Abstract

The Trezona carbon isotope excursion is recorded on five different continents in platform carbonates deposited prior to the end-Cryogenian Marinoan glaciation (>635 Ma) and represents a change in carbon isotope values of 16–18‰. Based on the spatial and temporal reproducibility, the excursion previously has been interpreted as tracking the carbon isotopic composition of dissolved inorganic carbon in the global ocean before the descent into a snowball Earth. However, in modern restricted shallow marine and freshwater settings, carbon isotope values have a similarly large range, which is mostly independent from open ocean chemistry and instead reflects local processes. In this study, we combine calcium, magnesium, and strontium isotope geochemistry with a numerical model of carbonate diagenesis to disentangle the degree to which the Trezona excursion reflects changes in global seawater chemistry versus local shallow-water platform environments. Our analysis demonstrates that the most extreme carbon isotope values (∼-10‰ versus +10‰) are preserved in former platform aragonite that was neomorphosed to calcite during sediment-buffered conditions and record the primary carbon isotope composition of platform-top surface waters. In contrast, the downturn and recovery of the Trezona excursion are recorded in carbonates that were altered during early fluid-buffered diagenesis and commonly are dolomitized. We also find that the nadir of the Trezona excursion is associated with a fractional increase in siliciclastic sediments, whereas the recovery from the excursion correlates with a relative increase in carbonate. This relationship suggests that the extreme negative isotopic shift in platform aragonite occurred in concert with periods of increased input of siliciclastic sediments, changes in water depth, and possibly nutrients to platform environments. Although the process for generating extremely negative carbon isotope values in Neoproterozoic platform carbonates remains enigmatic, we speculate that these excursions reflect kinetic isotope effects associated with CO2 invasion in platform waters during periods of intense primary productivity.

Highlights

  • The Cryogenian Period (∼720–635 Ma) of the Neoproterozoic Era is characterized by major reorganizations of Earth surface processes and is bracketed by two Snowball Earth events, the older Sturtian and the younger Marinoan glaciation (Hoffman and Schrag, 2002)

  • We investigate the variability of carbonate δ44/40Ca values across the Trezona excursion, a large negative δ13C excursion recorded on multiple continents prior to the Marinoan glaciation

  • This study demonstrates that stratigraphic changes in Cryogenian platform carbonate δ13C values are characterized by intervals of fluid-versus sediment-buffered diagenesis linked to changes in the relative input of carbonate and siliciclastic sediments

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Summary

Introduction

The Cryogenian Period (∼720–635 Ma) of the Neoproterozoic Era is characterized by major reorganizations of Earth surface processes and is bracketed by two Snowball Earth events, the older Sturtian and the younger Marinoan glaciation (Hoffman and Schrag, 2002). Tionary and climatic changes remain enigmatic due to the sparsity of radiometric age constraints and the challenges of interpreting geochemical records from ancient platform carbonates. To overcome the lack of both radiometric age constraints and biostratigraphy in Neoproterozoic successions, δ13C stratigraphy has been used as a global correlation tool. Cryogenian carbonates are characterized by significant variability in the isotopic ratios of 13C/12C (δ13C), with excursions of similar shape and magnitude recorded in multiple locations (Halverson et al, 2005).

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