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Tarduno JA, Cottrell RD, Bono RK, Rayner N, Davis WJ, Zhou T, Nimmo F, Hofmann A, Jodder J, Ibañez-Mejia M, Watkeys MK, Oda H, Mitra G. Hadaean to Palaeoarchaean stagnant-lid tectonics revealed by zircon magnetism. Nature 2023; 618:531-536. [PMID: 37316722 PMCID: PMC10266976 DOI: 10.1038/s41586-023-06024-5] [Citation(s) in RCA: 3] [Impact Index Per Article: 1.5] [Reference Citation Analysis] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 05/08/2022] [Accepted: 03/27/2023] [Indexed: 06/16/2023]
Abstract
Plate tectonics is a fundamental factor in the sustained habitability of Earth, but its time of onset is unknown, with ages ranging from the Hadaean to Proterozoic eons1-3. Plate motion is a key diagnostic to distinguish between plate and stagnant-lid tectonics, but palaeomagnetic tests have been thwarted because the planet's oldest extant rocks have been metamorphosed and/or deformed4. Herein, we report palaeointensity data from Hadaean-age to Mesoarchaean-age single detrital zircons bearing primary magnetite inclusions from the Barberton Greenstone Belt of South Africa5. These reveal a pattern of palaeointensities from the Eoarchaean (about 3.9 billion years ago (Ga)) to Mesoarchaean (about 3.3 Ga) eras that is nearly identical to that defined by primary magnetizations from the Jack Hills (JH; Western Australia)6,7, further demonstrating the recording fidelity of select detrital zircons. Moreover, palaeofield values are nearly constant between about 3.9 Ga and about 3.4 Ga. This indicates unvarying latitudes, an observation distinct from plate tectonics of the past 600 million years (Myr) but predicted by stagnant-lid convection. If life originated by the Eoarchaean8, and persisted to the occurrence of stromatolites half a billion years later9, it did so when Earth was in a stagnant-lid regime, without plate-tectonics-driven geochemical cycling.
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Affiliation(s)
- John A Tarduno
- Department of Earth and Environmental Sciences, University of Rochester, Rochester, NY, USA.
- Department of Physics and Astronomy, University of Rochester, Rochester, NY, USA.
- Laboratory for Laser Energetics, University of Rochester, Rochester, NY, USA.
- Geological Sciences, University of KwaZulu-Natal, Durban, South Africa.
| | - Rory D Cottrell
- Department of Earth and Environmental Sciences, University of Rochester, Rochester, NY, USA
| | - Richard K Bono
- Geomagnetism Laboratory, University of Liverpool, Liverpool, UK
- Department of Earth, Ocean and Atmospheric Science, Florida State University, Tallahassee, FL, USA
| | - Nicole Rayner
- Natural Resources Canada, Geological Survey of Canada, Ottawa, Ontario, Canada
| | - William J Davis
- Natural Resources Canada, Geological Survey of Canada, Ottawa, Ontario, Canada
| | - Tinghong Zhou
- Department of Earth and Environmental Sciences, University of Rochester, Rochester, NY, USA
| | - Francis Nimmo
- Department of Earth and Planetary Sciences, University of California, Santa Cruz, Santa Cruz, CA, USA
| | - Axel Hofmann
- Department of Geology, University of Johannesburg, Auckland Park, South Africa
| | - Jaganmoy Jodder
- Department of Geology, University of Johannesburg, Auckland Park, South Africa
- Evolutionary Studies Institute, University of the Witwatersrand, Wits, South Africa
| | | | - Michael K Watkeys
- Geological Sciences, University of KwaZulu-Natal, Durban, South Africa
| | - Hirokuni Oda
- Research Institute of Geology and Geoinformation, Geological Survey of Japan, National Institute of Advanced Industrial Science and Technology (AIST), Tsukuba, Japan
| | - Gautam Mitra
- Department of Earth and Environmental Sciences, University of Rochester, Rochester, NY, USA
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Matsuyama I, Mitrovica JX, Manga M, Perron JT, Richards MA. Rotational stability of dynamic planets with elastic lithospheres. ACTA ACUST UNITED AC 2006. [DOI: 10.1029/2005je002447] [Citation(s) in RCA: 46] [Impact Index Per Article: 2.4] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/09/2022]
Affiliation(s)
- I. Matsuyama
- Department of Astronomy and Astrophysics; University of Toronto; Toronto, Ontario Canada
| | - J. X. Mitrovica
- Department of Physics; University of Toronto; Toronto, Ontario Canada
| | - M. Manga
- Department of Earth and Planetary Science; University of California; Berkeley California USA
| | - J. T. Perron
- Department of Earth and Planetary Science; University of California; Berkeley California USA
| | - M. A. Richards
- Department of Earth and Planetary Science; University of California; Berkeley California USA
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Bunge HP, Richards MA, Baumgardner JR. A sensitivity study of three-dimensional spherical mantle convection at 108Rayleigh number: Effects of depth-dependent viscosity, heating mode, and an endothermic phase change. ACTA ACUST UNITED AC 1997. [DOI: 10.1029/96jb03806] [Citation(s) in RCA: 214] [Impact Index Per Article: 7.6] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/09/2022]
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Richards MA, Ricard Y, Lithgow-Bertelloni C, Spada G, Sabadini R. An Explanation for Earth's Long-Term Rotational Stability. Science 1997; 275:372-5. [PMID: 8994030 DOI: 10.1126/science.275.5298.372] [Citation(s) in RCA: 68] [Impact Index Per Article: 2.4] [Reference Citation Analysis] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 02/03/2023]
Abstract
Paleomagnetic data show less than approximately 1000 kilometers of motion between the paleomagnetic and hotspot reference frames-that is, true polar wander-during the past 100 million years, which implies that Earth's rotation axis has been very stable. This long-term rotational stability can be explained by the slow rate of change in the large-scale pattern of plate tectonic motions during Cenozoic and late Mesozoic time, provided that subducted lithosphere is a major component of the mantle density heterogeneity generated by convection. Therefore, it is unnecessary to invoke other mechanisms, such as sluggish readjustment of the rotational bulge, to explain the observed low rate of true polar wander.
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Affiliation(s)
- MA Richards
- M. A. Richards, Department of Geology and Geophysics, University of California, Berkeley, CA 94720, USA. Y. Ricard, Departement de Geologie, Ecole Normale Superieure, Lyon, France. C. Lithgow-Bertelloni, Department of Terrestrial Magnetism, Carnegie Institution of Washington, Washington, DC 20015-1305, USA. G. Spada, Dipartimento di Fisica, Settore Geofisica, Universita di Bologna, Bologna, Italy. R. Sabadini, Dipartimento di Scienze della Terra, Sezione Geofisica, Universita di Milano, Milano, Italy
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Abstract
An exceptionally low degree of melting of the upper mantle in the equatorial part of the mid-Atlantic Ridge is indicated by the chemical composition of mantle-derived mid-ocean ridge peridotites and basalts. These data imply that mantle temperatures below the equatorial Atlantic are at least approximately 150 degrees C cooler than those below the normal mid-Atlantic Ridge, suggesting that isotherms are depressed and the mantle is downwelling in the equatorial Atlantic. An equatorial minimum of the zero-age crustal elevation of the East Pacific Rise suggests a similar situation in the Pacific. If so, an oceanic upper mantle cold equatorial belt separates hotter mantle regimes and perhaps distinct chemical and isotopic domains in the Northern and Southern hemispheres. Gravity data suggest the presence of high density material in the oceanic equatorial upper mantle, which is consistent with its inferred low temperature and undepleted composition. The equatorial distribution of cold, dense upper mantle may be ultimately an effect of the Earth's rotation.
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