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Impact at the Permo-Triassic boundary: a critical evaluation
1Department of Paleobiology, Smithsonian Institution, Washington, DC 20560, USA. erwin.doug@nmnh.si.edu
Astrobiology
|June 14, 2003
Summary
The Permian-Triassic mass extinction, the largest in Earth's history, shows some evidence of an extraterrestrial impact. However, Earth-bound processes are a more likely cause for this significant extinction event.
Area of Science:
- Geology
- Paleontology
- Earth Science
Background:
- The Cretaceous-Tertiary (K-T) boundary impact event linked to mass extinction spurred research into other mass extinctions.
- Claims of impact evidence for the Permian-Triassic (P-T) mass extinction have faced significant challenges in reproducibility.
Purpose of the Study:
- To evaluate the evidence for an extraterrestrial impact as the cause of the Permian-Triassic mass extinction.
- To explore alternative, Earth-bound explanations for the P-T extinction event.
Main Methods:
- Review of existing geological and paleontological data related to the P-T mass extinction.
- Analysis of evidence for rapid extinction, carbon isotope shifts, and terrestrial-marine extinction correlations.
- Consideration of the Siberian flood basalts and complex carbon cycle shifts.
Main Results:
- While some evidence, such as rapid extinction and carbon shifts, is consistent with an impact, it is not definitively proven.
- The coincidence with the Siberian flood basalts and the complexity of the carbon shift present challenges to the impact hypothesis.
- Earth-bound processes offer a compelling alternative explanation for the P-T mass extinction.
Conclusions:
- The Permian-Triassic mass extinction, despite some impact-like signals, is more likely attributed to terrestrial processes.
- Understanding the failure of ecosystems through Earth-bound events provides greater insight than identifying another impact.
- Further research into Earth's internal dynamics is crucial for understanding major extinction events.