CALL FOR PROPOSALS:

ORGANIZERS

  • Harvey Thorleifson, Chair
    Minnesota Geological Survey
  • Carrie Jennings, Vice Chair
    Minnesota Geological Survey
  • David Bush, Technical Program Chair
    University of West Georgia
  • Jim Miller, Field Trip Chair
    University of Minnesota Duluth
  • Curtis M. Hudak, Sponsorship Chair
    Foth Infrastructure & Environment, LLC

 

Paper No. 9
Presentation Time: 11:00 AM

EARLY CRETACEOUS BASELINE ATMOSPHERIC pCO2 AND BUILDUP ESTIMATED FROM A CALCRETE SUCCESSION, CEDAR MOUNTAIN FORMATION, UTAH, USA


MURPHY, Laura R., Department of Anthropology, University of Kansas, 1415 Jayhawk Blvd, Lawrence, KS 66045, LUDVIGSON, Greg, Kansas Geological Survey, The University of Kansas, 1930 Constant Ave, Lawrence, KS 66047-3726, JOECKEL, R.M., CSD, School of Natural Resources, Department of Earth and Atmospheric Sciences, and U.N. State Museum, University of Nebraska-Lincoln, Lincoln, NE 68583-0996 and GONZALEZ, Luis A., Department of Geology, University of Kansas, 1475 Jayhawk Blvd., Rm. 120, Lindley Hall, Lawrence, KS 66045, murphy15@ku.edu

We calculate a baseline Aptian-Albian atmospheric pCO2 of 1,000 ppm by applying the equation of Ekart et al. (1999, AJS 299:805-827) to isotopic analyses of pedogenic and palustrine carbonates from eight correlated chemostratigraphic positions. The positions are from the Ap7 C-isotope feature of Herrle et al. (2004, EPSL 218:149-161) to the C15 C-isotope feature of Bralower et al. (1999, JFR 29:418-437) at two sections in the Cedar Mountain Formation (Ruby Ranch Road and Muddy Creek, eastern Utah). These sections encompass the Aptian-Albian Ap7-C15 (~125-100 Ma) interval (Ludvigson et al., 2010, JSR 80:955-974). Significantly, our results indicate a buildup in atmospheric pCO2 of ~350 ppm above baseline values during the C9-C11 positive carbon isotope excursion. Furthermore, this excursion corresponds with our reported shifts in δ13C values determined from coordinated carbonate and sedimentary organic carbon. We realize that S(z), the soil-derived component of total soil CO2 at depth z, significantly varies with season, depth, soil type, and paleolatitude. Thus, unlike other studies that use a constant S(z), we report a range of pCO2 values using several S(z) estimates. Direct comparison of our pCO2 measurements to compiled estimates from the same interval determined on pedogenic carbonates, stomata, and liverworts recently published (Royer, 2010, PNAS 107:517-518) emphasizes the need for a non-uniform S(z) approach. Finally, we correlate our pCO2 with high-resolution marine chemostratigraphic records (δ13C(carb), δ13C(org), 87Sr/86Sr), and magma flux output from the Kergulean Plateau (Indian Ocean). The 116 to 111 Ma rise and fall in pCO2 during the C9-C11 carbon isotope excursion, for which we have identified a pCO2 buildup, coincides with the well-documented mid-Cretaceous strontium isotope low, and with a peak in magma production at the Kerguelan Large Igneous Province. Therefore, we interpret a tectonic driver for this global change event.
Meeting Home page GSA Home Page