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  4. Orogenic growth in the atlas mountains of SW Marocco - Insights from low-temperature thermochronometry and in situ cosmogenic dating
Project Title
Orogenic growth in the atlas mountains of SW Marocco - Insights from low-temperature thermochronometry and in situ cosmogenic dating
Internal ID
32710
Principal Investigator
Kalt, Angelika  
Status
Completed
Start Date
October 1, 2006
End Date
September 30, 2008
Investigators
Ivy-Ochs, Susan
Wieler, Rainer
Organisations
Centre d'hydrogéologie et de géothermie  
Identifiants
https://libra.unine.ch/handle/20.500.14713/2177
-
https://libra.unine.ch/handle/123456789/1946
Keywords
uplift erosion exhumation neotectonics north-africa marocco Denudation Morocco Anti- and High-Atlas Tectonics Fission-Track - and (U-Th)/He Thermochronometry in situ cosmogenic exposure dating North Africa Anti-Atlas High Atlas fission track dating (U-Th)/He thermochronometry in-situ cosmogenic exposure dating
Description
New U-Th/He data on apatites from the High Atlas of SW Morocco provide for the first time constraints on the exhumation history of the Atlas chain. U-Th/He ages on apatite range between 37 and 14 Ma for the axial zone of the High Atlas, between 39 and 13 Ma in the Sub-Atlas Zones and finally between 125 and 120 Ma in the Anti-Atlas. Age-altitude relationships in the axial zone of the High-Atlas suggest that exhumation attained 0.2 km/my for the Middle Miocene whereas the Anti-Atlas belt to the south either 1) did not undergo any protracted phase since the Late Jurassic-Early Cretaceous, or 2) undergoes such phase very recently that cannot be traced even with the lowest-temperature thermochronometer (U-Th/He on apatite). Preliminary data from the Sub-Atlas zones on both sides of the High-Atlas indicate that a 2-3 kms thick sedimentary pile of post-Cretaceous age is missing. The timing of this erosion is still unknown but will be constrained by thermal modeling through future Apatite Fission-Track and additional U-Th/He data, whereas sub-recent erosion rates are being determined by the production of in situ cosmogenic analyses on present-day river sands.
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