175 D29. Recent Advances in Quaternary Geology and Geomorphology
Tuesday, 11 October 2022
1:30 PM - 5:30 PM
506
WEATHERING-RELATED CLAST SIZE AND SHAPE EVOLUTION IN ARID AND SEMI-ARID SITES IN CALIFORNIA THROUGHOUT THE QUATERNARY
Paper number: 175-12
Program: Technical Sessions
Time: 4:15 PM – 4:30 PM
Authors
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Martha Cary EppesUniversity of North Carolina at Charlotte, Charlotte, NC
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Russell KeaniniUniversity of North Carolina at Charlotte, Charlotte, NC
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Amit MushkinGeological Survey of Israel, Jerusalem
Abstract
Here, we used modified Wolman pebble count data to provide chronosequences of clast size and shape evolution over the past 117 kyr in arid and semi-arid California (Mojave Desert and Owens Valley). Combining surface clast-size data with thousands of manually measured crack lengths and morphologies from 1663 boulders we determined that: 1) cracking rates decrease significantly over the first ~6 kyr of rock exposure from 0.4 – 1.8 cm growth every thousand years (cm/kyr) to ≤ 0.1 cm/kyr after ~20 kyr of exposure; 2) crack morphologies broadly predict the shape of sediments produced, with surface-parallel cracking peaking just before elongated clasts are produced; and 3) different rock types experience different cracking rates and produce different clast sizes and shapes. For example, granitoid rocks typically weather to grus while fine-grained volcanics weather to larger, more elongated shards. Predictably, overall mean clast sizes generally decrease over time, and by 30 kyr exposure the median clast size of all lithologies at both sites stabilizes to between 1.6 – 3.0 cm long axis length.
These data can help inform the size evolution of surficial clasts over geologic time and provide further constraint on understanding fresh rock surface area exposure, which may inform our understanding of chemical processes and nutrient availability. We hope these data can also be incorporated into sedimentological and paleoclimate interpretations of abandoned deposited and buried sediments by informing how the clast sizes may have been modified post-abandonment.
Geological Society of America Abstracts with Programs. Vol. 54, No. 6
doi: 10.1130/abs/2022AM-379436
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