Medial Cretaceous Subduction Erosion of Southwestern North America: New Hypothesis for the Formation of the Catalina Schist M. Grove1 Department of Earth & Space Sciences, University of California, Los Angeles, 3806 Geology, Los Angeles, CA 90095, Tel. (310) 794-5457; FAX: (310) 825-2779
[email protected] G.E. Bebout Department of Earth & Environmental Sciences, Lehigh University, 31 Williams Dr, Bethlehem, PA 18015. C.E. Jacobson Department of Geological and Atmospheric Sciences, 253 Science I, Iowa State University, Ames, IA 50011-3212 D.L. Kimbrough Department of Geological Sciences, San Diego State University, 5500 Campanile Drive, San Diego CA 92182-1020 R.L. King Department of Earth & Environmental Sciences, Lehigh University, 31 Williams Dr, Bethlehem, PA 18015. O.M. Lovera Department of Earth & Space Sciences, University of California, Los Angeles, 3806 Geology, Los Angeles, CA 90095. 1Corresponding author Submitted August 4, 2006 to GSA Special Paper Formation and applications of the sedimentary record in arc collision zones Edited by Amy E. Draut, Peter D. Clift, and David W. Scholl Abstract The high P/T Catalina Schist underlies the inner southern California borderland outboard of southwestern North America and records amphibolite facies recrystallization and partial melting at ca. 115 Ma and 40 km depth. While inverted metamorphism down to lawsonite albite facies across low-angle faults has most commonly been regarded as a product of nascent subduction, new detrital zircon U-Pb ages (33 samples; N = 645) demonstrate that the Catalina Schist was derived from successively accreted sediment shed from the evolving northern Peninsular Ranges batholith. Zircons from high-grade metasediments represent early Aptian, craton-enriched detritus shed predominantly from the batholith’s pre-Cretaceous flysch wallrocks and the Late Jurassic to Early Cretaceous volcanic cover.