GSA Annual Meeting in Indianapolis, Indiana, USA - 2018

Paper No. 207-10
Presentation Time: 4:10 PM

RECONSTRUCTING LATE MIOCENE-EARLY PLIOCENE PALEOCLIMATE OF SONOITA CREEK BASIN, AZ


CARNES, Lorraine K., School of Earth and Space Exploration, Arizona State University, ISTB4 - BLDG75, 781 E Terrace Mall, Tempe, AZ 85287-6004 and HEIMSATH, Arjun M., School of Earth and Space Exploration, Arizona State University, ISTB4, Tempe, AZ 85287

The relative importance of climate vs tectonics driving landscape evolution is complex and nontrivial. The tectonically quiescent Sky Islands (high elevation/low relief mountains) of SE Arizona enable a unique opportunity to explore the impact of climate on landscape evolution over the past 10Ma. Here we present preliminary results from a paleoclimate study using 13C and 18O isotopes preserved in Miocene-Pliocene (6-3Ma) carbonate horizons in Sonoita Creek basin. We sampled five paleosol horizons containing carbonate nodules to analyze 13C and 18O isotopic ratios in a bulk sample isotope ratio mass spectrometer. The isotopic values are reported in context of the Vienna PeeDee Belemnite (VPDB) global standard, and range from -3.2 to -0.9‰ for 13C and -5.4 to -3.5‰ for 18O. These isotopic values are consistent with the Wang (1993) paleoclimate study in the nearby St. David Formation, indicating that calcrete formation occurred from the per descensum model of pedogeic caliche formation in which carbonate nodules develop in the zone of carbonate accumulation above the water table. We therefore attribute the ẟ18O isotope to reflect soil the oxygen isotopic composition of meteoric water and the ẟ13C to reflect the proportion of C3:C4 biomass present during formation. This proof of concept study enables a novel, high resolution landscape evolution analysis using a suite of paleoclimate, paleomagnetic, and cosmogenic 10Be paleoerosion rate data. In addition to these preliminary results, we present our study design of sampling every calcareous paleosol of the Sonoita Creek basin fill (~34 horizons) to reconstruct the paleoclimate record during sediment deposition. We will also provide an independent time constraint with a magnetostratigraphic study to correlate polarity reversals in the basin fill with the Geomagnetic Polarity Time Scale. Finally, we present our methodology for collecting suites of sediment samples constrained within single paleosol horizons to determine 10Be cosmogenic paleoerosion rates. Our goal with this project is to relate paleoerosion rates to climate to understand the erosional history of the basin and range topography of SE Arizona.