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dc.contributor.authorFrançois, C.
dc.contributor.authorDebaille, V.
dc.contributor.authorPaquette, JL.
dc.contributor.authorBaudet, D.
dc.contributor.authorJavaux, EJ.
dc.date2019
dc.date.accessioned2024-03-14T13:20:40Z
dc.date.available2024-03-14T13:20:40Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/12327
dc.descriptionUnderstanding the geodynamic processes of the Early Earth is crucial because they have strong implications for the habitability of the Earth but also for other planets. The Earth is the only proven planet in the solar system displaying lithospheric plate tectonics. However, plate tectonics on Earth did not always function as today, and the Archean was likely characterized by a stagnant-lid regime. Characterizing the transition from ancient to modern-style geodynamic regimes, including subduction process, is therefore important to understand the evolution of our own planet but also to compare our model to other rocky planets in our solar system. Here, we have characterized the oldest high pressure and low temperature eclogite worldwide (2089±13 Ma)discovered in the Democratic Republic of the Congo (Kasai Block). Eclogites are generally only produced in subduction geodynamic setting. Moreover, we have identified the protolith of this eclogite, a gabbro, which formed 2216±26 Ma ago in a narrow basin opening in a continental environment, and was then buried at∼55km in the mantle by subduction, before being exhumed to the surface during a complete Wilson cycle lasting about 130 Ma. This discovery evidences a modern-style plate tectonics operating since at least 2.2-2.1 Ga. This highlights the fundamental differences between the ancient Earth, without plate tectonics, and the modern Earth, as we know it today. The appearance of plate tectonics had important impacts on Life evolution on our planet, with an increasing supply of nutrients by erosion, increasing diversity of ecological niches and geographic isolation leading to increasing biodiversity, variable climatic conditions and oceanic circulation, as well as volcanic gases of different composition that may have influenced the composition of our atmosphere.
dc.languageeng
dc.titleOnset of plate tectonics on Earth and implications for habitability
dc.typeArticle
dc.subject.frascatiEarth and related Environmental sciences
dc.audienceScientific
dc.subject.freeGeodynamics and mineral resources
dc.source.titleEGU
dc.source.volumeabstracts 21
dc.source.page9256
Orfeo.peerreviewedNo
dc.identifier.doi10.13140/RG.2.2.28976.20480
dc.identifier.rmca5584


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