T293 Hello (Ancient) World!: Exploring the Neoproterozoic to Cambrian Interval by Quantitatively Probing the Rock Record

Wednesday, 25 September 2019
1:30 PM - 5:30 PM
Room 226ABC, North Building

ESTIMATING THE DURATION AND TEMPO OF THE CAMBRIAN EXPLOSION

Paper number: T293-12
Program: Technical Sessions
Time: 4:10 PM – 4:30 PM

Authors

Abstract

Despite recent advances in the understanding of the Cambrian explosion, many details of the event remain unclear, including the rate of diversification, the order of appearances of major clades, and the number and timing of pulses of origination. Here we present a statistically rigorous timeline for the appearances of skeletal animals during the first ~20 million years of the Cambrian Period (Terreneuvian Epoch). Our results build on earlier work by Maloof et al. (2010) that used radiometrically calibrated carbon isotope chemostratigraphy to reconstruct the pattern of appearances through this interval at two-million-year resolution. That work suggested that the diversification of skeletal animals began early and extended throughout this interval, with pulses of appearances near 540–538 Ma, 534–530 Ma, and 524–522 Ma. However, it is not clear to what extent these patterns are influenced by preservational biases, the Signor-Lipps effect, and uncertainties in correlation and dating.

We investigate the robustness of these findings after accounting for several sources of uncertainty in dating the origination times of fossil taxa. To do this, we use a Monte Carlo simulation that incorporates multiple potential correlations between sections, margins of error in radiometric dating, non-uniform sedimentation rates, and confidence intervals that account for the incompleteness of the fossil record. We also use novel statistical methods to estimate the duration of the diversification, and to identify the most likely number of pulses of origination and their timing.

Geological Society of America Abstracts with Programs. Vol. 51, No. 5

doi: 10.1130/abs/2019AM-340187

© Copyright 2019 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.