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Plate tectonics drives the compositional diversity of Earth's convecting mantle through subduction of lithosphere. In this context, the role of evolving global geodynamics and plate (re)organization on the spatial and temporal distribution of compositional heterogeneities in the convecting mantle is poorly understood. Here, using the geochemical compositions of intracontinental basalts formed over the past billion years, we show that intracontinental basalts with subchondritic initial neodymium-144/neodymium-143 values become common only after 300 million years, broadly coeval with the global appearance of kimberlites with geochemically enriched isotopic signatures. These step changes in the sources of intraplate magmatism stem from a rapid increase in the supply of deeply subducted lithosphere during the protracted formation of Pangea following the widespread onset of "modern" (cold and deep) subduction in the late Neoproterozoic. We argue that the delay (~300 million years) in the appearance of enriched intraplate magmas reflects the time required for the sinking and (re)incorporation of slabs into the sources of mantle-derived magmas.
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http://dx.doi.org/10.1126/sciadv.adq7476 | DOI Listing |
Sci Rep
September 2025
Department of Earth and Planetary Sciences, ETH Zürich, Zürich, 8092, Switzerland.
The occurrence of tectonic plate reorganization events is evident throughout the geologic record and appears to be associated with the cessation of mature and/or initiation of new subduction. Subduction initiation that produced the bend in the Hawaii-Emperor seamount chain resulted in the most recent upheaval of plate motion and engendered dramatic changes in plate velocities. Here, applying a method for identifying plate boundaries in a numerical global mantle convection model, we calculate Euler vector time series of self-consistently generated plates over a period of approximately 144 Myr.
View Article and Find Full Text PDFNatl Sci Rev
August 2025
Oulu Mining School, University of Oulu, Oulu 90014, Finland.
Determining the composition, formation mechanisms and stability of the Hadean continental crust is essential for understanding the early geological history of Earth. Detrital zircons, largely from Jack Hills of Western Australia, provide the dominant direct records for the nature of continental crust during the Hadean eon and its formation processes. Although isotope and trace element compositions of these zircons are extensively determined, the major and trace element compositions of their host rocks and corresponding parental magmas remain largely debated, making the nature and evolution of the early Earth's crust ambiguous.
View Article and Find Full Text PDFACS Omega
August 2025
School of Earth Sciences, East China University of Technology, Nanchang, Jiangxi 330013, China.
The Manglai uranium deposit is located in the Tabei Sag within the Manit Depression, centrally positioned in the eastern Erlian Basin at the core of an ancient valley uranium metallogenic belt. This study analyzed the geochemical properties of 22 clastic and mudstone samples from the Lower Cretaceous Saihan Formation in the Manglai deposit to assess its tectonic setting, provenance direction, redox conditions, and paleoclimatic environment. Key findings reveal that (1) The primary sediment source of the Saihan Formation in the Manglai deposit consists of felsic igneous rocks, situated mainly in a passive continental margin setting.
View Article and Find Full Text PDFScience
August 2025
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA.
A planet's interior is a time capsule, preserving clues to its early history. We report the discovery of kilometer-scale heterogeneities throughout Mars' mantle, detected seismically through pronounced wavefront distortion of energy arriving from deeply probing marsquakes. These heterogeneities, likely remnants of the planet's formation, imply a mantle that has undergone limited mixing driven by sluggish convection.
View Article and Find Full Text PDFCommun Earth Environ
August 2025
Department of Earth and Planetary Sciences, Institute of Geophysics, ETH Zürich, Sonneggstrasse 5, 8092 Zürich, Switzerland.
Subduction initiation is a pivotal process in the Wilson cycle, yet its mechanisms remain elusive. Using 3D coupled thermo-mechanical and surface processes models, we investigated how the duration of the plate motion reversal from rifting to plate convergence and the structural versus thermal inheritance influence the location of compression-induced subduction initiation. Our results reveal that abrupt plate motion changes lead to ridge inversion-driven subduction, controlled by the inherited thermal- and melt-induced weakening.
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