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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 €

0

EC-Contrib. €

0

Partnership

0

Views

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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.

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

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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