MAD-ESEC

Magmas at Depth: an Experimental Study at Extreme Conditions

 Coordinatore UNIVERSITE PIERRE ET MARIE CURIE - PARIS 6 

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 Nazionalità Coordinatore France [FR]
 Totale costo 1˙332˙160 €
 EC contributo 1˙332˙160 €
 Programma FP7-IDEAS-ERC
Specific programme: "Ideas" implementing the Seventh Framework Programme of the European Community for research, technological development and demonstration activities (2007 to 2013)
 Code Call ERC-2010-StG_20091028
 Funding Scheme ERC-SG
 Anno di inizio 2011
 Periodo (anno-mese-giorno) 2011-06-01   -   2017-05-31

 Partecipanti

# participant  country  role  EC contrib. [€] 
1    THE UNIVERSITY OF EDINBURGH

 Organization address address: OLD COLLEGE, SOUTH BRIDGE
city: EDINBURGH
postcode: EH8 9YL

contact info
Titolo: Ms.
Nome: Angela
Cognome: Noble
Email: send email
Telefono: +44 131 650 9024
Fax: +44 131 650 9023

UK (EDINBURGH) beneficiary 724˙755.06
2    UNIVERSITE PIERRE ET MARIE CURIE - PARIS 6

 Organization address address: Place Jussieu 4
city: PARIS
postcode: 75252

contact info
Titolo: Dr.
Nome: Chrystèle
Cognome: Sanloup
Email: send email
Telefono: +33 1 44 27 52 07
Fax: +33 1 44 27 39 11

FR (PARIS) hostInstitution 607˙404.94
3    UNIVERSITE PIERRE ET MARIE CURIE - PARIS 6

 Organization address address: Place Jussieu 4
city: PARIS
postcode: 75252

contact info
Titolo: Ms.
Nome: Ouerdia
Cognome: Oumohand
Email: send email
Telefono: +33 1 44 27 26 56
Fax: +33 1 44 27 74 67

FR (PARIS) hostInstitution 607˙404.94

Mappa


 Word cloud

Esplora la "nuvola delle parole (Word Cloud) per avere un'idea di massima del progetto.

silicate    melts    evolution    earth    ray    magmas    planetary    differentiation    molten    situ       chemical    broad    magma       fundamental    techniques    magmatic   

 Obiettivo del progetto (Objective)

'Magmas, i.e. silicate melts, have played a key role in the chemical and thermal evolution of the Earth and other planets. The Earth's interior today is the outcome of mass transfers which occurred primarily in its early history and still occur now via magmatic events. Present day magmatic and volcanic processes are controlled by the properties of molten silicate at high pressure, considering that magmas are produced at depth. However, the physical properties of molten silicates remain largely unexplored across the broad range of relevant P-T conditions, and their chemical properties are very often assumed constant and equal to those known at ambient conditions. This blurs out our understanding of planetary differentiation and current magmatic processes. The aim of this proposal is to place fundamental constraints on magma generation and transport in planetary interiors by measuring the properties of silicate melts in their natural high pressures (P) and high temperatures (T) conditions using a broad range of in situ key diagnostic probes (X-ray and neutron scattering techniques, X-ray absorption, radiography, Raman spectroscopy). The completion of this proposal will result in a comprehensive key database in the composition-P-T space that will form the foundation for modelling planetary formation and differentiation, and will provide answers to the very fundamental questions on magma formation, ascent or trapping at depth in the current and past Earth. This experimental program is allowed by the recent advancements in in situ high P-T techniques, and comes in conjunction with a large and fruitful theoretical effort; time has thus come to understand Earth's melts and their keys to Earth's evolution.'

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