Convection and transfers in a textured partially-molten planet from the magma ocean stage to present-day solid-state convection
SOFT-PLANET aims to understand planetary evolution by linking mantle convection, rheology, and surface morphology through innovative soft material experiments and visualization techniques.
Projectdetails
Introduction
How and when plate tectonics (PT) developed on Earth, and why the Earth is currently the only rocky planet of the solar system with PT, are two of the main enigmas of Earth and Planetary Sciences. The evolution of a planet is conditioned by heat transfer in its most viscous envelope, the mantle.
Heat Transfer and Convection
This heat transfer is mostly due to convection, and strongly depends on the convective patterns, which in turn depend critically on mantle rheology. However, the link between rock rheology at small time- and length-scales, and mantle "effective" rheology at the long/large scales of mantle convection is still missing.
Meso-scale Structure
I propose that it resides in the meso-scale structure of the mantle and lithosphere that are acquired through convective motions and partial melting. Hence, deciphering the evolution of the Earth or any other planet requires describing and understanding the interplay between:
- "Texture" (i.e. material multi-scale organization)
- Rheology
- Two-phase flow
- Convection
Recent Findings
Our team recently showed that aqueous nanoparticle colloids, fluids commonly used by soft matter physicists, can reproduce planetary phenomena such as one-sided subduction and the two-phase flow dynamics of mid-ocean ridges.
Project Overview
Building on this, SOFT-PLANET will combine convection in these soft materials with state-of-the-art visualization techniques to relate:
- Surface morphology (including faults, wrinkle ridges, and volcanism)
- Lithospheric structure
- Internal flow patterns
We will characterize the development of texture and rheology from the nano-scale to the macro-scale of convection.
Goals of SOFT-PLANET
SOFT-PLANET will map the different regimes of convection that can develop and will derive a physical understanding of each. This new physical framework, together with geomorphology observations, will be used to decipher the current state of Venus and the divergent evolution of Venus, Mars, and the Earth.
Financiële details & Tijdlijn
Financiële details
Subsidiebedrag | € 3.418.549 |
Totale projectbegroting | € 3.418.549 |
Tijdlijn
Startdatum | 1-7-2023 |
Einddatum | 30-6-2028 |
Subsidiejaar | 2023 |
Partners & Locaties
Projectpartners
- CENTRE NATIONAL DE LA RECHERCHE SCIENTIFIQUE CNRSpenvoerder
- UNIVERSITE PARIS-SACLAY
Land(en)
Vergelijkbare projecten binnen European Research Council
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The formation and evolution of the primordial planetary felsic crustPLANETAFELSIC aims to model the formation and evolution of primordial felsic crusts on Earth, Mars, and Venus to enhance understanding of early planetary habitability and guide future exploration. | ERC Advanced... | € 2.883.478 | 2025 | Details |
New isotope tracers of rocky planet forming environmentsThis project aims to uncover the origins and evolution of precursor materials for terrestrial planets by analyzing chondrules in meteorites using advanced isotopic and imaging techniques. | ERC Consolid... | € 1.970.878 | 2024 | Details |
Rebuilding the foundations of planet formation: proto-planetary disc evolutionThe project aims to develop a new model of proto-planetary disc evolution driven by winds, enhancing our understanding of planet formation by integrating observational data with theoretical frameworks. | ERC Starting... | € 1.495.755 | 2022 | Details |
Virtual planets to unravel how mantle convection shapes geosphere, climate and life co-evolution
This project aims to uncover how mantle convection influences Earth's surface environment and biodiversity through advanced 3D simulations and machine learning over geological time scales.
Formation and Evolution of the Earth with Volatile Elements
This project aims to quantify volatile elements in Earth's core and bulk silicate Earth through experiments, enhancing models of planetary evolution and atmospheric development.
The formation and evolution of the primordial planetary felsic crust
PLANETAFELSIC aims to model the formation and evolution of primordial felsic crusts on Earth, Mars, and Venus to enhance understanding of early planetary habitability and guide future exploration.
New isotope tracers of rocky planet forming environments
This project aims to uncover the origins and evolution of precursor materials for terrestrial planets by analyzing chondrules in meteorites using advanced isotopic and imaging techniques.
Rebuilding the foundations of planet formation: proto-planetary disc evolution
The project aims to develop a new model of proto-planetary disc evolution driven by winds, enhancing our understanding of planet formation by integrating observational data with theoretical frameworks.