Differences in physiological tolerance to global warming caused the Permian–Triassic transition between the Paleozoic and Modern faunas

J J. Andres Marquez (Department of Earth & Planetary Sciences, Doerr School of Sustainability, Stanford University) J Justin L. Penn (Department of Geosciences, Princeton University) R Richard G. Stockey (Department of Earth & Planetary Sciences, Doerr School of Sustainability, Stanford University) T Thomas H. Boag (Department of Earth & Planetary Sciences, Doerr School of Sustainability, Stanford University) M Murray I. Duncan (Department of Earth & Planetary Sciences, Doerr School of Sustainability, Stanford University) K Kyra N. McClure (Department of Earth & Planetary Sciences, Doerr School of Sustainability, Stanford University) K Kendall Matsumoto (Earth Systems, Doerr School of Sustainability, Stanford University) K Kemi F. Ashing-Giwa (Department of Earth & Planetary Sciences, Doerr School of Sustainability, Stanford University) C Christopher P. Noll (Department of Earth & Planetary Sciences, Doerr School of Sustainability, Stanford University) C Curtis Deutsch (Department of Geosciences, Princeton University) J Jonathan L. Payne (Department of Earth & Planetary Sciences, Doerr School of Sustainability, Stanford University) E Erik A. Sperling (Department of Earth & Planetary Sciences, Doerr School of Sustainability, Stanford University)

Abstract

The rapid global climate change at the end of the Permian Period (~251.9 Mya) coincided with the greatest macroevolutionary faunal turnover event in Earth’s history. As the oceans warmed, lost dissolved oxygen, and became more acidic, the dominant animal groups in the Paleozoic fauna (including brachiopods and crinoids) suffered differentially high rates of extinction, allowing the Modern fauna (including bivalves and gastropods) to rise to ecological dominance. The end-Permian kill mechanism(s) are not fully understood, but differences in extinction intensity among Linnaean classes suggest an important physiological component. Here, we use a trait-based model of species’ metabolic O 2 balance to demonstrate that temperature-dependent hypoxia can explain the taxonomic selectivity of the end-Permian mass extinction. Direct respirometry experiments and physiological trait estimates derived from biogeographic data reveal that species belonging to the Paleozoic fauna have a higher temperature dependence of hypoxia than those belonging to the Modern fauna. In simulations of the climate transition, this trait difference leads to a greater loss of aerobic habitat for Paleozoic fauna, consistent with their observed greater extinction intensity. These results demonstrate that differences in average physiological tolerances to environmental change across biogeography, taxonomy, and functional ecology drove end-Permian extinction patterns and could eventually characterize the modern biodiversity crisis. Temperature-dependent hypoxia is the only kill mechanism that has been shown to explain the magnitude, biogeography, and now taxonomic selectivity of the end-Permian mass extinction, ultimately underlying the permanent shift in marine ecosystems across this transition.

Article Details

Volume / Issue Vol. 123, Issue 28
Published July 14, 2026
ISSN 0027-8424
Publisher National Academy of Sciences

Authors (12)

J

J. Andres Marquez

Department of Earth & Planetary Sciences, Doerr School of Sustainability, Stanford University

J

Justin L. Penn

Department of Geosciences, Princeton University

R

Richard G. Stockey

Department of Earth & Planetary Sciences, Doerr School of Sustainability, Stanford University

T

Thomas H. Boag

Department of Earth & Planetary Sciences, Doerr School of Sustainability, Stanford University

M

Murray I. Duncan

Department of Earth & Planetary Sciences, Doerr School of Sustainability, Stanford University

K

Kyra N. McClure

Department of Earth & Planetary Sciences, Doerr School of Sustainability, Stanford University

K

Kendall Matsumoto

Earth Systems, Doerr School of Sustainability, Stanford University

K

Kemi F. Ashing-Giwa

Department of Earth & Planetary Sciences, Doerr School of Sustainability, Stanford University

C

Christopher P. Noll

Department of Earth & Planetary Sciences, Doerr School of Sustainability, Stanford University

C

Curtis Deutsch

Department of Geosciences, Princeton University

J

Jonathan L. Payne

Department of Earth & Planetary Sciences, Doerr School of Sustainability, Stanford University

E

Erik A. Sperling

Department of Earth & Planetary Sciences, Doerr School of Sustainability, Stanford University