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Development of the accretionary prism along Peru and material flux after subduction of Nazca Ridge

Development of the accretionary prism along Peru and material flux after subduction of Nazca Ridge Results from Ocean Drilling Program Leg 112 indicated tectonic erosion of the Peruvian convergent margin during subduction of the Nazca Ridge followed by renewed accretion against the erosional scar. Seismic images and swath mapping morphology show a regional geology shaped as subduction of Nazca Ridge migrated 800 km along the Peru Trench. The accretionary prism is imaged at two stages of development since upper Miocene time with depth‐migrated seismic records in which the “back stop” is well defined. From these data, material flux can be quantified. After the ridge crest subducted and accretion dominated over erosion, the prism grew rapidly to 10‐ to 15‐km width. During rapid growth, the margin taper was large and about 60 percent of the sediment supply accreted. As the prism growth slowed, only 30 percent accreted despite an increased trench sediment supply. Since the convergence rate changed little, the inverse relation between sediment supply and prism growth rate suggests that other processes allow most of the sediment input to be subducted. The decreased prism growth may be partially controlled by varying the structure of the back stop. The force required to activate faults cutting across the back stop is probably greater than the force allowed by basal friction across the plate boundary. Thus the shear stress transmitted across the plate boundary is insufficient to drive “out‐of‐sequence” thrust faults that would thicken the back stop or raise it beyond a limited height. A constant back stop height limits accretion, and the subduction window appears to open and accommodate increased trench sediment beneath the back stop rather than inducing a transport of sediment over the top of the back stop. Nazca Ridge subduction affected the convergent margin mass flux for about 8 Ma. Mass balancing indicates an order of magnitude increase in the current sediment volume subducted in the north compared to that near the ridge crest. When growth of the accretionary prism slowed, a greater terrigenous input through the trench was accommodated by sediment subduction. The resulting range of material flux is estimated to increase the sediment interlayer between the plates about 500 m which may affect coupling. http://www.deepdyve.com/assets/images/DeepDyve-Logo-lg.png Tectonics Wiley

Development of the accretionary prism along Peru and material flux after subduction of Nazca Ridge

Huene, R.; Pecher, I. A.; Gutscher, M.‐A.
Tectonics , Volume 15 (1) – Feb 1, 1996
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References (52)

Publisher
Wiley
Copyright
Copyright © 1996 by the American Geophysical Union.
ISSN
0278-7407
eISSN
1944-9194
DOI
10.1029/95TC02618
Publisher site
See Article on Publisher Site

Abstract

Results from Ocean Drilling Program Leg 112 indicated tectonic erosion of the Peruvian convergent margin during subduction of the Nazca Ridge followed by renewed accretion against the erosional scar. Seismic images and swath mapping morphology show a regional geology shaped as subduction of Nazca Ridge migrated 800 km along the Peru Trench. The accretionary prism is imaged at two stages of development since upper Miocene time with depth‐migrated seismic records in which the “back stop” is well defined. From these data, material flux can be quantified. After the ridge crest subducted and accretion dominated over erosion, the prism grew rapidly to 10‐ to 15‐km width. During rapid growth, the margin taper was large and about 60 percent of the sediment supply accreted. As the prism growth slowed, only 30 percent accreted despite an increased trench sediment supply. Since the convergence rate changed little, the inverse relation between sediment supply and prism growth rate suggests that other processes allow most of the sediment input to be subducted. The decreased prism growth may be partially controlled by varying the structure of the back stop. The force required to activate faults cutting across the back stop is probably greater than the force allowed by basal friction across the plate boundary. Thus the shear stress transmitted across the plate boundary is insufficient to drive “out‐of‐sequence” thrust faults that would thicken the back stop or raise it beyond a limited height. A constant back stop height limits accretion, and the subduction window appears to open and accommodate increased trench sediment beneath the back stop rather than inducing a transport of sediment over the top of the back stop. Nazca Ridge subduction affected the convergent margin mass flux for about 8 Ma. Mass balancing indicates an order of magnitude increase in the current sediment volume subducted in the north compared to that near the ridge crest. When growth of the accretionary prism slowed, a greater terrigenous input through the trench was accommodated by sediment subduction. The resulting range of material flux is estimated to increase the sediment interlayer between the plates about 500 m which may affect coupling.

Journal

Tectonics – Wiley

Published: Feb 1, 1996

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