T201 The Franciscan Assemblage and Tectonostratigraphic Terranes of the Western United States II: A Tribute to M.C. Blake Jr.
Tuesday, 20 October 2009
1:30 PM - 5:30 PM
B110/111/112
GEOLOGY AND GEOCHEMISTRY OF THE DE ROUX UNIT AND POSSIBLY CORRELATIVE TECTONOSTRATIGRAPHIC TERRANES WITHIN THE CASCADE MOUNTAINS, WASHINGTON
Paper number: T201-8
Program: Technical Sessions
Time: 3:20 PM – 3:35 PM
Authors
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Robert B. MillerSan Jose State University, San Jose, CA
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Joe D. DragovichGeology and Earth Resources Division, Olympia, WA
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Ellen P. MetzgerSan Jose State University, San Jose, CA
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Jonathan S. MillerSan Jose State University, San Jose, CA
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Gregory D. HarperUniversity at Albany, Albany, NY
Abstract
The western mélange belt and Russell Ranch complex have similar metamorphic facies, and metaigneous & metasedimentary rock types as the De Roux unit. The western mélange belt is penetratively deformed, volcanically derived sandstones are more common than the De Roux, and sparse fossils give Jurassic-Early Cretaceous ages, with rare Permian limestone. A U-Th-Pb zircon age from a metatonalite is ~150-160 Ma. LA-ICP-MS detrital zircon dating from sandstone indicates a youngest age population of ~96 Ma, with a significant population at ~147 Ma. Sparse geochemistry of greenstone from the western mélange belt includes 3 IAT and 1 MORB, and 2 tuffs are CA. The Russell Ranch complex is less deformed then the De Roux and arkosic sandstones are more common. Radiolarians from chert are Late Jurassic-Early Cretaceous and a limestone clast in a breccia is Permian. Sparse geochemistry of greenstone from the Russell Ranch complex includes 9 WPB and 2 MORB. Deformed plutonic rocks of the Indian Creek complex are steeply faulted against the Russell Ranch complex; two U-Pb zircon ages from these plutonic rocks are ~154 Ma.
We suggest that the De Roux unit, western mélange belt and Russell Ranch complex are correlative. The structure, lithologies, metamorphic grade, and ages of these terranes suggest that they may be both olistostromal and tectonic in origin; and formed within an accretionary wedge.