Icarus

Papers
(The TQCC of Icarus is 8. 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 2022-08-01 to 2026-08-01.)
ArticleCitations
Inversion of ultraviolet occultation profiles in a dusty atmosphere: Analytic and numerical methods95
322P/SOHO: The counterpart of a historical comet in 254 CE?83
Planet Four: A Neural Network’s search for polar spring-time fans on Mars76
Comparing the radiolytic oxidation of sulfur and chloride within ice on Europa and Mars69
Editorial Board65
Cosmic hydrogen and ice loss lines54
An analogue study of impact craters on Titan: Implications for Titan's surface age51
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]50
Long-period dynamical evolution of the meteoroid stream originating in comet 21P/Giacobini-Zinner50
Influence of hydrothermal asteroidal conditions on the molecular structure and isotopic compositions of polycyclic aromatic hydrocarbons47
Subglacial catastrophic-flood origin of linear and curvilinear flat-rimmed pit chains on Mars: Evidence from geomorphological mapping and detailed landsystem analysis44
Jovian upper clouds and hazes from visible and near infrared spectroscopy using CARMENES43
Raman spectroscopic documentation of Mars analog basalt alteration by brines43
The 3D subsurface structures of the Atlas impact crater revealed by GRAIL gravity data41
Variations of the magnetic field and plasma parameters near the Martian induced magnetosphere boundary41
Morphological changes currently occurring in sand-filled gully channels on Mars: Implications for the role of substrates inside channels40
A dual-branch automatic classification network for lunar simple crater degradation grades integrating image and morphological parameters38
Shadow method retrievals of the atmospheric optical depth above Gale crater on Mars using HRSC images38
Drying induces Mars intermediate-sized cracks: New evidence and insight from geometrical quantification36
Investigation of the shocked Viñales ordinary chondrite (L6) meteorite fall – Implications for shock classification, fragmentation, and collision dynamics35
An integrated study of Rutherfurd crater: Composition, morphology, and chronology35
Insights into pyroxene-dominated surfaces and implications for ongoing space exploration missions34
Using surface displacements to probe Venus’ interior structure and atmospheric dynamics34
Corrigendum to “On the forced orbital plane of the Hilda asteroids” Icarus 49 (2026), 11695934
Landslide chronology on mars: A window into the past of Valles Marineris and martian slopes33
Exosphere-mediated migration of volatile species on airless bodies across the solar system33
The magnetic susceptibility of Pleistocene paleosols as a martian paleoenvironment analog33
New candidate cave entrances on the Moon found using deep learning32
Plenoptic imaging of meteorite shape change during plasma wind tunnel experiments31
Comprehensive analysis of Chandrayaan-3 landing site region focussing on morphology, hydration and gravity anomalies31
The annual cycle of water vapor above gale crater as retrieved by CRISM and compared to ChemCam passive sky spectroscopy30
Catastrophic rupture of lunar rocks: Implications for lunar rock size–frequency distributions30
Optical observations and dust modelling of comet 156P/Russell-LINEAR30
Chaotic tides as a solution to the Hyperion problem29
Evidence for landslides in Sisyphi Cavi (Noachis Terra, Mars): Slope evolution and role of endogenous preparatory factors29
Phosphates reveal high pH ocean water on Enceladus29
Diffusion limited escape of hydrogen from Mars27
Simulation of surface regolith gardening and impact associated melt layer production under ns-pulsed laser ablation27
Elemental composition of manganese- and phosphorus-rich nodules in the Knockfarril Hill member, Gale crater, Mars27
Submicroscopic iron-rich grains throughout impact glasses in Chang'E-5 regolith27
Jovian current disk crossings as observed by Juno JADE-I26
Seasonal variability of gravity wave activity in Mars's lower atmosphere from MGS–TES nadir observations26
A case for young igneous volcanism in the Terra Sirenum region, Mars26
Influence of observed seasonally varying composition on Titan’s stratospheric circulation26
An improved model of metal/silicate differentiation during Earth's accretion26
Iron isotope anomalies and the origin of the Earth25
Isolating the mechanisms for asteroid surface refreshing25
Inferences of water–ice cloud physics determined from MAVEN/IUVS aerosol retrievals and Mars GCM comparisons25
Bayesian inference on the isotopic building blocks of Mars and Earth25
Physical properties of accessible Near Earth Objects, including the primitive (68278) 2001 FC725
The yearly variability of the sodium exosphere of Mercury: A toy model25
Tectonic patterns on Vesta and Ceres revealed by polygonal impact craters24
Formation of steep-sided domes on Venus via eruption of high crystallinity magmas24
Identification of H2O ice at lunar south polar region based on deep learning24
The high-resolution imaging science experiment (HiRISE) in the MRO extended science phases (2009–2023)24
On a radiolytic origin of red organics at the surface of the Arrokoth Trans-Neptunian Object24
Exploring the variability of the venusian thermosphere with the IPSL Venus GCM23
Three-dimensional characterization of particle size, shape, and internal porosity for Apollo 11 and Apollo 14 lunar regolith and JSC-1A lunar regolith soil simulant23
Photochemistry of benzene (C6H6) hydrogen cyanide (HCN) co-condensed ices part 2: Formation of aerosols analogues of titan's atmosphere22
Editorial Board22
A new constraint on HCl abundance at the cloud top of Venus22
The effect of collisional erosion on the composition of Earth-analog planets in Grand Tack models: Implications for the formation of the Earth22
Ejecta cloud distributions for the statistical analysis of impact cratering events onto asteroids’ surfaces: A sensitivity analysis22
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 roll22
Range resolution enhancement of SHAllow RADar (SHARAD) data via bandwidth extrapolation technique: Enabling new features detection and improving geophysical investigation21
Mineral abrasion experiments at Mars relevant temperatures21
Chronology, composition, and mineralogy of mare basalts in the junction of Oceanus Procellarum, Mare Imbrium, Mare Insularum, and Mare Vaporum21
How much earlier would LSST have discovered currently known long-period comets?21
Characterising the efficiency of the hierarchical clustering method21
Do icy dust aggregates break up when they pass the snow line?21
First quantitative characterization of the Martian dust devil dimensions determined from InSight data21
Dyke swarm history of Eastern Eistla Regio, Venus and implications for its plume origin20
Secondary craters reveal differences in neighboring geologic units: An example on Mars20
Recent faulting at the Claritas Rupes scarp on Mars20
A reappraisal of the amorphization kinetics of water ice: Combined experimental and numerical investigations and amorphization cross-sections in the 90–120 K range20
Vortex crystals at Jupiter’s poles: Emergence controlled by initial small-scale turbulence20
New surface composition and temperature maps of Pluto from New Horizons LEISA data20
The effects of CO2 clouds on the thermal structure of the early Martian atmosphere20
Non-LTE spectroscopy of the tetradecad region of methane recorded in a hypersonic flow20
Saturn’s atmospheric response to the large influx of ring material inferred from Cassini INMS measurements19
Analyzing spatial distributions and alignments of pitted cone features in Utopia Planitia on Mars19
Scaling of convection in high-pressure ice layers of large icy moons and implications for habitability19
Near-Earth Asteroid orbit determination with Physics-Informed Extreme Learning Machine19
Possible formation pathways for zeolites in closed-basin lakes on noachian Mars: Insights from geochemical modeling19
Evaluation of the effects of meteoroid impacts on properties of the Hermean exosphere19
Latitudinal and radial dependence of the lunar sodium exospheric temperature and linewidths19
Sound velocities of Anorthite at high pressures and temperatures: Implications for estimating porosity in upper lunar crust19
Impact strength of cm-to-decimeter scale weak porous targets: Implication for lifetime of boulders on asteroids19
A Mars orbital catalog of aqueous alteration signatures (MOCAAS)19
The role of subsurface ocean dynamics and phase transitions in forming the topography of icy moons19
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
The Martian ionosphere at solar minimum: Empirical model validation using MAVEN ROSE data19
Validation of SPH code Spheral to model interacting solid bodies in a supersonic flow19
Non-thermal escape of the martian CO218
The morphometry of small impact craters on Bennu: Relationships to geologic units, boulders, and impact armoring18
3D morphometry of Martian craters from HRSC DEMs using a multi-scale semantic segmentation network and morphological analysis18
Preface: Ices in the Solar system; origin, evolution and distribution18
Distal impact-related surface flows associated with the well-preserved Tokmok Crater, Noachis Terra, Mars18
Large volcanoes on Venus: Morphology, morphometry, and stratigraphy18
Where on the Moon was the eruption that produced the recently reported ∼ 120 million year old volcanic glass beads?18
Detailed chemical composition analysis of the Soi crater region on Titan18
Asteroids were born bigger: An implication of surface mass ablation during gas-assisted implantation into the asteroid belt18
Comparisons of the core and mantle compositions of earth analogs from different terrestrial planet formation scenarios18
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 cerium18
Mechanical behaviour of sulphur-based Martian regolith concrete processed under CO2-rich conditions17
The photochemistry of irradiated Enceladus ice analogues: Implications for the formation of ozone and carbon trioxide17
Interaction between oppositely signed vortices on adjacent domains in Jupiter17
Observation of the Southern Polar cap during MY34-36 with ExoMars-TGO NOMAD LNO17
Micro-FTIR reflectance spectroscopy of Ryugu, CI chondrites and volatile-rich clasts – Comparing spectral features in the Mid-IR (2.5–16.5 μm) region17
Moderate D/H ratios in methane ice on Eris and Makemake as evidence of hydrothermal or metamorphic processes in their interiors: Geochemical analysis17
Tidal dissipation within an elongated asteroid with satellite, and application to asteroid (216) Kleopatra17
Variability of temperatures and gravity wave activity in the Martian thermosphere during low solar irradiance17
Compositional diversity in the Mare Marginis and Mare Smythii: An insight into the volcanism in the region17
Dark ray craters on Ganymede: Impactor or endogenous origin17
A numerical model for the atmospheric entry of hydrated, phyllosilicate-rich micrometeorites17
Statistical chronometry of meteorites. I. A Test of 26Al homogeneity and the Pb-Pb age of the solar system’s 17
Integral equation modeling for dielectric retrieval of the lunar surface using Chandrayaan-2 fully-Polarimetric L-band dual frequency SAR (DFSAR) data17
The formation of gypsum ridges in the endorheic Qaidam Basin and implications for irregular polygonal ridges on Mars17
Editorial Board17
Distribution of atmospheric aerosols during the 2007 Mars dust storm (MY 28): Solar infrared occultation observations by SPICAM17
Surface grain size of alluvial fans on Mars from thermal inertia, as an indicator of depositional style16
Cross-attention induced multilayer domain adaptation network for extraction of sub-kilometer craters from HiRIC images16
Impact induced H2-rich climates on early Mars explored with a global climate model16
Separation of quasi-continuous and periodic components of lineament formation at the Belus – Phoenix - Rhadamanthys Linea “triangle” on Europa16
Evolution of impact-generated hydrothermal systems in basaltic targets on Earth and implications for habitats on Mars16
Lunar elemental abundances as derived from Chandrayaan-216
The brightness of the CO Cameron bands in the martian discrete aurora: A study based on revised cross sections16
Large mass inflow rates in Saturn’s rings due to ballistic transport and mass loading16
Was the Solar System’s dynamical instability triggered by a (sub)stellar flyby?16
Condensation of major and trace elements in dust-rich environments16
Bulk composition and thermal evolution constrain the formation of organics in Ceres' subsurface ocean via geochemical modeling16
Generation and evolution of laser-induced shock waves under martian atmospheric conditions16
Hydrocarbon complexity and photochemical shielding of prebiotic feedstock molecules in exoplanet atmospheres16
Aeolian bedrock ridges in Gale crater, Mars16
Variations in surface adsorbed H2O on lunar soils and relevant minerals16
Convective flow in Ganymede’s subsurface ocean: Implications for the induced magnetic field and topography16
A modeling approach for water and sediment transport in Jezero crater on Mars based on new geomorphological evidence16
Present-day model of lunar meteoroids and their impact flashes for LUMIO mission15
Prediction of the collisions of meteoroids originating in comet 21P/Giacobini-Zinner with the Mercury, Venus, and Mars15
Three-dimensional imaging of martian glaciated terrain using Mars Reconnaissance Orbiter Shallow Radar (SHARAD) observations15
Dimension-ratio-based observability analysis of asteroid photometric model and optimization strategy for completely observable satellite detection15
Frequency-dependent Ganymede’s tidal Love number 15
Corrigendum to ‘Oort Cloud and sednoid formation in an embedded cluster, II: Dynamics and orbital evolutions’ [Icarus 410 (2024) 115915]15
Stochastic hyperbola fitting, probabilistic inversion, reverse-time migration and clustering: A novel interpretation toolbox for in-situ planetary radar15
Physical properties of subsurface water ice deposits in Mars’s Mid-Latitudes from the shallow radar15
Mars volatile inventory and outgassing history15
Late drainage along portions of Samara Valles, West of Jones Crater, Margaritifer Terra, Mars15
Geological analysis of the dome field in western Utopia Planitia, on Mars15
SPH simulations of high-speed collisions between asteroids and comets15
Ed. Board15
GOES GLM, biased bolides, and debiased distributions15
Upper estimate of possible sizes of Venusian lava tubes from the perspective of structural stability15
Magnetically controlled ionosphere of Mars: A model analysis with the vertical plasma drift effects15
Uncovering Ganymede's past: Tectonics at Nippur/Philus Sulci15
Outcrop scale evidence of late-fluid flows and secondary sulfate minerals on exhumed surfaces – Earth versus Mars comparison15
Automatic crater shape retrieval using unsupervised and semi-supervised systems15
Formation of the four terrestrial planets in the Jupiter–Saturn chaotic excitation scenario: fundamental properties and water delivery15
Dielectric properties of the lunar regolith estimated through a combined loss tangent and EM velocity distribution analysis of the Chang'e-4 GPR data set14
Radiatively coupled equatorial waves in Mars’ Aphelion Cloud Belt: Wavenumber–frequency analysis in Mars GCM simulations14
Characterization of aqueous alteration and formation of salty exposures at Ius Chasma, Mars14
A new approach to investigate the influence of space weathering and spectral resolution on the visibility of infrared spectral features in meteorites14
Martian cave detection via machine learning coupled with visible light imagery14
Evidence for widely-separated binary asteroids recorded by craters on Mars14
Pre and post-landing atmospheric optical depths at the Zhurong landing site on Mars retrieved using a single-image-based approach14
Mastcam-Z analog spectral imager (MASI): A Mastcam-Z testbed and field instrument14
Origin of ice in the Medusae Fossae Formation, equatorial Mars14
Tidal dissipation within Earth’s solidifying magma ocean: II. Atmospheric blanketing and its constraint on tidal heating14
Relationships between lobate debris aprons and lineated valley fill on Mars: Evidence for an extensive Amazonian valley glacial landsystem in Mamers Valles14
Effects of observation geometry and heating on the ultra-violet to near-infrared spectra of Mercury simulant14
The mystery of the missing mantle problem and insights from spectroscopy14
Numerical simulation of impact cratering and induced seismic waves in sand targets14
Thermal expansion of oldhamite, CaS: Implication for the surface of Mercury14
Global characterization of the early-season dust storm of Mars year 3614
Mare filled craters on the Moon14
Duration of high temperature-pressure conditions in impact-induced plumes on the Moon13
Titan’s refractory core evolution: Implications for organics in its subsurface ocean13
Selection of chemical species for Europa’s surface using Galileo/NIMS13
Tale of two sugars: Trehalose and hyaluronic acid in a frozen Enceladus-analog brine13
Effect of crater diameter measurement errors on the uncertainty of crater statistics13
Pulsed plasma discharge effects on efficiency and rate of penetration of melt probes in ice13
Evidence that Earth’s magnetotail affects dielectric breakdown weathering on the Moon13
Overview of the MetSpec project - Artificial meteors in ground testing13
Contribution of multiple scattering to the Lyman alpha radiance distribution in cometary comae13
Alkali metal depletion in the deep Jovian atmosphere: The role of anions13
Particle sizes in Saturn’s rings from UVIS stellar occultations 2. Outlier Populations in the C ring and Cassini Division13
Weakening of olivine by hydrogen implantation: Results of nano-indentation tests and some applications to planetary materials13
A reflectance calibration method for Multispectral Camera (MSCam) on the Zhurong rover13
Rotational/divergent flow and energy conversion of thermal tides in a Venus general circulation model13
Three-dimensional imaging of high-velocity-impact induced crack growth in carbonaceous meteorites13
Feasibility of meteor surveying from a Venus orbiter13
Illumination and regolith temperature for China's candidate lunar landing sites with multiple scattering considerations13
Volcanic gas plumes’ effect on the spectrum of Venus13
Phase ratio in single-scattering dust particles: Implication to future DESTINY+ study of asteroid (3200) Phaethon13
Evaluating an embryo origin for detached TNOs within full Kuiper belt formation models13
Evolution of copiapite group minerals over a Mars surface relevant temperature range and low vacuum: SC-SC reversible transformation, thermal expansion and magnetic properties12
Rheological properties and ages of lava flows on Alba Mons, Mars12
Exploring the dielectric loss of Martian regolith in the frequency domain using Zhurong radar data12
How does topography affect wind abrasion on Mars? Recently observed shifts in ventifact orientation at Gale crater12
The origin of the high-TiO 12
A denser and elevated Martian nightside ionosphere during Mars season Ls 180–360°12
On the possible activation of quasi-Hilda comets by Jovian tides12
Relating thermal inertia of basaltic lavas to morphology and texture12
The Mars Science Laboratory record of optical depth measurements via solar imaging12
High alumina basalts identification and their feature analysis in Mare Fecunditatis12
High-velocity oblique impact experiments on ice and snow spheres: Implications for the collisional evolution of icy planetesimals at different thermal evolution stages12
Editorial Board12
Activity in quasi-Hilda objects: A photometric approach12
Chondrule formation via impact jetting in the icy outer solar system12
Pluto's Sputnik basin as a peak-ring or multiring basin: A comparative study12
Compositional signatures of CM, CO, CV, and CK chondrites: Insights from Micro-FTIR spectroscopy and machine learning tools12
Photodegradation of the biomarker L-histidine induced by edge sites of a clay mineral in the Martian harsh UV environment12
Editorial Board12
Numerical model for the solidification of a chondrule melt12
Characterising water in Lunar and Martian regolith materials using nuclear magnetic resonance12
The many ages of Triton: New crater counts on the Voyager high-resolution image sequence and implications for impactor provenance12
Rock size-frequency distribution analysis at the Zhurong landing site based on Navigation and Terrain Camera images along the entire traverse12
Lunar surface modification revealed by in-situ photometric observations from Chang'E-612
Lifetime of cm-sized zodiacal dust from the physical and dynamical evolution of meteoroid streams12
Rotation period estimates for 14 asteroids with the Earth MOID less than 1.1 AU12
Gravitational disturbance on asteroidal ring systems by close encounter with a small object11
Age estimation of Trans-Neptunian Object pairs in close orbits11
Ionosphere of Mars during the consecutive solar minima 23/24 and 24/25 as seen by MARSIS-Mars Express11
A thermal origin for super-high-frequency marsquakes11
Early bombardment of the moon: Connecting the lunar crater record to the terrestrial planet formation11
A numerical study of the liquid motion in Titan’s subsurface ocean11
Thermodynamic modeling of calcium or magnesium chloride, chlorate, and perchlorate ternary mixtures deliquescence at Mars-relevant temperatures11
Formation conditions and chemical composition of early-condensed olivine in the solar protoplanetary disk11
A new perspective on Saturn’s polar vortices: Coupling the thermosphere and stratosphere11
A new method to improve the detection rate and astrometric accuracy of natural satellites located in the halo of Uranus11
Editorial Board11
Principal Component Analysis applied on MASCS/MESSENGER data for the spectral investigation of Mercury's surface11
Geological mapping and chronology of lunar landing sites: Apollo 1411
Reflectance spectra (1–5 μm) at low temperatures and different grain sizes of ammonium-bearing minerals relevant for icy bodies11
Spatial extent of dust storm boundaries in the Mars Dust Activity Database11
Complex Ice Chemistry: A comparative study of electron irradiated planetary ice analogues containing methane11
Laboratory measurements of the 15–46 cm wavelength opacity of water vapor under temperature conditions characteristic of the deep atmosphere of Jupiter11
Evidence of a Martian spatter cone south of Pavonis Mons11
Reprocessing of Pioneer Venus Orbiter radio occultation data: Principles and methodology using a test case11
The impact of cometary outbursts on the orbits of comets in the Oort cloud11
Unexpected mineral impact on organic evolution during simulated aqueous alteration in asteroids11
Global abiotic Sulfur cycling on Earth-like terrestrial planets11
Observations of alkaline emissions NaI, KI and LiI during first minutes after DART probe impact on Dimorphos11
Regolith properties and Stokes vector radar polarimetry models for the moon11
Adaptive isoline interval optimization for precise contour segmentation and instance-level detection of Martian impact craters11
Impact of UV radiation on the Raman and infrared spectral signatures of sulfates, phosphates and carbonates: Implications for Mars exploration11
Influence of the western inlet on the northern delta in Jezero crater, Mars: Topographic-compositional analysis and sediment transport modeling10
Investigating the most promising Yarkovsky candidates using Gaia DR2 astrometry10
Stationary dynamics of planetary ring edge modes at Saturn’s B ring edge10
Improved measurement of radar meteor shower mass indices10
Hydrodynamic volatile escape and moderately volatile isotope fractionation in giant impact ejecta10
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