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Cribb AT, Formoso KK, Woolley CH, Beech J, Brophy S, Byrne P, Cassady VC, Godbold AL, Larina E, Maxeiner PP, Wu YH, Corsetti FA, Bottjer DJ. Contrasting terrestrial and marine ecospace dynamics after the end-Triassic mass extinction event. Proc Biol Sci 2023; 290:20232232. [PMID: 38052241 PMCID: PMC10697803 DOI: 10.1098/rspb.2023.2232] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 02/02/2023] [Accepted: 11/14/2023] [Indexed: 12/07/2023] Open
Abstract
Mass extinctions have fundamentally altered the structure of the biosphere throughout Earth's history. The ecological severity of mass extinctions is well studied in marine ecosystems by categorizing marine taxa into functional groups based on 'ecospace' approaches, but the ecological response of terrestrial ecosystems to mass extinctions is less well understood due to the lack of a comparable methodology. Here, we present a new terrestrial ecospace framework that categorizes fauna into functional groups as defined by tiering, motility and feeding traits. We applied the new terrestrial and traditional marine ecospace analyses to data from the Paleobiology Database across the end-Triassic mass extinction-a time of catastrophic global warming-to compare changes between the marine and terrestrial biospheres. We found that terrestrial functional groups experienced higher extinction severity, that taxonomic and functional richness are more tightly coupled in the terrestrial, and that the terrestrial realm continued to experience high ecological dissimilarity in the wake of the extinction. Although signals of extinction severity and ecological turnover are sensitive to the quality of the terrestrial fossil record, our findings suggest greater ecological pressure from the end-Triassic mass extinction on terrestrial ecosystems than marine ecosystems, contributing to more prolonged terrestrial ecological flux.
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Affiliation(s)
- Alison T. Cribb
- Department of Earth Sciences, University of Southern California, Los Angeles, CA, USA
- School of Ocean and Earth Science, University of Southampton, Southampton, UK
| | - Kiersten K. Formoso
- Department of Earth Sciences, University of Southern California, Los Angeles, CA, USA
- The Dinosaur Institute, Natural History Museum of Los Angeles County, Los Angeles, CA, USA
| | - C. Henrik Woolley
- Department of Earth Sciences, University of Southern California, Los Angeles, CA, USA
- The Dinosaur Institute, Natural History Museum of Los Angeles County, Los Angeles, CA, USA
| | - James Beech
- Department of Earth Sciences, University of Southern California, Los Angeles, CA, USA
| | - Shannon Brophy
- Department of Earth Sciences, University of Southern California, Los Angeles, CA, USA
| | - Paul Byrne
- Department of Earth Sciences, University of Southern California, Los Angeles, CA, USA
- The Dinosaur Institute, Natural History Museum of Los Angeles County, Los Angeles, CA, USA
| | - Victoria C. Cassady
- Department of Earth Sciences, University of Southern California, Los Angeles, CA, USA
| | - Amanda L. Godbold
- Department of Earth Sciences, University of Southern California, Los Angeles, CA, USA
| | - Ekaterina Larina
- Department of Earth Sciences, University of Southern California, Los Angeles, CA, USA
- Department of Geological Sciences, Jackson School of Geosciences, University of Texas at Austin, Austin, TX, USA
| | - Philip-peter Maxeiner
- Department of Earth Sciences, University of Southern California, Los Angeles, CA, USA
| | - Yun-Hsin Wu
- Department of Earth Sciences, University of Southern California, Los Angeles, CA, USA
- The Dinosaur Institute, Natural History Museum of Los Angeles County, Los Angeles, CA, USA
| | - Frank A. Corsetti
- Department of Earth Sciences, University of Southern California, Los Angeles, CA, USA
| | - David J. Bottjer
- Department of Earth Sciences, University of Southern California, Los Angeles, CA, USA
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3
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Wu H, Zhang Y, Chen A, Stubbs TL. A Highly Diverse Olenekian Brachiopod Fauna from the Nanpanjiang Basin, South China, and Its Implications for the Early Triassic Biotic Recovery. BIOLOGY 2023; 12:biology12040622. [PMID: 37106822 PMCID: PMC10136273 DOI: 10.3390/biology12040622] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Key Words] [Grants] [Track Full Text] [Subscribe] [Scholar Register] [Received: 02/16/2023] [Revised: 04/13/2023] [Accepted: 04/17/2023] [Indexed: 04/29/2023]
Abstract
As one of the predominant benthic organisms in the Palaeozoic, brachiopod was largely eliminated in the Permian-Triassic boundary mass extinction, and then highly diversified in the Middle Triassic. Since fossil data from the Early Triassic are rarely reported, the recovery patterns of Early Triassic brachiopods remain unclear. This study documents a well-preserved fauna that is the most diverse Olenekian brachiopod fauna so far (age constrained by conodont biostratigraphy) from the Datuguan section of ramp facies in South China. This fauna is composed of 14 species within nine genera, including six genera (Hirsutella, Sulcatinella, Paradoxothyris, Dioristella, Neoretzia and Isocrania) found in the Early Triassic for the first time and three new species, including Paradoxothyris flatus sp. nov., Hirsutella sulcata sp. nov. and Sulcatinella elongata sp. nov. The Datuguan fauna indicates that the diversity of Olenekian brachiopod fauna has been underestimated, which can be caused by a combination of reduced habitats (in geographic size and sedimentary type) compared with the end-Permian, great bed thickness making it difficult to find fossils and most species in the fauna having low abundance. Based on the faunal change in the Datuguan section and environmental changes in South China, it can be inferred that brachiopod recovery in the studied section occurred in the latest Spathian rather than the Smithian when the environment started to ameliorate. Global brachiopod data also indicates that the initial recovery of brachiopods happened in the Spathian, and many genera that widely occurred in the Middle or Late Triassic had originated in the Olenekian.
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Affiliation(s)
- Huiting Wu
- School of Geoscience and Surveying Engineering, China University of Mining and Technology (Beijing), Beijing 100083, China
- State Key Laboratory of Palaeobiology and Stratigraphy, Nanjing Institute of Geology and Palaeontology, CAS, Nanjing 210008, China
| | - Yang Zhang
- State Key Laboratory of Palaeobiology and Stratigraphy, Nanjing Institute of Geology and Palaeontology, CAS, Nanjing 210008, China
- School of Earth Sciences and Resources, China University of Geosciences (Beijing), Beijing 100083, China
| | - Anfeng Chen
- School of Earth Sciences and Resources, China University of Geosciences (Beijing), Beijing 100083, China
| | - Thomas L Stubbs
- School of Earth Sciences, University of Bristol, Bristol BS1 5QD, UK
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4
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Huang Y, Chen ZQ, Roopnarine PD, Benton MJ, Zhao L, Feng X, Li Z. The stability and collapse of marine ecosystems during the Permian-Triassic mass extinction. Curr Biol 2023; 33:1059-1070.e4. [PMID: 36841237 DOI: 10.1016/j.cub.2023.02.007] [Citation(s) in RCA: 8] [Impact Index Per Article: 8.0] [Reference Citation Analysis] [Abstract] [Key Words] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 07/09/2022] [Revised: 11/20/2022] [Accepted: 02/01/2023] [Indexed: 02/27/2023]
Abstract
The history of Earth's biodiversity is punctuated episodically by mass extinctions. These are characterized by major declines of taxon richness, but the accompanying ecological collapse has rarely been evaluated quantitatively. The Permian-Triassic mass extinction (PTME; ∼252 mya), as the greatest known extinction, permanently altered marine ecosystems and paved the way for the transition from Paleozoic to Mesozoic evolutionary faunas. Thus, the PTME offers a window into the relationship between taxon richness and ecological dynamics of ecosystems during a severe extinction. However, the accompanying ecological collapse through the PTME has not been evaluated in detail. Here, using food-web models and a marine paleocommunity dataset spanning the PTME, we show that after the first extinction phase, community stability decreased only slightly despite the loss of more than half of taxonomic diversity, while community stability significantly decreased in the second phase. Thus, taxonomic and ecological changes were unequivocally decoupled, with species richness declining severely ∼61 ka earlier than the collapse of marine ecosystem stability, implying that in major catastrophes, a biodiversity crash may be the harbinger of a more devastating ecosystem collapse.
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Affiliation(s)
- Yuangeng Huang
- State Key Laboratory of Biogeology and Environmental Geology, China University of Geosciences (Wuhan), 68 Jincheng Street, Wuhan 430078, China; Department of Invertebrate Zoology and Geology, California Academy of Sciences, 55 Music Concourse Drive, San Francisco, CA 94118, USA
| | - Zhong-Qiang Chen
- State Key Laboratory of Biogeology and Environmental Geology, China University of Geosciences (Wuhan), 68 Jincheng Street, Wuhan 430078, China.
| | - Peter D Roopnarine
- State Key Laboratory of Biogeology and Environmental Geology, China University of Geosciences (Wuhan), 68 Jincheng Street, Wuhan 430078, China; Department of Invertebrate Zoology and Geology, California Academy of Sciences, 55 Music Concourse Drive, San Francisco, CA 94118, USA
| | - Michael J Benton
- School of Earth Sciences, University of Bristol, Queens Road, Bristol BS8 1RJ, UK
| | - Laishi Zhao
- State Key Laboratory of Geological Processes and Resource Geology, China University of Geosciences (Wuhan), 68 Jincheng Street, Wuhan 430078, China
| | - Xueqian Feng
- State Key Laboratory of Biogeology and Environmental Geology, China University of Geosciences (Wuhan), 68 Jincheng Street, Wuhan 430078, China
| | - Zhenhua Li
- School of Computer Science, China University of Geosciences (Wuhan), 68 Jincheng Street, Wuhan 430078, China
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