GSA Annual Meeting in Seattle, Washington, USA - 2017

Paper No. 129-10
Presentation Time: 4:25 PM

CONSTRAINING ORBITAL SOLUTIONS USING THE CRETAEOUS GEOLOGICAL RECORD


MA, Chao, Department of Geology and Geophysics, University of Utah, Salt Lake City, UT 84112, MEYERS, Stephen R., Department of Geoscience, University of Wisconsin, 1215 West Dayton St, Madison, WI 53076 and SAGEMAN, Bradley B., Earth and Planetary Sciences, Northwestern University, 2145 Sheridan Rd, Evanston, IL 60208, super11040@gmail.com

Cyclostratigraphy is widely used for constructing high-resolution geological time scales. Due to the chaotic behavior of the Solar System, however, the theoretical astronomical solution for the geologic past is only valid to ~50 Ma. In order to better constrain the theoretical orbital solutions for the past and test for chaotic transitions in Solar System behavior older than 50Ma, this study compiles two previously studied orbitally-forced geological records spanning 82-97 Ma from the Western Interior Seaway (USA). The new composite cyclostratigraphy: (1) provides an astronomically-calibrated high-resolution carbon isotope record from 82-97 Ma, (2) quantifies the influence of the Earth-Mars secular resonance, which is a sensitive indicator of Solar System chaos, and (3) indicates a chaotic transition of the Earth-Mars secular resonance from the 2.4 Myr cycle to the 1.2 Myr cycle, and back again, within the 82-97 Ma study interval.