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Sudden and Gradual Molluscan Extinctions in the Latest Cretaceous of Western European Tethys

Science
22 Nov 1996
Vol 274, Issue 5291
pp. 1360-1363

Abstract

Incompleteness of the fossil record has confounded attempts to establish the role of the end-Cretaceous bolide impact in the Late Cretaceous mass extinctions. Statistical analysis of latest Cretaceous outer-shelf macrofossils from western European Tethys reveals (i) a major extinction at or near the Cretaceous-Tertiary (K-T) boundary, probably caused by the impact, (ii) either a faunal abundance change or an extinction of up to nine ammonite species associated with a regression event shortly before the boundary, (iii) gradual extinction of most inoceramid bivalves well before the K-T boundary, and (iv) background extinction of approximately six ammonites throughout the latest Cretaceous.

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REFERENCES AND NOTES

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Based on graphic correlation of the major lithological boundaries.
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Forty-two diagnosable ammonite fossils are known from the interval (about 30 fossils per meter of section), compared with a recovery of 1.5 diagnosable ammonite fossils per meter over the preceding 200 m of section.
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The absence of ammonites in the marls of Member V is unlikely to be due to preservation failure, given that ammonites are found in the similar marls of Member III, which occurs lower in the section.
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Ammonite fossils have been found, on average, once every 18 m2 of outcrop in the top 1.3 m of the Cretaceous at Hendaye, France. Echinoids are recovered at a comparable rate of one specimen per 19 m2 of outcrop. At least one echinoid per collecting season, but no ammonites over seven seasons, has been recovered in about 50 m2 of outcrop excavated within the pre-K-T gap (1.3 to 3.0 m below the K-T boundary). At these recovery rates, the probability that ammonites were as abundant in the excavated interval as they were above the pre-K-T gap is only 0.06; however, the probability that the ammonites were a third as abundant in the excavated interval as they were above the pre-K-T gap is 0.39.
32
We thank A. Smith, M. Foote, D. Jablonski, D. Jacobs, B. Runnegar, and two anonymous reviewers for their comments. Supported by NSF grant EAR-9258045 to C.R.M. and by EAR-8904797 and EAR-8843926 to P.D.W.

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Published In

Science
Volume 274 | Issue 5291
22 November 1996

Submission history

Received: 29 May 1996
Accepted: 3 September 1996
Published in print: 22 November 1996

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Charles R. Marshall*
C. R. Marshall, Department of Earth and Space Sciences, Molecular Biology Institute, and Institute for Geophysics and Planetary Physics, University of California, Los Angeles, CA 90095-1567, USA.
Peter D. Ward
P. D. Ward, Department of Geological Sciences, AJ-20, University of Washington, Seattle, WA 98195, USA.

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