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Geology; July 2000; v. 28; no. 7; p. 643-646; DOI: 10.1130/0091-7613(2000)28<643:TOTEEH>2.0.CO;2
© 2000 Geological Society of America
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Tempo of the end-Permian event: High-resolution cyclostratigraphy at the Permian-Triassic boundary

Michael R. Rampino1, Andreas Prokoph2 and Andre Adler3

1 Earth and Environmental Science Program, New York University, 100 Washington Square East, New York, New York 10003, USA, and NASA, Goddard Institute for Space Studies, 2880 Broadway, New York, New York 10025, USA
2 Department of Earth Sciences, University of Ottawa, 365 Nicholas Street, Ottawa, Ontario K1N 6N5, Canada
3 Department of Physics, New York University, 2-4 Washington Place, New York, New York 10003, USA

The Permian-Triassic (P-T) boundary is marked by the most severe mass extinction in the geologic record. High-resolution cyclostratigraphy on a 104 yr scale across the P-T boundary in a core from the Carnic Alps (Austria) revealed significant cycles in the ratio ~40:10:4.7:2.3 m, identified with Milankovitch cycles of ~412:100:40:20 k.y. (eccentricity 1 and 2, obliquity, and precession). Wavelet analysis indicates continuity of deposition across the boundary, with an average accumulation rate of ~10 cm/k.y. The dramatic faunal changes at the P-T boundary can be constrained within an interval of <60 k.y. (possibly <8 k.y.), with the accompanying sharp negative global carbon-isotope shift within <30 k.y., suggesting a catastrophic cause.

Key Words: Permian-Triassic boundary • Milankovitch cycles • extinctions • cyclostratigraphy




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