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SPIDI SIGNED

Star-Planet-Inner Disk Interactions (SPIDI): unveiling the formation and evolution of inner planetary systems

Total Cost €

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EC-Contrib. €

0

Partnership

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 SPIDI project word cloud

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

quite    with    structures    young    signposts    candidates    ranging    powerful    earth    evolution    synthetic    govern    physical    arms    exhibit    nearly    dynamical    additional    presumably    devise    discovered    imaging    diverse    alma    probe    combined    yield    stellar    protoplanetary    planetary    signatures    spectroscopy    gt    spidi    galaxy    au    photometry    sphere    accretion    star    detect    spectacular    days    time    nascent    exoplanets    disk    simultaneous    observational    accepted    date    clues    astronomical    lt    vast    differs    indirectly    scales    ubiquity    confirmed    interferometry    gaps    spectropolarimetry    close    majority    planet    form    orbit    rings    domain    planets    migrate    surface    solar    inner    stars    models    interactions    images    origin    issue    techniques    parent    circumstellar    jupiter    distance    hosts    observations    vlt    period    larger    orbital    unable    region    edge    revolves    predict    released    disks    view    spiral    generally   

Project "SPIDI" data sheet

The following table provides information about the project.

Coordinator
CENTRE NATIONAL DE LA RECHERCHE SCIENTIFIQUE CNRS 

Organization address
address: RUE MICHEL ANGE 3
city: PARIS
postcode: 75794
website: www.cnrs.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]
 Project website http://www.spidi-eu.org
 Total cost 2˙362˙230 €
 EC max contribution 2˙362˙230 € (100%)
 Programme 1. H2020-EU.1.1. (EXCELLENT SCIENCE - European Research Council (ERC))
 Code Call ERC-2016-ADG
 Funding Scheme ERC-ADG
 Starting year 2018
 Duration (year-month-day) from 2018-01-01   to  2022-12-31

 Partnership

Take a look of project's partnership.

# participants  country  role  EC contrib. [€] 
1    CENTRE NATIONAL DE LA RECHERCHE SCIENTIFIQUE CNRS FR (PARIS) coordinator 2˙362˙230.00

Map

 Project objective

With more than 2,000 confirmed exoplanets discovered to date, and about 4,000 additional candidates, it is now widely accepted that nearly every star in the Galaxy hosts a planetary system. These systems greatly differs from our Solar System: a vast majority of exoplanets revolves at a distance less than the Earth’s orbit (1 astronomical unit, 1 AU), and many orbit very close to their parent star indeed (<0.1 AU). These inner planets, with an orbital period less than 100 days, are quite diverse, ranging from Earth-like to Jupiter-like. How do they form or migrate close their star is still an open issue. ALMA and VLT/SPHERE recently released spectacular images of circumstellar disks around young stars, which exhibit large-scale structures (>10 AU), including rings, gaps, and spiral arms that presumably are the signposts of planet formation. Yet, as powerful as they are, imaging techniques are yet unable to probe the inner disk region. The goal of the SPIDI project is to investigate the origin and evolution of inner planetary systems. Specifically, we will develop dynamical models of inner planets embedded in the accretion disk of young stars to investigate the physical processes that govern the star-disk-planet interactions from 1 AU down to the stellar surface. From these models, we will then predict the observational signatures of disk-embedded inner planetary systems, and devise and implement observations that will allow us to detect them. This can only be done indirectly through simultaneous time domain photometry, spectroscopy, spectropolarimetry, and interferometry. Combined with current results obtained on larger scales, the SPIDI project will thus yield a synthetic view of nascent planetary systems, down to the inner edge of protoplanetary disks. It will bring clues to the origin of our own inner Solar System, and more generally, address the formation process and ubiquity of inner planetary systems throughout the Galaxy.

 Publications

year authors and title journal last update
List of publications.
2019 N. Roggero
Wavelet Analysis of Taurus K2 Dipper Light Curves
published pages: , ISSN: , DOI:
Ewass kuoni-congress 2019-09-05
2018 S. H. P. Alencar, J. Bouvier, J.-F. Donati, E. Alecian, C. P. Folsom, K. Grankin, G. A. J. Hussain, C. Hill, A.-M. Cody, A. Carmona, C. Dougados, S. G. Gregory, G. Herczeg, F. Ménard, C. Moutou, L. Malo, M. Takami
Inner disk structure of the classical T Tauri star LkCa 15
published pages: A195, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201834263
Astronomy & Astrophysics 620 2019-09-05
2018 J. Bouvier
Take a closer look at... the SPIDI project
published pages: , ISSN: , DOI: 10.5281/zenodo.1488890
Zenodo November 15, 2018 2019-09-05
2018 B. Tessore, J. Bouvier, C. Pinte, F. Menard
Formation of strong emission lines in stellar accretion disks: The link between observations and models, Radiative signatures from the cosmos
published pages: , ISSN: , DOI:
2019-09-05
2019 G. Pantolmos, C. Zanni, J. Bouvier
Effects of the stellar-wind geometry on the stellar angular momentum loss, European Week of Astronomy & Space Science (EWASS)
published pages: , ISSN: , DOI:
Ewass kuoni-congress 2019-09-05
2018 F. Gallet, E. Bolmont, J. Bouvier, S. Mathis, C. Charbonnel
Planetary tidal interactions and the rotational evolution of low-mass stars
published pages: A80, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201833576
Astronomy & Astrophysics 619 2019-09-05
2019 G. Pantolmos, C. Zanni, J. Bouvier
Stellar wind torques during the T-Tauri phase of stars
published pages: , ISSN: , DOI:
Ewass kuoni-congress 2019-09-05
2018 J-F Donati, J Bouvier, S H Alencar, C Hill, A Carmona, C P Folsom, F Ménard, S G Gregory, G A Hussain, K Grankin, C Moutou, L Malo, M Takami, G J Herczeg
The magnetic propeller accretion regime of LkCa 15
published pages: L1-L5, ISSN: 1745-3933, DOI: 10.1093/mnrasl/sly207
Monthly Notices of the Royal Astronomical Society: Letters 483/1 2019-09-05
2018 P. Pinilla, M. Benisty, J. de Boer, C. F. Manara, J. Bouvier, C. Dominik, C. Ginski, R. A. Loomis, A. Sicilia Aguilar
Variable Outer Disk Shadowing around the Dipper Star RXJ1604.3–2130
published pages: 85, ISSN: 1538-4357, DOI: 10.3847/1538-4357/aae824
The Astrophysical Journal 868/2 2019-09-05
2019 F. Gallet, P. Delorme
Star-planet tidal interaction and the limits of gyrochronology
published pages: A120, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201834898
Astronomy & Astrophysics 626 2019-09-05
2018 B. Tessore, J. Bouvier, C. Pinte, F. Menard
Non-LTE atomic line formation in accretion disk around young stars
published pages: , ISSN: , DOI: 10.5281/zenodo.1488996
Zenodo 2019-09-05

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