Abstract

Post-subduction dextral faulting was restored to evaluate the spatial distribution of units of the Franciscan subduction complex of California that formed as a result of subduction accretion. The Franciscan and related rocks of western California exhibit significant along-strike variation in its recording of subduction-accretion processes. Most notably, two segments 830 km apart record subduction erosion associated with low-angle subduction events that took place at ca. 120 Ma and ca. 80–70 Ma in the north and south, respectively. This spatial relationship is not affected by restoration of post-subduction dextral slip because none of the slip passes between the two inboard tectonic windows. Between these segments the subduction complex records net accretion from ca.175 Ma to 12 Ma, but includes horizons recording non-accretion. None of the accreted units of the subduction complex are preserved over the entire length of the subduction complex. One unit, however, correlated on the basis of its structural level in the subduction complex and distinctive detrital zircon age spectra, accreted at about 80–83 Ma extends a strike length of 580 km, an amount increased to 850 km with restoration of post-subduction dextral faulting. The long-strike length of accretion of this unit demonstrates that detrital zircon age populations of subduction complex clastic rocks are poor indicators of strike-slip displacement. Some reaches of the subduction complex include schistose blueschist facies rocks (most Franciscan blueschist facies rocks are not schistose), whereas others do not, and some reaches lack blueschist facies rocks altogether. The significant along-strike variation in the Franciscan and related rock units reflects temporal and spatial differences in history of accretion, non-accretion, subduction erosion, and probably subduction dip. Similar time and space variation in processes and resultant geologic record should be expected for other subduction complexes of the world.

Highlights

  • INTRODUCTIONModern subduction zones exhibit along-strike variation from subduction-accretion (subduction fault slices into downgoing plate; referred to as “accretion” in this paper), non-accretion (subduction fault does not cut into either upper plate or downgoing plate), and subduction erosion (subduction fault cuts into upper plate) (e.g., von Huene, 1986; von Huene and Scholl, 1991; Clift and Vannucchi, 2004)

  • Modern subduction zones exhibit along-strike variation from subduction-accretion, non-accretion, and subduction erosion

  • Recognizing the details of along-strike variation of accretion, non-accretion, and subduction erosion along exhumed paleo subduction zones is difficult because of the need to restore post-subduction deformation and the challenges posed in identifying subduction erosion and non-accretionary horizons along paleo-subduction interfaces exhumed from depth ranges that are commonly >10 km beneath the sea floor

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Summary

INTRODUCTION

Modern subduction zones exhibit along-strike variation from subduction-accretion (subduction fault slices into downgoing plate; referred to as “accretion” in this paper), non-accretion (subduction fault does not cut into either upper plate or downgoing plate), and subduction erosion (subduction fault cuts into upper plate) (e.g., von Huene, 1986; von Huene and Scholl, 1991; Clift and Vannucchi, 2004). The most extensive unit in the Franciscan in terms of alongstrike extent occupies one of the lowest structural positions among prehnite-pumpellyite facies units in the main Franciscan outcrop belt, as well as constituting part of the Nacimiento Belt, has distinctive detrital zircon age spectra, and apparently was deposited and accreted about 80–83 Ma (Type E unit of Dumitru et al, 2016 in the Franciscan and Nacimiento Belt; Wakabayashi, 2015 for structural context) This clastic-dominated unit crops out along a strike distance of 580 km in present-day exposures and 830 km with restoration of postsubduction dextral faulting (northern and southern limits labeled as E(N) and E(S) respectively on Figures 1, 3). The general pattern of accretionary ages that young structurally downward (Ernst et al, 2009; Dumitru et al, 2010; Snow et al, 2010; Wakabayashi, 2015; Wakabayashi, 2021b) is unchanged by restoration of postsubduction faulting

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