Icarus

Papers
(The TQCC of Icarus is 7. The table below lists those papers that are above that threshold based on CrossRef citation counts [max. 250 papers]. The publications cover those that have been published in the past four years, i.e., from 2021-05-01 to 2025-05-01.)
ArticleCitations
Isolating the mechanisms for asteroid surface refreshing67
Plenoptic imaging of meteorite shape change during plasma wind tunnel experiments57
Evidence for landslides in Sisyphi Cavi (Noachis Terra, Mars): Slope evolution and role of endogenous preparatory factors56
Morphological changes currently occurring in sand-filled gully channels on Mars: Implications for the role of substrates inside channels56
A case for young igneous volcanism in the Terra Sirenum region, Mars54
Raman spectroscopic documentation of Mars analog basalt alteration by brines53
Influence of hydrothermal asteroidal conditions on the molecular structure and isotopic compositions of polycyclic aromatic hydrocarbons51
Dynamical evolution and thermal history of asteroids (3200) Phaethon and (155140) 2005 UD50
Diffusion limited escape of hydrogen from Mars49
Multiscale spectral discrimination of poorly crystalline and intermixed alteration phases using aerial and ground-based ExoMars rover emulator data48
Visible–near-infrared observations of organics and carbonates on (101955) Bennu: Classification method and search for surface context45
Optical observations and dust modelling of comet 156P/Russell-LINEAR44
322P/SOHO: The counterpart of a historical comet in 254 CE?43
Inferences of water–ice cloud physics determined from MAVEN/IUVS aerosol retrievals and Mars GCM comparisons42
The yearly variability of the sodium exosphere of Mercury: A toy model42
Investigation of the shocked Viñales ordinary chondrite (L6) meteorite fall – Implications for shock classification, fragmentation, and collision dynamics41
Expression of concern: “The spatial distributions of degraded craters and valley networks on Mars as a function of elevation: Their implications for Noachian climate” [Icarus 406 (2023) 115734]38
Comparing the radiolytic oxidation of sulfur and chloride within ice on Europa and Mars37
Chaotic tides as a solution to the Hyperion problem36
Implications for the energy source for an early dynamo in Vesta from experiments on electrical resistivity of liquid Fe-10wt%Ni at high pressures35
Planet Four: A Neural Network’s search for polar spring-time fans on Mars34
Long-period dynamical evolution of the meteoroid stream originating in comet 21P/Giacobini-Zinner34
Exosphere-mediated migration of volatile species on airless bodies across the solar system32
Inversion of ultraviolet occultation profiles in a dusty atmosphere: Analytic and numerical methods31
Variations of the magnetic field and plasma parameters near the Martian induced magnetosphere boundary30
Constraints on a potential aerial biosphere on Venus: II. Ultraviolet radiation30
Influence of observed seasonally varying composition on Titan’s stratospheric circulation30
Three-dimensional characterization of particle size, shape, and internal porosity for Apollo 11 and Apollo 14 lunar regolith and JSC-1A lunar regolith soil simulant29
Daily and seasonal processes shape hydrological activity and detectability of moisture in Antarctic, Mars-analog soils29
Machine learning as a tool to classify extra-terrestrial landslides: A dossier from Valles Marineris, Mars27
Seasonal variability of gravity wave activity in Mars's lower atmosphere from MGS–TES nadir observations27
The annual cycle of water vapor above gale crater as retrieved by CRISM and compared to ChemCam passive sky spectroscopy26
On a radiolytic origin of red organics at the surface of the Arrokoth Trans-Neptunian Object26
An improved model of metal/silicate differentiation during Earth's accretion25
Catastrophic rupture of lunar rocks: Implications for lunar rock size–frequency distributions25
Elemental composition of manganese- and phosphorus-rich nodules in the Knockfarril Hill member, Gale crater, Mars25
Subglacial catastrophic-flood origin of linear and curvilinear flat-rimmed pit chains on Mars: Evidence from geomorphological mapping and detailed landsystem analysis25
Exploring the variability of the venusian thermosphere with the IPSL Venus GCM24
Submicroscopic iron-rich grains throughout impact glasses in Chang'E-5 regolith24
Shadow method retrievals of the atmospheric optical depth above Gale crater on Mars using HRSC images23
Jovian current disk crossings as observed by Juno JADE-I23
The high-resolution imaging science experiment (HiRISE) in the MRO extended science phases (2009–2023)23
Chronological and compositional mapping of the Mare Orientale basin using Chandrayaan-1 – M3 and LRO datasets23
Comprehensive analysis of Chandrayaan-3 landing site region focussing on morphology, hydration and gravity anomalies23
Bayesian inference on the isotopic building blocks of Mars and Earth23
Recent boulder falls within the Finsen crater on the lunar far side: An assessment of the possible triggering rationale23
The magnetic susceptibility of Pleistocene paleosols as a martian paleoenvironment analog23
Cosmic hydrogen and ice loss lines22
The influence of equation of state on impact dynamics between Pluto-like bodies22
Do icy dust aggregates break up when they pass the snow line?22
Simulation of surface regolith gardening and impact associated melt layer production under ns-pulsed laser ablation22
Non-thermal escape of the martian CO222
Lava flow ages in northeastern Oceanus Procellarum: The need for calibrating crater counting procedures22
How much earlier would LSST have discovered currently known long-period comets?22
Ed. Board22
Saturn’s atmospheric response to the large influx of ring material inferred from Cassini INMS measurements21
Scaling of convection in high-pressure ice layers of large icy moons and implications for habitability21
Asteroids were born bigger: An implication of surface mass ablation during gas-assisted implantation into the asteroid belt21
MAVEN/IUVS observations of C I 156.1 nm and 165.7 nm dayglow: Direct detection of carbon and implications on photochemical escape21
Two types of jarosite in the early Cambrian sedimentary rocks: Insights for genesis and transformation of jarosite on Mars21
Ion density and phase space density distribution of planetary ions Na+, O+ and He+ in Mercury’s magnetosphere21
A new constraint on HCl abundance at the cloud top of Venus21
Detailed chemical composition analysis of the Soi crater region on Titan20
Analyzing spatial distributions and alignments of pitted cone features in Utopia Planitia on Mars20
Range resolution enhancement of SHAllow RADar (SHARAD) data via bandwidth extrapolation technique: Enabling new features detection and improving geophysical investigation20
Large volcanoes on Venus: Morphology, morphometry, and stratigraphy20
The effect of collisional erosion on the composition of Earth-analog planets in Grand Tack models: Implications for the formation of the Earth20
The Martian ionosphere at solar minimum: Empirical model validation using MAVEN ROSE data20
Editorial Board20
Evidence for the protection of N-heterocycles from gamma radiation by Mars analogue minerals20
Ejecta cloud distributions for the statistical analysis of impact cratering events onto asteroids’ surfaces: A sensitivity analysis19
Possible formation pathways for zeolites in closed-basin lakes on noachian Mars: Insights from geochemical modeling19
Impact strength of cm-to-decimeter scale weak porous targets: Implication for lifetime of boulders on asteroids19
The morphometry of small impact craters on Bennu: Relationships to geologic units, boulders, and impact armoring19
Non-LTE spectroscopy of the tetradecad region of methane recorded in a hypersonic flow18
Vortex crystals at Jupiter’s poles: Emergence controlled by initial small-scale turbulence18
Recent faulting at the Claritas Rupes scarp on Mars18
Mineral abrasion experiments at Mars relevant temperatures18
Latitudinal and radial dependence of the lunar sodium exospheric temperature and linewidths18
A new numerical model of the HF antenna of the Mars Reconnaissance Orbiter’s (MRO) Shallow Radar (SHARAD) and first results from a test at a high-angle spacecraft roll18
VIS-IR spectroscopy of magnesium chlorides at cryogenic temperatures17
First quantitative characterization of the Martian dust devil dimensions determined from InSight data17
Rare earth element assessment in Jezero crater using the Planetary Instrument for X-ray Lithochemistry on the Mars 2020 rover Perseverance: A case study of cerium17
Venus upper atmosphere revealed by a GCM: II. Model validation with temperature and density measurements17
Ricochets on asteroids II: Sensitivity of laboratory experiments of low velocity grazing impacts on substrate grain size17
A Mars orbital catalog of aqueous alteration signatures (MOCAAS)17
Modeling global-scale mass flows on the Lagrangian satellites of Dione and Tethys17
Chronology, composition, and mineralogy of mare basalts in the junction of Oceanus Procellarum, Mare Imbrium, Mare Insularum, and Mare Vaporum17
The role of subsurface ocean dynamics and phase transitions in forming the topography of icy moons17
Aeolian bedrock ridges in Gale crater, Mars16
A contemporary view of the ordinary chondrite boot I: Band parameter analysis dependency16
Preface: Ices in the Solar system; origin, evolution and distribution16
Mechanical behaviour of sulphur-based Martian regolith concrete processed under CO2-rich conditions16
Io's SO2 atmosphere from HST Lyman-α images: 1997 to 201816
Photochemistry of benzene (C6H6) hydrogen cyanide (HCN) co-condensed ices part 2: Formation of aerosols analogues of titan's atmosphere16
Micro-FTIR reflectance spectroscopy of Ryugu, CI chondrites and volatile-rich clasts – Comparing spectral features in the Mid-IR (2.5–16.5 μm) region16
Compositional control on impact crater formation on mid-sized planetary bodies: Dawn at Ceres and Vesta, Cassini at Saturn16
VNIR reflectance spectra of silicate-graphite mixtures: The effect of graphite content and particle size16
3D morphometry of Martian craters from HRSC DEMs using a multi-scale semantic segmentation network and morphological analysis16
Mars volatile inventory and outgassing history15
Cross-attention induced multilayer domain adaptation network for extraction of sub-kilometer craters from HiRIC images15
Impact induced H2-rich climates on early Mars explored with a global climate model15
Present-day model of lunar meteoroids and their impact flashes for LUMIO mission15
Distribution of atmospheric aerosols during the 2007 Mars dust storm (MY 28): Solar infrared occultation observations by SPICAM15
Identification of a new spectral signature at 3 μ15
Tidal dissipation within an elongated asteroid with satellite, and application to asteroid (216) Kleopatra15
The brightness of the CO Cameron bands in the martian discrete aurora: A study based on revised cross sections15
Dark primitive asteroids account for a large share of K/Pg-scale impacts on the Earth15
Comparisons of the core and mantle compositions of earth analogs from different terrestrial planet formation scenarios15
A numerical model for the atmospheric entry of hydrated, phyllosilicate-rich micrometeorites15
Bulk composition and thermal evolution constrain the formation of organics in Ceres' subsurface ocean via geochemical modeling15
Variability of temperatures and gravity wave activity in the Martian thermosphere during low solar irradiance15
Statistical chronometry of meteorites. I. A Test of 26Al homogeneity and the Pb-Pb age of the solar system’s 15
Laser-Induced Breakdown Spectroscopy (LIBS) characterization of granular soils: Implications for ChemCam analyses at Gale crater, Mars15
Where on the Moon was the eruption that produced the recently reported ∼ 120 million year old volcanic glass beads?15
Large mass inflow rates in Saturn’s rings due to ballistic transport and mass loading15
Dark ray craters on Ganymede: Impactor or endogenous origin15
Separation of quasi-continuous and periodic components of lineament formation at the Belus – Phoenix - Rhadamanthys Linea “triangle” on Europa14
Europa's hemispheric color dichotomy as a constraint on non-synchronous rotation14
Magnetic induction heating of planetary satellites: Analytical formulae and applications14
Generation and evolution of laser-induced shock waves under martian atmospheric conditions14
GOES GLM, biased bolides, and debiased distributions14
Evidence for hydrated minerals in the VNIR spectra of G-class asteroids: A first look14
The upper-thermal stability of an iron-rich smectite: Implications for smectite formation on Mars14
Observation of the Southern Polar cap during MY34-36 with ExoMars-TGO NOMAD LNO14
Stochastic hyperbola fitting, probabilistic inversion, reverse-time migration and clustering: A novel interpretation toolbox for in-situ planetary radar14
Variations in surface adsorbed H2O on lunar soils and relevant minerals14
A modeling approach for water and sediment transport in Jezero crater on Mars based on new geomorphological evidence14
Evolution of impact-generated hydrothermal systems in basaltic targets on Earth and implications for habitats on Mars14
Modeling of observations of the OH nightglow in the venusian mesosphere14
Compositional diversity in the Mare Marginis and Mare Smythii: An insight into the volcanism in the region14
Space weathering on inner planetary surface analogues induced by swift multicharged heavy ion bombardment14
Moderate D/H ratios in methane ice on Eris and Makemake as evidence of hydrothermal or metamorphic processes in their interiors: Geochemical analysis14
Integral equation modeling for dielectric retrieval of the lunar surface using Chandrayaan-2 fully-Polarimetric L-band dual frequency SAR (DFSAR) data14
Lunar elemental abundances as derived from Chandrayaan-214
Surface grain size of alluvial fans on Mars from thermal inertia, as an indicator of depositional style14
SPH simulations of high-speed collisions between asteroids and comets13
Feasibility of meteor surveying from a Venus orbiter13
Origin of ice in the Medusae Fossae Formation, equatorial Mars13
Automatic crater shape retrieval using unsupervised and semi-supervised systems13
Frequency-dependent Ganymede’s tidal Love number k13
Evidence for widely-separated binary asteroids recorded by craters on Mars13
A new estimate for the age of highly-siderophile element retention in the lunar mantle from late accretion13
On the cooling rate evolution of asteroid fragments13
Ed. Board13
Ed. Board13
Three-dimensional imaging of martian glaciated terrain using Mars Reconnaissance Orbiter Shallow Radar (SHARAD) observations13
Mare filled craters on the Moon13
Igneous rock powder identification using colour cameras: A powerful method for space exploration13
Corrigendum to ‘Oort Cloud and sednoid formation in an embedded cluster, II: Dynamics and orbital evolutions’ [Icarus 410 (2024) 115915]13
Pre and post-landing atmospheric optical depths at the Zhurong landing site on Mars retrieved using a single-image-based approach13
Alkali metal depletion in the deep Jovian atmosphere: The role of anions13
The unique spectral and geomorphological characteristics of pitted impact deposits associated with Marcia crater on Vesta13
Bennu's global surface and two candidate sample sites characterized by spectral clustering of OSIRIS-REx multispectral images13
Ed. Board13
Formation of the four terrestrial planets in the Jupiter–Saturn chaotic excitation scenario: fundamental properties and water delivery13
Ed. Board13
Possible polyphase periglaciation and glaciation adjacent to the Moreux impact-crater, Mars13
Thermal expansion of oldhamite, CaS: Implication for the surface of Mercury13
Relationships between lobate debris aprons and lineated valley fill on Mars: Evidence for an extensive Amazonian valley glacial landsystem in Mamers Valles13
Uncovering Ganymede's past: Tectonics at Nippur/Philus Sulci13
Global characterization of the early-season dust storm of Mars year 3612
Selection of chemical species for Europa’s surface using Galileo/NIMS12
Absolute model ages of three craters in the vicinity of the Chang'E-5 landing site and their geologic implications12
Martian cave detection via machine learning coupled with visible light imagery12
Boulders on Mercury12
The mystery of the missing mantle problem and insights from spectroscopy12
The density structure of Titan’s outer ice shell12
Late drainage along portions of Samara Valles, West of Jones Crater, Margaritifer Terra, Mars12
Overview of the MetSpec project - Artificial meteors in ground testing12
Water uptake by chlorate salts under Mars-relevant conditions12
A denser and elevated Martian nightside ionosphere during Mars season Ls 180–360°12
Global geologic map of asteroid (101955) Bennu indicates heterogeneous resurfacing in the past 500,000 years12
Carbon photochemical escape rates from the modern Mars atmosphere12
Seepage-evaporation controlled depletion of initially water-filled reservoirs on Earth and Mars: Analytic versus HYDRUS modeling12
Ephemeris and hazard assessment for near-Earth asteroid (101955) Bennu based on OSIRIS-REx data12
Rotation period estimates for 14 asteroids with the Earth MOID less than 1.1 AU12
Illumination and regolith temperature for China's candidate lunar landing sites with multiple scattering considerations12
Corrigendum to ‘Successes and challenges of factor analysis/target transformation application to visible-to-near-infrared hyperspectral data’: [Icarus 365 (2021) 114402]12
Modification of icy planetesimals by early thermal evolution and collisions: Constraints for formation time and initial size of comets and small KBOs12
Evidence that Earth’s magnetotail affects dielectric breakdown weathering on the Moon12
Exploring the dielectric loss of Martian regolith in the frequency domain using Zhurong radar data12
Rotational/divergent flow and energy conversion of thermal tides in a Venus general circulation model12
Morphologic differences in radial grooves on martian layered (fluidized) ejecta: Implications for emplacement processes and conditions12
Investigation of mineral assemblages in a newly identified endorheic playa near Huygens basin on Mars and their astrobiological implications12
Volatiles on Mercury: The case of hollows and the pyroclastic vent of Tyagaraja crater12
Pluto's Sputnik basin as a peak-ring or multiring basin: A comparative study12
Magnetically controlled ionosphere of Mars: A model analysis with the vertical plasma drift effects12
Lifetime of cm-sized zodiacal dust from the physical and dynamical evolution of meteoroid streams12
Characterization of aqueous alteration and formation of salty exposures at Ius Chasma, Mars12
Chondrule formation via impact jetting in the icy outer solar system12
Prediction of the collisions of meteoroids originating in comet 21P/Giacobini-Zinner with the Mercury, Venus, and Mars12
Simulated SPHEREx spectra of asteroids and their implications for asteroid size and reflectance estimation12
Weakening of olivine by hydrogen implantation: Results of nano-indentation tests and some applications to planetary materials12
Pulsed plasma discharge effects on efficiency and rate of penetration of melt probes in ice12
Impact of UV radiation on the Raman and infrared spectral signatures of sulfates, phosphates and carbonates: Implications for Mars exploration11
A satellite orbit drift in binary near-Earth asteroids (66391) 1999 KW4 and (88710) 2001 SL9 — Indication of the BYORP effect11
The puzzling north polar region of Uranus: Continued zero-shear winds and increasing brightness from 2015 through 2022 according to 7 years of Keck AO imaging11
Elasticity of selected icy satellite candidate materials (CO2, C6H6, MgSO4·7H2O and CaSO4·2H2O) revisited by dispersion corrected density functional theory11
Ejecta distribution and momentum transfer from oblique impacts on asteroid surfaces11
Modeling results for the composition and typology of non-primary venusian anorthosite11
How does topography affect wind abrasion on Mars? Recently observed shifts in ventifact orientation at Gale crater11
Mare basalt flooding events surrounding Chang'e-4 landing site as revealed by Zhinyu crater ejecta11
Thermodynamic modeling of calcium or magnesium chloride, chlorate, and perchlorate ternary mixtures deliquescence at Mars-relevant temperatures11
Improved method of hydrous mineral detection by latitudinal distribution of 0.7-μm surface reflectance absorption on the asteroid Ryugu11
A new perspective on Saturn’s polar vortices: Coupling the thermosphere and stratosphere11
An improved method combining Fisher transformation and multiple endmember spectral mixture analysis for lunar mineral abundance quantification using spectral data11
Laboratory measurements of the 15–46 cm wavelength opacity of water vapor under temperature conditions characteristic of the deep atmosphere of Jupiter11
Unexpected mineral impact on organic evolution during simulated aqueous alteration in asteroids11
Particle sizes in Saturn’s rings from UVIS stellar occultations 2. Outlier Populations in the C ring and Cassini Division11
Complex Ice Chemistry: A comparative study of electron irradiated planetary ice analogues containing methane11
Chandrayaan-2 Large Area Soft X-ray Spectrometer (CLASS): Calibration, In-flight performance and first results11
A reflectance calibration method for Multispectral Camera (MSCam) on the Zhurong rover11
Experimental study of clusters in dense granular gas and implications for the particle stopping time in protoplanetary disks11
Three-dimensional imaging of high-velocity-impact induced crack growth in carbonaceous meteorites11
Rock size-frequency distribution analysis at the Zhurong landing site based on Navigation and Terrain Camera images along the entire traverse11
The many ages of Triton: New crater counts on the Voyager high-resolution image sequence and implications for impactor provenance11
One dimension photochemical models in global mean conditions in question: Application to Titan11
A novel auger-based system for extraterrestrial in-situ water resource extraction11
Regions of slow apparent motion of close approaching asteroids: The case of 2019 OK11
A thermal origin for super-high-frequency marsquakes11
Venus’ upper atmosphere revealed by a GCM: I. Structure and variability of the circulation11
Rheological properties and ages of lava flows on Alba Mons, Mars11
Evidence of a Martian spatter cone south of Pavonis Mons11
The Mars Science Laboratory record of optical depth measurements via solar imaging11
Phase ratio in single-scattering dust particles: Implication to future DESTINY+ study of asteroid (3200) Phaethon11
Editorial Board11
The excited spin state of Dimorphos resulting from the DART impact11
High-velocity oblique impact experiments on ice and snow spheres: Implications for the collisional evolution of icy planetesimals at different thermal evolution stages11
Martian nonmigrating atmospheric tides in the thermosphere and ionosphere at solar minimum11
Reflectance spectra (1–5 μm) at low temperatures and different grain sizes of ammonium-bearing minerals relevant for icy bodies11
Measurement of D/H and 13C/12C ratios in methane ice on Eris and Makemake: Evidence for internal activity10
The impact of asteroid shapes and topographies on their reflectance spectroscopy10
Editorial Board10
Editorial Board10
Moats in the residual south polar cap of Mars: Ages, formation, and evolution10
Mie theory-based light scattering analysis of entrained grains in Io's Tvashtar plume observed during new horizons' 2007 flyby10
Spatial extent of dust storm boundaries in the Mars Dust Activity Database10
The effect of planetary flybys on singly synchronous binary asteroids10
Numerical model for the solidification of a chondrule melt10
Investigating the feasibility of an impact-induced Martian Dichotomy10
Lunar polar volatile remobilization in regolith-filled craters10
Characterising water in Lunar and Martian regolith materials using nuclear magnetic resonance10
Uranus and Neptune as methane planets: Producing icy giants from refractory planetesimals10
Update on SO2, detection of OCS, CS, CS2, and SO3, and upper limits of H2S and HOCl in the Venus mesosphere using SOIR on board Venus Express10
Ed. Board10
Gravitational disturbance on asteroidal ring systems by close encounter with a small object10
Tidal constraints on the low-viscosity zone of the Moon10
Molecular hydrogen in the upper atmospheres of Saturn and Titan10
Stationary dynamics of planetary ring edge modes at Saturn’s B ring edge10
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