Cargando…
Crustal rejuvenation stabilised Earth’s first cratons
The formation of stable, evolved (silica-rich) crust was essential in constructing Earth’s first cratons, the ancient nuclei of continents. Eoarchaean (4000–3600 million years ago, Ma) evolved crust occurs on most continents, yet evidence for older, Hadean evolved crust is mostly limited to rare Had...
Autores principales: | Mulder, Jacob A., Nebel, Oliver, Gardiner, Nicholas J., Cawood, Peter A., Wainwright, Ashlea N., Ivanic, Timothy J. |
---|---|
Formato: | Online Artículo Texto |
Lenguaje: | English |
Publicado: |
Nature Publishing Group UK
2021
|
Materias: | |
Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8192532/ https://www.ncbi.nlm.nih.gov/pubmed/34112785 http://dx.doi.org/10.1038/s41467-021-23805-6 |
Ejemplares similares
-
A non-zircon Hf isotope record in Archean black shales from the Pilbara craton confirms changing crustal dynamics ca. 3 Ga ago
por: Nebel-Jacobsen, Yona, et al.
Publicado: (2018) -
When crust comes of age: on the chemical evolution of Archaean, felsic continental crust by crustal drip tectonics
por: Nebel, O., et al.
Publicado: (2018) -
Seismological constraints on the crustal structures generated by continental rejuvenation in northeastern China
por: Zheng, Tian-Yu, et al.
Publicado: (2015) -
Redox preconditioning deep cratonic lithosphere for kimberlite genesis – evidence from the central Slave Craton
por: Yaxley, G. M., et al.
Publicado: (2017) -
Thermal state and evolving geodynamic regimes of the Meso- to Neoarchean North China Craton
por: Sun, Guozheng, et al.
Publicado: (2021)