GSA Annual Meeting in Seattle, Washington, USA - 2017

Paper No. 192-4
Presentation Time: 9:05 AM

THE UPPER PART OF THE SUEVITE AND INTERMEDIATE LAYER AT SITE M0077A, IODP-ICDP EXPEDITION 364 INTO THE PEAK RING OF THE CHICXULUB CRATER (YUCATAN, MEXICO)


CLAEYS, Philippe1, DE WINTER, Niels J.1, GODERIS, Steven1, SINNESAEL, Matthias1, WITTMANN, Axel2 and SMIT, Jan3, (1)Analytical Environmental and Geo-Chemistry (AMGC), Vrije Universiteit Brussel, Brussels, 1050, Belgium, (2)LeRoy Eyring Center For Solid State Science, Arizona State University, Tempe, AZ 85287, (3)Faculty of Earth and Life Sciences, Vrije Universiteit, de Boelelaan 1085, Amsterdam, 1081HV, Netherlands, phclaeys@vub.be

IODP-ICDP hole M0077A recovered a core into the peak ring of Chicxulub offshore Yucatán composed of 3 main lithological units: 1) Paleogene sediments, 2) suevite/impact melt rocks and 3) granitic peak ring rocks intruded by pre-impact dikes and intercalated with suevites and impact-melt. This abstract examines the geochemistry of the intermediate unit between the impactites to the overlying Paleogene sediments (core 40 R-1). This ~ 80 cm unit is composed of fine laminated clay and carbonate-rich siltstones that may record the K/Pg boundary PGE anomaly. The contacts with the above lying marlstone-dominated Paleogene sediments and the underlying suevite unit are sharp and clearly visible. The upper and finer part of the suevite sequence is composed of carbonate-rich, sand-sized sorted and graded material, which indicate settling and reworking by high-energy processes (seiche, tsunami, slope failure…). This unit contains few altered impact-melt fragments, with elongated shapes and vesicles and many carbonate clasts of various sizes, with well-preserved Maastrichtian foraminifera floating in a fine carbonate matrix. It resembles the suevite found in the hole Yucatan-6, level N13, drilled onshore also in the peak-ring area, which contains feathery calcite - diagnostic for rapidly quenched carbonate liquids - that has not (yet?) been identified in M0077A. Just above the sharp contact, the lowermost part of the intermediate unit (617.30-617.34 mbsf) contains multiple mm-thick layers, clearly enriched in Ni, over a thickness of ~ 1 cm. Based on LA-ICP-MS concentration profiles and EMPA imaging, these Ni-rich layers are linked to the presence of Fe-Ni-Co-Cu-Pb-Zn sulfide mineralizations that are associated with very small (µm) platinum nuggets, but no clear Ir anomalies is detected. These sulfides probably reflect the existence of an impact-generated hydrothermal system, circulating fluids and solid components in the crust and releasing S- and volatile-rich fluids. Focus is now placed on the upper section of the intermediate settling unit, where additional siderophile element enrichments occur. The identification a clear Ir anomaly with chondritic inter-element ratios should reveal the source and processes responsible for the observed elevated concentrations.

Co-authors: IODP-ICDP Expedition 364 Scientists