Search Publications

Insight from the Noachian-aged fractured crust to the volcanic evolution of Mars: A case study from the Thaumasia graben and Claritas Fossae
DOI: 10.1016/j.icarus.2023.115770 Bibcode: 2024Icar..40715770P

Hauber, Ernst; Stephan, Katrin; Pieterek, Bartosz +1 more

Although most of the large volcanic landforms on Mars have been extensively studied, this is not the case for kilometer-sized landforms whose origin remains uncertain and which might provide important insights into the evolution of Martian volcanism. Previously, different populations of small-scale putative scoria cone volcanoes have been describe…

2024 Icarus
MEx 3
Sublimation and infrared spectral properties of ammonium cyanide
DOI: 10.1016/j.icarus.2024.116007 Bibcode: 2024Icar..41316007G

Gerakines, Perry A.; Yarnall, Yukiko Y.; Hudson, Reggie L.

The ammonium ion (NH4+) has been suggested to be present in interstellar ices and has been observed on the surfaces of planetary bodies using infrared (IR) spectroscopy as the primary means of identification. Evidence for several ammonium salts has also been found in the dust and surface ices of comet 67P/Churyumov-Gerasimenk…

2024 Icarus
Rosetta 3
First holistic modelling of meteoroid ablation and fragmentation: A case study of the Orionids recorded by the Canadian Automated Meteor Observatory
DOI: 10.1016/j.icarus.2023.115842 Bibcode: 2024Icar..40815842V

Vida, Denis; Brown, Peter G.; Campbell-Brown, Margaret +1 more

18 mm-sized Orionid meteoroids were captured in 2019 and 2020 by the Canadian Automated Observatory's mirror tracking system. Meteor position measurements were made to an accuracy of ∼1m and the meteors were tracked to a limiting magnitude of about + 7 . 5 at the faintest point. The trajectory estimation shows the intrinsic physical dispersion of …

2024 Icarus
Rosetta 3
Possibly seismically triggered avalanches after the S1222a Marsquake and S1000a impact event
DOI: 10.1016/j.icarus.2023.115942 Bibcode: 2024Icar..41115942L

Rodriguez, S.; Lognonné, P.; Perrin, C. +9 more

Ground motion from seismic events detected by the SEIS/InSight seismometer on Mars could potentially trigger dust avalanches. Our research strongly suggests that the seismic event S1000a may have triggered a significant number of dust avalanches. In contrast, following the seismic event S1222a, there was only a modest increase in avalanche occurre…

2024 Icarus
MEx 2
Glacial sculpting of a martian cratered landscape on the northeastern flank of the Hellas basin
DOI: 10.1016/j.icarus.2024.116211 Bibcode: 2024Icar..42016211G

Moore, Jeffrey M.; Wilson, Sharon A.; Howard, Alan D. +2 more

The interiors and exteriors of the >25 km diameter Batson, Nako, Salkhad, and Jori craters (and McCauley crater to a lesser degree) on the northeastern rim of Hellas basin, Mars, were extensively modified by glacio-fluvial and glacio-lacustrine activity during the Middle and Late Amazonian, from some time before 1.4 Ga to the present as reveale…

2024 Icarus
ExoMars-16 MEx 2
Lunar elemental abundances as derived from Chandrayaan-2
DOI: 10.1016/j.icarus.2023.115898 Bibcode: 2024Icar..41015898N

Bhatt, M.; Narendranath, S.; Pillai, Netra S. +6 more

The distribution of Mg, Al, Si, Ca and Fe on the lunar surface are important to understand the petrological characteristics of the Moon and its geological evolution. We derived new elemental distribution maps using the Chandrayaan-2 Large Area Soft X-ray Spectrometer (CLASS) experiment onboard the Chandrayaan-2 Orbiter. These are the first set of …

2024 Icarus
Chandrayaan-1 2
Polyphase tectonics on Mars: Insight from the Claritas Fossae
DOI: 10.1016/j.icarus.2024.115972 Bibcode: 2024Icar..41115972B

Tosi, Silvano; Balbi, Evandro; Ferretti, Gabriele +2 more

The Claritas Fossae (CF) is an elongated system of scarps and depressions >900 km long, representing the western boundary of the Thaumasia Region to the south of the Tharsis volcanic province. Although there is general agreement on the tectonic nature of such major physiographic feature, the processes that led to its formation are still debated…

2024 Icarus
MEx 2
Comets, sliding of surface dust on illuminated surfaces
DOI: 10.1016/j.icarus.2023.115861 Bibcode: 2024Icar..41015861K

Kossacki, Konrad J.; Wesołowski, Marcin; Mikołajków, Tomasz +1 more

In our paper we presented the results of our laboratory experiments dealing with the formation and sliding of the desiccated nonvolatile granular material down the samples of potential cometary analogs. The studied samples were composed of porous aggregates containing water ice, quartz sand and charcoal. Their surfaces were initially free of desic…

2024 Icarus
Rosetta 2
Characterization of aqueous alteration and formation of salty exposures at Ius Chasma, Mars
DOI: 10.1016/j.icarus.2023.115800 Bibcode: 2024Icar..40815800W

Flahaut, Jessica; Weitz, Catherine M.; Bishop, Janice L. +6 more

Intriguing outcrops in Ius Chasma provide a window into past aqueous processes in Valles Marineris, Mars. Hydrous sulfate minerals are abundant throughout this region, but one area in Ius Chasma includes phyllosilicates, opal, and additional materials with unusual spectral features. This study at Geryon Montes, an east-west horst that divides Ius …

2024 Icarus
MEx 2
Atmospheric gravity waves in Venus dayside clouds from VIRTIS-M images
DOI: 10.1016/j.icarus.2024.116076 Bibcode: 2024Icar..41516076S

Cardesín-Moinelo, Alejandro; Hueso, Ricardo; Peralta, Javier +3 more

We perform a survey of the Visible and Infrared Thermal Imaging Spectrometer-Mapper (VIRTIS-M) images onboard the Venus Express space mission, at four narrow wavelength bands that target different altitude regions on the cloud deck of Venus' atmosphere (280–320, 365–400, 580–600, 900–920 nm). Our goal was to detect and characterize atmospheric gra…

2024 Icarus
VenusExpress 2