2011 GSA Annual Meeting in Minneapolis (912 October 2011)
Paper No. 237-1
Presentation Time: 8:00 AM-8:20 AM


MEYERS, Stephen R., Department of Geoscience, University of Wisconsin, 1215 West Dayton St, Madison, WI 53076, smeyers@geology.wisc.edu, SINGER, Brad S., Geoscience, University of Wisconsin-Madison, 1215 W. Dayton St, Madison, WI 53076, SIEWERT, Sarah E., Geoscience, University of Wisconsin-Madison, 1215 W. Dayton St, Madison, WI 53706, SAGEMAN, Bradley B., Earth and Planetary Sciences, Northwestern University, 1850 Campus Drive, Evanston, IL 60208, CONDON, Daniel, NERC Isotope Geoscience Laboratory, British Geological Survey, Keyworth, Nottingham, NG12 5GG, United Kingdom, JICHA, Brian R., Department of Geoscience, University of Wisconsin-Madison, 1215 W. Dayton St, Madison, WI 53706, SAWYER, David A., USGS, MS 980, Box 25046, Denver, CO 80225, and OBRADOVICH, John D., U.S. Geological Survey, MS 980, Box 25046, Denver, CO 80225

The Cretaceous Western Interior Basin (WIB) preserves an extraordinary record of orbitally-influenced sedimentation, and also contains volcanic ashes that provide most of the radioisotopic ages that underpin the upper Cretaceous time scale, rooted in the pioneering 40Ar/39Ar geochronology of Obradovich (1993). Following recent advances in U-Pb geochronology, 40Ar/39Ar geochronology and astrochronology, reevaluation of the WIB deposits provides an opportunity to dramatically refine the Cretaceous time scale, while also allowing a comparison – and ideally an intercalibration – of these high-resolution techniques. To accomplish this goal, we have generated U-Pb (CA ID-TIMS) and 40Ar/39Ar (laser fusion) data from zircons and sanidines in WIB bentonites spanning the Cenomanian-Campanian stages, and have evaluated them within the context of floating astrochronologies that encompass ~9 Ma of time. The radioisotopic analyses utilize newly collected material, as well as legacy sanidine samples of Obradovich (1993), from more than 20 individual volcanic ashes in the WIB. For some bentonites, we have analyzed material from several locations throughout the WIB, to assess the temporal correlation from the perspective of both sanidine and zircon. Our approach considers sources of uncertainty associated with the radioisotopic ages (analytical, tracer solution or age of neutron fluence standard, decay constants), including geologic uncertainties (e.g., magma residence, inheritance, stratigraphic correlation), and uncertainties in the astrochronology. Results highlight the strengths and weaknesses of each geochronometer, and illustrate strategies for coupling them to resolve shortcomings and ambiguities associated with the individual methods. Overall, the new data support the astronomically-calibrated age of 28.2 Ma for the Fish Canyon sanidine standard (Kuiper et al., 2008), and result in new stage boundary ages with 2σ total uncertainties (radioisotopic/geologic/astrochronologic) that range from ~2-5 per mil. This presentation will examine strategies for deploying the WIB “floating” orbital time scales to better constrain radioisotopic ages (for individual bentonites) and stage boundary ages, as well as approaches for optimally “anchoring” the astrochronologies in time.

2011 GSA Annual Meeting in Minneapolis (912 October 2011)
General Information for this Meeting
Session No. 237
EARTHTIME Geochronology: Improving Age Interpretations through Integration and Intercalibration
Minneapolis Convention Center: Room 102D-F
8:00 AM-12:00 PM, Wednesday, 12 October 2011

Geological Society of America Abstracts with Programs, Vol. 43, No. 5, p. 567

© Copyright 2011 The Geological Society of America (GSA), all rights reserved. Permission is hereby granted to the author(s) of this abstract to reproduce and distribute it freely, for noncommercial purposes. Permission is hereby granted to any individual scientist to download a single copy of this electronic file and reproduce up to 20 paper copies for noncommercial purposes advancing science and education, including classroom use, providing all reproductions include the complete content shown here, including the author information. All other forms of reproduction and/or transmittal are prohibited without written permission from GSA Copyright Permissions.