Hola,
¿eres nuevo aquí?

Regístrate gratis y conecta tu empresa con financiación pública, partners y proyectos.

Tengo cuenta

Regístrate

Ver video

CRUSLID

Financiado

Formation magmatic evolution and present day structure of the CRUsts of Stagnan...

Formation magmatic evolution and present day structure of the CRUsts of Stagnant LID planets The low density of the Earth’s continental crust has been proposed to be at the origin of plate tectonics. Physical studies on the continental crust have shown that its low density was acquired by differentiation of the crust and... ver más

30/09/2027

ENS DE LYON

2M€

Presupuesto del proyecto: 2M€

Líder del proyecto

ECOLE NORMALE SUPERIEURE DE LYON No se ha especificado una descripción o un objeto social para esta compañía.

TRL 4-5

Ver 4 Participantes

Financiación concedida El organismo H2020 notifico la concesión del proyecto el día 2021-01-20

ERC-2020-COG: ERC CONSOLIDATOR GRANTS

I+D

Cerrada hace 4 años

0% 100% 100%

Información adicional privada

No hay información privada compartida para este proyecto. Habla con el coordinador.

4 Participantes

ENS DE LYON

1.61M€ | Lider

MIMECRI

356.58K€ | Participante

UNIVERSITE LYON 1 CLAUDE BER...

N.D. | Participante

Conecta tu I+D

¿Tienes un proyecto y buscas un partner? Gracias a nuestro motor inteligente podemos recomendarte los mejores socios y ponerte en contacto con ellos. Te lo explicamos en este video

Proyectos interesantes

SOFT-PLANET Convection and transfers in a textured partially-molten plan... 3M€ Cerrado

CGL2013-41860-P MODELO INTERDISCIPLINARIO Y DINAMICO PARA EL NUCLEO INTERNO... 36K€ Cerrado

IJC2018-036074-I Estructura y Dinámica de la Tierra y Cristalografía 93K€ Cerrado

Balcony BALancing Craton thickness by self-cOmpression, graiN size e... 211K€ Cerrado

ATR2023-143517 Ciencias de la Tierra y del agua 957K€ Cerrado

RYC2021-031053-I GEOCHEMICAL AND PHASE-EQUILIBRIA MODELLING ON FLUID TRANSFER... 236K€ Cerrado

Duración del proyecto: 80 meses Fecha Inicio: 2021-01-20
Fecha Fin: 2027-09-30

Líder del proyecto

ECOLE NORMALE SUPERIEURE DE LYON No se ha especificado una descripción o un objeto social para esta compañía.

TRL 4-5

Presupuesto del proyecto 2M€

Descripción del proyecto The low density of the Earth’s continental crust has been proposed to be at the origin of plate tectonics. Physical studies on the continental crust have shown that its low density was acquired by differentiation of the crust and loss of dense mafic residues. What is the composition and vertical structure of the crusts of the other terrestrial planets, which do not show plate tectonics? How did they form and what are the modifications they have undergone following their formations? Are they far from being of continental-type? To answer these questions, I propose to study from a physical perspective the crust structure and the processes of crust formation and evolution on terrestrial planets other than Earth using innovative thermal, mechanical and dynamical models combined with new planetary observations. Temperature is a crucial control variable as it dictates phase changes, buoyancy, mechanical properties and stress state. In the crust and stagnant lithosphere of terrestrial planets, temperature is controlled by the distribution of heat producing elements. Lithosphere cooling being the most likely cause of quakes on stagnant-lid planets, we propose to constrain the concentration and distribution of heat producing elements on Mars and the Moon by comparing recorded and predicted seismicity from thermal evolution models. From these thermal evolution models, we will also evaluate the potential for planetary crust differentiation and evolution. From magma ascent models, sensitive to crust density and mechanical state, combined with systematic in quantitative observations of volcanic structures and deposits on terrestrial planets, we will constrain the crust structure and thermal state. Finally, we will develop new models of primitive crust formation in a stagnant lid regime of convection to evaluate the characteristics of primitive crusts on terrestrial bodies.

Conecta tu I+D

Entra hoy

¿Olvidé mi contraseña?

Financiación

Empresas

CTIs/Universidades

Proyectos

Investigadores