Tharsis Montes Mars: Evidence of Massive Recent Erosion Caused by Volcano-Ice Interactions

Physics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

5415 Erosion And Weathering, 5419 Hydrology And Fluvial Processes, 5480 Volcanism (6063, 8148, 8450)

Scientific paper

The Tharsis Montes volcanoes, Arsia, Pavonis and Ascreus, share many volcano-tectonic features, including fissure swarms that extend NE and SW away from their centers. Lavas and sedimentary deposits have built up fan shaped aprons that overlie or partly bury the fissures swarms to a distance of over 500 km from the volcano massifs. The pattern with depressions observed on the NE and SW sides of the Tharsis Montes suggests a common origin. The fissure swarms coincide with large-scale negative landforms, some 25 km wide and over 2 km deep. These negative landforms can further be divided into lineated channels and isolated circular depressions or pit craters. While tectonic movements have surely been a major factor in forming the depressions the overall character of this network resembles erosional channels. Volcanism culminated most likely within the fissures swarms where surface lavas are visibly draped by a cover of sedimentary origin. Teardrop shaped crater remnants with erosional collar grooves are found in these deep depressions, e.g. Pavonis Mons. The derived teardrop orientation is downstream within the depressions and oblique to local wind directional pattern. The volcano-tectonic pattern, erosional morphology and pit craters all conform to an origin where volcanism has produced meltwater that in turn has led to jokulhlaups, both within the Montes calderas, the fissure swarms and even on the flank volcano slopes. Research has shown that the age of volcano units, based on crater counting, is lowest on the fissure swarm floors. Volcano-ice interactions within the calderas are likely to have forced copious quantities of melt water into the fissures swarms and caused large-scale erosion there. A genetic relationship is suggested between the erosional valley systems and the locus of maximum volcanism within the fissures swarms. The process of jokulhlaups resulting from magma-ice interactions can account for the generation of this erosional pattern. Large scale melting of ice within Tharsis calderas and leakage of meltwater from there through fissure swarms can account for the erosional phenomena observed within the NE-SW Montes depressions.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Tharsis Montes Mars: Evidence of Massive Recent Erosion Caused by Volcano-Ice Interactions does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Tharsis Montes Mars: Evidence of Massive Recent Erosion Caused by Volcano-Ice Interactions, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Tharsis Montes Mars: Evidence of Massive Recent Erosion Caused by Volcano-Ice Interactions will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-749079

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.