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Eskers in a complete, wet-based glacial system in the Phlegra Montes region, Mars
DOI: 10.1016/j.epsl.2015.09.023 Bibcode: 2015E&PSL.431...96G

Balme, Matthew; Gallagher, Colman

Although glacial landsystems produced under warm/wet based conditions are very common on Earth, even here, observations of subglacial landforms such as eskers emerging from extant glaciers are rare. This paper describes a system of sinuous ridges emerging from the in situ but now degraded piedmont terminus of a Late Amazonian-aged (∼150 Ma) glacie…

2015 Earth and Planetary Science Letters
MEx 33
Landform assemblage in Isidis Planitia, Mars: Evidence for a 3 Ga old polythermal ice sheet
DOI: 10.1016/j.epsl.2014.12.002 Bibcode: 2015E&PSL.411..253G

Bourgeois, Olivier; Pochat, Stéphane; Souček, Ondřej +1 more

The floor of Isidis Planitia, a giant impact basin located close to the martian equator, exhibits a landform assemblage, nicknamed Thumbprint Terrain, made of Arcuate Ridges, Aligned Cones, Isolated Cones, Cone Fields, associated with a peripheral network of Sinuous Ridges, Linear Depressions, and Mounds. From a new comprehensive mapping initiativ…

2015 Earth and Planetary Science Letters
MEx 23
Evidence for Amazonian highly viscous lavas in the southern highlands on Mars
DOI: 10.1016/j.epsl.2015.01.033 Bibcode: 2015E&PSL.415..200B

Hauber, Ernst; Brož, Petr; Platz, Thomas +1 more

We have identified small-scale volcanic edifices, two cones and three domes with associated flows, within Terra Sirenum, a region situated in the martian southern highlands. Based on thermal, morphological, and morphometrical properties, and the determination of absolute model ages, we conclude that these features were formed by volcanic activity …

2015 Earth and Planetary Science Letters
MEx 20
A 3 Ga old polythermal ice sheet in Isidis Planitia, Mars: Dynamics and thermal regime inferred from numerical modeling
DOI: 10.1016/j.epsl.2015.06.038 Bibcode: 2015E&PSL.426..176S

Bourgeois, Olivier; Pochat, Stéphane; Souček, Ondřej +1 more

Isidis Planitia is a 1350 km wide impact crater located close to the martian equator. To test the hypothesis that the 2.8 to 3.4 Ga old Thumbprint Terrain preserved on the floor of this basin is a glacial landform assemblage, we perform a numerical simulation of glaciation with a thermo-mechanically coupled model of ice sheet dynamics. As model in…

2015 Earth and Planetary Science Letters
MEx 17
Multiple origins for olivine at Copernicus crater
DOI: 10.1016/j.epsl.2015.03.039 Bibcode: 2015E&PSL.420...95D

Head, James W.; Dhingra, Deepak; Pieters, Carle M.

Multiple origins for olivine-bearing lithologies at Copernicus crater are recognized based on integrated analysis of data from Chandrayaan-1 Moon Mineralogy Mapper (M3), Lunar Reconnaissance Orbiter (LRO) Narrow Angle Camera (NAC) and Kaguya Terrain Camera (TC). We report the diverse morphological and spectral character of previously kn…

2015 Earth and Planetary Science Letters
Chandrayaan-1 15
Volcanic terrain and the possible periglacial formation of "excess ice" at the mid-latitudes of Utopia Planitia, Mars
DOI: 10.1016/j.epsl.2015.04.033 Bibcode: 2015E&PSL.423..182S

Soare, R. J.; El-Maarry, M. R.; Conway, S. J. +2 more

At the mid-latitudes of Utopia Planitia (UP), Mars, a suite of spatially-associated landforms exhibit geomorphological traits that, on Earth, would be consistent with periglacial processes and the possible freeze-thaw cycling of water. The suite comprises small-sized polygonally-patterned ground, polygon-junction and -margin pits, and scalloped, r…

2015 Earth and Planetary Science Letters
MEx 12