Icarus

Papers
(The median citation count of Icarus is 3. 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 2021-06-01 to 2025-06-01.)
ArticleCitations
Morphological changes currently occurring in sand-filled gully channels on Mars: Implications for the role of substrates inside channels67
Multiscale spectral discrimination of poorly crystalline and intermixed alteration phases using aerial and ground-based ExoMars rover emulator data57
Evidence for landslides in Sisyphi Cavi (Noachis Terra, Mars): Slope evolution and role of endogenous preparatory factors57
Diffusion limited escape of hydrogen from Mars57
A case for young igneous volcanism in the Terra Sirenum region, Mars57
Optical observations and dust modelling of comet 156P/Russell-LINEAR54
Visible–near-infrared observations of organics and carbonates on (101955) Bennu: Classification method and search for surface context54
322P/SOHO: The counterpart of a historical comet in 254 CE?51
The yearly variability of the sodium exosphere of Mercury: A toy model49
Inferences of water–ice cloud physics determined from MAVEN/IUVS aerosol retrievals and Mars GCM comparisons48
Comparing the radiolytic oxidation of sulfur and chloride within ice on Europa and Mars45
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]45
Planet Four: A Neural Network’s search for polar spring-time fans on Mars43
An analogue study of impact craters on Titan: Implications for Titan's surface age43
Tectonic patterns on Vesta and Ceres revealed by polygonal impact craters42
Inversion of ultraviolet occultation profiles in a dusty atmosphere: Analytic and numerical methods41
Variations of the magnetic field and plasma parameters near the Martian induced magnetosphere boundary40
Machine learning as a tool to classify extra-terrestrial landslides: A dossier from Valles Marineris, Mars38
Three-dimensional characterization of particle size, shape, and internal porosity for Apollo 11 and Apollo 14 lunar regolith and JSC-1A lunar regolith soil simulant37
The annual cycle of water vapor above gale crater as retrieved by CRISM and compared to ChemCam passive sky spectroscopy36
Daily and seasonal processes shape hydrological activity and detectability of moisture in Antarctic, Mars-analog soils35
Seasonal variability of gravity wave activity in Mars's lower atmosphere from MGS–TES nadir observations35
Subglacial catastrophic-flood origin of linear and curvilinear flat-rimmed pit chains on Mars: Evidence from geomorphological mapping and detailed landsystem analysis34
Cosmic hydrogen and ice loss lines32
Shadow method retrievals of the atmospheric optical depth above Gale crater on Mars using HRSC images32
Simulation of surface regolith gardening and impact associated melt layer production under ns-pulsed laser ablation31
Lava flow ages in northeastern Oceanus Procellarum: The need for calibrating crater counting procedures30
An improved model of metal/silicate differentiation during Earth's accretion30
Elemental composition of manganese- and phosphorus-rich nodules in the Knockfarril Hill member, Gale crater, Mars29
The magnetic susceptibility of Pleistocene paleosols as a martian paleoenvironment analog27
Constraints on a potential aerial biosphere on Venus: II. Ultraviolet radiation27
Chaotic tides as a solution to the Hyperion problem26
Investigation of the shocked Viñales ordinary chondrite (L6) meteorite fall – Implications for shock classification, fragmentation, and collision dynamics26
Plenoptic imaging of meteorite shape change during plasma wind tunnel experiments26
Influence of hydrothermal asteroidal conditions on the molecular structure and isotopic compositions of polycyclic aromatic hydrocarbons26
Isolating the mechanisms for asteroid surface refreshing26
On a radiolytic origin of red organics at the surface of the Arrokoth Trans-Neptunian Object25
Long-period dynamical evolution of the meteoroid stream originating in comet 21P/Giacobini-Zinner25
Catastrophic rupture of lunar rocks: Implications for lunar rock size–frequency distributions24
Exosphere-mediated migration of volatile species on airless bodies across the solar system24
Dynamical evolution and thermal history of asteroids (3200) Phaethon and (155140) 2005 UD24
Exploring the variability of the venusian thermosphere with the IPSL Venus GCM23
Raman spectroscopic documentation of Mars analog basalt alteration by brines23
Influence of observed seasonally varying composition on Titan’s stratospheric circulation23
Comprehensive analysis of Chandrayaan-3 landing site region focussing on morphology, hydration and gravity anomalies23
Recent boulder falls within the Finsen crater on the lunar far side: An assessment of the possible triggering rationale23
Chronological and compositional mapping of the Mare Orientale basin using Chandrayaan-1 – M3 and LRO datasets23
The high-resolution imaging science experiment (HiRISE) in the MRO extended science phases (2009–2023)23
Formation of steep-sided domes on Venus via eruption of high crystallinity magmas23
Jovian current disk crossings as observed by Juno JADE-I23
How much earlier would LSST have discovered currently known long-period comets?22
Implications for the energy source for an early dynamo in Vesta from experiments on electrical resistivity of liquid Fe-10wt%Ni at high pressures22
Bayesian inference on the isotopic building blocks of Mars and Earth22
Submicroscopic iron-rich grains throughout impact glasses in Chang'E-5 regolith22
The influence of equation of state on impact dynamics between Pluto-like bodies21
MAVEN/IUVS observations of C I 156.1 nm and 165.7 nm dayglow: Direct detection of carbon and implications on photochemical escape21
3D morphometry of Martian craters from HRSC DEMs using a multi-scale semantic segmentation network and morphological analysis21
Chronology, composition, and mineralogy of mare basalts in the junction of Oceanus Procellarum, Mare Imbrium, Mare Insularum, and Mare Vaporum21
Asteroids were born bigger: An implication of surface mass ablation during gas-assisted implantation into the asteroid belt21
Do icy dust aggregates break up when they pass the snow line?21
Large volcanoes on Venus: Morphology, morphometry, and stratigraphy20
Analyzing spatial distributions and alignments of pitted cone features in Utopia Planitia on Mars20
Editorial Board20
Detailed chemical composition analysis of the Soi crater region on Titan20
The Martian ionosphere at solar minimum: Empirical model validation using MAVEN ROSE data20
Evidence for the protection of N-heterocycles from gamma radiation by Mars analogue minerals19
Range resolution enhancement of SHAllow RADar (SHARAD) data via bandwidth extrapolation technique: Enabling new features detection and improving geophysical investigation19
The effect of collisional erosion on the composition of Earth-analog planets in Grand Tack models: Implications for the formation of the Earth19
Impact strength of cm-to-decimeter scale weak porous targets: Implication for lifetime of boulders on asteroids19
Secondary craters reveal differences in neighboring geologic units: An example on Mars19
Vortex crystals at Jupiter’s poles: Emergence controlled by initial small-scale turbulence18
Non-LTE spectroscopy of the tetradecad region of methane recorded in a hypersonic flow18
The morphometry of small impact craters on Bennu: Relationships to geologic units, boulders, and impact armoring18
Possible formation pathways for zeolites in closed-basin lakes on noachian Mars: Insights from geochemical modeling18
Mineral abrasion experiments at Mars relevant temperatures18
Recent faulting at the Claritas Rupes scarp on Mars18
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
Ejecta cloud distributions for the statistical analysis of impact cratering events onto asteroids’ surfaces: A sensitivity analysis18
Latitudinal and radial dependence of the lunar sodium exospheric temperature and linewidths17
Saturn’s atmospheric response to the large influx of ring material inferred from Cassini INMS measurements17
A Mars orbital catalog of aqueous alteration signatures (MOCAAS)17
First quantitative characterization of the Martian dust devil dimensions determined from InSight data17
Venus upper atmosphere revealed by a GCM: II. Model validation with temperature and density measurements17
Two types of jarosite in the early Cambrian sedimentary rocks: Insights for genesis and transformation of jarosite on Mars17
Ricochets on asteroids II: Sensitivity of laboratory experiments of low velocity grazing impacts on substrate grain size17
Scaling of convection in high-pressure ice layers of large icy moons and implications for habitability17
The role of subsurface ocean dynamics and phase transitions in forming the topography of icy moons17
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
Modeling global-scale mass flows on the Lagrangian satellites of Dione and Tethys17
A new constraint on HCl abundance at the cloud top of Venus16
Preface: Ices in the Solar system; origin, evolution and distribution16
Dark primitive asteroids account for a large share of K/Pg-scale impacts on the Earth16
Aeolian bedrock ridges in Gale crater, Mars16
VIS-IR spectroscopy of magnesium chlorides at cryogenic temperatures16
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
Mars volatile inventory and outgassing history16
Ion density and phase space density distribution of planetary ions Na+, O+ and He+ in Mercury’s magnetosphere16
Non-thermal escape of the martian CO216
A contemporary view of the ordinary chondrite boot I: Band parameter analysis dependency16
Comparisons of the core and mantle compositions of earth analogs from different terrestrial planet formation scenarios16
Stochastic hyperbola fitting, probabilistic inversion, reverse-time migration and clustering: A novel interpretation toolbox for in-situ planetary radar15
Cross-attention induced multilayer domain adaptation network for extraction of sub-kilometer craters from HiRIC images15
Modeling of observations of the OH nightglow in the venusian mesosphere15
Integral equation modeling for dielectric retrieval of the lunar surface using Chandrayaan-2 fully-Polarimetric L-band dual frequency SAR (DFSAR) data15
Bulk composition and thermal evolution constrain the formation of organics in Ceres' subsurface ocean via geochemical modeling15
Present-day model of lunar meteoroids and their impact flashes for LUMIO mission15
Variability of temperatures and gravity wave activity in the Martian thermosphere during low solar irradiance15
Laser-Induced Breakdown Spectroscopy (LIBS) characterization of granular soils: Implications for ChemCam analyses at Gale crater, Mars15
A numerical model for the atmospheric entry of hydrated, phyllosilicate-rich micrometeorites15
Dark ray craters on Ganymede: Impactor or endogenous origin15
Identification of a new spectral signature at 3 μ15
Tidal dissipation within an elongated asteroid with satellite, and application to asteroid (216) Kleopatra15
Lunar elemental abundances as derived from Chandrayaan-215
Distribution of atmospheric aerosols during the 2007 Mars dust storm (MY 28): Solar infrared occultation observations by SPICAM15
Automatic crater shape retrieval using unsupervised and semi-supervised systems14
VNIR reflectance spectra of silicate-graphite mixtures: The effect of graphite content and particle size14
Observation of the Southern Polar cap during MY34-36 with ExoMars-TGO NOMAD LNO14
Surface grain size of alluvial fans on Mars from thermal inertia, as an indicator of depositional style14
A modeling approach for water and sediment transport in Jezero crater on Mars based on new geomorphological evidence14
Where on the Moon was the eruption that produced the recently reported ∼ 120 million year old volcanic glass beads?14
Compositional diversity in the Mare Marginis and Mare Smythii: An insight into the volcanism in the region14
Impact induced H2-rich climates on early Mars explored with a global climate model14
Three-dimensional imaging of martian glaciated terrain using Mars Reconnaissance Orbiter Shallow Radar (SHARAD) observations14
Ed. Board14
GOES GLM, biased bolides, and debiased distributions14
Separation of quasi-continuous and periodic components of lineament formation at the Belus – Phoenix - Rhadamanthys Linea “triangle” on Europa14
Evolution of impact-generated hydrothermal systems in basaltic targets on Earth and implications for habitats on Mars14
Moderate D/H ratios in methane ice on Eris and Makemake as evidence of hydrothermal or metamorphic processes in their interiors: Geochemical analysis14
Europa's hemispheric color dichotomy as a constraint on non-synchronous rotation14
Formation of the four terrestrial planets in the Jupiter–Saturn chaotic excitation scenario: fundamental properties and water delivery14
The upper-thermal stability of an iron-rich smectite: Implications for smectite formation on Mars14
Mare filled craters on the Moon14
Statistical chronometry of meteorites. I. A Test of 26Al homogeneity and the Pb-Pb age of the solar system’s 14
Ed. Board14
Large mass inflow rates in Saturn’s rings due to ballistic transport and mass loading14
Space weathering on inner planetary surface analogues induced by swift multicharged heavy ion bombardment14
Generation and evolution of laser-induced shock waves under martian atmospheric conditions14
Evidence for hydrated minerals in the VNIR spectra of G-class asteroids: A first look14
Mechanical behaviour of sulphur-based Martian regolith concrete processed under CO2-rich conditions14
The brightness of the CO Cameron bands in the martian discrete aurora: A study based on revised cross sections14
Variations in surface adsorbed H2O on lunar soils and relevant minerals14
Origin of ice in the Medusae Fossae Formation, equatorial Mars14
Thermal expansion of oldhamite, CaS: Implication for the surface of Mercury13
Characterization of aqueous alteration and formation of salty exposures at Ius Chasma, Mars13
Magnetically controlled ionosphere of Mars: A model analysis with the vertical plasma drift effects13
SPH simulations of high-speed collisions between asteroids and comets13
Igneous rock powder identification using colour cameras: A powerful method for space exploration13
On the cooling rate evolution of asteroid fragments13
Relationships between lobate debris aprons and lineated valley fill on Mars: Evidence for an extensive Amazonian valley glacial landsystem in Mamers Valles13
A new estimate for the age of highly-siderophile element retention in the lunar mantle from late accretion13
Illumination and regolith temperature for China's candidate lunar landing sites with multiple scattering considerations13
Bennu's global surface and two candidate sample sites characterized by spectral clustering of OSIRIS-REx multispectral images13
Corrigendum to ‘Oort Cloud and sednoid formation in an embedded cluster, II: Dynamics and orbital evolutions’ [Icarus 410 (2024) 115915]13
Uncovering Ganymede's past: Tectonics at Nippur/Philus Sulci13
Evidence for widely-separated binary asteroids recorded by craters on Mars13
Late drainage along portions of Samara Valles, West of Jones Crater, Margaritifer Terra, Mars13
The mystery of the missing mantle problem and insights from spectroscopy13
Alkali metal depletion in the deep Jovian atmosphere: The role of anions13
Ed. Board13
Possible polyphase periglaciation and glaciation adjacent to the Moreux impact-crater, Mars13
The unique spectral and geomorphological characteristics of pitted impact deposits associated with Marcia crater on Vesta13
Weakening of olivine by hydrogen implantation: Results of nano-indentation tests and some applications to planetary materials12
Rock size-frequency distribution analysis at the Zhurong landing site based on Navigation and Terrain Camera images along the entire traverse12
Feasibility of meteor surveying from a Venus orbiter12
Pluto's Sputnik basin as a peak-ring or multiring basin: A comparative study12
Ephemeris and hazard assessment for near-Earth asteroid (101955) Bennu based on OSIRIS-REx data12
Volatiles on Mercury: The case of hollows and the pyroclastic vent of Tyagaraja crater12
Pulsed plasma discharge effects on efficiency and rate of penetration of melt probes in ice12
Investigation of mineral assemblages in a newly identified endorheic playa near Huygens basin on Mars and their astrobiological implications12
A denser and elevated Martian nightside ionosphere during Mars season Ls 180–360°12
Selection of chemical species for Europa’s surface using Galileo/NIMS12
Exploring the dielectric loss of Martian regolith in the frequency domain using Zhurong radar data12
A reflectance calibration method for Multispectral Camera (MSCam) on the Zhurong rover12
Corrigendum to ‘Successes and challenges of factor analysis/target transformation application to visible-to-near-infrared hyperspectral data’: [Icarus 365 (2021) 114402]12
Global geologic map of asteroid (101955) Bennu indicates heterogeneous resurfacing in the past 500,000 years12
Phase ratio in single-scattering dust particles: Implication to future DESTINY+ study of asteroid (3200) Phaethon12
Prediction of the collisions of meteoroids originating in comet 21P/Giacobini-Zinner with the Mercury, Venus, and Mars12
Modification of icy planetesimals by early thermal evolution and collisions: Constraints for formation time and initial size of comets and small KBOs12
Chondrule formation via impact jetting in the icy outer solar system12
Morphologic differences in radial grooves on martian layered (fluidized) ejecta: Implications for emplacement processes and conditions12
Boulders on Mercury12
Pre and post-landing atmospheric optical depths at the Zhurong landing site on Mars retrieved using a single-image-based approach12
Rotational/divergent flow and energy conversion of thermal tides in a Venus general circulation model12
Modeling results for the composition and typology of non-primary venusian anorthosite12
Frequency-dependent Ganymede’s tidal Love number k12
Seepage-evaporation controlled depletion of initially water-filled reservoirs on Earth and Mars: Analytic versus HYDRUS modeling12
Absolute model ages of three craters in the vicinity of the Chang'E-5 landing site and their geologic implications12
Rotation period estimates for 14 asteroids with the Earth MOID less than 1.1 AU12
Water uptake by chlorate salts under Mars-relevant conditions12
Global characterization of the early-season dust storm of Mars year 3612
Overview of the MetSpec project - Artificial meteors in ground testing12
Martian cave detection via machine learning coupled with visible light imagery12
Geological analysis of the dome field in western Utopia Planitia, on Mars12
Characterising water in Lunar and Martian regolith materials using nuclear magnetic resonance11
Evidence of a Martian spatter cone south of Pavonis Mons11
A new perspective on Saturn’s polar vortices: Coupling the thermosphere and stratosphere11
Editorial Board11
An improved method combining Fisher transformation and multiple endmember spectral mixture analysis for lunar mineral abundance quantification using spectral data11
Elasticity of selected icy satellite candidate materials (CO2, C6H6, MgSO4·7H2O and CaSO4·2H2O) revisited by dispersion corrected density functional theory11
Particle sizes in Saturn’s rings from UVIS stellar occultations 2. Outlier Populations in the C ring and Cassini Division11
Simulated SPHEREx spectra of asteroids and their implications for asteroid size and reflectance estimation11
The origin of the high-TiO211
Venus’ upper atmosphere revealed by a GCM: I. Structure and variability of the circulation11
Unexpected mineral impact on organic evolution during simulated aqueous alteration in asteroids11
Excitation, emission, and synchronous fluorescence for astrochemical applications: Experiments and computer simulations of synchronous spectra of polycyclic aromatic hydrocarbons and their mixtures11
Ed. Board11
One dimension photochemical models in global mean conditions in question: Application to Titan11
High-velocity oblique impact experiments on ice and snow spheres: Implications for the collisional evolution of icy planetesimals at different thermal evolution stages11
A novel auger-based system for extraterrestrial in-situ water resource extraction11
The many ages of Triton: New crater counts on the Voyager high-resolution image sequence and implications for impactor provenance11
Editorial Board11
Lifetime of cm-sized zodiacal dust from the physical and dynamical evolution of meteoroid streams11
The Mars Science Laboratory record of optical depth measurements via solar imaging11
Evidence that Earth’s magnetotail affects dielectric breakdown weathering on the Moon11
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
A thermal origin for super-high-frequency marsquakes11
Automatic mapping and spatial analysis of high spatial resolution closed terrain depressions and mounds on martian landscapes11
NEOExchange - an online portal for NEO and Solar System science11
Editorial Board11
Martian nonmigrating atmospheric tides in the thermosphere and ionosphere at solar minimum11
Thermodynamic modeling of calcium or magnesium chloride, chlorate, and perchlorate ternary mixtures deliquescence at Mars-relevant temperatures11
Reflectance spectra (1–5 μm) at low temperatures and different grain sizes of ammonium-bearing minerals relevant for icy bodies11
Rheological properties and ages of lava flows on Alba Mons, Mars11
Ejecta distribution and momentum transfer from oblique impacts on asteroid surfaces11
The density structure of Titan’s outer ice shell11
The excited spin state of Dimorphos resulting from the DART impact11
Three-dimensional imaging of high-velocity-impact induced crack growth in carbonaceous meteorites11
Laboratory measurements of the 15–46 cm wavelength opacity of water vapor under temperature conditions characteristic of the deep atmosphere of Jupiter11
Geological mapping and chronology of lunar landing sites: Apollo 1411
Regions of slow apparent motion of close approaching asteroids: The case of 2019 OK11
Corrigendum to “The Activity of Comet 29P/Schwassmann–Wachmann 1 Monitored through Its CO J=2→1 Radio Line” [Icarus Volume 150, Issue 1, March 2001, Pages 140–150]10
Moats in the residual south polar cap of Mars: Ages, formation, and evolution10
Characterization of groundwater chemistry beneath Gale Crater on early Mars by hydrothermal experiments10
Possible particle ejection contributions to the shape and spin stability of small near-Earth asteroids10
Rapid rounding of icy clasts during simulated fluvial transport in the Titan Tumbler10
Investigation of the incremental benefits of eccentric collisions in kinetic deflection of potentially hazardous asteroids10
Preliminary investigation of debris propagation dynamics in the Jovian system using the circular restricted 3- and N-body problems10
Topographic response to ocean heat flux anomaly on the icy moons of Jupiter and Saturn10
Lunar polar volatile remobilization in regolith-filled craters10
Random models for exploring planet compositions I: Uranus as an example10
Tracing seasonal trends across Pluto’s craters: New Horizons Ralph/MVIC results10
Composition variations of major lunar elements: Possible impacts on lunar albedo spectra10
Astrometric observations of Phoebe from 2010 to 2019 based on Gaia DR310
New and improved orbits of some historical comets: 6TH and 7TH centuries10
Geomorphic analysis of lobate debris aprons on Pluto from New Horizons images10
Assessment and review of modern lunar crescent visibility criterion10
Investigating the most promising Yarkovsky candidates using Gaia DR2 astrometry10
A photometric study of members of the NEOs Atiras population10
Quantification of amorphous Si, Al, and Fe in palagonitic Mars analogs by chemical extraction and X-ray spectroscopy10
Volatile transport modeling on Triton with new observational constraints10
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