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ICED SIGNED

Initial conditions of exoplanet formation in protoplanetary disks

Total Cost €

0

EC-Contrib. €

0

Partnership

0

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 ICED project word cloud

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

group    composition    numerical    spectroscopy    predicted    radii    planets    career    astronomy    wavelength    marketability    accomplished    exoplanets    training    located    interpreting    gaseous    physics    1au    formed    natal    atmospheric    atomic    phases    time    disks    grains    connections    situ    molecular    goals    disk    stellar    host    network    stars    infrared    solid    central    condensation    jwst    discovery    building    observing    compositions    atmosphere    gradients    planetary    techniques    orbital    form    migrated    sublimation    visibility    characterization    international    courses    confirm    skills    pure    senior    grain    turn    sufficient    masses    map    dust    positions    material    core    planet    location    flux    determined    moving    there    models    ing    radiative    function    dependent    thermal    gas    blocks    synthesis    transfer    multiple    bulk    accreted    farther    spectral    substantial    chemical    clear    scenarios    exoplanetary    massive    population    physical    exoplanet   

Project "ICED" data sheet

The following table provides information about the project.

Coordinator
UNIVERSITEIT VAN AMSTERDAM 

Organization address
address: SPUI 21
city: AMSTERDAM
postcode: 1012WX
website: www.uva.nl

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 Netherlands [NL]
 Total cost 177˙598 €
 EC max contribution 177˙598 € (100%)
 Programme 1. H2020-EU.1.3.2. (Nurturing excellence by means of cross-border and cross-sector mobility)
 Code Call H2020-MSCA-IF-2016
 Funding Scheme MSCA-IF-EF-ST
 Starting year 2017
 Duration (year-month-day) from 2017-10-01   to  2019-09-30

 Partnership

Take a look of project's partnership.

# participants  country  role  EC contrib. [€] 
1    UNIVERSITEIT VAN AMSTERDAM NL (AMSTERDAM) coordinator 177˙598.00

Map

 Project objective

There is now a substantial population of exoplanets with well-determined masses, radii, and orbital parameters in a range of host stellar systems. JWST will bring an increase in exoplanets with atmospheric spectroscopy measurements, moving the field from pure discovery to population synthesis and characterization. Many of the best-studied planetary systems are massive and located within 1AU of their central stars; it is not clear whether all of these planets migrated from farther out in their natal disks to this location or if they could have formed in situ. Both scenarios should produce distinct compositions resulting from multiple strong, time-dependent chemical gradients in their disks due to thermal sublimation and grain processing effects. These effects likely set the bulk chemical composition of the planet’s core and atmosphere, which are accreted from different material in the disk. By determining the physical conditions within 1AU, I will confirm whether they are sufficient to support in situ planet formation. I will also map the distribution of key planetary building blocks in both the solid phase (dust grains) and gas phase. This will be accomplished by interpreting disks’ flux as a function of wavelength with radiative transfer models including detailed sublimation and condensation physics, and comparing observed spectral features in both the solid and gaseous phases in molecular and atomic form to those predicted by models. This project will provide training through research in numerical methods and exoplanet characterization techniques, which are important in the long term for my career goals to lead a research group in planetary formation. Through development courses, I will improve my marketability for senior research positions and in turn transfer my infrared observing skills and US and European network connections to the host. This project increases the visibility of the host and European exoplanetary astronomy on an international scale.

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

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