Sonoma Orogeny—A Reassessment

Abstract

The Late Permian to earliest Triassic Sonoma orogeny has long been envisioned as the result of an arc-continent collision that closed the Havallah oceanic basin, creating the Golconda allochthon, which was emplaced eastward onto the western edge of the continental margin along the Golconda thrust. Critical reevaluation of available stratigraphic, biostratigraphic, and structural data raise some fundamental issues with this scenario, including: (1) The Golconda allochthon experienced multiple phases of deformation both older and younger than the Sonoma orogeny; (2) the tectonostratigraphic successions in the Golconda allochthon record a disrupted depositional history; (3) these punctuated events and unconformities are mirrored by simultaneous punctuated tectonic disruptions of the adjacent continental margin; (4) some of the lithotectonic units within the Golconda allochthon have clear ties to a magmatic arc. These observations indicated that the Havallah basin did not originate as a simple, post-Antler orogeny rift basin, nor is the Mediterranean model for opening of a basin a solution to the initiation of this basin. Instead they imply a more complex paleogeography for the Havallah basin. The Late Permian–earliest Triassic closure of the Havallah basin did result in the development of the Golconda allochthon sensu stricto, but final emplacement of the Golconda allochthon was likely an Early–Middle Jurassic event.