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Boulila S, Peters SE, Müller RD, Haq BU, Hara N. Earth's interior dynamics drive marine fossil diversity cycles of tens of millions of years. Proc Natl Acad Sci U S A 2023; 120:e2221149120. [PMID: 37428908 PMCID: PMC10629558 DOI: 10.1073/pnas.2221149120] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Key Words] [MESH Headings] [Grants] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 12/13/2022] [Accepted: 05/24/2023] [Indexed: 07/12/2023] Open
Abstract
The fossil record reveals that biotic diversity has fluctuated quasi-cyclically through geological time. However, the causal mechanisms of biotic diversity cycles remain unexplained. Here, we highlight a common, correlatable 36 ± 1 Myr (million years) cycle in the diversity of marine genera as well as in tectonic, sea-level, and macrostratigraphic data over the past 250 Myr of Earth history. The prominence of the 36 ± 1 Myr cycle in tectonic data favors a common-cause mechanism, wherein geological forcing mechanisms drive patterns in both biological diversity and the preserved rock record. In particular, our results suggest that a 36 ± 1 Myr tectono-eustatically driven sea-level cycle may originate from the interaction between the convecting mantle and subducting slabs, thereby pacing mantle-lithospheric deep-water recycling. The 36 ± 1 Myr tectono-eustatic driver of biodiversity is likely related to cyclic continental inundations, with expanding and contracting ecological niches on shelves and in epeiric seas.
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Affiliation(s)
- Slah Boulila
- Sorbonne Université, CNRS, Institut des Sciences de la Terre Paris, ParisF-75005, France
- Astronomie et Systèmes Dynamiques/Institut de Mécanique Céleste et de Calcul des Ephémérides, CNRS-UMR8028, Observatoire de Paris, Paris Sciences & Lettres University, Sorbonne Université, Paris75014, France
| | - Shanan E. Peters
- Department of Geoscience, University of Madison, Madison, WI53706
| | - R. Dietmar Müller
- EarthByte Group, School of Geosciences, University of Sydney, Sydney, NSW2006, Australia
| | - Bilal U. Haq
- Sorbonne Université, CNRS, Institut des Sciences de la Terre Paris, ParisF-75005, France
- Smithsonian Institution, Washington,DC20024
| | - Nathan Hara
- Département d’astronomie, Université de Genève, Genève1290, Switzerland
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Miller KG, Browning JV, Schmelz WJ, Kopp RE, Mountain GS, Wright JD. Cenozoic sea-level and cryospheric evolution from deep-sea geochemical and continental margin records. SCIENCE ADVANCES 2020; 6:eaaz1346. [PMID: 32440543 PMCID: PMC7228749 DOI: 10.1126/sciadv.aaz1346] [Citation(s) in RCA: 85] [Impact Index Per Article: 17.0] [Reference Citation Analysis] [Abstract] [Grants] [Track Full Text] [Download PDF] [Figures] [Subscribe] [Scholar Register] [Received: 08/14/2019] [Accepted: 03/16/2020] [Indexed: 05/14/2023]
Abstract
Using Pacific benthic foraminiferal δ18O and Mg/Ca records, we derive a Cenozoic (66 Ma) global mean sea level (GMSL) estimate that records evolution from an ice-free Early Eocene to Quaternary bipolar ice sheets. These GMSL estimates are statistically similar to "backstripped" estimates from continental margins accounting for compaction, loading, and thermal subsidence. Peak warmth, elevated GMSL, high CO2, and ice-free "Hothouse" conditions (56 to 48 Ma) were followed by "Cool Greenhouse" (48 to 34 Ma) ice sheets (10 to 30 m changes). Continental-scale ice sheets ("Icehouse") began ~34 Ma (>50 m changes), permanent East Antarctic ice sheets at 12.8 Ma, and bipolar glaciation at 2.5 Ma. The largest GMSL fall (27 to 20 ka; ~130 m) was followed by a >40 mm/yr rise (19 to 10 ka), a slowing (10 to 2 ka), and a stillstand until ~1900 CE, when rates began to rise. High long-term CO2 caused warm climates and high sea levels, with sea-level variability dominated by periodic Milankovitch cycles.
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Affiliation(s)
- Kenneth G. Miller
- Department of Earth and Planetary Sciences, Rutgers University, Piscataway, NJ 08854, USA
- Institute of Earth, Ocean, and Atmospheric Sciences, Rutgers University, New Brunswick, NJ 08901, USA
- Corresponding author.
| | - James V. Browning
- Department of Earth and Planetary Sciences, Rutgers University, Piscataway, NJ 08854, USA
- Institute of Earth, Ocean, and Atmospheric Sciences, Rutgers University, New Brunswick, NJ 08901, USA
| | - W. John Schmelz
- Department of Earth and Planetary Sciences, Rutgers University, Piscataway, NJ 08854, USA
- Institute of Earth, Ocean, and Atmospheric Sciences, Rutgers University, New Brunswick, NJ 08901, USA
| | - Robert E. Kopp
- Department of Earth and Planetary Sciences, Rutgers University, Piscataway, NJ 08854, USA
- Institute of Earth, Ocean, and Atmospheric Sciences, Rutgers University, New Brunswick, NJ 08901, USA
| | - Gregory S. Mountain
- Department of Earth and Planetary Sciences, Rutgers University, Piscataway, NJ 08854, USA
- Institute of Earth, Ocean, and Atmospheric Sciences, Rutgers University, New Brunswick, NJ 08901, USA
| | - James D. Wright
- Department of Earth and Planetary Sciences, Rutgers University, Piscataway, NJ 08854, USA
- Institute of Earth, Ocean, and Atmospheric Sciences, Rutgers University, New Brunswick, NJ 08901, USA
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