 置信度 0.78 physics.ao-ph
• An Ice Age JWST inventory of dense molecular cloud ices
  Icy grain mantles are the main reservoir of the volatile elements that link chemical processes in dark, interstellar clouds with the formation of planets and composition of their atmospheres. The initial ice composition is set in the cold, dense parts of molec…
  arxiv M. K. McClure, W. R. M. Rocha, K. M. Pontoppidan, N. Crouzet 等 2023-01-22T15:28:37Z 置信度 0.78 astro-ph.GAastro-ph.EPastro-ph.SR
• Using Scattered Near-Infrared Light to Map Water Ice in Prestellar Cores with SPHEREx
  We present the first coreshine-derived, spatially-resolved maps of the 3 $μ$m H$_2$O ice absorption feature in four prestellar cores, using SPHEREx spectra. Ices are a key component of dense cores in molecular clouds, playing a central role in the chemistry of…
  arxiv Tamojeet Roychowdhury, Jennifer B. Bergner, Jens Kauffmann, Thushara G. S. Pillai 等 2026-07-27T18:00:06Z 置信度 0.78 astro-ph.GA
• Experimental Studies of Artificial Spin Ice
  Artificial spin ices were originally introduced as analogs of the pyrochlore spin ices, but have since become a much richer field . The original attraction of building nanotechnological analogs of the pyrochlores were threefold: to allow room temperature studi…
  arxiv Christopher Marrows 2016-11-02T19:43:04Z 置信度 0.78 cond-mat.dis-nncond-mat.mtrl-sci
• Why could ice ages be unpredictable?
  It is commonly accepted that the variations of Earth's orbit and obliquity control the timing of Pleistocene glacial-interglacial cycles. Evidence comes from power spectrum analysis of palaeoclimate records and from inspection of the timing of glacial and degl…
  arxiv Michel Crucifix 2013-02-06T19:49:45Z 置信度 0.78 physics.geo-phnlin.CDphysics.ao-ph
• Regelation: why does ice melt under pressure?
  Unlike other unusual materials whose bonds contract under compression, the O:H nonbond undergoes contraction and the H-O bond elongation towards O:H and H-O length symmetry in water and ice. The energy drop of the H-O bond dictates the melting point Tm depress…
  arxiv Chang Q Sun 2015-01-28T03:34:30Z 置信度 0.78 cond-mat.softphysics.flu-dyn
• The Turkish Ice Cream Robot: Examining Playful Deception in Social Human-Robot Interactions
  Playful deception, a common feature in human social interactions, remains underexplored in Human-Robot Interaction (HRI). Inspired by the Turkish Ice Cream (TIC) vendor routine, we investigate how bounded, culturally familiar forms of deception influence user …
  arxiv Hyeonseong Kim, Roy El-Helou, Seungbeen Lee, Sungjoon Choi 等 2025-09-26T02:24:34Z 置信度 0.78 cs.ROcs.HC
• Transition in the Acid-Base Component of Surface Free Energy of Ice upon the Premelting of its Second Molecular Bilayer
  Molecular disordering of the ice surface occurs below the bulk melting temperature of 273 K, termed surface premelting. The top-most molecular layer begins gradually premelting at 200 K, and has been linked to its low coefficient of friction through an increas…
  arxiv Nathaniel Orndorf, Saranshu Singla, Ali Dhinojwala 2020-05-09T16:21:54Z 置信度 0.78 physics.chem-phcond-mat.soft
• Graph neural network for colliding particles with an application to sea ice floe modeling
  This paper introduces a novel approach to sea ice modeling using Graph Neural Networks (GNNs), utilizing the natural graph structure of sea ice, where nodes represent individual ice pieces, and edges model the physical interactions, including collisions. This …
  arxiv Ruibiao Zhu 2026-02-18T06:31:04Z 置信度 0.78 cs.LGcs.AIcs.CVphysics.comp-ph
• Ice Giant System Exploration in the 2020s: An Introduction
  The international planetary science community met in London in January 2020, united in the goal of realising the first dedicated robotic mission to the distant Ice Giants, Uranus and Neptune, as the only major class of Solar System planet yet to be comprehensi…
  arxiv L. N. Fletcher, A. A. Simon, M. D. Hofstadter, C. S. Arridge 等 2020-08-26T12:51:08Z 置信度 0.78 astro-ph.IMastro-ph.EP
• Impact crater morphology and the structure of Europa's ice shell
  We performed numerical simulations of impact crater formation on Europa to infer the thickness and structure of its ice shell. The simulations were performed using iSALE to test both the conductive ice shell over ocean and the conductive lid over warm convecti…
  arxiv Elizabeth A. Silber, Brandon C. Johnson 2017-11-24T14:51:03Z 置信度 0.78 astro-ph.EP
• Water ice at low to midlatitudes on Mars
  In this paper, we analyze water ice occurrences at the surface of Mars using near-infrared observations, and we study their distribution with a climate model. Latitudes between 45°S and 50°N are considered. Data from the Observatoire pour la Minéralogie, l'Eau…
  arxiv Mathieu Vincendon, François Forget, John Mustard 2011-03-01T17:08:27Z 置信度 0.78 astro-ph.EP
• 1I/'Oumuamua as an N2 ice fragment of an exo-pluto surface. II. Generation of N2 ice fragments and the origin of 'Oumuamua
  The origin of the interstellar object 1I/'Oumuamua, has defied explanation. In a companion paper (Jackson & Desch, 2021), we show that a body of N2 ice with axes 45 m x 44 m x 7.5 m at the time of observation would be consistent with its albedo, non-gravit…
  arxiv Steven J. Desch, Alan P. Jackson 2021-03-16T02:50:31Z 置信度 0.78 astro-ph.EP
• A Revised Description of the Cosmic Ray-Induced Desorption of Interstellar Ices
  Non-thermal desorption of ices on interstellar grains is required to explain observations of molecules that are not synthesized efficiently in the gas phase in cold dense clouds. Perhaps the most important non-thermal desorption mechanism is one induced by cos…
  arxiv O. Sipilä, K. Silsbee, P. Caselli 2021-06-08T18:00:01Z 置信度 0.78 astro-ph.GA
• Detecting extra-galactic supernova neutrinos in the Antarctic ice
  Building on the technological success of the IceCube neutrino telescope, we outline a prospective low-energy extension that utilizes the clear ice of the South Pole. Aiming at a 10 Mton effective volume and a 10 MeV threshold, the detector would provide suffic…
  arxiv Sebastian Böser, Marek Kowalski, Lukas Schulte, Nora Linn Strotjohann 等 2013-04-09T12:33:06Z 置信度 0.78 astro-ph.IMastro-ph.HEhep-exphysics.ins-det
• Hidden force floating ice
  Because of the segmental specific-heat disparity of the hydrogen bond (O:H-O) and the Coulomb repulsion between oxygen ions, cooling elongates the O:H-O bond at freezing by stretching its containing angle and shortening the H-O bond with an association of larg…
  arxiv Chang Q. Sun 2015-01-17T08:04:50Z 置信度 0.78 cond-mat.soft
• Near-tropical subsurface ice on Mars
  Near-surface perennial water ice on Mars has been previously inferred down to latitudes of about 45° and could result from either water vapor diffusion through the regolith under current conditions or previous ice ages precipitations. In this paper we show tha…
  arxiv Mathieu Vincendon, John Mustard, François Forget, Mikhail Kreslavsky 等 2011-03-02T09:50:31Z 置信度 0.78 astro-ph.EP
• Generalised Longitudinal Susceptibility for Magnetic Monopoles in Spin Ice
  The generalised longitudinal susceptibility $χ({\bf q}, ω)$ affords a sensitive measure of the spatial and temporal correlations of magnetic monopoles in spin ice. Starting with the monopole model, a mean field expression for $χ({\bf q}, ω)$ is derived as well…
  arxiv Steven T. Bramwell 2011-12-01T18:16:35Z 置信度 0.78 cond-mat.str-el
• Ice cream and orbifold Riemann-Roch
  We give an orbifold Riemann-Roch formula in closed form for the Hilbert series of a quasismooth polarized n-fold X,D, under the assumption that X is projectively Gorenstein with only isolated orbifold points. Our formula is a sum of parts each of which is inte…
  arxiv Anita Buckley, Miles Reid, Shengtian Zhou 2012-08-02T11:26:38Z 置信度 0.78 math.AG
• Classical-Quantum Mappings for Geometrically Frustrated Systems: Spin Ice in a [100] Field
  Certain classical statistical systems with strong local constraints are known to exhibit Coulomb phases, where long-range correlation functions have power-law forms. Continuous transitions from these into ordered phases cannot be described by a naive applicati…
  arxiv Stephen Powell, J. T. Chalker 2008-03-29T13:35:55Z 置信度 0.78 cond-mat.stat-mech
• Meteoroid Bombardment of Lunar Poles
  While the floors of deep lunar craters are largely shielded from solar radiation and thus provide an ideal thermal environment for water ice accumulation, meteoroids on highly inclined orbits can easily access permanently shadowed regions and alter the surface…
  arxiv Petr Pokorny, Menelaos Sarantos, Diego Janches, Erwan Mazarico 2020-03-27T21:22:53Z 置信度 0.78 astro-ph.EP
• Molecular dynamics simulations of ice and methane hydrate by means of the rotation coordinate TIP5P-Ewald model
  Molecular dynamics simulations are utilized to study the microwave heating of methane hydrate by the five-body rotation coordinate system with the TIP5P-Ewald model. The structure I of methane hydrate is constructed, and the ice and free methane or methane hyd…
  arxiv Motohiko Tanaka 2023-11-02T12:23:56Z 置信度 0.78 physics.chem-ph
• Formation of Water-rich Giant Planet Satellites at Decretion Disk Ice Lines
  The volatile budgets of giant planet satellites are critical to unraveling the origin of their building blocks within the circumplanetary disks that hosted them. The Galilean moons Ganymede and Callisto, as well as the Saturnian moon Titan, are known to be ano…
  arxiv Teng Ee Yap, David J. Stevenson 2026-02-24T22:11:29Z 置信度 0.78 astro-ph.EP
• Snow topography on undeformed Arctic sea ice captured by an idealized "snow dune" model
  Our ability to predict the future of Arctic sea ice is limited by ice's sensitivity to detailed surface conditions such as the distribution of snow and melt ponds. Snow on top of the ice decreases ice's thermal conductivity, increases its reflectivity (albedo)…
  arxiv Predrag Popović, Justin Finkel, Mary C. Silber, Dorian S. Abbot 2022-03-07T22:39:55Z 置信度 0.78 nlin.PSphysics.ao-phphysics.geo-ph
• Ice Giant Circulation Patterns: Implications for Atmospheric Probes
  Atmospheric circulation patterns derived from multi-spectral remote sensing can serve as a guide for choosing a suitable entry site for a future in situ probe mission. Since the Voyager-2 flybys in the 1980s, three decades of observations from ground- and spac…
  arxiv Leigh N. Fletcher, Imke de Pater, Glenn S. Orton, Mark D. Hofstadter 等 2019-07-05T15:47:00Z 置信度 0.78 astro-ph.EP
• On exact solutions and numerics for cold, shallow, and thermocoupled ice sheets
  This three section report can be regarded as an extended appendix to (Bueler, Brown, and Lingle 2006). First we give the detailed construction of an exact solution to a standard continuum model of a cold, shallow, and thermocoupled ice sheet. The construction …
  arxiv Ed Bueler, Jed Brown 2006-10-16T17:36:45Z 置信度 0.78 physics.geo-phphysics.comp-phphysics.flu-dyn
• The Intelligence College in Europe (ICE): An Effort to Create a European Intelligence Community
  In fulfilling the European security commitment, the actors of the so-called "Intelligence Community" play a central role. They provide political and military decision-makers with important analyses and information. The Intelligence College in Europe (ICE) is t…
  arxiv Uwe M. Borghoff, Lars Berger, François Fischer 2023-12-28T16:30:48Z 置信度 0.78 cs.CY
• Planetary Science by the NLSI LUNAR Team: The Lunar Core, Ionized Atmosphere, & Nanodust Weathering
  The Lunar University Network for Astrophysics Research (LUNAR) undertakes investigations across the full spectrum of science within the mission of the NASA Lunar Science Institute (NLSI), namely science of, on, and from the Moon. The LUNAR team's work on scien…
  arxiv Jack Burns, Joseph Lazio 2011-08-16T17:27:08Z 置信度 0.78 astro-ph.EP
• Lunar Resources: A Review
  There is growing interest in the possibility that the resource base of the Solar System might in future be used to supplement the economic resources of our own planet. As the Earth's closest celestial neighbour, the Moon is sure to feature prominently in these…
  arxiv Ian A. Crawford 2014-10-25T01:25:54Z 置信度 0.78 astro-ph.EP
• Lunar Reference Timescale
  Setting up a relativistic lunar reference frame is of a prime importance in the context of future exploration missions to the Moon. If the procedure for building a consistent reference frame within the framework of the general theory of relativity is well esta…
  arxiv Adrien Bourgoin, Pascale Defraigne, Frédéric Meynadier 2025-07-29T08:55:16Z 置信度 0.78 gr-qc
• Lunar semimonthly signal in cloud amount
  Based on NASA satellite infrared and visible range measurements, cloud amount ISCCP_D1 summer nighttime data, representing the tropospheric cloud activity at Central Russia are examined over 1994-2007, and the lunar signal in the cloud amount was extracted. Th…
  arxiv Nikolay Pertsev, Peter Dalin 2009-07-21T16:18:09Z 置信度 0.78 physics.ao-phphysics.geo-ph
• Origin of the lunar farside highlands from Earthshine-induced global circulation in lunar magma ocean
  The lunar farside highlands, referred to as the lunar farside thicker crust compared with the nearside crust, presents a challenge to the theory of formation and evolution of the Moon. Here, we show that, after the Moon reached synchronous rotation, Earthshine…
  arxiv Wenshuai Liu 2025-09-14T09:55:41Z 置信度 0.78 astro-ph.EPastro-ph.HE
• Review of research on lunar dust dynamics
  Lunar dust particles are generated by hypervelocity impacts of interplanetary micron-meteoroids onto the surface of the Moon, which seriously threatens the security of explorations. Studying the lunar dust dynamics helps to understand the origin and migration …
  arxiv Kun Yang, Weiming Feng, Luyuan Xu, Xiaodong Liu 2022-07-28T05:22:24Z 置信度 0.78 astro-ph.EP
• MoonMetaSync: Lunar Image Registration Analysis
  This paper compares scale-invariant (SIFT) and scale-variant (ORB) feature detection methods, alongside our novel feature detector, IntFeat, specifically applied to lunar imagery. We evaluate these methods using low (128x128) and high-resolution (1024x1024) lu…
  arxiv Ashutosh Kumar, Sarthak Kaushal, Shiv Vignesh Murthy 2024-10-14T22:05:48Z 置信度 0.78 cs.CVcs.AImath.AG
• Collisionless Encounters and the Origin of the Lunar Inclination
  The Moon is generally thought to have formed from the debris ejected by the impact of a planet-sized object with the proto-Earth towards the end of planetary accretion. Modeling of the impact process predicts that the lunar material was disaggregated into a ci…
  arxiv Kaveh Pahlevan, Alessandro Morbidelli 2016-03-21T17:49:03Z 置信度 0.78 astro-ph.EP
• Lunar Laser Ranging Science
  Analysis of Lunar Laser Ranging (LLR) data provides science results: gravitational physics and ephemeris information from the orbit, lunar science from rotation and solid-body tides, and Earth science. Sensitive tests of gravitational physics include the Equiv…
  arxiv James G. Williams, Dale H. Boggs, Slava G. Turyshev, J. Todd Ratcliff 2004-11-18T22:39:28Z 置信度 0.78 gr-qc
• Speciation and Dissolution of Hydrogen in the Proto-Lunar Disk
  Despite very high temperatures accompanying lunar origin, indigenous water in the form of OH has been unambiguously observed in Apollo samples in recent years. Such observations have prompted questions about the abundance and distribution of lunar hydrogen. He…
  arxiv Kaveh Pahlevan, Shun-ichiro Karato, Bruce Fegley 2016-03-21T18:21:12Z 置信度 0.78 astro-ph.EP
• Managing Activities at the Lunar Poles for Science
  The lunar poles are unique environments of both great scientific and, increasingly, commercial interest. Consequently, a tension exists between the twin objectives of (a) Exploring the lunar poles for both scientific and commercial purposes and ultimately supp…
  arxiv Ian A. Crawford, Parvathy Prem, Carle Peters, Mahesh Anand 2022-11-30T01:18:51Z 置信度 0.78 physics.soc-phastro-ph.EPastro-ph.IM
• Soil Test Apparatus for Lunar Surfaces
  We have studied several field geotechnical test instruments for their applicability to lunar soil simulants and analog soils. Their performance was evaluated in a series of tests in lunar simulants JSC-1A, NU-LHT-2M, and CHENOBI each prepared in carefully cont…
  arxiv Laila A. Rahmatian, Philip T. Metzger 2023-06-01T18:34:38Z 置信度 0.78 astro-ph.EPastro-ph.IMcond-mat.soft
• Ice-free geomorphometry of Enderby Land, East Antarctica: 2. Coastal oases
  Geomorphometric modeling and mapping of ice-free Antarctic areas can be applied for obtaining new quantitative knowledge about the topography of these unique landscapes and for the further use of morphometric information in Antarctic research. Within the frame…
  arxiv I. V. Florinsky, S. O. Zharnova 2025-09-05T14:32:58Z 置信度 0.78 physics.geo-ph
• Venting and Outgassing Simulations of Pressurized Lunar Modules: Contamination of the Lunar Environment
  One objective of Artemis science is to determine the impact human activities have on the lunar environment, which might compromise science objectives and measurements. We perform a preliminary analysis of the contamination associated with airlock venting and o…
  arxiv Stefano Boccelli, William M. Farrell, Prabal Saxena, Orenthal J. Tucker 2026-02-05T20:57:06Z 置信度 0.78 physics.space-phastro-ph.EPastro-ph.IMeess.SY
• Modelling long-term trends in lunar exposure to the Earth's plasmasheet
  This paper shows how the exposure of the Moon to the Earth's plasmasheet is subject to decadal variations due to lunar precession. The latter is a key property of the Moon's apparent orbit around the Earth - the nodes of that orbit precess around the ecliptic,…
  arxiv Mike Hapgood 2007-05-07T09:10:54Z 置信度 0.78 physics.space-ph
• Origin of the Moon and Lunar Water
  Three principal concepts regarding lunar formation have been examined: the accretion hypothesis, the mega-impact theory, and the multi-impact model. The multi-impact model amalgamates the salient facets of the mega-impact theory and the accretion hypothesis. A…
  arxiv Nick Gorkavyi 2023-10-25T20:06:14Z 置信度 0.78 astro-ph.EPphysics.ao-ph
• Critical percolation threshold restricts late-summer Arctic sea ice melt pond coverage
  During the summer, vast regions of Arctic sea ice are covered by meltwater ponds that significantly lower the ice reflectivity and accelerate melting. Ponds develop over the melt season through an initial rapid growth stage followed by drainage through macrosc…
  arxiv Predrag Popović, Mary C. Silber, Dorian S. Abbot 2022-03-08T14:04:23Z 置信度 0.78 nlin.PSnlin.AOphysics.ao-phphysics.flu-dynphysics.geo-ph
• The Damage to Lunar Orbiting Spacecraft Caused by the Ejecta of Lunar Landers
  This manuscript analyzes lunar lander soil erosion models and trajectory models to calculate how much damage will occur to spacecraft orbiting in the vicinity of the Moon. The soil erosion models have considerable uncertainty due to gaps in our understanding o…
  arxiv Philip T. Metzger, James G. Mantovani 2023-05-20T16:58:41Z 置信度 0.78 astro-ph.EPastro-ph.IMphysics.flu-dynphysics.space-ph
• Definition and Realization of the International Lunar Reference Frame
  All future lunar missions require a definition of the lunar reference system and a realization in the form of the lunar reference frame to ensure consistent products for positioning, navigation, cartography, and timing. This paper defines the origin, orientati…
  arxiv Krzysztof Sośnica, Agnès Fienga, Dmitry Pavlov, Nicolas Rambaux 等 2025-10-17T09:54:38Z 置信度 0.78 astro-ph.EPastro-ph.IM
• The International Lunar Reference System
  As the exploration of the Moon accelerates in the coming years, there is already an urgent need to standardise the Position, Navigation and Timing of spacecraft, and consequently for the definition of the lunar reference system and frame. This document gathers…
  arxiv Agnès Fienga 2026-07-30T07:01:42Z 置信度 0.78 astro-ph.EPastro-ph.IM
• Science on the Lunar Surface Facilitated by Low Latency Telerobotics from a Lunar Orbiting Platform-Gateway
  NASA and ESA are preparing a series of human exploration missions using the four-person Orion crew vehicle, launched by NASA's Space Launch System, and a Lunar Orbiting Platform-Gateway (LOP-G) that enable long duration (>30 days) operations in cis-lunar sp…
  arxiv Jack O. Burns, Terry Fong, David A. Kring, William D. Pratt 等 2017-05-26T19:35:12Z 置信度 0.78 astro-ph.IM
• The Spectroscopic Detectability of Argon in the Lunar Atmosphere
  Direct measurements of the abundance of argon in the lunar atmosphere were made in 1973 by instruments placed on the Moon during the Apollo 17 mission, but the total daytime abundance is unknown due to instrument saturation effects; thus, until we are able to …
  arxiv Joel Wm. Parker, S. Alan Stern, G. Randall Gladstone, J. Michael Shull 1998-10-20T20:49:10Z 置信度 0.78 astro-ph
• The effects of surface roughness on lunar Askaryan pulses
  The effects of lunar surface roughness, on both small and large scales, on Askaryan radio pulses generated by particle cascades beneath the lunar surface has never been fully estimated. Surface roughness affects the chances of a pulse escaping the lunar surfac…
  arxiv C. W. James 2016-08-25T10:20:00Z 置信度 0.78 astro-ph.HEastro-ph.IM
• Analyzing and Forecasting Success in the Men's Ice Hockey World (Junior) Championships Using a Dynamic Ranking Model
  What factors contribute to the success of national teams in the Men's Ice Hockey World Championships and the Men's Ice Hockey World Junior Championships? This study examines whether hosting the tournament provides a home advantage; the influence of past tourna…
  arxiv Vladimír Holý 2024-09-09T15:25:15Z 置信度 0.78 stat.AP
• Spectrum estimates of Hill's lunar problem
  We investigate the action spectrum of Hill's lunar problem by observing inclusions between the Liouville domains enclosed by the regularized energy hypersurfaces of the rotating Kepler problem and Hill's lunar problem. In this paper, we reinterpret the spectra…
  arxiv Junyoung Lee 2015-10-25T14:14:35Z 置信度 0.78 math.SG
• Principal Component Analysis for Lunar Crater Detection
  Optical navigation is a critical component for lunar orbiter and lander missions. Image-based crater identification has emerged as a promising technology for optical navigation due to the abundance of craters on the lunar surface and the availability of extens…
  arxiv Travis Driver, John A. Christian 2026-05-16T19:06:23Z 置信度 0.78 cs.CVcs.LG
• Lunar impact ejecta flux on the Earth
  The transfer of material between planetary bodies due to impact events is important for understanding planetary evolution, meteoroid impact fluxes, the formation of near-Earth objects (NEOs), and even the provenance of volatile and organic materials at Earth. …
  arxiv Jose Daniel Castro-Cisneros, Renu Malhotra, Aaron J. Rosengren 2025-04-22T00:46:46Z 置信度 0.78 astro-ph.EP
• A quantitative comparison of lunar orbital neutron data
  Data from the Lunar Exploration Neutron Detector (LEND) Collimated Sensors for Epithermal Neutrons (CSETN) are used in conjunction with a model based on results from the Lunar Prospector mission to quantify the extent of the background in the LEND CSETN. A sim…
  arxiv V. R. Eke, L. F. A. Teodoro, D. J. Lawrence, R. C. Elphic 等 2011-08-09T21:00:20Z 置信度 0.78 astro-ph.EP
• The timeline of the Lunar bombardment - revisited
  The timeline of the lunar bombardment in the first Gy of the Solar System remains unclear. Some basin-forming impacts occurred 3.9-3.7Gy ago. Many other basins formed before, but their exact ages are not precisely known. There are two possible interpretations …
  arxiv A. Morbidelli, D. Nesvorny, V. Laurenz, S. Marchi 等 2018-01-11T13:47:21Z 置信度 0.78 astro-ph.EP
• Single-Satellite Navigation on Lunar North Pole
  The Moon is a primary focus of space exploration. Current navigation methods face significant limitations in providing precise location data for lunar missions. In particular, existing methods often require direct Line of Sight to Earth, have limited capacity,…
  arxiv Tim Gong, Andrew Dempster 2025-04-04T00:01:51Z 置信度 0.78 eess.SP
• Constraints on the Source of Lunar Cataclysm Impactors
  Multiple impact basins formed on the Moon about 3.8 Gyr ago in what is known as the lunar cataclysm or late heavy bombardment. Many workers currently interpret the lunar cataclysm as an impact spike primarily caused by main-belt asteroids destabilized by delay…
  arxiv Matija Cuk, Brett J. Gladman, Sarah T. Stewart 2009-12-10T00:35:35Z 置信度 0.78 astro-ph.EP
• Origin of the lunar isotopic crisis from solidification of a stratified lunar magma ocean
  According to the giant impact theory, the Moon formed through accreting the debris disk produced by a collision between Theia and the proto-Earth. The giant impact theory can explain most of the properties of the Earth-Moon system, however, simulations with re…
  arxiv Wenshuai Liu 2025-09-08T10:24:36Z 置信度 0.78 astro-ph.EP
• Lunar south pole ice as heat sink for lunar cryofuel production system
  Recent Clementine bistatic radar data suggest that water ice may be present in a ‘‘forever shaded’’ depression or crater at the South Pole of the Moon. The ice is a feedstock for the electrolysis production of cryogenic oxygen and hydrogen rocket fuel for a tr…
  crossref Anthony Zuppero, Marland Stanley, S. Michael Modro, Pat Whitman 2008-05-14T16:06:49Z 置信度 0.70
• Polar Ice on the Moon
  crossref Akos Kereszturi 2023-05-13T10:02:24Z 置信度 0.70
• Can spacecraft-borne contamination compromise our understanding of lunar ice chemistry?
  Recent detections of water ice in the permanently shadowed regions (PSRs) at the lunar poles have reignited scientific and commercial interest in the exploration of Earth’s closest neighbour. The frigid temperatures in PSRs operate as cold traps for volatiles …
  crossref Francisca S. Paiva, Silvio Sinibaldi 2025-11-17T17:04:21Z 置信度 0.70
• Prospecting for Lunar Polar Ice from Very Low Lunar Orbit: How Low Can You Go?
  View Video Presentation: https://doi.org/10.2514/6.2022-4348.vid Neutron spectroscopy observations from very low-altitude orbits over the Moon’s south pole could improve the spatial resolution maps for water ice reserves. We explore these low-altitude orbits t…
  crossref Jackson Shannon, Charles Hibbitts, Kirby Runyon, Michael E. Nord 2022-10-15T21:19:55Z 置信度 0.70
• Mining Lunar Polar Ice for LO2/LH2 Propellant
  View Video Presentation: https://doi.org/10.2514/6.2021-4235.vid Water ice and other volatiles at the poles of the Moon present a vast supply of resources for lunar and cislunar activities, prime among them is the production of propellant. LO2/LH2 is the most …
  crossref Christopher B. Dreyer 2021-11-03T20:24:00Z 置信度 0.70
• Simulations suggest organic molecules can form in lunar ice
  crossref 2017-01-31T11:52:05Z 置信度 0.70
• Lunar Ice Might Be Easier to Reach Than We Thought
  An instrument aboard the Vikram lander suggests that buried water ice could be found at higher latitudes, making it more abundant and easier to extract than previously believed.
  crossref Damond Benningfield 2025-04-12T07:00:21Z 置信度 0.70
• Demonstration and Analysis of Thermal Management System (TMS) for Ice Extraction and Ice Collection for Lunar Ice Miners
  Advanced Cooling Technologies, Inc. in collaboration with Honeybee Robotics is developing a Thermal Management System (TMS) to facilitate ice extraction from icy-lunar regolith and efficient ice collection in a cold trap tank. The TMS has two main technologies…
  crossref Sai Kiran Hota, Quang Truong, Kuan-Lin Lee, Calin Tarau 等 2026-05-05T18:56:16Z 置信度 0.70
• Water Ice Lurks in Young—but Not Too Young—Lunar Craters
  Using topographic data, researchers have estimated the ages of water ice–containing craters near the Moon’s poles and ruled out volcanism as being a primary route for water delivery.
  crossref Katherine Kornei 2020-06-16T07:00:19Z 置信度 0.70
• Experimental Study of UV-Vis-NIR Detection of Lunar Water Ice in Different Stratigraphies
  Volatiles are critical for understanding their delivery to the Moon and as a resource for sustained lunar exploration. Water ice and potentially other volatiles exist in and proximal to permanently shadowed regions (PSRs). However, little is known of the form,…
  crossref Abhay Vidwans, Jeffrey Gillis-Davis 2025-03-04T16:33:37Z 置信度 0.70
• Lunar Polar Ice: Implications for Lunar Development
  The discovery of water ice at the lunar poles can spur lunar exploration and development and may be a factor in accelerating human exploration beyond the Earth-Moon system. Theoretical models predict the existence of ice in the cold traps, and the Clementine a…
  crossref Michael B. Duke 2002-07-26T11:58:29Z 置信度 0.70
• The Nature of Lunar Competition and Security Implications for Ice Mining
  crossref Andrew Dempster 2026-01-16T14:18:06Z 置信度 0.70
• Impact of Water Ice on Lunar Propellant Production
  *† The existence of water-ice on the Moon is an important resource for lunar bases. The hydrogen and oxygen can be useful for propellant production and human life support. This study assumes that a commercial market may be viable for the extraction and sale of…
  crossref Charles Reynerson 2012-12-19T00:08:30Z 置信度 0.70
• In-situ Detection and Quantitative Analysis Methods for Lunar Water Ice in PSRs
  Remote sensing has identified water-ice in the Moon’s polar regions; however, it cannot directly verify the existence and origin of lunar water in the permanently shadowed regions. The LUnar soil Water molecular Analyzer (LUWA) is a key payload on the mini-fly…
  crossref Xiang Li, Nailiang Cao, Ruifeng Kan 2026-03-13T19:50:41Z 置信度 0.70
• In-situ detection of water ice and volatiles in lunar permanently shadowed regions
  The LUnar soil Water molecular Analyzer (LUWA) is a payload aboard China's Chang'E-7 mission (to be launched in 2026), which will conduct first in-situ detection of water ice and volatiles within the permanently shadowed regions (PSRs) at the lunar south pole.…
  crossref Nailiang Cao, Xiang Li, Ruifeng Kan 2026-03-13T19:50:41Z 置信度 0.70
• Lunar Dust and Terrestrial Ice Nucleus Concentration
  crossref VLADIMIR VAND 2006-07-05T14:56:01Z 置信度 0.70
• Searching for Subsurface Lunar Water Ice using a Nuclear-Powered Rover
  The Vision for Space Exploration has identified the Earth’s moon as a future destination for human explorers as a stepping‐stone for further manned deep space exploration. The feasibility of building and maintaining a human presence on the moon could be direct…
  crossref James E. Randolph 2005-03-16T23:42:15Z 置信度 0.70
• Mini-RF Observations of Lunar Polar Craters and Implications for Ice Distribution
  <p>The possibility that water ice could be present in lunar polar craters has long been postulated.  More recently, measurements from instruments on a number of spacecraft have all pointed to the presence of water at the lunar poles;…
  crossref Lauren Jozwiak, G. Wes Patterson 2020-03-09T18:43:21Z 置信度 0.70
• Design and Verification of a Novel Sampling System for Lunar Water Ice Exploration
  Aiming at the problem that it is difficult to collect the subsurface lunar water ice samples quickly due to the cementation-hardening of ice and soil at extremely low temperature in the permanent shadow regions, a novel lunar water ice sampling system is propo…
  crossref Ruqi Ma, Weiwei Zhang, Rulin Ma, Wengcheng Ni 等 2023-03-01T18:26:01Z 置信度 0.70
• Experimental Investigation of Regolith-Ice Mixtures under Cryogenic Vacuum Conditions for Lunar and Planetary Exploration
  IntroductionA good understanding of the properties of water-ice and regolith mixtures is of paramount importance to support the development of upcoming scientific missions to the Moon and for future in-situ resource utilization (ISRU). Although water was alrea…
  crossref Thilo Witzel, Rok Šeško, Philipp Reiss 2025-07-09T15:45:11Z 置信度 0.70
• The Role of Crustal Magnetic Anomalies and Topography in Shaping Lunar South Polar Water Ice
  Lunar magnetic anomalies are abundant near the south pole, where several moderate-strength anomalies spatially overlap permanently shadowed regions. This environment provides a unique setting to assess how crustal magnetic fields and complex topography regulat…
  crossref Jan Deca, Lon Hood, Shuai Li 2026-03-13T23:03:52Z 置信度 0.70
• Revisiting Lunar Water Ice Content Retrieval Using Lunar Remote Sensing Data
  During a few recent lunar missions, a possibility of water ice existing in the permanently shadowed regions on the moon has come forward. The content of water ice on the moon is an open question in the current moon study. It is known that the existence of ice …
  crossref Vaidehi Patel, Jayesh Pabari, Jignesh Patel 2014-06-04T05:34:38Z 置信度 0.70
• Volatile Ice Presence Analysis through Mass Wasting Events Mapping in Lunar Permanently Shadowed Regions
  Mass wasting events on the Moon have been documented since the Apollo era and are distributed across its surface. On Earth, the morphology and runout distance of landslides, particularly flowlike landslides such as debris and mud flows, are strongly influenced…
  crossref Riccardo Pedrelli, Valentin Bickel, Jordan Aaron, Ariel Deutsch 2025-03-14T19:28:01Z 置信度 0.70
• Detection of Water Ice in the Lunar Regolith via Microwave Radiometry
  Recent lunar observations have concluded that significant water ice deposits may exists in the regolith, especially in the permanently shadowed regions near the lunar poles. Detection and utilization of these reserves is very important to sustain the continuou…
  crossref Mustafa Aksoy 2021-10-15T17:33:25Z 置信度 0.70
• Overview and Results from NASA's Break The Ice Lunar Challenge
  NASA's Prizes, Challenges, and Crowdsourcing (PCC) program portfolio is designed to connect the public to the agency's missions. The program encourages creative solutions from a diverse range of solvers which serve to advance the agency's technology developmen…
  crossref Kurt W. Leucht, Tracie J. Prater, Naveen Vetcha 2025-07-14T17:40:12Z 置信度 0.70
• Molecular Dynamics Simulations of Dielectric Breakdown of Lunar Regolith: Implications for Water Ice Formation on Lunar Surface
  Abstract Molecular dynamics simulations are carried out to investigate dielectric breakdown of lunar regolith induced by space weather events and its potential effects on water ice formation on lunar surface. We find that dielectric breakdown can trigger the w…
  crossref Ziyu Huang, Ken‐ichi Nomura, Aiichiro Nakano, Joseph Wang 2021-01-15T10:02:38Z 置信度 0.70
• Ice on the Moon boosts hopes for future lunar missions
  crossref Tony Reichhardt 2002-07-26T08:37:13Z 置信度 0.70
• A more robust interpretation of water ice isotope signature from lunar polar missions: theoretical model for isotope fractionation during water ice sublimation in very low pressure systems at cryogenic temperatures.
  <p>Targeting the deployment of sustainable human and robotic exploration on the Moon by the end of this decade, there is a pressing need for better understanding the lunar water cycle and the availability of water for ISRU. The O-H isotope signat…
  crossref Veneranda López Días, Laurent Pfister, Christophe Hissler, François Barnich 2022-03-27T23:29:46Z 置信度 0.70
• Lunar polar ice - Methods for mining the new resource for exploration
  The presence of ice in permanently shadowed depressions near the lunar poles and determination of its properties will significantly influence both the near- and long-term prospects for lunar exploration and development. Since data from the Lunar Prospector spa…
  crossref Robert Gustafson, Eric Rice 2013-09-30T21:30:54Z 置信度 0.70
• Numerical simulation of temperature rise and sublimation of water-ice during drilling in lunar polar ice-soils
  The lunar polar regions are rich in resources, particularly the water resources that are urgently needed for the establishment of a lunar research station. One of the Chang'e 7 missions is utilize a drilling sampling method to collect in-situ ice-soil samples,…
  crossref Sibo Liu, Fenghong Gao, Jinsheng Cui 2024-09-27T20:41:30Z 置信度 0.70
• Beyond lunar ice cube: next generation 12U orbiting lunar water explorer
  We present a concept for a robust 12U version of an orbiting cubesat explorer for lunar water as a follow on to the Lunar Ice Cube mission with an upgraded IR spectrometer, CLEW, described in earlier work (ref). CLEW has significantly enhanced spectral range a…
  crossref Pamela E. Clark, Nate Fite, Cliff Brambora, Tilak Hewagama 等 2025-09-17T20:14:58Z 置信度 0.70
• SAR-based Investigation of Water Ice in Lunar Polar Permanently Shadowed Regions (PSRs)
  THE nature and distribution of deposits in the lunar PSRs have long been subjects of scientific debate. Although the Lunar Crater Observation and Sensing Spacecraft (LCROSS) impact experiment provided evidence for the existence of cold-trapped volatiles, Areci…
  crossref Haiying Li, Zhou Qin, Bin Liu, Jianjun Liu 等 2025-07-09T15:12:38Z 置信度 0.70