T64 No Dates: No Rates—Utilizing Geochronometers to Quantify Rates of Geomorphic Processes or Archaeological Development over a Wide Range of Temporal and Spatial Scales (Posters)
Sunday, 22 October 2017
9:00 AM - 5:30 PM
Halls 4EF
DATING DUST: USING OSL TO CONSTRAIN THE TIMING OF SEDIMENT ACCUMULATION ON HILLSLOPES IN THE MOJAVE DESERT
Paper number: T64-8
Program: Technical Sessions
Time: 9:00 AM – 5:30 PM
Authors
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Lyman P. PersicoWhitman College, Walla Walla, WA
Abstract
The timing of deposition of the eolian material can be dated by optically stimulated luminescence (OSL). Three sediment samples were collected from a 1.5-meter-thick section of exposed colluvium at depths of 20, 60, and 95 centimeters on the south-facing slope. OSL samples were collected at night because the metal tube could not penetrate the rock colluvium. We also sampled a mid Holocene terrace 3 meters above the modern channel, which also has a dust component to further test the reliability of method. Preliminary results indicate that colluviation on both north- and south-facing slopes occurred in the Pleistocene and that dust is filling and mixing in pore spaces of colluvium. The grain size of the fine-grained sediment is dominated by fine sand and silt with modes at 75, 200, and 500 microns. OSL samples were sieved to 50-150 micron and 150-250 micron sub samples, and OSL analysts performed for the different size fractions. The age of the 50-150 micron sediment is ~6-12 ka, and the age of the 150-250 micron sediment is ~15-20 ka. Young ages at depth show that both fine sand and silt are translocated into the B horizons. Ages of different modes suggest changes in dust source at different depositional times. The more xeric conditions on the south-facing slopes limit vegetation cover. During precipitation events, there is more overland flow and erosion. Stripping on south-facing slopes has increased the amount of bare bedrock, further enhancing overland flow and erosion.
Geological Society of America Abstracts with Programs. Vol. 49, No. 6
doi: 10.1130/abs/2017AM-307561
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