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 2022-06-01 to 2026-06-01.)
ArticleCitations
Inversion of ultraviolet occultation profiles in a dusty atmosphere: Analytic and numerical methods92
322P/SOHO: The counterpart of a historical comet in 254 CE?79
Inferences of water–ice cloud physics determined from MAVEN/IUVS aerosol retrievals and Mars GCM comparisons72
Planet Four: A Neural Network’s search for polar spring-time fans on Mars67
Comparing the radiolytic oxidation of sulfur and chloride within ice on Europa and Mars63
Simulation of surface regolith gardening and impact associated melt layer production under ns-pulsed laser ablation63
Jovian current disk crossings as observed by Juno JADE-I51
Plenoptic imaging of meteorite shape change during plasma wind tunnel experiments47
Editorial Board45
The annual cycle of water vapor above gale crater as retrieved by CRISM and compared to ChemCam passive sky spectroscopy45
Cosmic hydrogen and ice loss lines42
An analogue study of impact craters on Titan: Implications for Titan's surface age41
Long-period dynamical evolution of the meteoroid stream originating in comet 21P/Giacobini-Zinner40
Evidence for landslides in Sisyphi Cavi (Noachis Terra, Mars): Slope evolution and role of endogenous preparatory factors39
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
Subglacial catastrophic-flood origin of linear and curvilinear flat-rimmed pit chains on Mars: Evidence from geomorphological mapping and detailed landsystem analysis37
Influence of hydrothermal asteroidal conditions on the molecular structure and isotopic compositions of polycyclic aromatic hydrocarbons37
Formation of steep-sided domes on Venus via eruption of high crystallinity magmas35
On a radiolytic origin of red organics at the surface of the Arrokoth Trans-Neptunian Object35
Diffusion limited escape of hydrogen from Mars35
Raman spectroscopic documentation of Mars analog basalt alteration by brines34
Jovian upper clouds and hazes from visible and near infrared spectroscopy using CARMENES34
An improved model of metal/silicate differentiation during Earth's accretion33
The high-resolution imaging science experiment (HiRISE) in the MRO extended science phases (2009–2023)32
Chaotic tides as a solution to the Hyperion problem31
Investigation of the shocked Viñales ordinary chondrite (L6) meteorite fall – Implications for shock classification, fragmentation, and collision dynamics31
An integrated study of Rutherfurd crater: Composition, morphology, and chronology31
Insights into pyroxene-dominated surfaces and implications for ongoing space exploration missions30
The magnetic susceptibility of Pleistocene paleosols as a martian paleoenvironment analog29
Optical observations and dust modelling of comet 156P/Russell-LINEAR29
Corrigendum to “On the forced orbital plane of the Hilda asteroids” Icarus 49 (2026), 11695929
Influence of observed seasonally varying composition on Titan’s stratospheric circulation29
Exosphere-mediated migration of volatile species on airless bodies across the solar system29
Using surface displacements to probe Venus’ interior structure and atmospheric dynamics29
A case for young igneous volcanism in the Terra Sirenum region, Mars29
Isolating the mechanisms for asteroid surface refreshing27
Seasonal variability of gravity wave activity in Mars's lower atmosphere from MGS–TES nadir observations27
Exploring the variability of the venusian thermosphere with the IPSL Venus GCM27
Bayesian inference on the isotopic building blocks of Mars and Earth27
Submicroscopic iron-rich grains throughout impact glasses in Chang'E-5 regolith26
Comprehensive analysis of Chandrayaan-3 landing site region focussing on morphology, hydration and gravity anomalies26
New candidate cave entrances on the Moon found using deep learning26
Landslide chronology on mars: A window into the past of Valles Marineris and martian slopes26
The yearly variability of the sodium exosphere of Mercury: A toy model25
Variations of the magnetic field and plasma parameters near the Martian induced magnetosphere boundary25
Morphological changes currently occurring in sand-filled gully channels on Mars: Implications for the role of substrates inside channels24
Daily and seasonal processes shape hydrological activity and detectability of moisture in Antarctic, Mars-analog soils24
Elemental composition of manganese- and phosphorus-rich nodules in the Knockfarril Hill member, Gale crater, Mars24
The 3D subsurface structures of the Atlas impact crater revealed by GRAIL gravity data24
Tectonic patterns on Vesta and Ceres revealed by polygonal impact craters23
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
Shadow method retrievals of the atmospheric optical depth above Gale crater on Mars using HRSC images23
Phosphates reveal high pH ocean water on Enceladus23
Catastrophic rupture of lunar rocks: Implications for lunar rock size–frequency distributions23
A dual-branch automatic classification network for lunar simple crater degradation grades integrating image and morphological parameters23
Identification of H2O ice at lunar south polar region based on deep learning23
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 cerium22
Editorial Board22
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 abundance22
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
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 analysis21
How much earlier would LSST have discovered currently known long-period comets?21
A Mars orbital catalog of aqueous alteration signatures (MOCAAS)21
Photochemistry of benzene (C6H6) hydrogen cyanide (HCN) co-condensed ices part 2: Formation of aerosols analogues of titan's atmosphere21
Mineral abrasion experiments at Mars relevant temperatures21
First quantitative characterization of the Martian dust devil dimensions determined from InSight data21
Do icy dust aggregates break up when they pass the snow line?21
Range resolution enhancement of SHAllow RADar (SHARAD) data via bandwidth extrapolation technique: Enabling new features detection and improving geophysical investigation20
Chronology, composition, and mineralogy of mare basalts in the junction of Oceanus Procellarum, Mare Imbrium, Mare Insularum, and Mare Vaporum20
The morphometry of small impact craters on Bennu: Relationships to geologic units, boulders, and impact armoring20
Near-Earth Asteroid orbit determination with Physics-Informed Extreme Learning Machine19
A reappraisal of the amorphization kinetics of water ice: Combined experimental and numerical investigations and amorphization cross-sections in the 90–120 K range19
Impact strength of cm-to-decimeter scale weak porous targets: Implication for lifetime of boulders on asteroids19
Latitudinal and radial dependence of the lunar sodium exospheric temperature and linewidths19
The effects of CO2 clouds on the thermal structure of the early Martian atmosphere19
Dyke swarm history of Eastern Eistla Regio, Venus and implications for its plume origin19
Asteroids were born bigger: An implication of surface mass ablation during gas-assisted implantation into the asteroid belt19
Saturn’s atmospheric response to the large influx of ring material inferred from Cassini INMS measurements19
Vortex crystals at Jupiter’s poles: Emergence controlled by initial small-scale turbulence19
Secondary craters reveal differences in neighboring geologic units: An example on Mars19
Detailed chemical composition analysis of the Soi crater region on Titan19
Characterising the efficiency of the hierarchical clustering method19
Analyzing spatial distributions and alignments of pitted cone features in Utopia Planitia on Mars18
Possible formation pathways for zeolites in closed-basin lakes on noachian Mars: Insights from geochemical modeling18
Recent faulting at the Claritas Rupes scarp on Mars18
The role of subsurface ocean dynamics and phase transitions in forming the topography of icy moons18
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
Validation of SPH code Spheral to model interacting solid bodies in a supersonic flow18
Sound velocities of Anorthite at high pressures and temperatures: Implications for estimating porosity in upper lunar crust18
Large volcanoes on Venus: Morphology, morphometry, and stratigraphy18
3D morphometry of Martian craters from HRSC DEMs using a multi-scale semantic segmentation network and morphological analysis18
Non-thermal escape of the martian CO218
Non-LTE spectroscopy of the tetradecad region of methane recorded in a hypersonic flow18
The Martian ionosphere at solar minimum: Empirical model validation using MAVEN ROSE data18
Scaling of convection in high-pressure ice layers of large icy moons and implications for habitability18
On the rotation of M-type asteroids: Statistical evidence for higher rotation rates18
Aeolian bedrock ridges in Gale crater, Mars17
Compositional diversity in the Mare Marginis and Mare Smythii: An insight into the volcanism in the region17
Generation and evolution of laser-induced shock waves under martian atmospheric conditions17
Lunar elemental abundances as derived from Chandrayaan-217
Mars volatile inventory and outgassing history17
Cross-attention induced multilayer domain adaptation network for extraction of sub-kilometer craters from HiRIC images17
Observation of the Southern Polar cap during MY34-36 with ExoMars-TGO NOMAD LNO17
GOES GLM, biased bolides, and debiased distributions17
Comparisons of the core and mantle compositions of earth analogs from different terrestrial planet formation scenarios17
Evolution of impact-generated hydrothermal systems in basaltic targets on Earth and implications for habitats on Mars17
Separation of quasi-continuous and periodic components of lineament formation at the Belus – Phoenix - Rhadamanthys Linea “triangle” on Europa17
A numerical model for the atmospheric entry of hydrated, phyllosilicate-rich micrometeorites17
The brightness of the CO Cameron bands in the martian discrete aurora: A study based on revised cross sections17
Distribution of atmospheric aerosols during the 2007 Mars dust storm (MY 28): Solar infrared occultation observations by SPICAM16
Interaction between oppositely signed vortices on adjacent domains in Jupiter16
Dark ray craters on Ganymede: Impactor or endogenous origin16
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
Mechanical behaviour of sulphur-based Martian regolith concrete processed under CO2-rich conditions16
Tidal dissipation within an elongated asteroid with satellite, and application to asteroid (216) Kleopatra16
Integral equation modeling for dielectric retrieval of the lunar surface using Chandrayaan-2 fully-Polarimetric L-band dual frequency SAR (DFSAR) data16
Bulk composition and thermal evolution constrain the formation of organics in Ceres' subsurface ocean via geochemical modeling16
The formation of gypsum ridges in the endorheic Qaidam Basin and implications for irregular polygonal ridges on Mars16
Large mass inflow rates in Saturn’s rings due to ballistic transport and mass loading16
Editorial Board16
Statistical chronometry of meteorites. I. A Test of 26Al homogeneity and the Pb-Pb age of the solar system’s 16
Present-day model of lunar meteoroids and their impact flashes for LUMIO mission16
Where on the Moon was the eruption that produced the recently reported ∼ 120 million year old volcanic glass beads?16
Upper estimate of possible sizes of Venusian lava tubes from the perspective of structural stability16
Physical properties of subsurface water ice deposits in Mars’s Mid-Latitudes from the shallow radar15
Three-dimensional imaging of martian glaciated terrain using Mars Reconnaissance Orbiter Shallow Radar (SHARAD) observations15
Late drainage along portions of Samara Valles, West of Jones Crater, Margaritifer Terra, Mars15
Prediction of the collisions of meteoroids originating in comet 21P/Giacobini-Zinner with the Mercury, Venus, and Mars15
Stochastic hyperbola fitting, probabilistic inversion, reverse-time migration and clustering: A novel interpretation toolbox for in-situ planetary radar15
The photochemistry of irradiated Enceladus ice analogues: Implications for the formation of ozone and carbon trioxide15
A contemporary view of the ordinary chondrite boot I: Band parameter analysis dependency15
Variability of temperatures and gravity wave activity in the Martian thermosphere during low solar irradiance15
Ed. Board15
SPH simulations of high-speed collisions between asteroids and comets15
On the cooling rate evolution of asteroid fragments15
Ed. Board15
Variations in surface adsorbed H2O on lunar soils and relevant minerals15
A modeling approach for water and sediment transport in Jezero crater on Mars based on new geomorphological evidence15
Moderate D/H ratios in methane ice on Eris and Makemake as evidence of hydrothermal or metamorphic processes in their interiors: Geochemical analysis15
Condensation of major and trace elements in dust-rich environments15
Formation of the four terrestrial planets in the Jupiter–Saturn chaotic excitation scenario: fundamental properties and water delivery15
Automatic crater shape retrieval using unsupervised and semi-supervised systems15
Magnetically controlled ionosphere of Mars: A model analysis with the vertical plasma drift effects15
Uncovering Ganymede's past: Tectonics at Nippur/Philus Sulci15
Impact induced H2-rich climates on early Mars explored with a global climate model15
Convective flow in Ganymede’s subsurface ocean: Implications for the induced magnetic field and topography15
Surface grain size of alluvial fans on Mars from thermal inertia, as an indicator of depositional style15
Was the Solar System’s dynamical instability triggered by a (sub)stellar flyby?15
Relationships between lobate debris aprons and lineated valley fill on Mars: Evidence for an extensive Amazonian valley glacial landsystem in Mamers Valles14
Corrigendum to ‘Oort Cloud and sednoid formation in an embedded cluster, II: Dynamics and orbital evolutions’ [Icarus 410 (2024) 115915]14
Contribution of multiple scattering to the Lyman alpha radiance distribution in cometary comae14
Radiatively coupled equatorial waves in Mars’ Aphelion Cloud Belt: Wavenumber–frequency analysis in Mars GCM simulations14
Global characterization of the early-season dust storm of Mars year 3614
A new approach to investigate the influence of space weathering and spectral resolution on the visibility of infrared spectral features in meteorites14
Selection of chemical species for Europa’s surface using Galileo/NIMS14
Geological analysis of the dome field in western Utopia Planitia, on Mars14
The mystery of the missing mantle problem and insights from spectroscopy14
Titan’s refractory core evolution: Implications for organics in its subsurface ocean14
Evidence for widely-separated binary asteroids recorded by craters on Mars14
Martian cave detection via machine learning coupled with visible light imagery14
Effects of observation geometry and heating on the ultra-violet to near-infrared spectra of Mercury simulant14
Dimension-ratio-based observability analysis of asteroid photometric model and optimization strategy for completely observable satellite detection14
Pre and post-landing atmospheric optical depths at the Zhurong landing site on Mars retrieved using a single-image-based approach14
Outcrop scale evidence of late-fluid flows and secondary sulfate minerals on exhumed surfaces – Earth versus Mars comparison14
Mastcam-Z analog spectral imager (MASI): A Mastcam-Z testbed and field instrument14
Thermal expansion of oldhamite, CaS: Implication for the surface of Mercury14
Duration of high temperature-pressure conditions in impact-induced plumes on the Moon13
Dielectric properties of the lunar regolith estimated through a combined loss tangent and EM velocity distribution analysis of the Chang'e-4 GPR data set13
Global geologic map of asteroid (101955) Bennu indicates heterogeneous resurfacing in the past 500,000 years13
The origin of the high-TiO 13
Particle sizes in Saturn’s rings from UVIS stellar occultations 2. Outlier Populations in the C ring and Cassini Division13
Illumination and regolith temperature for China's candidate lunar landing sites with multiple scattering considerations13
Evidence that Earth’s magnetotail affects dielectric breakdown weathering on the Moon13
Mare filled craters on the Moon13
A reflectance calibration method for Multispectral Camera (MSCam) on the Zhurong rover13
Origin of ice in the Medusae Fossae Formation, equatorial Mars13
Characterization of aqueous alteration and formation of salty exposures at Ius Chasma, Mars13
Photodegradation of the biomarker L-histidine induced by edge sites of a clay mineral in the Martian harsh UV environment13
Tidal dissipation within Earth’s solidifying magma ocean: II. Atmospheric blanketing and its constraint on tidal heating13
A denser and elevated Martian nightside ionosphere during Mars season Ls 180–360°13
Feasibility of meteor surveying from a Venus orbiter13
Frequency-dependent Ganymede’s tidal Love number 13
Numerical simulation of impact cratering and induced seismic waves in sand targets13
Rotational/divergent flow and energy conversion of thermal tides in a Venus general circulation model13
Alkali metal depletion in the deep Jovian atmosphere: The role of anions13
Relating thermal inertia of basaltic lavas to morphology and texture12
Rotation period estimates for 14 asteroids with the Earth MOID less than 1.1 AU12
Pulsed plasma discharge effects on efficiency and rate of penetration of melt probes in ice12
Compositional signatures of CM, CO, CV, and CK chondrites: Insights from Micro-FTIR spectroscopy and machine learning tools12
Editorial Board12
Volcanic gas plumes’ effect on the spectrum of Venus12
Three-dimensional imaging of high-velocity-impact induced crack growth in carbonaceous meteorites12
Lifetime of cm-sized zodiacal dust from the physical and dynamical evolution of meteoroid streams12
Evaluating an embryo origin for detached TNOs within full Kuiper belt formation models12
Phase ratio in single-scattering dust particles: Implication to future DESTINY+ study of asteroid (3200) Phaethon12
Pluto's Sputnik basin as a peak-ring or multiring basin: A comparative study12
Machine Learning in meteor science: Challenges and future directions12
The many ages of Triton: New crater counts on the Voyager high-resolution image sequence and implications for impactor provenance12
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
On the possible activation of quasi-Hilda comets by Jovian tides12
Rock size-frequency distribution analysis at the Zhurong landing site based on Navigation and Terrain Camera images along the entire traverse12
Chondrule formation via impact jetting in the icy outer solar system12
Overview of the MetSpec project - Artificial meteors in ground testing12
Polygonal impact craters on planetary surfaces – A review12
Weakening of olivine by hydrogen implantation: Results of nano-indentation tests and some applications to planetary materials12
The Mars Science Laboratory record of optical depth measurements via solar imaging12
Lunar surface modification revealed by in-situ photometric observations from Chang'E-612
Exploring Mons Mouton (lunar south circumpolar region): Reconstruction of the 3D geology and stratigraphy of a prominent Lunar Mountain region11
The influence of passing field stars on the solar system’s dynamical future11
Gravitational disturbance on asteroidal ring systems by close encounter with a small object11
Martian nonmigrating atmospheric tides in the thermosphere and ionosphere at solar minimum11
Rheological properties and ages of lava flows on Alba Mons, Mars11
Observations of alkaline emissions NaI, KI and LiI during first minutes after DART probe impact on Dimorphos11
Unexpected mineral impact on organic evolution during simulated aqueous alteration in asteroids11
Adaptive isoline interval optimization for precise contour segmentation and instance-level detection of Martian impact craters11
Thermodynamic modeling of calcium or magnesium chloride, chlorate, and perchlorate ternary mixtures deliquescence at Mars-relevant temperatures11
Editorial Board11
A new method to improve the detection rate and astrometric accuracy of natural satellites located in the halo of Uranus11
Editorial Board11
Characterising water in Lunar and Martian regolith materials using nuclear magnetic resonance11
Numerical model for the solidification of a chondrule melt11
Impact of UV radiation on the Raman and infrared spectral signatures of sulfates, phosphates and carbonates: Implications for Mars exploration11
Mie theory-based light scattering analysis of entrained grains in Io's Tvashtar plume observed during new horizons' 2007 flyby11
Reprocessing of Pioneer Venus Orbiter radio occultation data: Principles and methodology using a test case11
Principal Component Analysis applied on MASCS/MESSENGER data for the spectral investigation of Mercury's surface11
High alumina basalts identification and their feature analysis in Mare Fecunditatis11
High-velocity oblique impact experiments on ice and snow spheres: Implications for the collisional evolution of icy planetesimals at different thermal evolution stages11
Activity in quasi-Hilda objects: A photometric approach11
Micromechanical properties of Chang'e-5 lunar soil minerals: Comparison with meteorite and terrestrial analogs11
Formation conditions and chemical composition of early-condensed olivine in the solar protoplanetary disk11
Complex Ice Chemistry: A comparative study of electron irradiated planetary ice analogues containing methane11
Measurement of viscous erosion rate from plume surface interactions in low-pressure environments10
Quantification of amorphous Si, Al, and Fe in palagonitic Mars analogs by chemical extraction and X-ray spectroscopy10
Variations in lunar regolith properties with depth as revealed by Chang'e-5 samples10
Moats in the residual south polar cap of Mars: Ages, formation, and evolution10
The bulk composition and initial size of Mercury10
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
Investigation of the incremental benefits of eccentric collisions in kinetic deflection of potentially hazardous asteroids10
Possible particle ejection contributions to the shape and spin stability of small near-Earth asteroids10
Editorial Board10
Micro-meteoroids impact vaporization as source for Ca and CaO exosphere along Mercury's orbit10
Investigating the most promising Yarkovsky candidates using Gaia DR2 astrometry10
Topographic response to ocean heat flux anomaly on the icy moons of Jupiter and Saturn10
Characterization of groundwater chemistry beneath Gale Crater on early Mars by hydrothermal experiments10
Lunar polar volatile remobilization in regolith-filled craters10
Astrometric observations of Phoebe from 2010 to 2019 based on Gaia DR310
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