TY - JOUR
T1 - Microbial life in the nascent Chicxulub crater
AU - Schaefer, Bettina
AU - Grice, Kliti
AU - Coolen, Marco J.L.
AU - Summons, Roger E.
AU - Cui, Xingqian
AU - Bauersachs, Thorsten
AU - Schwark, Lorenz
AU - Böttcher, Michael E.
AU - Bralower, Timothy J.
AU - Lyons, Shelby L.
AU - Freeman, Katherine H.
AU - Cockell, Charles S.
AU - Gulick, Sean P.S.
AU - Morgan, Joanna V.
AU - Whalen, Michael T.
AU - Lowery, Christopher M.
AU - Vajda, Vivi
N1 - Funding Information:
legacy IODP funding (364 postcruise funding, 2016– 2018) of “The Chicxulub post-impact crater record: Duration of a giant hydrothermal system and window into the resurgence and evolution of marine and terrestrial life” project. Schwark and Bauersachs received support via Deutsche Forschungsgemeinschaft grant Schw554/26. Freeman and Bralower, Gulick and Lowery, and Whalen were supported by U.S. National Science Foundation grants OCE 1736951, 1737351, and 1737199, respectively. Joanna Morgan was supported by UK NERC grant: NE/P005217/1. Thanks go to Julio Sepúlveda for helpful comments on an earlier version of this manuscript. We thank the anonymous reviewers for their constructive comments, which helped to improve this manuscript. This is University of Texas Institute for Geophysics Contribution #3529.
Funding Information:
The research used samples and data provided by the International Ocean Discovery Program (IODP). Expedition 364 was implemented by the European Consortium for Ocean Research Drilling (ECORD) and jointly funded by the IODP and the International Continental Scientific Drilling Program (ICDP), with contributions and logistical support from the Yucatan State Government and Universidad Nacional Aut?noma de M?xico (UNAM). We thank Peter Hopper and Alex Holman for their technical support with GC-MS analyses, and Iris Schmiedinger for isotope mass spectrometric analysis. Grice, Coolen, and Summons thank the Australian Research Council (ARC) for an ARC Discovery grant (DP180100982) titled "The recovery of life recorded at the end-Cretaceous impact crater. " Schaefer thanks Curtin University for an Australian postgraduate award. Coolen and Grice thank IODP and Australian and New Zealand legacy IODP funding (364 postcruise funding, 2016-2018) of "The Chicxulub post-impact crater record: Duration of a giant hydrothermal system and window into the resurgence and evolution of marine and terrestrial life" project. Schwark and Bauersachs received support via Deutsche Forschungsgemeinschaft grant Schw554/26. Freeman and Bralower, Gulick and Lowery, and Whalen were supported by U.S. National Science Foundation grants OCE 1736951, 1737351, and 1737199, respectively. Joanna Morgan was supported by UK NERC grant: NE/P005217/1. Thanks go to Julio Sep?lveda for helpful comments on an earlier version of this manuscript. We thank the anonymous reviewers for their constructive comments, which helped to improve this manuscript. This is University of Texas Institute for Geophysics Contribution #3529.
Funding Information:
The research used samples and data provided by the International Ocean Discovery Program (IODP). Expedition 364 was implemented by the European Consortium for Ocean Research Drilling (ECORD) and jointly funded by the IODP and the International Continental Scientific Drilling Program (ICDP), with contributions and logistical support from the Yucatan State Government and Universidad Nacio-nal Autónoma de México (UNAM). We thank Peter Hopper and Alex Holman for their technical support with GC-MS analyses, and Iris Schmiedinger for isotope mass spectrometric analysis. Grice, Coolen, and Summons thank the Australian Research Council (ARC) for an ARC Discovery grant (DP180100982) titled “The recovery of life recorded at the end-Cretaceous impact crater.” Schaefer thanks Curtin University for an Australian postgraduate award. Coolen and Grice thank IODP and Australian and New Zealand
Publisher Copyright:
© 2020.
PY - 2020
Y1 - 2020
N2 - The Chicxulub crater was formed by an asteroid impact at ca. 66 Ma. The impact is considered to have contributed to the end-Cretaceous mass extinction and reduced productivity in the world's oceans due to a transient cessation of photosynthesis. Here, biomarker profiles extracted from crater core material reveal exceptional insights into the post-impact upheaval and rapid recovery of microbial life. In the immediate hours to days after the impact, ocean resurge flooded the crater and a subsequent tsunami delivered debris from the surrounding carbonate ramp. Deposited material, including biomarkers diagnostic for land plants, cyanobacteria, and photosynthetic sulfur bacteria, appears to have been mobilized by wave energy from coastal microbial mats. As that energy subsided, days to months later, blooms of unicellular cyanobacteria were fueled by terrigenous nutrients. Approximately 200 k.y. later, the nutrient supply waned and the basin returned to oligotrophic conditions, as evident from N2-fixing cyanobacteria biomarkers. At 1 m.y. after impact, the abundance of photosynthetic sulfur bacteria supported the development of water-column photic zone euxinia within the crater.
AB - The Chicxulub crater was formed by an asteroid impact at ca. 66 Ma. The impact is considered to have contributed to the end-Cretaceous mass extinction and reduced productivity in the world's oceans due to a transient cessation of photosynthesis. Here, biomarker profiles extracted from crater core material reveal exceptional insights into the post-impact upheaval and rapid recovery of microbial life. In the immediate hours to days after the impact, ocean resurge flooded the crater and a subsequent tsunami delivered debris from the surrounding carbonate ramp. Deposited material, including biomarkers diagnostic for land plants, cyanobacteria, and photosynthetic sulfur bacteria, appears to have been mobilized by wave energy from coastal microbial mats. As that energy subsided, days to months later, blooms of unicellular cyanobacteria were fueled by terrigenous nutrients. Approximately 200 k.y. later, the nutrient supply waned and the basin returned to oligotrophic conditions, as evident from N2-fixing cyanobacteria biomarkers. At 1 m.y. after impact, the abundance of photosynthetic sulfur bacteria supported the development of water-column photic zone euxinia within the crater.
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U2 - 10.1130/G46799.1
DO - 10.1130/G46799.1
M3 - Article
AN - SCOPUS:85084111533
SN - 0091-7613
VL - 48
SP - 328
EP - 332
JO - Geology
JF - Geology
IS - 4
ER -