GP003-07
Ten Million Years of Paleoclimatic Variability Recorded in Permian Loessite of Eastern Equatorial Pangea

Monday, 14 December 2020: 07:18
Virtual
Lily S Pfeifer1, Linda A Hinnov2, Christian Zeeden3, Christian Rolf4, Christian Laag3 and Gerilyn S Soreghan5, (1)University of Oklahoma Norman Campus, Norman, OK, United States, (2)George Mason University Fairfax, Fairfax, VA, United States, (3)Leibniz Institute for Applied Geophysics, Section 5, Hannover, Germany, (4)Leibniz Institute for Applied Geophysics, Hannover, Germany, (5)Univ of Oklahoma, Norman, OK, United States
Abstract:
Analysis and modeling of a ~1000-m-thick stratigraphic series of rock magnetic data from the loessite of the Permian Salagou Formation (south-central France) reveal distinctive Milankovitch-scale paleoclimatic variability through the middle to late Cisuralian (ca. 285—275 Ma). Evidence for predominant orbital eccentricity-scale cyclicity (~10-m-thick) and subordinate obliquity and precession-scale variability (~3.5 and ~1.8 m-thick) occurs in two magnetic susceptibility (MS) series. Laboratory rock magnetic data suggest that the driver of the MS signal in the Salagou Formation is hematite and not magnetite or maghemite common in Quaternary loess. This suggests arid and/or oxidizing climate conditions at the time of loess deposition and/or post-depositional oxidation of magnetite and maghemite. We propose that the rock magnetic signal is pedogenically driven, and that the continental Salagou Formation represents approximately 10 million years of astronomically controlled wet-dry climate cycles. Application of two objective methods designed for cyclic stratigraphy with uncertain timescales indicates depositional rates ranging from 9 cm/kyr in the lower Sagalou Formation to 14 cm/kyr in the mid-upper Salagou Formation.