NOBLE

"The Origin, Accretion and Differentiation of Extreme Volatiles in Terrestrial Planets"

Coordinatore	THE CHANCELLOR, MASTERS AND SCHOLARS OF THE UNIVERSITY OF OXFORD    more Spiacenti, non ci sono informazioni su questo coordinatore. Contattare Fabio per maggiori infomrazioni, grazie.
Nazionalità Coordinatore	United Kingdom [UK]
Totale costo	2˙747˙271 €
EC contributo	2˙747˙271 €
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-AdG_20100224
Funding Scheme	ERC-AG
Anno di inizio	2011
Periodo (anno-mese-giorno)	2011-04-01   -   2017-03-31

 Partecipanti

#	participant	country	role	EC contrib. [€]
1	THE UNIVERSITY OF MANCHESTER  Organization address address: OXFORD ROAD city: MANCHESTER postcode: M13 9PL contact info Titolo: Ms. Nome: Liz Cognome: Fay Email: send email Telefono: 441613000000 Fax: 441613000000	UK (MANCHESTER)	beneficiary	1˙381˙564.29
2	THE CHANCELLOR, MASTERS AND SCHOLARS OF THE UNIVERSITY OF OXFORD  Organization address address: University Offices, Wellington Square city: OXFORD postcode: OX1 2JD contact info Titolo: Ms. Nome: Gill Cognome: Wells Email: send email Telefono: +44 1865 289800 Fax: +44 1865 289801	UK (OXFORD)	hostInstitution	1˙365˙706.71
3	THE CHANCELLOR, MASTERS AND SCHOLARS OF THE UNIVERSITY OF OXFORD  Organization address address: University Offices, Wellington Square city: OXFORD postcode: OX1 2JD contact info Titolo: Prof. Nome: Christopher John Cognome: Ballentine Email: send email Telefono: +44 1 865272000 Fax: +44 1 865272072	UK (OXFORD)	hostInstitution	1˙365˙706.71

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 Obiettivo del progetto (Objective)

'Identifying the processes by which the terrestrial planets acquired, retained and redistributed extreme volatile elements remains a fundamental science question. Although the halogens, Br, Cl and I, represent a powerful potential tracer, the concentrations of Br and I within most samples is too low for most laboratories - and the halogens have been ignored. We detail a Manchester innovation which enables halogens in these samples to be readily analysed.

We propose to: 1) Make the first direct experimental measurements of the partitioning behaviour of the halogens relevant to terrestrial mantle melting and planetesimal differentiation; 2) Establish the character of halogens available for accretion from chondrites; 3) Investigate the effect of planetesimal differentiation on the halogens from evolved meteorite glass/mineral systems; 4) Identify the role of massive impactors from lunar volcanic glasses; and 5) Identify the effect of planetary surface processes in the absence of life from alteration products in Martian meteorites.

On the Earth we will establish the first halogen mid ocean ridge and ocean island basalt halogen data base. This will enable us to: 1) Characterise the respective mantle source halogen-noble gases; 2) Test models of volatile element recycling into the mantle by exploiting the high I/Cl of the ocean sediments caused by organic sequestration; 3) Identify whether the relationship between halogens and noble gases in subducted fluids (pilot data) is preserved in the mantle; 4) Use the mantle iodine concentration together with 129Xe as a tool to quantify the mass of dead iodine recycled into the respective reservoirs. 5) Identify or devise mantle convection and primordial reservoir source models compatible with the new data set.'