GSA Annual Meeting in Phoenix, Arizona, USA - 2019

Paper No. 293-10
Presentation Time: 4:10 PM

ESTIMATING THE DURATION AND TEMPO OF THE CAMBRIAN EXPLOSION (Invited Presentation)


WANG, Steve C.1, PORTER, Susannah M.2, MALOOF, Adam C.3, MOORE, John L.4, ZHANG, Eric H.1, CHOI, Kevin T.5, ZAVEZ, Melissa J.6, SHORAKA, Madison H.1 and SEN, Harsha7, (1)Mathematics and Statistics, Swarthmore College, 500 College Ave, Swarthmore, PA 19081, (2)Department of Earth Science, University of California Santa Barbara, Santa Barbara, CA 93106, (3)Geosciences, Princeton University, Princeton, NJ 08544, (4)Earth Science, University of California, Santa Barbara, Santa Barbara, CA 93106, (5)Economics, Swarthmore College, 500 College Ave, Swarthmore, PA 19081; Mathematics and Statistics, Swarthmore College, 500 College Ave, Swarthmore, PA 19081, (6)Computer Science, Swarthmore College, 500 College Ave, Swarthmore, PA 19081, (7)Biology, Swarthmore College, 500 College Ave, Swarthmore, PA 19081

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.