T3 Advances in Nontraditional Stable Isotope Measurements and Utility as Proxies in Modern and Paleo-Settings
Sunday, 22 September 2024
8:00 AM - 12:00 PM
207A
CARBONATE CLUMPED ISOTOPES OF ARAGONITIC FOSSILS FROM THE LATE CRETACEOUS WESTERN INTERIOR SEAWAY AND THE ROLE OF BOND REORDERING IN SIGNAL PRESERVATION
Paper number: T3-4
Program: Technical Sessions
Time: 8:35 AM – 8:55 AM
Authors
-
J. Kirk CochranStony Brook University, Stony Brook, NY
-
Neil LandmanAmerican Museum of Natural History, New York, NY
-
Gregory HenkesStony Brook University, Stony Brook, NY
Abstract
In North America, well-preserved ammonite fossils are commonly found in Upper Cretaceous sediments from the Western Interior Seaway (WIS). New measurements of δ13C, δ18O, and Δ47 from 12 exceptionally well-preserved ammonite fossils from WIS sediments in South Dakota yield unrealistically warm clumped isotope paleotemperatures (T(Δ47)), some as high as 45 °C. In contrast, published fossil T(Δ47) from contemporaneous WIS sediments infer water temperatures of 20-25 °C. Most of the shells we have analyzed are petrographically pristine and 100% aragonite, ruling out cryptic diagenesis, excluding the conversion of some aragonite to calcite, but leaving open the possibility of clumped isotope bond reordering.
To derive the kinetics of aragonite clumped isotope bond reordering, we show the results of aragonite heated to 250-350 °C for different time intervals. Our results show that at lower temperatures, aragonite bond reordering can lead to clumped isotope alteration without aragonite converting to calcite, implying kinetics of aragonite bond reordering are faster than aragonite-to-calcite conversion. These new experimental results demonstrate that aragonite more rapidly breaks 13C-18O bonds than does calcite, putting its geologic thermal stability below the canonical ~100°C threshold for millions of years of burial heating. Ultimately this may affect the reliability of implementing clumped isotopes on aragonitic fossils for paleotemperature reconstruction.
Geological Society of America Abstracts with Programs. Vol. 56, No. 5
doi: 10.1130/abs/2024AM-403286
© Copyright 2024 The Geological Society of America (GSA), all rights reserved. Permission is hereby granted to the author(s) of this abstract to reproduce and distribute it freely, for noncommercial purposes. Permission is hereby granted to any individual scientist to download a single copy of this electronic file and reproduce up to 20 paper copies for noncommercial purposes advancing science and education, including classroom use, providing all reproductions include the complete content shown here, including the author information. All other forms of reproduction and/or transmittal are prohibited without written permission from GSA Copyright Permissions.