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From atmospheric to exoplanet formation retrievals
With new and upcoming observing facilities (JWST and the ELTs), the exoplanet community is poised to precisely measure the chemical inventory of exoplanet atmospheres. This will allow, for the first time, to start investigating whether one of the greatest promises of atmospheric characterization studies holds up: inverting the atmospheric composition ...Paul Mollière +12 more
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Cosmic Collisions Yield Clues about Exoplanet Formation
Scientific American, 2022openaire +1 more source
Thermal Evolution and Crust Formation of Tidally-Locked Rocky Exoplanets
Many of the observed rocky exoplanets orbiting close to their host stars are likely tidally locked, with one hemisphere in permanent daylight and the other in complete darkness. Phase curve observations of GI-486b, TRAPPIST-1b and c, and LHS 3844b suggest that such planets may exhibit extreme temperature contrasts between their day and night sides ...Dilawaiz Saghir +2 more
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Exoplanets: detection, formation, properties, habitability
Choice Reviews Online, 2008openaire +1 more source
BSc thesis, Timescale of Ocean Formation on Rocky Exoplanets
Data from the 1D interior-atmosphere coupled evolution framework PROTEUS: evolution of Earth-like exoplanets in the Solar system and data and plots derived from PROTEUS data concerning the timescale and composition of oceans on these ...openaire +1 more source
Connecting the Observed Properties of Exoplanet Populations to Their Formation
2020The wealth of exoplanetary data as displayed on the mass-semimajor axis and mass-radius distributions reveal a tremendous amount of information constraining our understanding of their formation. We link the variety of outcomes shown in exoplanet populations to the observed ranges of protoplanetary disk properties using the core accretion model of ...
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Formation and Evolution of Exoplanets, edited by Rory Barnes
Contemporary Physics, 2012openaire +1 more source
Lowlid formation and plate tectonics on exoplanets
Stamenkovic, Vlada +2 moreopenaire +1 more source

