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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.

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

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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