Affiliation:
1. School of Earth & Ocean Sciences, University of Victoria, Victoria, British Columbia, Canada V8P 5C2
2. Department of Earth & Planetary Sciences, Harvard University, Cambridge, MA 02138, USA
Abstract
Abstract
Lithospheric cusps occur where arcs are joined end to end. Where a subducting
plate moves directly into a cusp, the slab experiences lateral constriction due to
the cusp geometry. Buckled slabs of Cenozoic age occur at cusps (also known as
‘syntaxes’) in the Arabian, Indian, Pacific, Juan de Fuca and other plates. Here I
report an Ediacaran example from the cusp of the Congo Craton where Pan-African
collision zones meet at a right angle in NW Namibia. The craton was blanketed by
syn- and post-rift Neoproterozoic marine carbonate, disconformably overlain by
collision-related foredeep clastics. The disconformity has little stratigraphic
relief in a 900 km-long fold belt rimming the craton, except within 60 km of the
cusp apex where foredeep deposits bury a megakarst landscape floored by exhumed
crystalline basement. Forebulge uplift, estimated from palaeokarst relief, was
≥1.85 km. This far exceeds characteristic forebulge heights of
c. 0.5 km and matches the deepest part of the Grand
Canyon of Arizona (USA). Coeval with megakarst development, map-scale mass slides
moved coherently westwards and southwards towards the advancing accretionary
prisms. Rapid burial by foredeep clastics preserved the megakarst palaeosurface
and associated mass slides; folding them brought protection from complete
destructive resurfacing for eons.
Publisher
Geological Society of London
Subject
Geology,Ocean Engineering,Water Science and Technology
Cited by
8 articles.
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