DIAGENETIC δ34SCAS VARIABILITY IN METEORICALLY ALTERED DOLOSTONES: A CASE STUDY FROM THE UPPER ORDOVICIAN OF THE GREAT BASIN
Using the Anticosti data as a “least-altered” Hirnantian δ34SCAS benchmark, we test the fidelity of the δ34SCAS signal in strata that have undergone significant post-depositional alteration. We have recently used δ13C chemostratigraphy and sequence stratigraphy to identify Hirnantian strata in the Ely Springs Dolostone, a meteorically altered shallow water carbonate exposed in the Great Basin, USA. Here we present δ34SCAS data from two of these Upper Ordovician sections; the section at South Egan Range occupies a mid-shelf location, whereas the deeper section at Pancake Range represents the shelf-slope margin. Carbonate-associated sulfate concentrations are low (<120 ppm), as is typical of meteorically altered carbonates. Like the Anticosti limestones, the dolostones do not host a δ34SCAS excursion in the Hirnantian, and a ~5‰ scatter persists around the long-term secular trends. However there is a ~10‰ offset between the two sections. Isotope ratios of the shelf edge deposits are ~23‰, similar to those of well-preserved limestones, whereas the mid-shelf deposits fluctuate around ~33‰. Mid-shelf sediment at South Egan Range may have incorporated pore water sulfate enriched in 34S through microbial sulfate reduction as a result of limited mixing with the open ocean during the sea level lowstand associated with the Hirnantian glacial maximum. These results suggest that while dolostones have the potential to preserve primary δ 34SCAS signals, diagenetic overprints may vary across a sedimentary basin.