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 2021-10-01 to 2025-10-01.)
ArticleCitations
Formation of steep-sided domes on Venus via eruption of high crystallinity magmas79
A case for young igneous volcanism in the Terra Sirenum region, Mars69
322P/SOHO: The counterpart of a historical comet in 254 CE?67
Inferences of water–ice cloud physics determined from MAVEN/IUVS aerosol retrievals and Mars GCM comparisons66
Tectonic patterns on Vesta and Ceres revealed by polygonal impact craters61
Inversion of ultraviolet occultation profiles in a dusty atmosphere: Analytic and numerical methods58
An analogue study of impact craters on Titan: Implications for Titan's surface age58
The high-resolution imaging science experiment (HiRISE) in the MRO extended science phases (2009–2023)54
Seasonal variability of gravity wave activity in Mars's lower atmosphere from MGS–TES nadir observations50
Bayesian inference on the isotopic building blocks of Mars and Earth50
The yearly variability of the sodium exosphere of Mercury: A toy model49
Optical observations and dust modelling of comet 156P/Russell-LINEAR48
Exosphere-mediated migration of volatile species on airless bodies across the solar system44
Landslide chronology on mars: A window into the past of Valles Marineris and martian slopes42
Cosmic hydrogen and ice loss lines42
Editorial Board42
Evidence for landslides in Sisyphi Cavi (Noachis Terra, Mars): Slope evolution and role of endogenous preparatory factors40
Comprehensive analysis of Chandrayaan-3 landing site region focussing on morphology, hydration and gravity anomalies35
Using surface displacements to probe Venus’ interior structure and atmospheric dynamics35
Planet Four: A Neural Network’s search for polar spring-time fans on Mars34
Constraints on a potential aerial biosphere on Venus: II. Ultraviolet radiation34
An improved model of metal/silicate differentiation during Earth's accretion34
Jovian current disk crossings as observed by Juno JADE-I33
Comparing the radiolytic oxidation of sulfur and chloride within ice on Europa and Mars33
Plenoptic imaging of meteorite shape change during plasma wind tunnel experiments31
Variations of the magnetic field and plasma parameters near the Martian induced magnetosphere boundary31
Submicroscopic iron-rich grains throughout impact glasses in Chang'E-5 regolith30
Chaotic tides as a solution to the Hyperion problem29
Simulation of surface regolith gardening and impact associated melt layer production under ns-pulsed laser ablation29
Raman spectroscopic documentation of Mars analog basalt alteration by brines27
Subglacial catastrophic-flood origin of linear and curvilinear flat-rimmed pit chains on Mars: Evidence from geomorphological mapping and detailed landsystem analysis27
The magnetic susceptibility of Pleistocene paleosols as a martian paleoenvironment analog27
Shadow method retrievals of the atmospheric optical depth above Gale crater on Mars using HRSC images27
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]26
The annual cycle of water vapor above gale crater as retrieved by CRISM and compared to ChemCam passive sky spectroscopy26
Investigation of the shocked Viñales ordinary chondrite (L6) meteorite fall – Implications for shock classification, fragmentation, and collision dynamics26
Influence of observed seasonally varying composition on Titan’s stratospheric circulation26
Isolating the mechanisms for asteroid surface refreshing25
Multiscale spectral discrimination of poorly crystalline and intermixed alteration phases using aerial and ground-based ExoMars rover emulator data25
Implications for the energy source for an early dynamo in Vesta from experiments on electrical resistivity of liquid Fe-10wt%Ni at high pressures25
Daily and seasonal processes shape hydrological activity and detectability of moisture in Antarctic, Mars-analog soils24
Visible–near-infrared observations of organics and carbonates on (101955) Bennu: Classification method and search for surface context24
On a radiolytic origin of red organics at the surface of the Arrokoth Trans-Neptunian Object24
Lava flow ages in northeastern Oceanus Procellarum: The need for calibrating crater counting procedures24
Recent boulder falls within the Finsen crater on the lunar far side: An assessment of the possible triggering rationale24
Chronological and compositional mapping of the Mare Orientale basin using Chandrayaan-1 – M3 and LRO datasets24
Influence of hydrothermal asteroidal conditions on the molecular structure and isotopic compositions of polycyclic aromatic hydrocarbons23
Catastrophic rupture of lunar rocks: Implications for lunar rock size–frequency distributions23
Long-period dynamical evolution of the meteoroid stream originating in comet 21P/Giacobini-Zinner23
Machine learning as a tool to classify extra-terrestrial landslides: A dossier from Valles Marineris, Mars22
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
Morphological changes currently occurring in sand-filled gully channels on Mars: Implications for the role of substrates inside channels22
Elemental composition of manganese- and phosphorus-rich nodules in the Knockfarril Hill member, Gale crater, Mars22
Diffusion limited escape of hydrogen from Mars22
Photochemistry of benzene (C6H6) hydrogen cyanide (HCN) co-condensed ices part 2: Formation of aerosols analogues of titan's atmosphere21
Do icy dust aggregates break up when they pass the snow line?21
3D morphometry of Martian craters from HRSC DEMs using a multi-scale semantic segmentation network and morphological analysis21
How much earlier would LSST have discovered currently known long-period comets?21
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 abundance21
Exploring the variability of the venusian thermosphere with the IPSL Venus GCM21
A new constraint on HCl abundance at the cloud top of Venus20
VIS-IR spectroscopy of magnesium chlorides at cryogenic temperatures20
Scaling of convection in high-pressure ice layers of large icy moons and implications for habitability20
Chronology, composition, and mineralogy of mare basalts in the junction of Oceanus Procellarum, Mare Imbrium, Mare Insularum, and Mare Vaporum20
Large volcanoes on Venus: Morphology, morphometry, and stratigraphy20
Ricochets on asteroids II: Sensitivity of laboratory experiments of low velocity grazing impacts on substrate grain size20
The morphometry of small impact craters on Bennu: Relationships to geologic units, boulders, and impact armoring20
The role of subsurface ocean dynamics and phase transitions in forming the topography of icy moons19
The Martian ionosphere at solar minimum: Empirical model validation using MAVEN ROSE data19
Modeling global-scale mass flows on the Lagrangian satellites of Dione and Tethys19
Asteroids were born bigger: An implication of surface mass ablation during gas-assisted implantation into the asteroid belt19
Non-thermal escape of the martian CO218
Analyzing spatial distributions and alignments of pitted cone features in Utopia Planitia on Mars18
Saturn’s atmospheric response to the large influx of ring material inferred from Cassini INMS measurements18
Editorial Board18
Ion density and phase space density distribution of planetary ions Na+, O+ and He+ in Mercury’s magnetosphere18
The effect of collisional erosion on the composition of Earth-analog planets in Grand Tack models: Implications for the formation of the Earth18
Impact strength of cm-to-decimeter scale weak porous targets: Implication for lifetime of boulders on asteroids18
The influence of equation of state on impact dynamics between Pluto-like bodies18
Vortex crystals at Jupiter’s poles: Emergence controlled by initial small-scale turbulence17
Range resolution enhancement of SHAllow RADar (SHARAD) data via bandwidth extrapolation technique: Enabling new features detection and improving geophysical investigation17
First quantitative characterization of the Martian dust devil dimensions determined from InSight data17
Rare earth element assessment in Jezero crater using the Planetary Instrument for X-ray Lithochemistry on the Mars 2020 rover Perseverance: A case study of cerium17
A Mars orbital catalog of aqueous alteration signatures (MOCAAS)17
Evidence for the protection of N-heterocycles from gamma radiation by Mars analogue minerals17
Mineral abrasion experiments at Mars relevant temperatures17
Secondary craters reveal differences in neighboring geologic units: An example on Mars17
Latitudinal and radial dependence of the lunar sodium exospheric temperature and linewidths17
Possible formation pathways for zeolites in closed-basin lakes on noachian Mars: Insights from geochemical modeling17
Non-LTE spectroscopy of the tetradecad region of methane recorded in a hypersonic flow17
Distal impact-related surface flows associated with the well-preserved Tokmok Crater, Noachis Terra, Mars17
Recent faulting at the Claritas Rupes scarp on Mars17
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 roll17
Detailed chemical composition analysis of the Soi crater region on Titan17
Ejecta cloud distributions for the statistical analysis of impact cratering events onto asteroids’ surfaces: A sensitivity analysis17
MAVEN/IUVS observations of C I 156.1 nm and 165.7 nm dayglow: Direct detection of carbon and implications on photochemical escape17
Two types of jarosite in the early Cambrian sedimentary rocks: Insights for genesis and transformation of jarosite on Mars17
A contemporary view of the ordinary chondrite boot I: Band parameter analysis dependency16
A numerical model for the atmospheric entry of hydrated, phyllosilicate-rich micrometeorites16
The photochemistry of irradiated Enceladus ice analogues16
Where on the Moon was the eruption that produced the recently reported ∼ 120 million year old volcanic glass beads?16
A modeling approach for water and sediment transport in Jezero crater on Mars based on new geomorphological evidence16
Mechanical behaviour of sulphur-based Martian regolith concrete processed under CO2-rich conditions16
Evidence for hydrated minerals in the VNIR spectra of G-class asteroids: A first look16
Evolution of impact-generated hydrothermal systems in basaltic targets on Earth and implications for habitats on Mars16
Preface: Ices in the Solar system; origin, evolution and distribution16
Micro-FTIR reflectance spectroscopy of Ryugu, CI chondrites and volatile-rich clasts – Comparing spectral features in the Mid-IR (2.5–16.5 μm) region15
GOES GLM, biased bolides, and debiased distributions15
Impact induced H2-rich climates on early Mars explored with a global climate model15
Integral equation modeling for dielectric retrieval of the lunar surface using Chandrayaan-2 fully-Polarimetric L-band dual frequency SAR (DFSAR) data15
Dark ray craters on Ganymede: Impactor or endogenous origin15
Lunar elemental abundances as derived from Chandrayaan-215
Cross-attention induced multilayer domain adaptation network for extraction of sub-kilometer craters from HiRIC images15
Bulk composition and thermal evolution constrain the formation of organics in Ceres' subsurface ocean via geochemical modeling15
The brightness of the CO Cameron bands in the martian discrete aurora: A study based on revised cross sections15
Aeolian bedrock ridges in Gale crater, Mars15
Variations in surface adsorbed H2O on lunar soils and relevant minerals15
Condensation of major and trace elements in dust-rich environments15
Large mass inflow rates in Saturn’s rings due to ballistic transport and mass loading15
Space weathering on inner planetary surface analogues induced by swift multicharged heavy ion bombardment14
Distribution of atmospheric aerosols during the 2007 Mars dust storm (MY 28): Solar infrared occultation observations by SPICAM14
Modeling of observations of the OH nightglow in the venusian mesosphere14
Moderate D/H ratios in methane ice on Eris and Makemake as evidence of hydrothermal or metamorphic processes in their interiors: Geochemical analysis14
Variability of temperatures and gravity wave activity in the Martian thermosphere during low solar irradiance14
Compositional diversity in the Mare Marginis and Mare Smythii: An insight into the volcanism in the region14
Present-day model of lunar meteoroids and their impact flashes for LUMIO mission14
VNIR reflectance spectra of silicate-graphite mixtures: The effect of graphite content and particle size14
Origin of ice in the Medusae Fossae Formation, equatorial Mars14
Three-dimensional imaging of martian glaciated terrain using Mars Reconnaissance Orbiter Shallow Radar (SHARAD) observations14
The upper-thermal stability of an iron-rich smectite: Implications for smectite formation on Mars14
Separation of quasi-continuous and periodic components of lineament formation at the Belus – Phoenix - Rhadamanthys Linea “triangle” on Europa14
Comparisons of the core and mantle compositions of earth analogs from different terrestrial planet formation scenarios14
Dark primitive asteroids account for a large share of K/Pg-scale impacts on the Earth14
Tidal dissipation within an elongated asteroid with satellite, and application to asteroid (216) Kleopatra14
Surface grain size of alluvial fans on Mars from thermal inertia, as an indicator of depositional style14
Mars volatile inventory and outgassing history14
Stochastic hyperbola fitting, probabilistic inversion, reverse-time migration and clustering: A novel interpretation toolbox for in-situ planetary radar14
Identification of a new spectral signature at 3 μ14
Statistical chronometry of meteorites. I. A Test of 26Al homogeneity and the Pb-Pb age of the solar system’s 14
Generation and evolution of laser-induced shock waves under martian atmospheric conditions14
Observation of the Southern Polar cap during MY34-36 with ExoMars-TGO NOMAD LNO14
Corrigendum to ‘Oort Cloud and sednoid formation in an embedded cluster, II: Dynamics and orbital evolutions’ [Icarus 410 (2024) 115915]13
Selection of chemical species for Europa’s surface using Galileo/NIMS13
Pre and post-landing atmospheric optical depths at the Zhurong landing site on Mars retrieved using a single-image-based approach13
Dimension-ratio-based observability analysis of asteroid photometric model and optimization strategy for completely observable satellite detection13
Illumination and regolith temperature for China's candidate lunar landing sites with multiple scattering considerations13
Formation of the four terrestrial planets in the Jupiter–Saturn chaotic excitation scenario: fundamental properties and water delivery13
Volatiles on Mercury: The case of hollows and the pyroclastic vent of Tyagaraja crater13
Water uptake by chlorate salts under Mars-relevant conditions13
Magnetically controlled ionosphere of Mars: A model analysis with the vertical plasma drift effects13
Ed. Board13
Thermal expansion of oldhamite, CaS: Implication for the surface of Mercury13
Frequency-dependent Ganymede’s tidal Love number k13
On the cooling rate evolution of asteroid fragments13
Ed. Board13
Global characterization of the early-season dust storm of Mars year 3613
Feasibility of meteor surveying from a Venus orbiter13
Effects of observation geometry and heating on the ultra-violet to near-infrared spectra of Mercury simulant13
Relationships between lobate debris aprons and lineated valley fill on Mars: Evidence for an extensive Amazonian valley glacial landsystem in Mamers Valles13
Prediction of the collisions of meteoroids originating in comet 21P/Giacobini-Zinner with the Mercury, Venus, and Mars13
Ephemeris and hazard assessment for near-Earth asteroid (101955) Bennu based on OSIRIS-REx data13
SPH simulations of high-speed collisions between asteroids and comets13
Automatic crater shape retrieval using unsupervised and semi-supervised systems13
The unique spectral and geomorphological characteristics of pitted impact deposits associated with Marcia crater on Vesta13
Investigation of mineral assemblages in a newly identified endorheic playa near Huygens basin on Mars and their astrobiological implications13
Igneous rock powder identification using colour cameras: A powerful method for space exploration13
Late drainage along portions of Samara Valles, West of Jones Crater, Margaritifer Terra, Mars13
Absolute model ages of three craters in the vicinity of the Chang'E-5 landing site and their geologic implications13
The mystery of the missing mantle problem and insights from spectroscopy13
Uncovering Ganymede's past: Tectonics at Nippur/Philus Sulci13
Alkali metal depletion in the deep Jovian atmosphere: The role of anions13
Evidence for widely-separated binary asteroids recorded by craters on Mars13
Global geologic map of asteroid (101955) Bennu indicates heterogeneous resurfacing in the past 500,000 years13
Ed. Board13
Martian cave detection via machine learning coupled with visible light imagery13
Mare filled craters on the Moon13
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 Express12
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
Simulated SPHEREx spectra of asteroids and their implications for asteroid size and reflectance estimation12
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
Ejecta distribution and momentum transfer from oblique impacts on asteroid surfaces12
Pluto's Sputnik basin as a peak-ring or multiring basin: A comparative study12
Particle sizes in Saturn’s rings from UVIS stellar occultations 2. Outlier Populations in the C ring and Cassini Division12
Exploring the dielectric loss of Martian regolith in the frequency domain using Zhurong radar data12
The excited spin state of Dimorphos resulting from the DART impact12
A reflectance calibration method for Multispectral Camera (MSCam) on the Zhurong rover12
Gravitational disturbance on asteroidal ring systems by close encounter with a small object12
Early bombardment of the moon: Connecting the lunar crater record to the terrestrial planet formation12
Activity in quasi-Hilda objects: A photometric approach12
A denser and elevated Martian nightside ionosphere during Mars season Ls 180–360°12
Editorial Board12
Phase ratio in single-scattering dust particles: Implication to future DESTINY+ study of asteroid (3200) Phaethon12
Weakening of olivine by hydrogen implantation: Results of nano-indentation tests and some applications to planetary materials12
Characterization of aqueous alteration and formation of salty exposures at Ius Chasma, Mars12
A new perspective on Saturn’s polar vortices: Coupling the thermosphere and stratosphere12
Corrigendum to ‘Successes and challenges of factor analysis/target transformation application to visible-to-near-infrared hyperspectral data’: [Icarus 365 (2021) 114402]12
How does topography affect wind abrasion on Mars? Recently observed shifts in ventifact orientation at Gale crater12
Volcanic gas plumes’ effect on the spectrum of Venus12
Seepage-evaporation controlled depletion of initially water-filled reservoirs on Earth and Mars: Analytic versus HYDRUS modeling12
The Mars Science Laboratory record of optical depth measurements via solar imaging12
Numerical model for the solidification of a chondrule melt12
Evidence of a Martian spatter cone south of Pavonis Mons12
Overview of the MetSpec project - Artificial meteors in ground testing12
Evidence that Earth’s magnetotail affects dielectric breakdown weathering on the Moon12
The many ages of Triton: New crater counts on the Voyager high-resolution image sequence and implications for impactor provenance12
Three-dimensional imaging of high-velocity-impact induced crack growth in carbonaceous meteorites12
Rotational/divergent flow and energy conversion of thermal tides in a Venus general circulation model12
Pulsed plasma discharge effects on efficiency and rate of penetration of melt probes in ice12
The origin of the high-TiO212
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
Boulders on Mercury12
The impact of cometary outbursts on the orbits of comets in the Oort cloud12
Mie theory-based light scattering analysis of entrained grains in Io's Tvashtar plume observed during new horizons' 2007 flyby12
Thermodynamic modeling of calcium or magnesium chloride, chlorate, and perchlorate ternary mixtures deliquescence at Mars-relevant temperatures11
Excitation, emission, and synchronous fluorescence for astrochemical applications: Experiments and computer simulations of synchronous spectra of polycyclic aromatic hydrocarbons and their mixtures11
Editorial Board11
Reflectance spectra (1–5 μm) at low temperatures and different grain sizes of ammonium-bearing minerals relevant for icy bodies11
An improved method combining Fisher transformation and multiple endmember spectral mixture analysis for lunar mineral abundance quantification using spectral data11
A numerical study of the liquid motion in Titan’s subsurface ocean11
Automatic mapping and spatial analysis of high spatial resolution closed terrain depressions and mounds on martian landscapes11
Elasticity of selected icy satellite candidate materials (CO2, C6H6, MgSO4·7H2O and CaSO4·2H2O) revisited by dispersion corrected density functional theory11
Observations of alkaline emissions NaI, KI and LiI during first minutes after DART probe impact on Dimorphos11
Impact of UV radiation on the Raman and infrared spectral signatures of sulfates, phosphates and carbonates: Implications for Mars exploration11
Characterising water in Lunar and Martian regolith materials using nuclear magnetic resonance11
Principal Component Analysis applied on MASCS/MESSENGER data for the spectral investigation of Mercury's surface11
A thermal origin for super-high-frequency marsquakes11
The effect of planetary flybys on singly synchronous binary asteroids11
Regions of slow apparent motion of close approaching asteroids: The case of 2019 OK11
Uranus and Neptune as methane planets: Producing icy giants from refractory planetesimals11
Spatial extent of dust storm boundaries in the Mars Dust Activity Database11
The influence of passing field stars on the solar system’s dynamical future11
Martian nonmigrating atmospheric tides in the thermosphere and ionosphere at solar minimum11
New and improved orbits of some historical comets: 6TH and 7TH centuries11
A novel auger-based system for extraterrestrial in-situ water resource extraction11
Geological mapping and chronology of lunar landing sites: Apollo 1411
Complex Ice Chemistry: A comparative study of electron irradiated planetary ice analogues containing methane11
Rheological properties and ages of lava flows on Alba Mons, Mars11
Laboratory measurements of the 15–46 cm wavelength opacity of water vapor under temperature conditions characteristic of the deep atmosphere of Jupiter11
The impact of asteroid shapes and topographies on their reflectance spectroscopy11
Ionosphere of Mars during the consecutive solar minima 23/24 and 24/25 as seen by MARSIS-Mars Express11
High-velocity oblique impact experiments on ice and snow spheres: Implications for the collisional evolution of icy planetesimals at different thermal evolution stages11
Unexpected mineral impact on organic evolution during simulated aqueous alteration in asteroids11
Ed. Board11
High alumina basalts identification and their feature analysis in Mare Fecunditatis11
Investigating the feasibility of an impact-induced Martian Dichotomy11
Measurement of D/H and 13C/12C ratios in methane ice on Eris and Makemake: Evidence for internal activity11
Editorial Board11
Global estimates of lunar surface chemistry derived from LRO diviner data10
0.38093996047974