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ECOGAL SIGNED

Understanding our Galactic ecosystem: From the disk of the Milky Way to the formation sites of stars and planets

Total Cost €

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EC-Contrib. €

0

Partnership

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 ECOGAL project word cloud

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

unifying    single    constituents    exploring    template    varying    combination    galaxy    ultimately    parts    milky    witness    observational    synergy    observations    governed    stars    diffuse    star    gas    paradigm    cradles    distant    equilibrium    permeates    galactic    dynamical    regulate    trace    born    found    hierarchy    theoretical    creates    magnetic    govern    calibrated    radiation    back    medium    cascade    wavelengths    agents    ecogal    evolution    environment    isolation    astronomy    environments    interstellar    disks    limits    influence    interplay    clear    modeling    reservoir    entire    gravity    progress    clouds    dramatically    transformative    universe    astrophysics    model    stellar    instrument    scales    link    treat    unites    predictive    ism    dust    shift    life    loops    planets    goals    primary    forefront    turbulence    disk    astroinformatics    birth    physical    forming    groups    competing    feedback    ecosystem    planet    planetary    numerical    linear    coexist    protoplanetary   

Project "ECOGAL" data sheet

The following table provides information about the project.

Coordinator
COMMISSARIAT A L ENERGIE ATOMIQUE ET AUX ENERGIES ALTERNATIVES 

Organization address
address: RUE LEBLANC 25
city: PARIS 15
postcode: 75015
website: www.cea.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 12˙659˙177 €
 EC max contribution 12˙659˙177 € (100%)
 Programme 1. H2020-EU.1.1. (EXCELLENT SCIENCE - European Research Council (ERC))
 Code Call ERC-2019-SyG
 Funding Scheme ERC-SyG
 Starting year 2020
 Duration (year-month-day) from 2020-05-01   to  2026-04-30

 Partnership

Take a look of project's partnership.

# participants  country  role  EC contrib. [€] 
1    COMMISSARIAT A L ENERGIE ATOMIQUE ET AUX ENERGIES ALTERNATIVES FR (PARIS 15) coordinator 3˙272˙637.00
2    EUROPEAN SOUTHERN OBSERVATORY - ESO EUROPEAN ORGANISATION FOR ASTRONOMICAL RESEARCH IN THE SOUTHERN HEMISPHERE DE (GARCHING) participant 3˙542˙965.00
3    RUPRECHT-KARLS-UNIVERSITAET HEIDELBERG DE (HEIDELBERG) participant 2˙718˙498.00
4    ISTITUTO NAZIONALE DI ASTROFISICA IT (ROMA) participant 2˙474˙451.00
5    CENTRE NATIONAL DE LA RECHERCHE SCIENTIFIQUE CNRS FR (PARIS) participant 362˙500.00
6    THE UNIVERSITY OF MANCHESTER UK (MANCHESTER) participant 288˙125.00

Map

 Project objective

Stars and planets are born from a large reservoir of diffuse gas and dust that permeates the Galaxy, the interstellar medium (ISM). The process is governed by the complex interplay of often competing physical agents such as gravity, turbulence, magnetic fields, and radiation. The system is organized in a hierarchy of scales, that link the disk of the Milky Way, to star-forming clouds, and eventually to protoplanetary disks, the cradles of planetary systems. Stellar feedback creates highly non-linear feedback loops that strongly influence the dynamical evolution across the entire cascade of scales. We witness a paradigm shift in galactic astronomy and astrophysics. Approaches that treat the constituents of the Galaxy in equilibrium and consider the various scales in isolation reach clear limits. A comprehensive understanding of our Milky Way requires us to consider the Galaxy as one single complex ecosystem, where dramatically different environments coexist and where varying conditions are found for star and planet formation, and ultimately for life. Exploring and understanding the Galactic ecosystem as well as the physical processes that govern its evolution define the research activities of ECOGAL. Our primary goal is to build a unifying predictive model of star and planet formation in the Milky Way. Based on a unique combination of theoretical modeling and multi-wavelengths observations, we will trace the properties of planet-forming disks back to their environment in different parts of the Galaxy, determine the physical processes that regulate the birth to stars and determine their key parameters, deliver a well calibrated galaxy template which can be used to study systems in the distant Universe. To reach these goals, ECOGAL unites four key research groups in Europe at the forefront in observational astronomy, numerical astrophysics, instrument development, and astroinformatics, whose synergy enables transformative progress in our understanding of our Galaxy.

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

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