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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.

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

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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