T169 Chemostratigraphy: Physical and Temporal Applications
Tuesday, 24 September 2019
8:00 AM - 12:00 PM
Room 224B, North Building
STRONTIUM ISOTOPES IN CARBONATE FROM THE EAGLE FORD GROUP AT THE CENOMANIAN-TURONIAN BOUNDARY IN NORTH-CENTRAL TEXAS: A POSSIBLE PROXY FOR SEAWATER COMPOSITION
Paper number: T169-12
Program: Technical Sessions
Time: 10:50 AM – 11:05 AM
Authors
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W.R. PremoU.S. Geological Survey, Denver, CO
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L.A. NeymarkU.S. Geological Survey, Denver, CO
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J.E. BirdwellU.S. Geological Survey, Denver, CO
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K.J. WhiddenU.S. Geological Survey, Denver, CO
Abstract
Samples were removed from the core by sawing. Carbonate-rich material and shells were isolated by breaking the samples into small fragments using stainless-steel tools under a binocular microscope. Samples were leached with 1M acetic acid for 1 h at room temperature, followed by a second leach with 3M acetic acid for 3 days at 120 °C. Both leachates were decanted and analyzed for strontium isotope composition by thermal ionization mass spectrometry; the final residues, dissolved in a mixture of HF and HNO3, were also analyzed for Sr isotopes.
The first leach contained more radiogenic Sr with higher 87Sr/86Sr than the second leach, and the residues were much more radiogenic than both leachates. This is consistent with the concept of the first leach removing adhered, easily dissolved carbonate that may be post-deposition; in this case, we think, the second leach is the best representation of the composition of parent seawater. The results on residues show that addition of Sr derived from silicates to carbonate leachates would lead to erroneously larger 87Sr/86Sr values. The analyses of the second leachate indicate decreasing 87Sr/86Sr across the C-T boundary, partially consistent with the seawater 87Sr/86Sr curve. Some samples from the upper Eagle Ford show larger values indicating either a shift in seawater 87Sr/86Sr or that these samples are more affected by diagenesis or silicate-derived Sr.
Geological Society of America Abstracts with Programs. Vol. 51, No. 5
doi: 10.1130/abs/2019AM-336694
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