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 2021-11-01 to 2025-11-01.)
ArticleCitations
An analogue study of impact craters on Titan: Implications for Titan's surface age79
Inversion of ultraviolet occultation profiles in a dusty atmosphere: Analytic and numerical methods72
Formation of steep-sided domes on Venus via eruption of high crystallinity magmas69
A case for young igneous volcanism in the Terra Sirenum region, Mars67
322P/SOHO: The counterpart of a historical comet in 254 CE?63
Inferences of water–ice cloud physics determined from MAVEN/IUVS aerosol retrievals and Mars GCM comparisons60
Exosphere-mediated migration of volatile species on airless bodies across the solar system59
Tectonic patterns on Vesta and Ceres revealed by polygonal impact craters59
Seasonal variability of gravity wave activity in Mars's lower atmosphere from MGS–TES nadir observations56
Catastrophic rupture of lunar rocks: Implications for lunar rock size–frequency distributions51
Machine learning as a tool to classify extra-terrestrial landslides: A dossier from Valles Marineris, Mars51
The yearly variability of the sodium exosphere of Mercury: A toy model51
Lava flow ages in northeastern Oceanus Procellarum: The need for calibrating crater counting procedures47
On a radiolytic origin of red organics at the surface of the Arrokoth Trans-Neptunian Object45
Exploring the variability of the venusian thermosphere with the IPSL Venus GCM44
Phosphates reveal high pH ocean water on Enceladus42
Bayesian inference on the isotopic building blocks of Mars and Earth41
Elemental composition of manganese- and phosphorus-rich nodules in the Knockfarril Hill member, Gale crater, Mars36
Chronological and compositional mapping of the Mare Orientale basin using Chandrayaan-1 – M3 and LRO datasets35
Morphological changes currently occurring in sand-filled gully channels on Mars: Implications for the role of substrates inside channels35
Submicroscopic iron-rich grains throughout impact glasses in Chang'E-5 regolith35
Subglacial catastrophic-flood origin of linear and curvilinear flat-rimmed pit chains on Mars: Evidence from geomorphological mapping and detailed landsystem analysis34
The magnetic susceptibility of Pleistocene paleosols as a martian paleoenvironment analog34
Influence of observed seasonally varying composition on Titan’s stratospheric circulation34
The annual cycle of water vapor above gale crater as retrieved by CRISM and compared to ChemCam passive sky spectroscopy33
Shadow method retrievals of the atmospheric optical depth above Gale crater on Mars using HRSC images32
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]31
Visible–near-infrared observations of organics and carbonates on (101955) Bennu: Classification method and search for surface context30
Isolating the mechanisms for asteroid surface refreshing30
Long-period dynamical evolution of the meteoroid stream originating in comet 21P/Giacobini-Zinner29
Raman spectroscopic documentation of Mars analog basalt alteration by brines29
Variations of the magnetic field and plasma parameters near the Martian induced magnetosphere boundary28
Planet Four: A Neural Network’s search for polar spring-time fans on Mars28
An improved model of metal/silicate differentiation during Earth's accretion27
Plenoptic imaging of meteorite shape change during plasma wind tunnel experiments27
Chaotic tides as a solution to the Hyperion problem27
Comparing the radiolytic oxidation of sulfur and chloride within ice on Europa and Mars27
Identification of H2O ice at lunar south polar region based on deep learning26
Diffusion limited escape of hydrogen from Mars26
Recent boulder falls within the Finsen crater on the lunar far side: An assessment of the possible triggering rationale26
Daily and seasonal processes shape hydrological activity and detectability of moisture in Antarctic, Mars-analog soils25
New candidate cave entrances on the Moon found using deep learning25
The high-resolution imaging science experiment (HiRISE) in the MRO extended science phases (2009–2023)25
Simulation of surface regolith gardening and impact associated melt layer production under ns-pulsed laser ablation25
Landslide chronology on mars: A window into the past of Valles Marineris and martian slopes24
Cosmic hydrogen and ice loss lines24
Editorial Board24
Investigation of the shocked Viñales ordinary chondrite (L6) meteorite fall – Implications for shock classification, fragmentation, and collision dynamics23
Optical observations and dust modelling of comet 156P/Russell-LINEAR23
Evidence for landslides in Sisyphi Cavi (Noachis Terra, Mars): Slope evolution and role of endogenous preparatory factors23
Jovian current disk crossings as observed by Juno JADE-I22
Comprehensive analysis of Chandrayaan-3 landing site region focussing on morphology, hydration and gravity anomalies22
Insights into pyroxene-dominated surfaces and implications for ongoing space exploration missions22
Three-dimensional characterization of particle size, shape, and internal porosity for Apollo 11 and Apollo 14 lunar regolith and JSC-1A lunar regolith soil simulant22
Implications for the energy source for an early dynamo in Vesta from experiments on electrical resistivity of liquid Fe-10wt%Ni at high pressures22
Influence of hydrothermal asteroidal conditions on the molecular structure and isotopic compositions of polycyclic aromatic hydrocarbons22
Editorial Board21
The Martian ionosphere at solar minimum: Empirical model validation using MAVEN ROSE data21
Do icy dust aggregates break up when they pass the snow line?21
Asteroids were born bigger: An implication of surface mass ablation during gas-assisted implantation into the asteroid belt21
Constraints on a potential aerial biosphere on Venus: II. Ultraviolet radiation21
The effect of collisional erosion on the composition of Earth-analog planets in Grand Tack models: Implications for the formation of the Earth20
Ricochets on asteroids II: Sensitivity of laboratory experiments of low velocity grazing impacts on substrate grain size20
The influence of equation of state on impact dynamics between Pluto-like bodies20
Large volcanoes on Venus: Morphology, morphometry, and stratigraphy20
Non-thermal escape of the martian CO220
First quantitative characterization of the Martian dust devil dimensions determined from InSight data20
Detailed chemical composition analysis of the Soi crater region on Titan19
Mineral abrasion experiments at Mars relevant temperatures19
Laboratory experiments on the visible to near- infrared (VNIR) spectroscopy of water ice and lunar highland simulant mixtures: Effects of particle size, particle shape, phase angle, and ice abundance19
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 roll19
Vortex crystals at Jupiter’s poles: Emergence controlled by initial small-scale turbulence19
The effects of CO2 clouds on the thermal structure of the early Martian atmosphere19
Impact strength of cm-to-decimeter scale weak porous targets: Implication for lifetime of boulders on asteroids19
Recent faulting at the Claritas Rupes scarp on Mars19
Photochemistry of benzene (C6H6) hydrogen cyanide (HCN) co-condensed ices part 2: Formation of aerosols analogues of titan's atmosphere19
Secondary craters reveal differences in neighboring geologic units: An example on Mars18
Non-LTE spectroscopy of the tetradecad region of methane recorded in a hypersonic flow18
Range resolution enhancement of SHAllow RADar (SHARAD) data via bandwidth extrapolation technique: Enabling new features detection and improving geophysical investigation18
Two types of jarosite in the early Cambrian sedimentary rocks: Insights for genesis and transformation of jarosite on Mars18
MAVEN/IUVS observations of C I 156.1 nm and 165.7 nm dayglow: Direct detection of carbon and implications on photochemical escape18
Evidence for the protection of N-heterocycles from gamma radiation by Mars analogue minerals18
Latitudinal and radial dependence of the lunar sodium exospheric temperature and linewidths17
A new constraint on HCl abundance at the cloud top of Venus17
Possible formation pathways for zeolites in closed-basin lakes on noachian Mars: Insights from geochemical modeling17
The role of subsurface ocean dynamics and phase transitions in forming the topography of icy moons17
Modeling global-scale mass flows on the Lagrangian satellites of Dione and Tethys17
How much earlier would LSST have discovered currently known long-period comets?17
A Mars orbital catalog of aqueous alteration signatures (MOCAAS)17
Ejecta cloud distributions for the statistical analysis of impact cratering events onto asteroids’ surfaces: A sensitivity analysis17
Saturn’s atmospheric response to the large influx of ring material inferred from Cassini INMS measurements17
3D morphometry of Martian craters from HRSC DEMs using a multi-scale semantic segmentation network and morphological analysis17
Scaling of convection in high-pressure ice layers of large icy moons and implications for habitability17
Analyzing spatial distributions and alignments of pitted cone features in Utopia Planitia on Mars17
Ion density and phase space density distribution of planetary ions Na+, O+ and He+ in Mercury’s magnetosphere17
The morphometry of small impact craters on Bennu: Relationships to geologic units, boulders, and impact armoring17
Chronology, composition, and mineralogy of mare basalts in the junction of Oceanus Procellarum, Mare Imbrium, Mare Insularum, and Mare Vaporum16
A contemporary view of the ordinary chondrite boot I: Band parameter analysis dependency16
GOES GLM, biased bolides, and debiased distributions16
Evolution of impact-generated hydrothermal systems in basaltic targets on Earth and implications for habitats on Mars16
Modeling of observations of the OH nightglow in the venusian mesosphere16
The brightness of the CO Cameron bands in the martian discrete aurora: A study based on revised cross sections16
VIS-IR spectroscopy of magnesium chlorides at cryogenic temperatures16
Evidence for hydrated minerals in the VNIR spectra of G-class asteroids: A first look16
Cross-attention induced multilayer domain adaptation network for extraction of sub-kilometer craters from HiRIC images16
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
Physical properties of subsurface water ice deposits in Mars’s Mid-Latitudes from the shallow radar16
Lunar elemental abundances as derived from Chandrayaan-216
Preface: Ices in the Solar system; origin, evolution and distribution16
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 cerium16
Separation of quasi-continuous and periodic components of lineament formation at the Belus – Phoenix - Rhadamanthys Linea “triangle” on Europa16
Variations in surface adsorbed H2O on lunar soils and relevant minerals16
Stochastic hyperbola fitting, probabilistic inversion, reverse-time migration and clustering: A novel interpretation toolbox for in-situ planetary radar16
Bulk composition and thermal evolution constrain the formation of organics in Ceres' subsurface ocean via geochemical modeling15
A numerical model for the atmospheric entry of hydrated, phyllosilicate-rich micrometeorites15
Statistical chronometry of meteorites. I. A Test of 26Al homogeneity and the Pb-Pb age of the solar system’s 15
Observation of the Southern Polar cap during MY34-36 with ExoMars-TGO NOMAD LNO15
Present-day model of lunar meteoroids and their impact flashes for LUMIO mission15
Tidal dissipation within an elongated asteroid with satellite, and application to asteroid (216) Kleopatra15
Space weathering on inner planetary surface analogues induced by swift multicharged heavy ion bombardment15
Where on the Moon was the eruption that produced the recently reported ∼ 120 million year old volcanic glass beads?15
Compositional diversity in the Mare Marginis and Mare Smythii: An insight into the volcanism in the region15
Mars volatile inventory and outgassing history15
Variability of temperatures and gravity wave activity in the Martian thermosphere during low solar irradiance15
Large mass inflow rates in Saturn’s rings due to ballistic transport and mass loading15
The upper-thermal stability of an iron-rich smectite: Implications for smectite formation on Mars15
Moderate D/H ratios in methane ice on Eris and Makemake as evidence of hydrothermal or metamorphic processes in their interiors: Geochemical analysis15
Dark ray craters on Ganymede: Impactor or endogenous origin15
VNIR reflectance spectra of silicate-graphite mixtures: The effect of graphite content and particle size15
Integral equation modeling for dielectric retrieval of the lunar surface using Chandrayaan-2 fully-Polarimetric L-band dual frequency SAR (DFSAR) data14
Corrigendum to ‘Oort Cloud and sednoid formation in an embedded cluster, II: Dynamics and orbital evolutions’ [Icarus 410 (2024) 115915]14
Identification of a new spectral signature at 3 μ14
Impact induced H2-rich climates on early Mars explored with a global climate model14
Formation of the four terrestrial planets in the Jupiter–Saturn chaotic excitation scenario: fundamental properties and water delivery14
Ed. Board14
SPH simulations of high-speed collisions between asteroids and comets14
Effects of observation geometry and heating on the ultra-violet to near-infrared spectra of Mercury simulant14
Interaction between oppositely signed vortices on adjacent domains in Jupiter14
A modeling approach for water and sediment transport in Jezero crater on Mars based on new geomorphological evidence14
Dark primitive asteroids account for a large share of K/Pg-scale impacts on the Earth14
Mechanical behaviour of sulphur-based Martian regolith concrete processed under CO2-rich conditions14
Alkali metal depletion in the deep Jovian atmosphere: The role of anions14
Relationships between lobate debris aprons and lineated valley fill on Mars: Evidence for an extensive Amazonian valley glacial landsystem in Mamers Valles14
On the cooling rate evolution of asteroid fragments14
Igneous rock powder identification using colour cameras: A powerful method for space exploration14
Dimension-ratio-based observability analysis of asteroid photometric model and optimization strategy for completely observable satellite detection14
Distribution of atmospheric aerosols during the 2007 Mars dust storm (MY 28): Solar infrared occultation observations by SPICAM14
Surface grain size of alluvial fans on Mars from thermal inertia, as an indicator of depositional style14
Generation and evolution of laser-induced shock waves under martian atmospheric conditions14
Comparisons of the core and mantle compositions of earth analogs from different terrestrial planet formation scenarios14
Prediction of the collisions of meteoroids originating in comet 21P/Giacobini-Zinner with the Mercury, Venus, and Mars14
Evidence for widely-separated binary asteroids recorded by craters on Mars14
Ed. Board14
The unique spectral and geomorphological characteristics of pitted impact deposits associated with Marcia crater on Vesta14
Ed. Board14
Aeolian bedrock ridges in Gale crater, Mars14
Characterization of aqueous alteration and formation of salty exposures at Ius Chasma, Mars13
Volatiles on Mercury: The case of hollows and the pyroclastic vent of Tyagaraja crater13
Illumination and regolith temperature for China's candidate lunar landing sites with multiple scattering considerations13
Ephemeris and hazard assessment for near-Earth asteroid (101955) Bennu based on OSIRIS-REx data13
Contribution of multiple scattering to the Lyman alpha radiance distribution in cometary comae13
Global geologic map of asteroid (101955) Bennu indicates heterogeneous resurfacing in the past 500,000 years13
Frequency-dependent Ganymede’s tidal Love number k13
Evidence that Earth’s magnetotail affects dielectric breakdown weathering on the Moon13
Three-dimensional imaging of martian glaciated terrain using Mars Reconnaissance Orbiter Shallow Radar (SHARAD) observations13
Absolute model ages of three craters in the vicinity of the Chang'E-5 landing site and their geologic implications13
Water uptake by chlorate salts under Mars-relevant conditions13
Pre and post-landing atmospheric optical depths at the Zhurong landing site on Mars retrieved using a single-image-based approach13
Automatic crater shape retrieval using unsupervised and semi-supervised systems13
Late drainage along portions of Samara Valles, West of Jones Crater, Margaritifer Terra, Mars13
Magnetically controlled ionosphere of Mars: A model analysis with the vertical plasma drift effects13
Uncovering Ganymede's past: Tectonics at Nippur/Philus Sulci13
How does topography affect wind abrasion on Mars? Recently observed shifts in ventifact orientation at Gale crater13
Investigation of mineral assemblages in a newly identified endorheic playa near Huygens basin on Mars and their astrobiological implications13
Weakening of olivine by hydrogen implantation: Results of nano-indentation tests and some applications to planetary materials13
Overview of the MetSpec project - Artificial meteors in ground testing13
Feasibility of meteor surveying from a Venus orbiter13
Selection of chemical species for Europa’s surface using Galileo/NIMS13
Global characterization of the early-season dust storm of Mars year 3613
Geological analysis of the dome field in western Utopia Planitia, on Mars13
The mystery of the missing mantle problem and insights from spectroscopy13
The origin of the high-TiO213
Outcrop scale evidence of late-fluid flows and secondary sulfate minerals on exhumed surfaces – Earth versus Mars comparison13
Lifetime of cm-sized zodiacal dust from the physical and dynamical evolution of meteoroid streams13
Thermal expansion of oldhamite, CaS: Implication for the surface of Mercury13
Martian cave detection via machine learning coupled with visible light imagery13
Mare filled craters on the Moon13
Origin of ice in the Medusae Fossae Formation, equatorial Mars13
An improved method combining Fisher transformation and multiple endmember spectral mixture analysis for lunar mineral abundance quantification using spectral data12
Adaptive isoline interval optimization for precise contour segmentation and instance-level detection of Martian impact craters12
A denser and elevated Martian nightside ionosphere during Mars season Ls 180–360°12
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 imaging12
Ejecta distribution and momentum transfer from oblique impacts on asteroid surfaces12
Three-dimensional imaging of high-velocity-impact induced crack growth in carbonaceous meteorites12
Chondrule formation via impact jetting in the icy outer solar system12
Corrigendum to ‘Successes and challenges of factor analysis/target transformation application to visible-to-near-infrared hyperspectral data’: [Icarus 365 (2021) 114402]12
Phase ratio in single-scattering dust particles: Implication to future DESTINY+ study of asteroid (3200) Phaethon12
The many ages of Triton: New crater counts on the Voyager high-resolution image sequence and implications for impactor provenance12
Automatic mapping and spatial analysis of high spatial resolution closed terrain depressions and mounds on martian landscapes12
Rheological properties and ages of lava flows on Alba Mons, Mars12
Simulated SPHEREx spectra of asteroids and their implications for asteroid size and reflectance estimation12
Activity in quasi-Hilda objects: A photometric approach12
Boulders on Mercury12
Editorial Board12
Exploring the dielectric loss of Martian regolith in the frequency domain using Zhurong radar data12
Pluto's Sputnik basin as a peak-ring or multiring basin: A comparative study12
Pulsed plasma discharge effects on efficiency and rate of penetration of melt probes in ice12
Rock size-frequency distribution analysis at the Zhurong landing site based on Navigation and Terrain Camera images along the entire traverse12
The Mars Science Laboratory record of optical depth measurements via solar imaging12
Ionosphere of Mars during the consecutive solar minima 23/24 and 24/25 as seen by MARSIS-Mars Express12
A numerical study of the liquid motion in Titan’s subsurface ocean12
High-velocity oblique impact experiments on ice and snow spheres: Implications for the collisional evolution of icy planetesimals at different thermal evolution stages12
Regolith properties and Stokes vector radar polarimetry models for the moon12
Seepage-evaporation controlled depletion of initially water-filled reservoirs on Earth and Mars: Analytic versus HYDRUS modeling12
A new perspective on Saturn’s polar vortices: Coupling the thermosphere and stratosphere12
The excited spin state of Dimorphos resulting from the DART impact12
Ed. Board12
A reflectance calibration method for Multispectral Camera (MSCam) on the Zhurong rover12
Volcanic gas plumes’ effect on the spectrum of Venus12
Rotation period estimates for 14 asteroids with the Earth MOID less than 1.1 AU12
Particle sizes in Saturn’s rings from UVIS stellar occultations 2. Outlier Populations in the C ring and Cassini Division12
Rotational/divergent flow and energy conversion of thermal tides in a Venus general circulation model12
Unexpected mineral impact on organic evolution during simulated aqueous alteration in asteroids12
Regions of slow apparent motion of close approaching asteroids: The case of 2019 OK12
Martian nonmigrating atmospheric tides in the thermosphere and ionosphere at solar minimum11
Measurement of D/H and 13C/12C ratios in methane ice on Eris and Makemake: Evidence for internal activity11
Complex Ice Chemistry: A comparative study of electron irradiated planetary ice analogues containing methane11
Editorial Board11
Numerical model for the solidification of a chondrule melt11
Uranus and Neptune as methane planets: Producing icy giants from refractory planetesimals11
Excitation, emission, and synchronous fluorescence for astrochemical applications: Experiments and computer simulations of synchronous spectra of polycyclic aromatic hydrocarbons and their mixtures11
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 Express11
A thermal origin for super-high-frequency marsquakes11
Editorial Board11
Impact of UV radiation on the Raman and infrared spectral signatures of sulfates, phosphates and carbonates: Implications for Mars exploration11
Early bombardment of the moon: Connecting the lunar crater record to the terrestrial planet formation11
High alumina basalts identification and their feature analysis in Mare Fecunditatis11
The impact of asteroid shapes and topographies on their reflectance spectroscopy11
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
Mie theory-based light scattering analysis of entrained grains in Io's Tvashtar plume observed during new horizons' 2007 flyby11
Characterising water in Lunar and Martian regolith materials using nuclear magnetic resonance11
Laboratory measurements of the 15–46 cm wavelength opacity of water vapor under temperature conditions characteristic of the deep atmosphere of Jupiter11
A new method to improve the detection rate and astrometric accuracy of natural satellites located in the halo of Uranus11
Principal Component Analysis applied on MASCS/MESSENGER data for the spectral investigation of Mercury's surface11
Observations of alkaline emissions NaI, KI and LiI during first minutes after DART probe impact on Dimorphos11
Elasticity of selected icy satellite candidate materials (CO2, C6H6, MgSO4·7H2O and CaSO4·2H2O) revisited by dispersion corrected density functional theory11
Spatial extent of dust storm boundaries in the Mars Dust Activity Database11
Evidence of a Martian spatter cone south of Pavonis Mons11
Geological mapping and chronology of lunar landing sites: Apollo 1411
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