Search Publications

Ionosphere of Mars during the consecutive solar minima 23/24 and 24/25 as seen by MARSIS-Mars Express
DOI: 10.1016/j.icarus.2021.114616 Bibcode: 2023Icar..39314616S

Witasse, Olivier; Sánchez-Cano, Beatriz; Kofman, Wlodek +4 more

The Mars' ionospheric behavior during two consecutive solar minima (23/24 and 24/25) is investigated with the same dataset. In particular, we use the Mars Advanced Radar for Subsurface and Ionospheric Sounding (MARSIS) on board Mars Express to investigate the total electron content behavior of the whole atmosphere in relation to the solar irradian…

2023 Icarus
MEx 3
Permafrost molards as an analogue for ejecta-ice interactions at Hale Crater, Mars
DOI: 10.1016/j.icarus.2022.115363 Bibcode: 2023Icar..39115363M

Lucas, Antoine; Conway, Susan; Noblet, Axel +7 more

When the Hale impact crater penetrated the martian cryosphere 1Ga, landforms indicating post-impact volatile mobilisation were generated. We have found landforms in the ejecta blanket of Hale Crater similar to 'permafrost molards' found in periglacial environments on Earth, and probably related to the past or present presence of volatiles at/near …

2023 Icarus
MEx 3
Global surficial water content stored in hydrated silicates at Mars from OMEGA/MEx
DOI: 10.1016/j.icarus.2023.115537 Bibcode: 2023Icar..39815537R

Poulet, François; Cardesín-Moinelo, Alejandro; Martin, Patrick +2 more

Assessing the water content at the surface of Mars is key to understand the history of water and past climate of the planet but it also is very important for future exploration and potential In Situ Resource Utilization (ISRU). Numerous locations on the surface, known to harbor hydrated minerals, have been detected and their mineralogical assembla…

2023 Icarus
MEx 3
A race against the clock: Constraining the timing of cometary bombardment relative to Earth's growth
DOI: 10.1016/j.icarus.2023.115754 Bibcode: 2023Icar..40615754J

Nesvorný, David; Avice, Guillaume; Raymond, Sean N. +3 more

Comets are considered a potential source of inner solar system volatiles, but the timing of this delivery relative to that of Earth's accretion is still poorly understood. Measurements of xenon isotopes in comet 67P/Churyumov-Gerasimenko revealed that comets partly contributed to the Earth's atmosphere. However, there is no conclusive evidence of …

2023 Icarus
Rosetta 2
Subglacial catastrophic-flood origin of linear and curvilinear flat-rimmed pit chains on Mars: Evidence from geomorphological mapping and detailed landsystem analysis
DOI: 10.1016/j.icarus.2023.115439 Bibcode: 2023Icar..39515439K

Yin, An; Kakaria, Reva

Flat-rimmed pits lacking emanating flow-like features on pit margins are typically clustered as linear or curvilinear chains on Mars. Their formation has been attributed to faulting, volcanism, or roof collapse of subsurface voids. Here we test these end-member models by conducting landform analysis and systematic geomorphological mapping in the c…

2023 Icarus
MEx 2
Chicxulub-like Gale impact into an ocean/land interface on Mars: An explanation for the formation of Mount Sharp
DOI: 10.1016/j.icarus.2022.115306 Bibcode: 2023Icar..39015306D

Dohm, James M.; Williams, Jean-Pierre; Fink, Wolfgang +2 more

A geologic investigation of Gale Crater and surrounding terrain was conducted combining orbital data with reported in situ information collected through the Mars Science Laboratory (MSL Curiosity) rover cameras to better explain the anomalous features in and nearby Gale Crater with the primary focus being the formational history of Aeolis Mons, in…

2023 Icarus
MEx 2
A new shape model of the bilobate comet 67P/Churyumov-Gerasimenko
DOI: 10.1016/j.icarus.2023.115566 Bibcode: 2023Icar..40115566C

Chen, Min; Huang, Xianfeng; Yan, Jianguo +2 more

In this article, we performed the stereo-photogrammetric processing on over 5200 Rosetta/OSIRIS-NAC images to derive a global high-resolution 3D model of the bilobate comet 67P/Churyumov-Gerasimenko, which is visually richer and more convincing than the existing models (i.e., SPG-SHAP4S, SPC-SHAP5 and SPG-SHAP7). This shape model was used to gener…

2023 Icarus
Rosetta 2
The Bolometric Bond Albedo of Enceladus
DOI: 10.1016/j.icarus.2023.115429 Bibcode: 2023Icar..39415429L

West, Robert A.; Nixon, Conor A.; Fry, Patrick M. +13 more

The bolometric Bond albedo is a fundamental parameter of planets and moons. Here, combined observations from the Cassini spacecraft and the Hubble Space Telescope are used to determine the bolometric Bond albedo of Enceladus. We provide the full-disk reflectance of Enceladus across all phase angles (0° -180°) from 150 nm to 5131 nm, a spectral ran…

2023 Icarus
Cassini eHST 2
Spatial and temporal distribution of sinuous ridges in southeastern Terra Sabaea and the northern region of Hellas Planitia, Mars
DOI: 10.1016/j.icarus.2022.115399 Bibcode: 2023Icar..39415399G

Williams, Rebecca M. E.; Anderson, Ryan B.; Gullikson, Amber L.

Sinuous ridges are an important yet understudied component of Mars' hydrologic history. We have produced a map of sinuous ridges, valleys and channels, and tectonic ridges across southeastern Terra Sabaea and into northern Hellas Planitia (10°-45° S, 35°-80° E) using a CTX mosaic. Although we mapped different types of ridges and negative relief fe…

2023 Icarus
MEx 2
Topographical analysis of a candidate subglacial water region in Ultimi Scopuli, Mars
DOI: 10.1016/j.icarus.2022.115394 Bibcode: 2023Icar..39215394S

Mitri, Giuseppe; Genova, Antonio; Sulcanese, Davide +3 more

Radar signals of the MARSIS (Mars Advanced Radar for Subsurface and Ionosphere Sounding) instrument at the base of the South Polar Layered Deposits (SPLD) in the region known as Ultimi Scopuli, on Mars, have been interpreted as reflections from putative subglacial standing bodies of liquid water. The interpretation of the MARSIS radar signals is n…

2023 Icarus
MEx 2