TY - JOUR
T1 - Origin of a global carbonate layer deposited in the aftermath of the Cretaceous-Paleogene boundary impact
AU - Bralower, Timothy J.
AU - Cosmidis, Julie
AU - Heaney, Peter J.
AU - Kump, Lee R.
AU - Morgan, Joanna V.
AU - Harper, Dustin T.
AU - Lyons, Shelby L.
AU - Freeman, Katherine H.
AU - Grice, Kliti
AU - Wendler, Jens E.
AU - Zachos, James C.
AU - Artemieva, Natalia
AU - Chen, Si Athena
AU - Gulick, Sean P.S.
AU - House, Christopher H.
AU - Jones, Heather L.
AU - Lowery, Christopher M.
AU - Nims, Christine
AU - Schaefer, Bettina
AU - Thomas, Ellen
AU - Vajda, Vivi
N1 - Funding Information:
This research used samples and data provided by IODP Expedition 364 was jointly funded by the European Consortium for Ocean Research Drilling (ECORD) and ICDP, with contributions and logistical support from the Yucatán State Government and Universidad Nacional Autónoma de México (UNAM). Research was funded by NASA NNX12AD83G, NSF-OCE 1736951, and Post Expedition Awards from IODP to TB and KF and NSF-OCE 1737351 to CL and SG. Funding was also received from the Swedish Research Council (VR grant 2015-4264 to VV. KG and BS were supported by an Australian Research Council (ARC - DP180100982) and Australian and New Zealand legacy IODP funding (364), 2016-2018. JM received NERC funding (NE/P005217/1). We thank Holger Kuhlmann, Lallan Gupta, Chad Broyles, and Phil Rumford for help with sampling ocean cores, Julie Anderson and Wes Auker for help with the SEM, Jenn Grey for assistance with TEM, Max Wetherington for assistance with Raman, and Professor Bin Lian for sharing published photographs of cyanobacteria in Fig. 2. We acknowledge discussions with Paul Bown, Michael Henehan, Paul Pearson, Howie Spero and Jeremy Young. We thank Michael Henehan for extremely helpful feedback on an earlier version of this manuscript as well as comments by two other reviewers. We thank Aileen McNamee and Carly Gazze for technical help. Land section samples were generously supplied by Hermann Bermudez, Eduardo Kousoutkos, Julio Sepúlveda, and Laia Alegret; samples from Site 384 were lent by Hans Thierstein, and picked foraminifera from Site 1049 were supplied by Brian Huber. This is UTIG Contribution #3664 and Center for Planetary Systems Habitability #0009.
Funding Information:
Heather Jones received her integrated Master's degree in Geology from the University of Southampton (UK) where she first discovered her love for calcareous nannoplankton. She recently received her PhD in Geosciences from Penn State University, which was partly funded by a Schlanger Ocean Drilling Fellowship. Heather is heavily involved with the International Ocean Discovery Program (IODP), having sailed as a nannofossil biostratigrapher on Expedition 364 (Chicxulub impact crater), and more recently as a physical properties specialist on Expedition 378 (South Pacific Paleogene Climate). She is broadly interested in the ecological and evolutionary response of calcareous nannoplankton to extreme environmental perturbation throughout the geologic record.
Funding Information:
This research used samples and data provided by IODP Expedition 364 was jointly funded by the European Consortium for Ocean Research Drilling (ECORD) and ICDP, with contributions and logistical support from the Yucatán State Government and Universidad Nacional Autónoma de México (UNAM). Research was funded by NASA NNX12AD83G , NSF-OCE 1736951 , and Post Expedition Awards from IODP to TB and KF and NSF-OCE 1737351 to CL and SG. Funding was also received from the Swedish Research Council (VR grant 2015-4264 to VV. KG and BS were supported by an Australian Research Council (ARC - DP180100982 ) and Australian and New Zealand legacy IODP funding (364), 2016-2018 . JM received NERC funding ( NE/P005217/1 ). We thank Holger Kuhlmann, Lallan Gupta, Chad Broyles, and Phil Rumford for help with sampling ocean cores, Julie Anderson and Wes Auker for help with the SEM, Jenn Grey for assistance with TEM, Max Wetherington for assistance with Raman, and Professor Bin Lian for sharing published photographs of cyanobacteria in Fig. 2 . We acknowledge discussions with Paul Bown, Michael Henehan, Paul Pearson, Howie Spero and Jeremy Young. We thank Michael Henehan for extremely helpful feedback on an earlier version of this manuscript as well as comments by two other reviewers. We thank Aileen McNamee and Carly Gazze for technical help. Land section samples were generously supplied by Hermann Bermudez, Eduardo Kousoutkos, Julio Sepúlveda, and Laia Alegret; samples from Site 384 were lent by Hans Thierstein, and picked foraminifera from Site 1049 were supplied by Brian Huber. This is UTIG Contribution #3664 and Center for Planetary Systems Habitability #0009.
Publisher Copyright:
© 2020 Elsevier B.V.
PY - 2020/10/15
Y1 - 2020/10/15
N2 - Microcrystalline calcite (micrite) dominates the sedimentary record of the aftermath of the Cretaceous–Paleogene (K–Pg) impact at 31 sites globally, with records ranging from the deep ocean to the Chicxulub impact crater, over intervals ranging from a few centimeters to more than seventeen meters. This micrite-rich layer provides important information about the chemistry and biology of the oceans after the impact. Detailed high-resolution scanning electron microscopy demonstrates that the layer contains abundant calcite crystals in the micron size range with a variety of forms. Crystals are often constructed of delicate, oriented agglomerates of sub-micrometer mesocrystals indicative of rapid precipitation. We compare the form of crystals with natural and experimental calcite to shed light on their origin. Close to the crater, a significant part of the micrite may derive from the initial backreaction of CaO vaporized during impact. In more distal sites, simple interlocking rhombohedral crystals resemble calcite precipitated from solution. Globally, we found unique calcite crystals associated with fossilized extracellular materials that strikingly resemble calcite precipitated by various types of bacteria in natural and laboratory settings. The micrite-rich layer contains abundant bacterial and eukaryotic algal biomarkers and most likely represents global microbial blooms initiated within millennia of the K–Pg mass extinction. Cyanobacteria and non-haptophyte microalgae likely proliferated as dominant primary producers in cold immediate post-impact environments. As surface-water saturation state rose over the following millennia due to the loss of eukaryotic carbonate producers and continuing river input of alkalinity, “whitings” induced by cyanobacteria replaced calcareous nannoplankton as major carbonate producers. We postulate that the blooms grew in supersaturated surface waters as evidenced by crystals that resemble calcite precipitates from solution. The microbial biomass may have served as a food source enabling survival of a portion of the marine biota, ultimately including life on the deep seafloor. Although the dominance of cyanobacterial and algal photosynthesis would have weakened the biological pump, it still would have removed sufficient nutrients from surface waters thus conditioning the ocean for the recovery of biota at higher trophic levels.
AB - Microcrystalline calcite (micrite) dominates the sedimentary record of the aftermath of the Cretaceous–Paleogene (K–Pg) impact at 31 sites globally, with records ranging from the deep ocean to the Chicxulub impact crater, over intervals ranging from a few centimeters to more than seventeen meters. This micrite-rich layer provides important information about the chemistry and biology of the oceans after the impact. Detailed high-resolution scanning electron microscopy demonstrates that the layer contains abundant calcite crystals in the micron size range with a variety of forms. Crystals are often constructed of delicate, oriented agglomerates of sub-micrometer mesocrystals indicative of rapid precipitation. We compare the form of crystals with natural and experimental calcite to shed light on their origin. Close to the crater, a significant part of the micrite may derive from the initial backreaction of CaO vaporized during impact. In more distal sites, simple interlocking rhombohedral crystals resemble calcite precipitated from solution. Globally, we found unique calcite crystals associated with fossilized extracellular materials that strikingly resemble calcite precipitated by various types of bacteria in natural and laboratory settings. The micrite-rich layer contains abundant bacterial and eukaryotic algal biomarkers and most likely represents global microbial blooms initiated within millennia of the K–Pg mass extinction. Cyanobacteria and non-haptophyte microalgae likely proliferated as dominant primary producers in cold immediate post-impact environments. As surface-water saturation state rose over the following millennia due to the loss of eukaryotic carbonate producers and continuing river input of alkalinity, “whitings” induced by cyanobacteria replaced calcareous nannoplankton as major carbonate producers. We postulate that the blooms grew in supersaturated surface waters as evidenced by crystals that resemble calcite precipitates from solution. The microbial biomass may have served as a food source enabling survival of a portion of the marine biota, ultimately including life on the deep seafloor. Although the dominance of cyanobacterial and algal photosynthesis would have weakened the biological pump, it still would have removed sufficient nutrients from surface waters thus conditioning the ocean for the recovery of biota at higher trophic levels.
UR - http://www.scopus.com/inward/record.url?scp=85089102470&partnerID=8YFLogxK
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U2 - 10.1016/j.epsl.2020.116476
DO - 10.1016/j.epsl.2020.116476
M3 - Article
AN - SCOPUS:85089102470
SN - 0012-821X
VL - 548
JO - Earth and Planetary Science Letters
JF - Earth and Planetary Science Letters
M1 - 116476
ER -