ISONEB

Isotopic records of solar nebula evolution and controls on planetary compositions

Coordinatore	UNIVERSITY OF BRISTOL    more Spiacenti, non ci sono informazioni su questo coordinatore. Contattare Fabio per maggiori infomrazioni, grazie.
Nazionalità Coordinatore	United Kingdom [UK]
Totale costo	3˙425˙271 €
EC contributo	3˙425˙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-2012-ADG_20120216
Funding Scheme	ERC-AG
Anno di inizio	2013
Periodo (anno-mese-giorno)	2013-07-01   -   2018-06-30

 Partecipanti

#	participant	country	role	EC contrib. [€]
1	THERMO FISHER SCIENTIFIC (BREMEN) GMBH  Organization address address: HANNA KUNATH STRASSE 11 city: BREMEN postcode: 28199 contact info Titolo: Mr. Nome: Volker Cognome: Blohberger Email: send email Telefono: 4942154930	DE (BREMEN)	beneficiary	1˙330˙000.00
2	NATURAL ENVIRONMENT RESEARCH COUNCIL  Organization address address: Polaris House, North Star Avenue city: SWINDON WILTSHIRE postcode: SN2 1EU contact info Titolo: Mrs. Nome: Sheryl Cognome: White Email: send email Telefono: +44 115 9363058	UK (SWINDON WILTSHIRE)	beneficiary	95˙040.00
3	UNIVERSITY OF BRISTOL  Organization address address: TYNDALL AVENUE SENATE HOUSE city: BRISTOL postcode: BS8 1TH contact info Titolo: Mrs. Nome: Audrey Cognome: Michael Email: send email Telefono: +44 117 3317371	UK (BRISTOL)	hostInstitution	2˙000˙231.00
4	UNIVERSITY OF BRISTOL  Organization address address: TYNDALL AVENUE SENATE HOUSE city: BRISTOL postcode: BS8 1TH contact info Titolo: Prof. Nome: Timothy Cognome: Elliott Email: send email Telefono: +44 117 9545426 Fax: +44 117 9253385	UK (BRISTOL)	hostInstitution	2˙000˙231.00

Mappa

 Word cloud

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 Obiettivo del progetto (Objective)

'This project has three linked strands that will combine to constrain the birth environment of the solar system and the nebular processes that shape bulk planetary compositions. Firstly, I will use ultra-high precision isotope ratio measurements in bulk meteorites to determine the stellar origin of the pre-solar of material that controls the gross compositional differences between planetary bodies. Secondly I will identify the mineralogical hosts of this isotopic variability, using in situ laser ablation analyses with a unique collision-cell multi-collector inductively coupled plasma mass-spectrometer, developed in close collaboration with an industrial partner (Thermo Fisher) as part of the project. Thirdly, I will establish a chronology for the mixing of the pre-solar material within the nebula, by dating individual meteorite components (chondrules) using ‘absolute’ Pb and relative 26Al-26Mg approaches and analysing the same aliquots for their mass-independent isotopic compositions. These observations will be quantitatively interpreted using novel numerical models of particle dynamics in the protoplanetary disk, in collaboration with Fred Cieala. This is an ambitious project that builds on the analytical prowess of the laboratory I have developed at Bristol and couples this with challenging technical developments and inter-disciplinary, modelling calculations. This work will radically improve our understanding of the history of the early solar system and the fundamental processes that shape its evolution.'