Abstract

The local topographic slope of the accretionary prism is often used together with the critical taper theory to determine the effective friction on subduction megathrust. In this context, extremely small topographic slopes associated with extremely low effective basal friction (μ ≤ 0.05) can be interpreted either as seismically locked portions of megathrust, which deforms episodically at dynamic slip rates or as a viscously creeping décollement. Existing mechanical models of the long-term evolution of accretionary prism, sandbox models, and numerical simulations alike, generally do not account for heat conservation nor for temperature dependant rheological transitions. Here, we solve for advection-diffusion of heat with imposed constant heat flow at the base of the model domain. This allows the temperature to increase with burial, and therefore to capture how the brittle-ductile transition and dehydration reactions within the décollement affect the dynamic of the accretionary prism and its topography. We investigate the effect of basal heat flow, shear heating, thermal blanketing by sediments, the thickness of the incoming sediments. We find that while reduction of the friction during dewatering reactions result as expected in a flat segment often in the fore-arc, the brittle-ductile transition result unexpectedly in a local increase of topographic slope. We show that this counter-intuitive backproduct of the numerical simulation can be explained and by the onset of internal ductile deformation in between the active thrusts. Our models, therefore, implies significant viscous deformation of sediments above a brittle décollement, at geological rates, and we discuss its consequences in term of interpretation of coupling ratios at subduction megathrust. We also find that, with increasing burial and ductile deformation, the internal brittle deformation tends to be accommodated by backthrusts until the basal temperature becomes sufficient to form a viscous channel, parallel to the décollement, which serves as root to a major splay fault and its back-thrust and delimits a region with small topographic slope. Morphologic resemblances of the brittle-ductile and ductile segments with fore-arc high and fore-arc basins of accretionary active margins respectively allow us to propose an alternative metamorphic origin of the fore-arc crust in this context.

Highlights

  • IntroductionFore-arc wedges are to the first order well described by the critical taper theory (CTT) (Davis et al, 1983; Dahlen et al, 25 1984)

  • Several studies have suggested a link between the morphology of fore-arc wedges and the seismic behavior of megathrusts, showing a correlation between large subduction earthquakes and fore-arc basins or deep-sea terraces (Wells et al, 2003) or with negative free-air gravity anomalies (Song and Simons, 2003; Wells et al, 2003).Fore-arc wedges are to the first order well described by the critical taper theory (CTT) (Davis et al, 1983; Dahlen et al, 25 1984)

  • – brittle décollement and viscous internal deformation of fault-bounded blocks, where the topographic slope is in excess compared to the CTT and these large slopes should not be interpreted as the downdip limit of the seismogenic zone;

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Summary

Introduction

Fore-arc wedges are to the first order well described by the critical taper theory (CTT) (Davis et al, 1983; Dahlen et al, 25 1984) This theory assumes that wedges are built by accretion of material equivalent to sand pushed by a moving bulldozer over a frictional basal décollement. This theory has been very successful in describing the equilibrium morphology of wedges in response to accretion and as a function of its effective internal and basal frictional strength (Davis et al, 1983; Dahlen et al, 1984). Prograde metamorphic reactions that affect clay minerals release water in the system, which is suspected to raise fluid pressure and diminish effective friction Clay contents, their nature, and their evolution during accretion may affect the effective friction of the décollement as a function of temperature history. Their nature, and their evolution during accretion may affect the effective friction of the décollement as a function of temperature history. 40 Several studies have related the depth-dependence of subduction megathrust seismicity to the diagenetic transformation of smectite to illite, two clay minerals (Vrolijk, 1990; Hyndman et al, 1995; Oleskevich et al, 1999; Moore and Saffer, 2001)

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