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Complementarity SIGNED

A unifying model: bulk chondrite complementarity by individual chondrule-matrix mentality

Total Cost €

0

EC-Contrib. €

0

Partnership

0

Views

0

 Complementarity project word cloud

Explore the words cloud of the Complementarity project. It provides you a very rough idea of what is the project "Complementarity" about.

data    proposes    constraints    suggest    fragments    constituents    regarding    silicate    indicate    planetary    meteorites    single    unprocessed    capacity    seemingly    accretion    particles    chondrules    exoplanetary    requiring    rims    circumstellar    bridge    probed    building    represented    astrophysical    universe    time    grains    raises    asteroids    hypothesis    chondrule    missions    transport    mechanisms    genetically    blocks    central    space    simulations    matrix    physicochemical    chondrites    verify    model    storage    frontiers    candidate    small    mass    genetic    chondritic    final    planets    subsequent    once    interplanetary    contrastingly    complementarity    isotope    tackle    reservoir    fundamental    relationships    chemical    sun    primitive    bulk    analytical    formed    disk    molten    link    dust    questions    spherules    return    cometary    history    accreted    relative    solar    poorly    bodies    turn    co    origin    individual    gas    mechanism    unify    star    life    evolution    components    opposing    planet    progress    invokes   

Project "Complementarity" data sheet

The following table provides information about the project.

Coordinator
INSTITUT DE PHYSIQUE DU GLOBE DE PARIS 

Organization address
address: RUE JUSSIEU 1
city: PARIS
postcode: 75238
website: http://www.ipgp.fr

contact info
title: n.a.
name: n.a.
surname: n.a.
function: n.a.
email: n.a.
telephone: n.a.
fax: n.a.

 Coordinator Country France [FR]
 Total cost 185˙076 €
 EC max contribution 185˙076 € (100%)
 Programme 1. H2020-EU.1.3.2. (Nurturing excellence by means of cross-border and cross-sector mobility)
 Code Call H2020-MSCA-IF-2017
 Funding Scheme MSCA-IF-EF-ST
 Starting year 2018
 Duration (year-month-day) from 2018-08-01   to  2020-07-31

 Partnership

Take a look of project's partnership.

# participants  country  role  EC contrib. [€] 
1    INSTITUT DE PHYSIQUE DU GLOBE DE PARIS FR (PARIS) coordinator 185˙076.00

Map

 Project objective

The so far unique role of our Solar System in the universe regarding its capacity for life raises fundamental questions about its formation history relative to exoplanetary systems. Central in this research is the accretion of asteroids and planets from a gas-rich circumstellar disk and the final distribution of their mass around the central star, our Sun. The key building blocks of the planets may be represented by chondrules, once molten silicate spherules that are the main constituents of chondritic meteorites, which in turn are primitive fragments of planetary bodies. Chondrule formation mechanism(s), as well as their subsequent storage and transport in the disk are still poorly understood and their origin and evolution can be probed through their link to unprocessed dust that accreted together with chondrules in chondrites. Contrastingly, while bulk chemical and isotope analyses of this dust (the matrix) and chondrules indicate that these components formed co-genetically in a single reservoir, individual analyses of chondrules suggest that they formed over a range of space and time, requiring storage and transport mechanisms. The candidate proposes to unify these seemingly opposing data in a single model that will result in significant and timely progress on the frontiers of Solar System research, including a bridge to astrophysical simulations that tackle planet formation and physicochemical constraints on the origin of chondrules. This model invokes bulk chondrule-matrix complementarity as a result of genetic relationships between individual chondrules and their dust rims. The necessary development of analytical methods to verify this hypothesis will contribute greatly to the advancement of small sample analyses, including cometary grains from sample return missions and interplanetary dust particles.

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The information about "COMPLEMENTARITY" are provided by the European Opendata Portal: CORDIS opendata.

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