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Rapid recovery of life at ground zero of the end-Cretaceous mass extinction

Christopher M. Lowery (), Timothy J. Bralower, Jeremy D. Owens, Francisco J. Rodríguez-Tovar, Heather Jones, Jan Smit, Michael T. Whalen, Phillipe Claeys, Kenneth Farley, Sean P. S. Gulick, Joanna V. Morgan, Sophie Green, Elise Chenot, Gail L. Christeson, Charles S. Cockell, Marco J. L. Coolen, Ludovic Ferrière, Catalina Gebhardt, Kazuhisa Goto, David A. Kring, Johanna Lofi, Rubén Ocampo-Torres, Ligia Perez-Cruz, Annemarie E. Pickersgill, Michael H. Poelchau, Auriol S. P. Rae, Cornelia Rasmussen, Mario Rebolledo-Vieyra, Ulrich Riller, Honami Sato, Sonia M. Tikoo, Naotaka Tomioka, Jaime Urrutia-Fucugauchi, Johan Vellekoop, Axel Wittmann, Long Xiao, Kosei E. Yamaguchi and William Zylberman
Additional contact information
Christopher M. Lowery: University of Texas at Austin
Timothy J. Bralower: Pennsylvania State University
Jeremy D. Owens: Florida State University
Francisco J. Rodríguez-Tovar: Universidad de Granada
Heather Jones: Pennsylvania State University
Jan Smit: Vrije Universiteit Amsterdam
Michael T. Whalen: University of Alaska Fairbanks
Phillipe Claeys: Vrije Universiteit Brussel
Kenneth Farley: MS 170-25, California Institute of Technology
Sean P. S. Gulick: University of Texas at Austin
Joanna V. Morgan: Imperial College London
Sophie Green: British Geological Survey
Elise Chenot: Université de Bourgogne-Franche Comté
Gail L. Christeson: University of Texas at Austin
Charles S. Cockell: University of Edinburgh
Marco J. L. Coolen: Curtin University
Ludovic Ferrière: Natural History Museum
Catalina Gebhardt: Helmholtz Centre of Polar and Marine Research
Kazuhisa Goto: Tohoku University
David A. Kring: Lunar and Planetary Institute
Johanna Lofi: CNRS, Université de Montpellier
Rubén Ocampo-Torres: L’Institut de Chimie et Procédés pour l’Énergie, l’Environnement et la Santé (ICPEES), Université de Strasbourg
Ligia Perez-Cruz: Universidad Nacional Autónoma De México
Annemarie E. Pickersgill: University of Glasgow
Michael H. Poelchau: University of Freiburg
Auriol S. P. Rae: Imperial College London
Cornelia Rasmussen: University of Texas at Austin
Mario Rebolledo-Vieyra: Independent consultant
Ulrich Riller: Universität Hamburg
Honami Sato: Chiba Institute of Technology
Sonia M. Tikoo: Rutgers University
Naotaka Tomioka: Japan Agency for Marine-Earth Science and Technology
Jaime Urrutia-Fucugauchi: Universidad Nacional Autónoma De México
Johan Vellekoop: Vrije Universiteit Brussel
Axel Wittmann: Arizona State University
Long Xiao: China University of Geosciences
Kosei E. Yamaguchi: Toho University
William Zylberman: Aix Marseille University

Nature, 2018, vol. 558, issue 7709, 288-291

Abstract: Abstract The Cretaceous/Palaeogene mass extinction eradicated 76% of species on Earth1,2. It was caused by the impact of an asteroid3,4 on the Yucatán carbonate platform in the southern Gulf of Mexico 66 million years ago 5 , forming the Chicxulub impact crater6,7. After the mass extinction, the recovery of the global marine ecosystem—measured as primary productivity—was geographically heterogeneous 8 ; export production in the Gulf of Mexico and North Atlantic–western Tethys was slower than in most other regions8–11, taking 300 thousand years (kyr) to return to levels similar to those of the Late Cretaceous period. Delayed recovery of marine productivity closer to the crater implies an impact-related environmental control, such as toxic metal poisoning 12 , on recovery times. If no such geographic pattern exists, the best explanation for the observed heterogeneity is a combination of ecological factors—trophic interactions 13 , species incumbency and competitive exclusion by opportunists 14 —and ‘chance’8,15,16. The question of whether the post-impact recovery of marine productivity was delayed closer to the crater has a bearing on the predictability of future patterns of recovery in anthropogenically perturbed ecosystems. If there is a relationship between the distance from the impact and the recovery of marine productivity, we would expect recovery rates to be slowest in the crater itself. Here we present a record of foraminifera, calcareous nannoplankton, trace fossils and elemental abundance data from within the Chicxulub crater, dated to approximately the first 200 kyr of the Palaeocene. We show that life reappeared in the basin just years after the impact and a high-productivity ecosystem was established within 30 kyr, which indicates that proximity to the impact did not delay recovery and that there was therefore no impact-related environmental control on recovery. Ecological processes probably controlled the recovery of productivity after the Cretaceous/Palaeogene mass extinction and are therefore likely to be important for the response of the ocean ecosystem to other rapid extinction events.

Date: 2018
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DOI: 10.1038/s41586-018-0163-6

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