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The End-Cretaceous Mass Extinction and the Chicxulub Impact in Texas
Author(s) -
Gerta Keller,
Thierry Adatte
Publication year - 2011
Language(s) - English
Resource type - Book series
DOI - 10.2110/sepmsp.100
Subject(s) - impact crater , extinction event , ejecta , geology , extinction (optical mineralogy) , paleontology , outcrop , impact structure , cretaceous , dozen , astronomy , physics , biological dispersal , population , demography , arithmetic , mathematics , supernova , sociology
One of the liveliest, contentious, and long-running scientific debates began over three decades ago with the discovery of an iridium anomaly in a thin clay layer at Gubbio, Italy, that led to the hypothesis that a large impact caused the end-Cretaceous mass extinction. For many scientists the discovery of an impact crater near Chicxulub on Yucatan in 1991 all but sealed the impact-kill hypothesis as proven with the impact as sole cause for the mass extinction. Ever since that time evidence to the contrary has generally been interpreted as an impact-tsunami disbturbance. A multi-disciplinary team of reserachers has tested this assertion in new cores and a dozen outcrops along the Brazos River, Texas. In this area undisturbed sediments reveal a complete time stratigraphic sequence containing the primary impact spherule ejecta layer in late Maastrichtian claystones deposited about 200-300 thousand years before the mass extinction.

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