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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
The formation of cone chains in the Chryse Planitia region on Mars and the thermodynamic aspects of this process
DOI: 10.1016/j.icarus.2023.115473 Bibcode: 2023Icar..39615473C

Czechowski, Leszek; Zalewska, Natalia; Zambrowska, Anita +3 more

This paper considers a small region in Chryse Planitia where several subparallel chains of cones are observed. Despite many papers on small Martian cones, the mechanism of their formation is not unequivocally explained, nor the reason for their arrangement in subparallel chains. In this paper, we test a few hypotheses stating that most of the cone…

2023 Icarus
MEx 2
Observations of a dust tail gap in comet C/2014 Q1 (PanSTARRS)
DOI: 10.1016/j.icarus.2022.115286 Bibcode: 2023Icar..39015286A

Afghan, Qasim; Jones, Geraint H.; Price, Oliver +1 more

Cometary dust tails display a wide array of structures, most believed to be caused by a variable dust production, size distributions, fragmentation processes, and interactions with the solar wind, e.g. Price et al. (2019). However, not all these structures are fully understood. Here we report the discovery of a curious new dust tail feature, first…

2023 Icarus
SOHO 2