GSA Connects 2022 meeting in Denver, Colorado

Paper No. 218-12
Presentation Time: 11:15 AM

PEEKING THROUGH THE SLAB WINDOW: EXHUMATION OF ACCRETIONARY SEDIMENTS OVER A SLAB WINDOW IN THE WILLOW CREEK AREA, SOUTHERN TALKEETNA MOUNTAINS, ALASKA


MULLER, Isabella, Dept of Geosciences, University of Alaska Fairbanks, 900 Yukon Dr, Fairbanks, AK 99775-9702, REGAN, Sean, Geophysical Institute, University of Alaska Fairbanks, Fairbanks, AK 99775-9702, HOLLAND, Mark E., Department of Life, Earth, and Environmental Sciences, West Texas A&M University, 2403 Russell Long Blvd., Canyon, AK 79015 and SUHEY, Jane, Geophysical Institute, University of Alaska Fairbanks, 900 Yukon Dr, Fairbanks, AK 99775-9702

Most of south-central Alaska is interpreted as a subduction-accretion complex built on the southern margin of the Wrangellia composite terrane (WCT). The Hatcher Pass schist (HPs) of the WCT is an enigmatic chlorite-muscovite schist with plagioclase and garnet porphyroblasts located in the Willow Creek area of the southern Talkeetna Mountains. Preliminary detrital zircon (DZ) data suggests that the HPs may be correlative to accretionary complex rocks (Valdez Group). We conducted 1:24,000 scale bedrock geologic mapping, microstructural and petrographic analysis, thermobarometry, forward petrologic modeling, and DZ analysis of the HPs to test the hypothesis that the HPs is a subducted equivalent of the Valdez Group. Structural mapping shows that the oldest known foliation (S1) underwent isoclinal recumbent folding (F2) that resulted in the development of a regionally pervasive fabric (S2). Fragmented boudins, porphyroblast asymmetry, and rare S-C geometries indicate top-to-the-east shearing. Two sets of open, upright folds with SW-NE and NW-SE trending axes postdate the development of S2 and define a type 1 interference pattern. We interpret F3-4 to have formed during doming (F3) and continued tectonic exhumation (corrugations; F4) along a south-vergent detachment juxtaposing the HPs against the overlying Arkose Ridge Formation. Forward modeling of garnet and plagioclase microchemical data with Theriak-Domino indicate that the HPs reached peak metamorphic conditions of 500-650 ℃ and 10 kbar in a fluid-oversaturated system prior to exhumation. DZ data indicates a maximum depositional age of ca. 81 Ma and supports correlation with the Valdez Group. Based on these data, we propose the following tectonic evolution for the HPs: 1) incorporation into a subduction channel after ca. 81 Ma; 2) burial to >30 km paleodepths; 3) structural exhumation ca. 61-50 Ma during deposition of the Arkose Ridge Formation. Exhumation may have been driven by formation of a slab window via break-off of the Kula Plate.