CALL FOR PROPOSALS:

ORGANIZERS

  • Harvey Thorleifson, Chair
    Minnesota Geological Survey
  • Carrie Jennings, Vice Chair
    Minnesota Geological Survey
  • David Bush, Technical Program Chair
    University of West Georgia
  • Jim Miller, Field Trip Chair
    University of Minnesota Duluth
  • Curtis M. Hudak, Sponsorship Chair
    Foth Infrastructure & Environment, LLC

 

Paper No. 2
Presentation Time: 2:00 PM

MINERALOGY AND GEOCHEMISTRY OF VESICULAR SOILS AS AN ARCHIVE OF DUST DEPOSITION AND PROXY FOR A REGIONAL DUST SOURCE, CENTRAL UTAH, U.S.A


HYNEK, Scott A., Geosciences, Penn State University, 302 Hosler Building, University Park, PA 16802, FERNANDEZ, Diego P., Geology and Geophysics, University of Utah, Frederick Albert Sutton Building, 115 S. 1460 E. Rm 383, Salt Lake City, UT 84112, MACKEY, Glen N., Geology and Geophysics, University of Utah, 115 S. 1460 E. Rm 383, Salt Lake City, UT 84112, CERLING, Thure E., Department of Geology and Geophysics, University of Utah, Salt Lake City, UT 84112 and EHLERINGER, James, Department of Biology, University of Utah, 247 South 1400 East, Salt Lake City, UT 84112, sah376@psu.edu

The Sevier Desert of central Utah is one of several known regional dust sources providing sediment for storms that affect Salt Lake City and adjacent Wasatch Mountains, northern Utah. Dust is a health concern in the Wasatch Front Megapolitan Region, and dust deposition in the Wasatch Mountains affects the albedo of the snowpack while simultaneously introducing anthropogenically derived trace elements into the closed Great Salt Lake drainage basin. The vesicular A (Av) horizon of soils developed on shoreline features of the latest Pleistocene Lake Bonneville provide an integrated record of dust deposition in central Utah since shoreline abandonment, 18–10 ka. Additionally, these Av soils characterize a regional signal for dust originating in the Sevier Desert, which may be compared to Holocene and Anthropocene dust deposition in northern Utah.

Quantitative Evaluation of Minerals by SCANning electron microscopy (QEMSCAN) analysis and optical microscopy were used to study the mineralogy of Av horizons, and their chemistry was determined by ICP-MS analysis of major, minor, and trace elements in 24 hour nitric acid leachates. These data identified depositional contributions from the host lithology, as well as near- and far-field eolian sources. Consequently, many minerals and elements show strong concentration gradients at the <10 km scale. No strong evidence was found that the Sevier (Dry) Lake bed is a disproportionately important dust source within the Sevier Desert. Vertical and horizontal sampling profiles within Av horizons did not demonstrate a high potential for recovering temporally resolved variations in dust composition. Lead was an exception; samples from the upper 2 cm contain approximately twice the concentration of lower samples. Some elemental concentrations, including Li, Mn, Ce, and Nd, were found to be less variable and might provide a proxy for dust sourced in Sevier Desert.

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