Evolution of Extensional Systems

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Evolution of Extensional Systems Faculty of Science Masaryk University Department of Geological Sciences Evolution of Extensional Systems Literature Thesis in Requirement for Masters Author: B.Sc. Cameron Sheya Supervisors: Assoc. Prof. RNDr. Rostislav Melichar, Dr., Prof Michal Nemˇcok, DrSc. Brno, Czech Republic 2010 Contents Table of Contentsi Preface ii 1 Classification of rift systems: Basics1 1.1 Continental Rifts................................1 1.1.1 Narrow Rifts..............................2 1.1.2 Wide rifts................................2 1.2 Pull-apart basins................................5 1.3 Back-arc Basins................................. 10 1.4 Cratonic Sags.................................. 11 2 Rift system linkages and geometries 16 2.1 Fault geometries and linkages......................... 16 2.2 Fault linkages.................................. 18 2.3 Sub-basin interactions and the role of extension geometry in the process.. 22 3 Pull-apart basin development and geometries 28 3.1 Basic basin evolution and resulting geometries................ 28 Bibliography 38 i Preface The purpose of this literature thesis is to create a concise report on the extension and associated basin types and their subsequent history in the orogenic foreland setting. This thesis was written with the intent of first classifying the types of extensional basins and then describing their evolution. The understanding of the basin dynamics throughout their history will help in interpreta- tions of past and present day tectonic regimes. Final chapters discuss characteristics and dynamics of foreland basins including potential inversion of pre-existing extensional basins. ii Chapter 1 Classification of rift systems: Basics 1.1 Continental Rifts Continental rifts are areas where extension of the continental lithosphere leads to a subsid- ing basin.It is broken by several normal faults or several sets of normal faults, which can lead to either passive or active upwelling of the hot asthenospheric material underneath the area of the rift (Allen & Allen, 1990, 2005; Brun, 1999). Good examples of continental rifts come from the Basin and Range Province in the Western United States (Hamilton, 1987) and East African rift (Rosendahl, 1987). Extension within these continental rift systems continuously evolves until subsequent re- gional tectonic process either changes the existing local tectonic regime into another, (e.g. change from rifting to thrusting) or some process halts the extension, (e.g. the lack of sufficient stresses to control faulting) (Withjack et al, 2002). Continental extension has several associated factors such as: • high heat flow in the extended basin (Allen & Allen, 1990; Behn et al, 2002); • high temperature gradient from the basin to the un-extended margins (Allen & Allen 1990); • negative gravity anomaly (Prieto, 1996, Allen & Allen 2005); • internal structural highs, which may sometimes become inverted sedimentary prove- nances for deposition in the basin (Allen & Allen, 1990); • possibility associated magmatism due to the upwelling of hotter material from the asthenosphere (Behn et al, 2002); 1 1.1 Continental Rifts 2 • if the basin itself has emplaced basalt or granite, it will result in a positive magnetic anomaly (Prieto, 1996) and; • changes in isostacy. Continental rifts can be classified into narrow and wide rifts (Allen & Allen, 1990; Brun, 1999). Narrow continental rifts are areas of extension in the lithosphere that result in a stretching instability when the geotherm is higher than normal and the crustal thickness is in the range of 30-40 km whereas wide rifts are wider than the thickness of the lithosphere in which they occur (figure 1.1 ; Brun, 1999). 1.1.1 Narrow Rifts Narrow rifts are typically found in areas that have thermal anomalies which are associated with: • previous thinning of the lithosphere; • in areas with high mantle strength (Gueydan et al., 2008); • localized magmatism either from tectonic reasons or the influence of a hotspot; and/or • regions of localized strain weakening that affects the stronger layers of the continental lithosphere (Buck, 1991). Passive margins are incorporated into the classification of narrow rifts due to the thickness of lithosphere in which they generally evolve. Pre-rift rheology and thermal conditions of the crust play an integral role in determining the type and geometry of the rift. Passive margins are similar to the aforementioned continental rift systems, however; the upwelling of the Moho and asthenosphere is more pronounced in the formation of a passive margin. This upwelling of the Moho and asthenosphere usually has a longer wavelength than the width of the rift itself. Passive margins usually have a width range from around 100 km to 400 km (Brun, 1999). Examples of this rift type are found on the entire coastal margin of Africa, eastern margin of North America and the coastal margins of Australia among other coastal regions throughout the world (figure 1.2). 1.1.2 Wide rifts Wide rifts are wider than the thickness of the lithosphere in which they occur (Allen & Allen, 1990; Brun, 1999). The extensional event in the wide rift settings take place 1.1 Continental Rifts 3 (a) (b) Figure 1.1: (a) Idealized narrow rift with examples of passive margins and oceanic rift stages; (b) wide rift system, note how the brittle lithosphere has been thickened due to a previous compressional event (Brun, 1999) 1.1 Continental Rifts 4 Figure 1.2: Global distribution of passive margins. Compiled from Melluso et al., 2002; Geoffroy, 2005; Watkeys, 2002; Leroy, 2008. 1.2 Pull-apart basins 5 after a period or multiple periods of lithospheric thickening that can be associated with a subduction or area of collision setting. Wide rifts are known to reach widths of up to 1000 km (Brun, 1999) and are usually separated into sub-basins. An example of a wide rift that has been separated into sub-basins is the Basin and Range Province in the Western United States. This rift contains several tilted horst blocks that separate the individual sub-basins (Hamilton, 1987). Wide rifts are usually characterized by a horst-and-graben architecture and the frequent occurrence of core complexes (Hamilton, 1987; Brun, 1999). The models of Gueyadan et al., (2008) have shown that wide rifts occur in areas where the lower crust is very ductile and weak which leads to a more wide spread fracturing of the brittle crust. Core complexes occur in areas with a very low angle normal detachment fault that allows the hotter and more ductile material to protrude through the tilted blocks of a wide rift sys- tem (Allmendinger and Platt, 1983; Brun et al., 1994; Brun, 1999). When a core complex is forming, the extension of the upper crust is largely localized whereas the extension of the lower crust is much more broadly distributed (Allmendinger and Platt, 1983). The ductile material of the lower crust is then exhumed and exposed by a system of low angle normal faults. The exhumed material is then eroded and uplifted which leads to the exhumation of highly metamorphosed rocks (Brun, 1999). These core complexes tend to occur in areas that have larger than normal heterogeneities in the crustal lithosphere (Brun, 1999). Wide rifts occur by definition over a large area, which accounts for large differences in the amount of strain throughout the whole basin (Hamilton, 1987). Therefore, there can be a multitude of different fault expressions, including low angle detachments of core complexes, and high-angle normal faults between the horsts and grabens, scattered throughout the basin as a whole (Allmendinger and Platt, 1983; Brun et al., 1994). 1.2 Pull-apart basins Pull-apart basins are structural depressions that are formed by localized zones of extension within an area of strike-slip deformation (figure 1.3 (a) ;(b); 1.4; Carey, 1958, Rahe et al., 1998). The areas of extension occur in the accommodation zone between two strike-slip branches that are nearing each other (Rahe et al., 1998; Sims, 1999). As the area between these two main controlling faults continues to become fractured, the subsequent linking and accommodation space created by this movement will create a subsiding extensional basin (Allen & Allen 1990). The resulting shape from the localized extension is usually rhombic (figure 1.3 (a) ;(b); 1.4; Price and Cosgrove, 1990; Rahe et al., 1998; Sims et al., 1999). The process of fault linking and subsequent extension and subsidence evolves as follows: • R shears begin to form throughout the accommodation zone between the two linking 1.2 Pull-apart basins 6 (b) (a) Figure 1.3: (a) Model set up from Rahe (1999) showing the initial parameters of a pull- apart system; (b) after deformation of the model in (a) showing the relative movements and area of accommodation (Rahe, 1999). strike-slip faults. The R shears have the same sense as the overall strike-slip regime (figure 1.5 (a); (b), Allen & Allen, 1990; Twiss & Moores, 1992). • as the basin continues to evolve, R' shears begin to propagate through the accom- modation zone. They have a displacement that is opposite to that of the overall strike-slip sense (figure 1.5 (a) ;(b); Allen & Allen, 1990; Sims et al., 1999). • subsequently, P shears begin to develop through the accommodation zone, having the same sense as the overall movement of the strike- slip system (figure 1.5 (a) ;(b); Allen & Allen, 1990). Tension fractures and normal faults are being developed inside the pull-apart basin apart from the mentioned R, R' and P shears (Allen & Allen 1990). • the final stage of linkages in a pull-apart basin is when the various fractures and faults hard-link the two controlling strike-slip faults together (Allen & Allen 1990). The evolution of a pull-apart can be divided into three stages (Rahe et al., 1998): 1. incipient; 2. early; and 3. mature. The incipient stage of a pull-apart is characterized by the initiation of graben or half graben which is oriented parallel to the oblique step located between the controlling strike-slip faults (figure 1.5 (a) ;(b);1.6; Rahe et al., 1998; Sims et al., 1999).
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