Paleogeographic reconstruction of regional accretionary complex architecture, Franciscan Complex, northwestern San Francisco Bay Area, California, USA

Author:

Raymond Loren A.12ORCID,Bero David A.13

Affiliation:

1. 1Coast Range Geological Mapping Institute, 3327 Cypress Way, Santa Rosa, California 95405, USA

2. 2Emeritus Professor, Department of Geological and Environmental Sciences, Appalachian State University, Boone, North Carolina 28608, USA

3. 3Emeritus Faculty, Department of Geology, Sonoma State University, 1801 East Cotati Avenue, Rohnert Park, California 94928, USA

Abstract

Abstract The Franciscan Complex of western California, USA, the archetypal subduction accretionary complex, cannot serve as a model subduction accretionary complex unless its local-to-regional architecture is clearly understood. Yet, architectural details are not clearly understood in many regions, including the northwestern San Francisco Bay Area. Here, Cenozoicage, dextral strike-slip faulting on faults of the San Andreas System fragmented the original architecture, forming crustal blocks and juxtaposing fragments of accretionary rock of different tectonostratigraphy. One little-known Cenozoicage fault and block boundary, the Tamarancho Shear Zone, separates northeastern crustal blocks that are dominated by Franciscan rocks from southwestern blocks with significantly different Franciscan accretionary tectonostratigraphy. The northeastern blocks have abbreviated accretionary stacks with at least one blueschist-facies accretionary unit, whereas the southwestern blocks lack blueschist-facies accretionary units and have either a westward-and-downward–younging Franciscan tectonostratigraphy or thrustsheet stacks composed of partial sequences of ocean-plate stratigraphy rocks. The northwestern San Francisco Bay Area Franciscan Complex is bounded on the southwest by the San Andreas fault (sensu stricto) and on the northeast by the Petaluma Valley–Point Richmond–Silver Creek fault. Using paleogeographic reconstruction, the original Franciscan Complex accretionary architecture of the northwestern San Francisco Bay Area can be partially reconstructed by removing block separations on San Andreas System faults and enhanced by unfolding Cenozoic folds. Accretionary units of the northwestern San Francisco Bay Area Franciscan Complex were originally assembled ~190 km southeast of their present locations, west of the southern Diablo Range. Reconstruction of the accretionary complex in that location and considerations of tectonostratigraphy require that the Novato Block, located northeast of the Tamarancho Shear Zone, and the Mt. Tamalpais Block, to its southwest, be separated along or across strike in the reconstructed accretionary complex. Either dual subduction zone or faulted plate geometries produced the northwestern San Francisco Bay Area segment of the accretionary complex, and each model highlights the possibilities of along- or across-strike variations in the structure and history of the accretionary complex.

Publisher

Geological Society of America

Subject

Stratigraphy,Geology

Reference110 articles.

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