Flat versus steep subduction: Contrasting modes for the formation and exhumation of high- to ultrahigh-pressure rocks in continental collision zones

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Abstract

Flat and steep subduction are end-member modes of oceanic subduction zones with flat subduction occurring at about 10% of the modern convergent margins and mainly around the Pacific. Continental (margin) subduction normally follows oceanic subduction with the remarkable event of formation and exhumation of high- to ultrahigh-pressure (HP–UHP) metamorphic rocks in the continental subduction/collision zones. We used 2D thermo-mechanical numerical models to study the contrasting subduction/collision styles as well as the formation and exhumation of HP–UHP rocks in both flat and steep subduction modes. In the reference flat subduction model, the two plates are highly coupled and only HP metamorphic rocks are formed and exhumed. In contrast, the two plates are less coupled and UHP rocks are formed and exhumed in the reference steep subduction model. In addition, faster convergence of the reference flat subduction model produces extrusion of UHP rocks. Slower convergence of the reference flat subduction model results in two-sided subduction/collision. The higher/lower convergence velocities of the reference steep subduction model can both produce exhumation of UHP rocks. A comparison of our numerical results with the Himalayan collisional belt suggests two possible scenarios: (1) A spatially differential subduction/collision model, which indicates that steep subduction dominates in the western Himalaya, while flat subduction dominates in the extensional central Himalaya; and (2) A temporally differential subduction/collision model, which favors earlier continental plate (flat) subduction with high convergence velocity in the western Himalaya, and later (flat) subduction with relatively low convergence velocity in the central Himalaya.

Research Highlights

►UHP rocks exhumation in steep subduction model ►HP rocks exhumation in flat subduction model ►UHP rocks exhumation in fast flat subduction model ►Spatially differential subduction/collision in western and central Himalaya ►Temporally differential subduction/collision in western and central Himalaya

Introduction

Oceanic subduction zones can be classified into normal-to-steep (high-angle) and flat (low-angle) subduction styles. Steep (normal) subduction usually has a dip angle of ≥ 30°at the top of the upper mantle (e.g., Turcotte and Schubert, 2002), whereas flat subduction is characterized by shallow dip angle and a high degree of coupling between the converging plates. In nature, flat subduction occurs at about 10% of the modern convergent margins and mainly around the Pacific, with the best known present-day examples located beneath western South America, in Peru and central Chile/NW Argentina (e.g., Gutscher et al., 2000a, Gutscher et al., 2000b, Lallemand et al., 2005). It has been proposed that flat subduction may have been widespread during the early stages in the Earth's history and contributed to the processes of continental growth in the Proterozoic and Archean (Abbott et al., 1994, Vlaar, 1983, Vlaar, 1985). However, the cause of flat subduction is the subject of an active discussion with several possible mechanisms having been proposed, e.g. the subduction of buoyant anomalies (such as bathymetric highs, aseismic ridges, or oceanic plateaus), rapid absolute motion of the overriding plate, interplate hydrostatic suction, a delay in the basalt to eclogite transition, the curvature of the margin, etc. (e.g. Gutscher et al., 2000b). In addition, several analogue (e.g., Chemenda et al., 2000, Espurt et al., 2008, Martinod et al., 2005) and numerical models (e.g., Van Hunen et al., 2002a, Van Hunen et al., 2002b, Van Hunen et al., 2004) have explored the conditions permitting the appearance of flat subduction zones as well as their consequences on overriding plate deformation. As discussed by van Hunen et al. (2004), flat subduction does not necessarily imply buoyant slabs. Other factors, such as overriding plate velocity and slab strength, may also play significant roles in controlling this process.

Continental (margin) subduction normally follows oceanic subduction under the convergent forces of lateral “ridge push” and/or oceanic “slab pull”. The remarkable event during early continental collision is the formation and exhumation of high- to ultrahigh-pressure (HP–UHP) metamorphic rocks. Occurrences of UHP terranes around the world have been increasingly recognized with more than 20 UHP terranes documented (e.g., Liou et al., 2004), which have repeatedly invigorated the concepts of deep subduction (> 100 km) and exhumation of crustal materials. Continental subduction/collision and exhumation of HP–UHP rocks are widely investigated with analogue (e.g., Boutelier et al., 2004, Chemenda et al., 1995, Chemenda et al., 1996) and numerical modeling method (e.g., Beaumont et al., 2001, Beaumont et al., 2009, Burg and Gerya, 2005, Burov et al., 2001, Gerya et al., 2008, Li and Gerya, 2009, Toussaint et al., 2004b, Warren et al., 2008a, Warren et al., 2008b, Yamato et al., 2007, Yamato et al., 2008). The tectonic styles of continental subduction can be either “one-sided” (overriding plate does not subduct) or “two-sided” (both plates subduct together) (Faccenda et al., 2008, Pope and Willett, 1998, Tao and O'Connell, 1992, Warren et al., 2008a), as well as several other possibilities, e.g. thickening, slab break-off, slab drips etc. (e.g., Toussaint et al., 2004a, Toussaint et al., 2004b). Models of HP–UHP rocks exhumation can be summarized into the following groups: (1) syn-collisional exhumation of a coherent and buoyant crustal slab, with formation of a weak zone at the entrance of the subduction channel (Chemenda et al., 1995, Chemenda et al., 1996, Li and Gerya, 2009, Toussaint et al., 2004b); (2) episodic ductile extrusion of HP–UHP rocks from the subduction channel to the surface or crustal depths (Beaumont et al., 2001, Warren et al., 2008a); and (3) continuous material circulation in the rheologically weak subduction channel stabilized at the plate interface, with materials exhumed from different depths (Burov et al., 2001, Gerya et al., 2002, Stöckhert and Gerya, 2005, Warren et al., 2008a, Yamato et al., 2007).

The previously-mentioned analogue and numerical models for continental subduction/collision associated with burial and exhumation of crustal rocks are mostly based on the steep (normal) subduction mode. It is unknown therefore what the characteristics of HP–UHP metamorphism and exhumation would be in the flat subduction mode. In order to address this issue, we used 2D thermo-mechanical numerical modeling to study the contrasting subduction/collision styles as well as the formation and exhumation of HP–UHP metamorphic rocks in both the flat and steep subduction modes. In addition, we investigated the sensitivities of the model predictions to the convergence velocity. The numerical model results are compared to the western and central Himalayas as this large, young continental collisional belt shows intriguing contrasts in subduction geometry and exhumation patterns along strike.

Section snippets

Numerical model design

The numerical simulations are conducted with the 2D code “I2VIS” (Gerya and Yuen, 2003a) based on finite differences and marker-in-cell techniques (see Appendix A.1 for details of the numerical methodology). Large scale models (4000 × 670 km, Fig. 1) are designed for studying the dynamic processes from oceanic subduction to continental collision associated with the formation and exhumation of HP–UHP rocks. The non-uniform 699 × 134 rectangular grid is designed with a resolution varying from 2 × 2 km in

Model results

Series of numerical experiments were conducted with variable dip angle of the initial weak zone as well as variable convergence velocity (Table 1). The configurations and parameters are shown in Figure 1 and Table S1, Table S2, Table S3.

Geological implications for the Himalayan collisional belt

The Himalayan range is one of the largest, latest and best documented continental collisional belts, and provides significant constraints on subduction/collision processes due to the many geological (e.g., DiPietro and Pogue, 2004, Kind et al., 2002, Leech et al., 2005, Royden et al., 2008, Tapponnier et al., 2001, Yin, 2006, Yin, 2009) and geophysical/seismological data available (e.g., Li et al., 2008, Nabelek et al., 2009, Negredo et al., 2007, Van der Voo et al., 1999).

The Himalayan belt

Why slab dip angle controls (U)HP exhumation

Numerical simulations show that the dip angle of the initial weak zone (“seed”) can result in either a flat or steep subduction style. If the weak seed has a low angle (e.g., 10° in Fig. 2, Fig. 3, Fig. 4), the high interplate hydrostatic suction (e.g., Gutscher et al., 2000b, Shemenda, 1993) results in strongly coupled plates, which will further lead to flat subduction. In this case, crustal materials of the subducting plate take a longer path (and time) to be subducted to a given depth

Conclusions

Numerical models show that the subduction angle plays an important role in controlling both continental collision modes and the metamorphic conditions of HP–UHP rocks. In the reference flat subduction model, the two converging plates are highly coupled with only HP rocks exhumed to the surface. In the reference steep subduction model, by contrast, the two plates are less coupled and UHP rocks are formed and exhumed. In addition, faster convergence of the reference flat subduction model produces

Acknowledgements

This work was supported by the fund from China Scholarship Council (CSC) and European Union Marie Curie ITN ‘Crystal2plate’ project (no. 215353) to ZHL; China National Natural Science Foundation project (40921001) and China Geological Survey project (1212010918035) to ZQX; and ETH Research Grants TH-0807-3, ETH-0609-2 and TopoEurope program to TVG. N. Ribe is thanked for discussion and polishing the English. Thorough and constructive reviews by S. Buiter, C. Beaumont and the editor Y. Ricard

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