Geological Society of America

T228 Mass Extinctions II: Past, Present, and Future?

Tuesday, 24 October 2017
1:30 PM - 5:30 PM
Room 608

PRE-MASS EXTINCTION DECLINE OF LATEST PERMIAN AMMONOIDS

Paper number: T228-10
Program: Technical Sessions
Time: 3:45 PM – 4:00 PM

Authors

Wolfgang Kiessling Presenting Author
Friedrich-Alexander-Universität Erlangen-Nürnberg, Erlangen
Martin Schobben
University of Leeds, Leeds
Abbas Ghaderi
Ferdowsi University of Mashhad, Mashhad
Vachik Hairapetian
Islamic Azad University, Isfahan
Lucyna Leda
Museum fuer Naturkunde, Berlin
Dieter Korn
Museum fuer Naturkunde, Berlin

Abstract

The devastating end-Permian mass extinction is widely considered to be caused by large-scale and rapid greenhouse gas release by Siberian volcanism. Although the proximate extinction mechanisms are disputed, there is widespread agreement that a major extinction pulse occurred just below the biostratigraphically defined Permian–Triassic boundary. Statistical analyses of stratigraphic ranges and their confidence intervals do not comply with a single end-Permian extinction pulse of ammonoids in Iran. Extinction was gradual or stepped over the last million years of the Permian period. Analyses of body sizes and morphological complexity support a gradual decline over the same interval. Similar pre-mass extinction declines and disturbances of the carbon cycle have been reported from other regions suggesting a widespread, but often overlooked environmental deterioration at global scale well before the main extinction pulse. Ammonoids may have responded more strongly than other marine invertebrates because they were more sensitive to physiological stress.

Geological Society of America Abstracts with Programs. Vol. 49, No. 6

doi: 10.1130/abs/2017AM-301914

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