Abstract

Early Proterozoic marine carbonates of the Rocknest Formation (1.93-1.89 Ga) have very depleted {delta}{sup 18}O values (about 8{per thousand}) relative to younger, Late Proterozoic marine carbonates that formed in similar depositional environments. Two isotopic trends are superimposed on the data for open-marine components. The first involves stabilization of tidal-flat sediments during early, possibly reflux-type dolomitization by evaporative pore fluids enriched in {delta}{sup 18}O. The second trend toward isotopically light {delta}{sup 18}O values was established during dolomitization of open-marine facies in contact either with meteoric waters (mixing zone) or under conditions of higher temperatures during burial. This resulted in precipitation of blocky, pore-occluding cements. The isotopically most enriched ooids are the best preserved normal marine components and may suggest that the {delta}{sup 18}O of seawater was about {minus}9.75{per thousand} {plus minus}1.0{per thousand} (SMOW) at 1.9 Ga. This composition would require a major change in the balance of high-temperature oxygen isotopic exchange between seawater and basalt and low-temperature weathering in order to explain the 8{per thousand} positive shift in inferred seawater {delta}{sup 18}O between 1.9 and 1.0 Ga. Alternatively, the depleted {delta}{sup 18}O values represent an approximately 30-35 C higher temperature of surface waters at 1.9 Ga. The heaviest carbonate {delta}{sup 13}Cmore » values are +1.75{per thousand}, more enriched than previously reported for the Early Proterozoic on the basis of bulk-rock data.« less

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