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One million cubic kilometers of fossil ice in Valles Marineris: Relicts of a 3.5Gy old glacial landsystem along the Martian equator.

Authors :
Gourronc, Marine
Bourgeois, Olivier
Mège, Daniel
Pochat, Stéphane
Bultel, Benjamin
Massé, Marion
Le Deit, Laetitia
Le Mouélic, Stéphane
Mercier, Denis
Source :
Geomorphology. Jan2014, Vol. 204, p235-255. 21p.
Publication Year :
2014

Abstract

Abstract: Self-consistent landform assemblages suggest that Valles Marineris, the giant valley system that stretches along the Martian equator, was entirely glaciated during Late Noachian to Early Hesperian times and still contains huge volumes of fossil ice. Some of these glacial landform assemblages are illustrated here, with representative examples selected in three regions: Ius Chasma, Central Candor Chasma and the junction between Coprates Chasma and Capri Chasma. A morphological boundary separating an upper spur-and-gully morphology from a smooth basal escarpment has been spectacularly preserved along valley walls throughout Valles Marineris. The boundary winds around topographic obstacles and displays long-wavelength variations in elevation. It is associated with lateral benches, hanging valleys and truncated spurs. Comparisons with terrestrial analogs indicate that it is most reasonably interpreted as a glacial trimline. Chasma floors are covered by various kinds of terrains, including hummocky terrains, platy terrains, lateral banks, layered benches and a draping mantle. Landforms in these terrains and their spatial relationship with the interpreted trimline suggest that they correspond to various disintegration stages of an ancient glacial fill, currently protected by a superficial cover of ablation till. Altogether, these landforms and terrains compose a full glacial landsystem with wet-based glaciers that were able to flow and slide over their beds. It was most probably fed by ice accumulating at low elevations directly from the atmosphere onto valley floors and walls, with only minor contributions from tributary glaciers flowing down from higher elevations. Similar fossil glacial landsystems dating back from the early Martian history are to be expected in many other low-latitude troughs such as chasmata, chaos, valleys, impact craters and other basins. [Copyright &y& Elsevier]

Details

Language :
English
ISSN :
0169555X
Volume :
204
Database :
Academic Search Index
Journal :
Geomorphology
Publication Type :
Academic Journal
Accession number :
91969878
Full Text :
https://doi.org/10.1016/j.geomorph.2013.08.009