Return to the Strangelove Ocean? Preliminary results of carbon and oxygen isotope compositions of post-impact sediments, IODP Expedition 364 "Chicxulub Impact Crater"

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http://abstractsearch.agu.org/meetings/2017/FM/PP23B-1302.html
Author(s): Yamaguchi, K. E.; Ikehara, M.; Hayama, Hiromasa; Takiguchi, Shogo; Masuda, S.; Ogura, Chihiro; Fujita, S.; Kurihara, Erina; Matsumoto, T.; Oshio, Shu; Ishihata, Kenta; Fuchizawa, Yuya; Noda, H.; Sakurai, Urara; Yamane, T.; Morgan, J. V.; Gulick, S. P. S.
Author Affiliation(s): Primary:
Toho University, Department of Chemistry, Chiba, Japan
Other:
Kochi University, Nankoku, Japan
Imperial College London, London, United Kingdom
University of Texas at Austin, Department of Geological Sciences, Austin, TX, United States
Volume Title: AGU 2017 fall meeting
Source: American Geophysical Union Fall Meeting, Vol.2017; American Geophysical Union 2017 fall meeting, New Orleans, LA, Dec. 11-15, 2017. Publisher: American Geophysical Union, Washington, DC, United States
Note: In English
Summary: The Chicxulub crater in the northern Yucatan Peninsula, Mexico was formed by the asteroid impact at the Cretaceous-Paleogene boundary (66.0 Ma). In early 2016 the IODP Exp. 364 successfully drilled the materials from the topographic peak ring within the crater that was previously identified by seismological observations. A continuous core was recovered. The ≈112m-thick uppermost part of the continuous core (505.7-1334.7 mbsf) is post-impact sediments, including the PETM, that are mainly composed of carbonate with intercalation of siliciclastics and variable contents of organic carbon. More than 300 samples from the post-impact section were finely powdered for a variety of geochemical analysis. Here we report their carbon and oxygen isotope compositions of the carbonate fraction (mostly in the lower part of the analyzed section) and carbon and nitrogen isotope compositions of organic matter (mostly in the middle-upper part of the analyzed section). Isotope mass spectrometer Isoprime was used for the former analysis, and EA-irMS (elemental analyzer - isotope ratio mass spectrometer) was used for the latter analysis, both at CMCR, Kochi Univ. Depth profile of oxygen isotope compositions of carbonate fraction is variable and somewhat similar to those of Zachos et al. (2001; Science). Carbon isotope compositions of carbonate and organic carbon in the lower part of the analyzed section exhibit some excursions that could correspond to the hyperthemals in the early Paleogene. Their variable nitrogen isotope compositions reflect temporal changes in the style of biogeochemical cycles involving denitrification and nitrogen fixation. Coupled temporal changes in the carbon isotope compositions of organic and carbonate carbon immediately after the K-Pg boundary might support a Strangelove ocean (Kump, 1991; Geology), however high export production (Ba/Ti, nannoplankton and calcisphere blooms, high planktic foram richness, and diverse and abundant micro- and macrobenthic organisms) at the base of the Danian limestone cored during Exp. 364 contradict a Strangelove Ocean.
Year of Publication: 2017
Research Program: IODP2 International Ocean Discovery Program
Key Words: 12 Stratigraphy, Historical Geology and Paleoecology; Chicxulub Crater; Expedition 364; Impact craters; Impact features; International Ocean Discovery Program; Paleo-oceanography
Record ID: 2018074795
Copyright Information: GeoRef, Copyright 2019 American Geosciences Institute. Reference includes data supplied by, and/or abstract, Copyright, American Geophysical Union, Washington, DC, United States

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