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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

0

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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.

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

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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