Summary
Atmospheric composition provides essential markers of the most fundamental properties of exoplanets, such as their formation mechanism or internal structure. New-generation exoplanet imagers have been designed to achieve high contrast for the detection of young giant planets in the near-infrared, but they only provide very low spectral resolutions (R
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More information & hyperlinks
Web resources: | https://cordis.europa.eu/project/id/757561 |
Start date: | 01-12-2017 |
End date: | 30-11-2023 |
Total budget - Public funding: | 1 496 730,00 Euro - 1 496 730,00 Euro |
Cordis data
Original description
Atmospheric composition provides essential markers of the most fundamental properties of exoplanets, such as their formation mechanism or internal structure. New-generation exoplanet imagers have been designed to achieve high contrast for the detection of young giant planets in the near-infrared, but they only provide very low spectral resolutions (RStatus
CLOSEDCall topic
ERC-2017-STGUpdate Date
27-04-2024
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