HiRISE | High-Resolution Imaging and Spectroscopy of Exoplanets

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 (R

Status

CLOSED

Call topic

ERC-2017-STG

Update Date

27-04-2024
Images
No images available.
Geographical location(s)
Structured mapping
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Horizon 2020
H2020-EU.1. EXCELLENT SCIENCE
H2020-EU.1.1. EXCELLENT SCIENCE - European Research Council (ERC)
ERC-2017
ERC-2017-STG