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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.

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

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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