2014 GSA Annual Meeting in Vancouver, British Columbia (19–22 October 2014)

Paper No. 92-9
Presentation Time: 10:35 AM


DETHIER, David P., Geosciences Dept, Williams College, Williamstown, MA 01267, OUIMET, William B., Dept. of Geography; Center for Integrative Geosciences, University of Connecticut, Storrs, CT 06269, KASTE, James, Geology, The College of William and Mary, McGlothlin-Street Hall, Williamsburg, VA 23188, SHEA, Neil, University of Connecticut, Center for Integrative Geosciences, Storrs, CT 06269, WYSHNYTZKY, Cianna E., School of Geography, Queen Mary University of London, Mile End Road, London, E1 4NS, United Kingdom, BIERMAN, Paul, Department of Geology and Rubenstein School of Environment and Natural Resources, University of Vermont, Delehanty Hall, 180 Colchester Ave, Burlington, VT 05405 and MONDRACH, Hannah, Center for Integrative Geosciences, University of Connecticut, Storrs, CT 06269, ddethier@williams.edu

Accumulation profiles and inventories of cosmogenic nuclides such as meteoric10Be, weapons-derived radionuclides such as 137Cs, and weathering-derived metals (Zr and pedogenic Fe (Fed)) allow estimates of soil residence time and erosion rates, and provide insight into geomorphic processes at short, millennial and longer time scales. Met 10Be and 137Cs profiles integrate surface erosion and vertical mixing whereas Fed and Zr reflect mainly bottom up accumulation and rates of vertical mixing. Manganese and Zn profiles reflect vegetative cycling and the control of mobility by organic matter. We report data from stable soils, mobile regolith on slopes, and alluvium from the Colorado Front Range where parent material is granitic, climate is cool, dry, and vegetation is coniferous. Profiles on stable surfaces generally reflect depositional and pedogenic processes, but on 24° slopes, vertical mixing of met10Be is incomplete in mobile regolith that has residence times of 10 to 20 ky. Zr values are irregular, likely reflecting local parent material variability, and accumulation profiles at many sites may derive from enrichment in fine, eolian-derived material, rather than strain. Catena studies using met10Be and 137Cs show that inventories are highest in toeslopes and in adjacent alluvial fans, demonstrating recent erosion and downslope transport of near-surface materials. Steady-state assumptions do not provide a complete description of slope evolution in the changing climates of latest Pleistocene and Holocene time. Reconnaissance sampling of toeslope and flood deposits suggests that near-surface processes following fires may profoundly alter the inventory of cosmogenic isotopes and organically mediated elements in hillslope soils. On the slow-weathering slopes of the Front Range, in-situ cosmogenic techniques may provide better descriptions of long-term slope evolution.