T177 Correlation of Global Stages, Series, and Systems into North American Stratigraphic Successions

Tuesday, 12 October 2021
1:30 PM - 5:30 PM
A106


COMBINED CA-ID-TIMS AND CARBON ISOTOPE CHEMOSTRATIGRAPHY TO CORRELATE CRETACEOUS CONTINENTAL STRATA OF THE RUBY RANCH MEMBER OF THE CEDAR MOUNTAIN FORMATION

Paper number: T177-12
Program: Technical Sessions
Time: 4:05 PM – 4:20 PM


Authors


Abstract

Determining the age of continental strata is vital to understanding the timing of climate changes and the development of ecosystems during the Cretaceous Terrestrial Revolution. The combination of geochronologic data with widespread carbon isotope chemostratigraphy provides time constraints for a lower Cretaceous continental unit, the Cedar Mountain Formation. Specifically, a unique palustrine-lacustrine sequence of the Ruby Ranch Member reveals a bulk organic carbon isotope record that ranges between -32.3‰ and -21.1‰ and averages -26.3‰ vs. VPDB. A positive C-isotope excursion occurs that is interpreted to represent the C10 carbon isotope excursion (Bralower et al. 1999; Ap12-15 and Al1 segments of Herrle et al. 2004) that has been identified in other locations worldwide (Herrle et al. 2004). An ash layer within the positive isotope excursion provides an estimated eruption age from CA-ID-TIMS of ca. 116 Ma. This is slightly older than the interpolated age of the base of the Hypacanthopilites jacobi Ammonite zone, thus providing a chemostratigraphic and geochronologic correlation to other biostratigraphically constrained Aptian-Albian units. This also firmly places the time of deposition for the Ruby Ranch Member of the Cedar Mountain Formation within the Aptian to Albian.

Geological Society of America Abstracts with Programs. Vol. 53, No. 6

doi: 10.1130/abs/2021AM-370386

© Copyright 2021 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.