Equatorial glaciations on Mars revealed by gravitational collapse of Valles Marineris wallslopes
- Research areas:
- Year:
- 2011
- Authors:
- Journal:
- EARTH AND PLANETARY SCIENCE LETTERS
- Volume:
- 310
- Number:
- 3-4
- Pages:
- 182-191
- Month:
- OCT 15
- ISSN:
- 0012-821X
- BibTex:
- Abstract:
- Martian global climate models that account for evidence of past
glaciations reported in tropical to mid-latitude regions of Mars predict
accumulation of water ice in Valles Marineris during past periods of
high obliquity. Observational evidence for such glaciations is given
here. Topographic basement ridges of tectonic origin are common in
Valles Marineris, and display sackung features, an assemblage of
tectonic patterns that are diagnostic of deep-seated gravitational slope
deformation. This deformation is most easily explained by paraglacial
ridge failure subsequent to ridge wall debuttressing and decohesion
following the retreat of glaciers. This interpretation is supported by
extensive bibliographic analysis of sackung triggers on Earth, by
morphological evidence of subglacial erosion of the lower parts of
Valles Marineris wallslopes, of periglacial erosion of their upper parts
and by the presence of various types of glacial landforms on the floors
of Valles Marineris troughs. The age of these equatorial glaciations is
found to be older than 1.4 Gy and younger than 3.5 Gy. (C) 2011 Elsevier
B.V. All rights reserved.