GSA Annual Meeting in Seattle, Washington, USA - 2017

Paper No. 192-11
Presentation Time: 11:25 AM


LOWERY, Christopher, Institute for Geophysics, Jackson School of Geosciences, University of Texas at Austin, JJ Pickle Research Campus, Bldg 196, 10100 Burnet Rd, Austin, TX 78758; Austin, TX 78758, JONES, Heather L., Department of Geosciences, Pennsylvania State University, State College, PA 16802, BRALOWER, Timothy J., Department of Geosciences, Pennsylvania State University, University Park, PA 16801, SMIT, Jan, Faculty of Earth and Life Sciences, Vrije Universiteit Amsterdam, De Boelelaan 1085, Amsterdam, 1081 HV, Netherlands, RODRIGUEZ-TOVAR, Francisco J., Departamento de Estratigrafía y Paleontología, Universidad de Granada, Av. Fuente Nueva, Granada, 18002, Spain, WHALEN, Michael T., Department of Geosciences, University of Alaska Fairbanks, Fairbanks, AK 99775, OWENS, Jeremy D., Department of Earth, Ocean & Atmospheric Science, Florida State University, 1017 Academic Way, Tallahassee, FL 32306 and EXPEDITION 364 SCIENTISTS, IODP-ICDP, IODP-ICDP, Breman, Germany,

The asteroid impact that formed the Chicxulub Crater caused the extinction of ~75% of genera on Earth and marks the end of the Mesozoic Era. Although the global pattern of recovery following this mass extinction has been well-described, core samples within the crater collected by IODP Exp. 364 provide the first opportunity to study primary succession in a large impact crater, and provide a test of several hypotheses about the extinction, specifically, whether metal toxicity was a significant kill mechanism and that these environmental effects were stronger closer to the crater. Here, we document the recovery of planktic and benthic foraminifera, calcareous nannoplankton, calcispheres, and trace fossil forming organisms.

The top of the impact sequence at Site M0077 is characterized by a transition from suevite breccia to an 80 cm brown fine-grained micrite, which is overlain by white Danian limestone. This 80 cm transitional unit contains reworked Cretaceous foraminifera and nannoplankton. Maastrichtian foraminifera are most diverse and abundant at the base of the unit and decline upsection. Toward the top of the unit, foraminifer species known to survive the boundary come to dominate a depauperate assemblage. The nannofossil assemblage is dominated by Cretaceous taxa of highly variable size and preservation, with rare survivor species. The upper 20 cm of the transitional unit is also characterized by the first appearance of trace fossils. The lowest sample in the limestone contains a foraminifer assemblage indicative of the base of Zone Pα, approximately 30 kyr after the impact. This level also contains a diverse assemblage of benthic foraminifera, indicating normal seafloor conditions, both in terms of organic matter flux and temperature, which suggests the impact-generated hydrothermal system was not strong enough to prevent the colonization of the seafloor by benthic life. Geochemical proxies also indicate a quick recovery of marine productivity at the base of the limestone unit. With the exception of a small increase near the top of the transitional unit, potentially toxic metals (Cu, Cr, Fe, Zn) are not elevated throughout the study interval. The rapid recovery (within 30 kyr) of life within the crater indicates that proximity to the impact was not a significant factor in the geographic pattern of recovery.