Opendata, web and dolomites

FETA

Fluid impacts in EarTh Accretion

Total Cost €

0

EC-Contrib. €

0

Partnership

0

Views

0

 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.

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

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.

Are you the coordinator (or a participant) of this project? Plaese send me more information about the "FETA" project.

For instance: the website url (it has not provided by EU-opendata yet), the logo, a more detailed description of the project (in plain text as a rtf file or a word file), some pictures (as picture files, not embedded into any word file), twitter account, linkedin page, etc.

Send me an  email (fabio@fabiodisconzi.com) and I put them in your project's page as son as possible.

Thanks. And then put a link of this page into your project's website.

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

More projects from the same programme (H2020-EU.1.3.2.)

EngPTC2 (2019)

Exploring new technologies for the next generation pulse tube cryocooler below 2K

Read More  

NSTree (2020)

Understanding substrate delivery for cell wall biosynthesis in plants

Read More  

MemoryAggregates (2020)

Mechanism of Whi3 Aggregation and its Age-dependent Malfunction

Read More