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FETA

Fluid impacts in EarTh Accretion

Total Cost €

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EC-Contrib. €

0

Partnership

0

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 FETA project word cloud

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

interpret    drops    origin    usa    reinvested    observations    diagrams    geophysical    organisation    setting    geochemical    combines    place    interior    generation    deep    ideal    prodigious    embryos    laws    progress    host    ocean    mechanics    experiments    accreted    environment    coherent    liquid    mass    collisions    researcher    planetary    metallic    gaps    physical    formed    protoplanet    fragment    metal    chemical    mixing    clues    analog    first    expertise    regime    projectile    scales    accretion    energy    plate    scaling    fluid    core    lab    numerical    simulations    magma    questions    life    planets    initiation    delivered    evolution    cratering    stage    differentiated    amounts    magnetic    equilibration    instance    acquired    complementary    indicate    impacts    silicate    time    turbulence    theory    fate    efficiency    turbulent    played    silicates    geodynamics    exoplanets    mantle    geochemistry    fundamental    bridging    released    tectonics    molten    constraints    melting    earth   

Project "FETA" data sheet

The following table provides information about the project.

Coordinator
THE CHANCELLOR MASTERS AND SCHOLARSOF THE UNIVERSITY OF CAMBRIDGE 

Organization address
address: TRINITY LANE THE OLD SCHOOLS
city: CAMBRIDGE
postcode: CB2 1TN
website: www.cam.ac.uk

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 United Kingdom [UK]
 Project website https://feta703767.wordpress.com/
 Total cost 183˙454 €
 EC max contribution 183˙454 € (100%)
 Programme 1. H2020-EU.1.3.2. (Nurturing excellence by means of cross-border and cross-sector mobility)
 Code Call H2020-MSCA-IF-2015
 Funding Scheme MSCA-IF-EF-RI
 Starting year 2016
 Duration (year-month-day) from 2016-11-01   to  2018-10-31

 Partnership

Take a look of project's partnership.

# participants  country  role  EC contrib. [€] 
1    THE CHANCELLOR MASTERS AND SCHOLARSOF THE UNIVERSITY OF CAMBRIDGE UK (CAMBRIDGE) coordinator 183˙454.00

Map

 Project objective

Geochemical and geophysical observations indicate that much of Earth’s mass was accreted during large impacts between planetary embryos already differentiated into a metallic core and a silicate mantle. These collisions played a crucial role in setting the stage for Earth evolution, including the initiation of plate tectonics, the generation of Earth’s magnetic field, and the development of life. Each impact delivered prodigious amounts of energy, melting the projectile and the protoplanet's mantle, and creating an environment where the metallic liquid core of the projectile was released within a molten silicate magma ocean. The fate of the projectile’s core following impact affected the efficiency of chemical equilibration between metal and silicates, and therefore the geochemistry of Earth’s deep interior. Recent studies have provided clues on the physical processes involved, however, major questions remain. For instance, does the projectile’s core remain coherent or does it fragment into drops during the impact ?

This project includes the first analog fluid mechanics experiments on large impacts that formed the Earth, and combines them with numerical simulations and theory. Complementary to simulations, experiments can produce turbulence, as expected during Earth accretion. Regime diagrams and scaling laws on turbulent mixing obtained from these experiments and simulations will provide key constraints to interpret geochemical observations in terms of accretion time scales and processes. Bridging gaps between fluid mechanics, geodynamics, impact cratering and geochemistry, this project is expected to bring fundamental progress in our understanding of the origin of the Earth, planets, and exoplanets. The researcher’s expertise in Earth accretion and in lab experiments, acquired in the USA, will be reinvested in Europe through this project. Because the work is in fluid mechanics, the host organisation is the ideal place for this project.

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

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