Paleophysiology and end-Permian mass extinction

被引:516
作者
Knoll, Andrew H. [1 ]
Barnbach, Richard K.
Payne, Jonathan L.
Pruss, Sara
Fischer, Woodward W.
机构
[1] Harvard Univ, Dept Organism & Evolutionary Biol, Cambridge, MA 02138 USA
[2] Smithsonian Inst, Natl Museum Nat Hist, Dept Paleobiol, Washington, DC 20560 USA
[3] Stanford Univ, Dept Geol & Environm Sci, Stanford, CA 94305 USA
[4] Harvard Univ, Dept Earth & Planetary Sci, Cambridge, MA 02138 USA
基金
美国国家科学基金会;
关键词
Permian; Triassic; mass extinction; physiology; paleontology;
D O I
10.1016/j.epsl.2007.02.018
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
Physiological research aimed at understanding current global change provides a basis for evaluating selective survivoyship associated with Permo-Triassic mass extinction. Comparative physiology links paleontological and palcoenvironmental observations, supporting the hypothesis that an end-Permian trigger, most likely Siberian Trap volcanism, touched off a set of physically-l inked perturbations that acted synergistically to disrupt the metabolisms of latest Permian organisms. Global wan-ning, anoxia, and toxic sulfide probably all contributed to end-Permian mass mortality, but hypercapnia (physiological effects of elevated P-CO2) best accounts for the selective survival of marine invertebrates. Paleophysiological perspectives further suggest that persistent or recurring hypercapnia/global warmth also played a principal role in delayed Triassic recovery. More generally, physiology provides an important way of paleobiological knowing in the age of Earth system science. (C) 2007 Elsevier B.V. All rights reserved.
引用
收藏
页码:295 / 313
页数:19
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