EGU23-15489
https://doi.org/10.5194/egusphere-egu23-15489
EGU General Assembly 2023
© Author(s) 2023. This work is distributed under
the Creative Commons Attribution 4.0 License.

Insights into the terminal Ediacaran marine carbonate record from shale-hosted carbonate carbon isotopes

Mariana Yilales1, Fred Bowyer1, Rachel Wood1, and Simon Poulton2
Mariana Yilales et al.
  • 1School of Geosciences, University of Edinburgh, United Kingdom of Great Britain – Scotland
  • 2School of Earth and Environment, University of Leeds, United Kingdom of Great Britain – England

The marine carbon isotope record (δ13C) used for chemostratigraphy and reconstruction of carbon cycle dynamics is constructed using carbonate rocks, but there is evidence that carbonate cements hosted within fine-grained clastics (shales and mudstones) in some settings may also express δ13C trends that covary with the record from carbonates. We present new carbon and oxygen isotopic data from shale-hosted carbonate cements (δ13Ccarb-sh and δ18Ocarb-sh, n = 107, <16 wt% CaCO3) of the terminal Ediacaran Nama Group, Namibia (≥550.5 to <539.6 Million years ago; Ma). These data are compared with the published carbon and oxygen isotopic record from coeval carbonates (δ13Ccarb and δ18Ocarb, n = 1611) and total organic carbon (TOC) concentrations. We show that δ13Ccarb-sh compositions in samples of intermediate to high CaCO3/TOC can approximate contemporaneous δ13Ccarb in open marine mixed carbonate-clastic settings. By contrast, δ13Ccarb-sh values in samples with low CaCO3/TOC that were deposited in clastic settings distant from the locus of carbonate deposition are more negative than contemporaneous δ13Ccarb. These data suggest that δ13Ccarb-sh may approach seawater composition in samples of low TOC when deposited in high dissolved inorganic carbon (DIC) settings, where carbonate can rapidly precipitate from seawater during early diagenesis. However, the use of δ13Ccarb-sh to infill gaps in the existing δ13Ccarb record remains uncertain, even when these criteria are fulfilled. Intervals of δ13C-δ18O co-variability in the Nama Group succession appear to correlate with units where seawater mixing with meteoric fluids was more likely during early diagenesis, such as clastic-dominated settings, which also show significant decreasing δ18O through time with gradual sub-basin infill.We further consider uncertainties in lithostratigraphic correlation of the upper Urusis Formation of the Nama Group that enable three new possible correlations to be proposed for δ13Ccarb-sh data within the terminal Ediacaran to lower Cambrian (<542.65 Ma to >535 Ma) regional and global δ13Ccarb records.

How to cite: Yilales, M., Bowyer, F., Wood, R., and Poulton, S.: Insights into the terminal Ediacaran marine carbonate record from shale-hosted carbonate carbon isotopes, EGU General Assembly 2023, Vienna, Austria, 24–28 Apr 2023, EGU23-15489, https://doi.org/10.5194/egusphere-egu23-15489, 2023.