2015 GSA Annual Meeting in Baltimore, Maryland, USA (1-4 November 2015)

Paper No. 104-7
Presentation Time: 9:55 AM

LAST GLACIAL TEMPERATURES IN THE SIERRA NEVADA INFERRED FROM COSMOGENIC NOBLE GAS PALEOTHERMOMETRY


TREMBLAY, Marissa M., Department of Earth and Planetary Science, University of California, Berkeley, Berkeley, CA 94720; Berkeley Geochronology Center, 2455 Ridge Road, Berkeley, CA 94709, SHUSTER, David L., Department of Earth and Planetary Science, 479 McCone Hall, University of California, Berkeley, CA 94720; Berkeley Geochronology Center, 2455 Ridge Road, Berkeley, CA 94709, BALCO, Greg, Berkeley Geochronology Center, 2455 Ridge Road, Berkeley, CA 94709 and BADEN, Curtis W., Department of Geological Sciences, Stanford University, Stanford, CA 94305, mtremblay@berkeley.edu

Understanding the climate of the Sierra Nevada, California, and greater western North America during the last glacial period is important for calibrating climate models in this drought-susceptible area. However, deconvolving effects of temperature and precipitation on paleoclimate proxies can be difficult and often qualitative. Here, we apply cosmogenic noble gas paleothermometry (CNGP) to samples from Mt. Langley in the Sierra Nevada to quantitatively reconstruct temperatures during the last glacial period. Helium and neon experience diffusive loss at Earth surface temperatures in common minerals like quartz and feldspars. CNGP utilizes the diffusive behavior of cosmogenic 3He and 21Ne in these minerals to quantify the thermal histories of rocks during exposure to cosmic ray particles at Earth’s surface. We collected samples at the summit of Mt. Langley, inferred to be ice free during the last glacial, and from a nearby cirque floor, inferred to be shielded from cosmic rays by ice until 13 ka, and measured cosmogenic 3He and 21Ne concentrations in quartz from these samples. We will use cosmogenic 21Ne, which is retained at surface temperatures, to constrain steady-state erosion rates of summit samples, and cosmogenic 3He, which exhibits open-system behavior, to quantify time-integrated temperatures during surface exposure. We will also quantify the kinetics of helium diffusion in these samples through step-degassing experiments on proton-irradiated quartz aliquots.