Research Article| January 01, 2015 Chemostratigraphy of an Ordovician–Silurian carbonate platform: δ13C records below glacioeustatic exposure surfaces David S. Jones; David S. Jones Geology Department, Amherst College, 11 Barrett Hill Road, Amherst, Massachusetts 01002, USA Search for other works by this author on: GSW Google Scholar Roger C. Creel; Roger C. Creel Geology Department, Amherst College, 11 Barrett Hill Road, Amherst, Massachusetts 01002, USA Search for other works by this author on: GSW Google Scholar Bernardo Rios; Bernardo Rios Geology Department, Amherst College, 11 Barrett Hill Road, Amherst, Massachusetts 01002, USA Search for other works by this author on: GSW Google Scholar Danielle P. Santiago Ramos Danielle P. Santiago Ramos Geology Department, Amherst College, 11 Barrett Hill Road, Amherst, Massachusetts 01002, USA *Current address: Department of Geosciences, Princeton University, Guyot Hall, Princeton, New Jersey 08544, USA. Search for other works by this author on: GSW Google Scholar Geology (2015) 43 (1): 59–62. https://doi.org/10.1130/G36236.1 Article history received: 02 Sep 2014 rev-recd: 30 Oct 2014 accepted: 05 Nov 2014 first online: 09 Mar 2017 Cite View This Citation Add to Citation Manager Share Icon Share Facebook Twitter LinkedIn MailTo Tools Icon Tools Get Permissions Search Site Citation David S. Jones, Roger C. Creel, Bernardo Rios, Danielle P. Santiago Ramos; Chemostratigraphy of an Ordovician–Silurian carbonate platform: δ13C records below glacioeustatic exposure surfaces. Geology 2015;; 43 (1): 59–62. doi: https://doi.org/10.1130/G36236.1 Download citation file: Ris (Zotero) Refmanager EasyBib Bookends Mendeley Papers EndNote RefWorks BibTex toolbar search Search Dropdown Menu toolbar search search input Search input auto suggest filter your search All ContentBy SocietyGeology Search Advanced Search Abstract The use of carbon isotope stratigraphy to construct time lines for stratigraphic correlation requires synchronous changes in carbon isotope ratios (δ13C) to be preserved in carbonate-dominated strata. Such changes are commonly interpreted to reflect primary secular variation in ocean chemistry. However, negative δ13C anomalies developed in Pliocene–Pleistocene carbonate platforms following glacioeustatic sea-level fall due to remineralization of terrestrial biomass during meteoric diagenesis. These anomalies are similar in structure and magnitude to some Neoproterozoic δ13C records, opening the possibility that the Neoproterozoic δ13C anomalies have a meteoric origin derived from a large terrestrial biosphere. Here we test the hypothesis that a large terrestrial biosphere existed prior to the Silurian–Devonian land-plant radiation by examining δ13C records of subaerial exposure surfaces formed in a shallow-water carbonate platform during the Ordovician–Silurian icehouse. The exposure surfaces include an unconformity at the Ordovician-Silurian boundary with terra rossa and dissolution-collapse breccia, and a lower Silurian quartz sand layer feeding a 50-m-deep system of karst pipes. There is no evidence for δ13C depletion beneath either exposure surface. Strontium concentrations in the rocks are low (10–120 ppm) and covary with δ18O; oxygen isotope ratios, however, do not positively correlate with δ13C. Our results suggest that there was no significant terrestrial biosphere during Ordovician–Silurian time, and by extension, that Neoproterozoic negative carbon isotope anomalies cannot be explained by meteoric diagenesis. You do not have access to this content, please speak to your institutional administrator if you feel you should have access.
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