Mineral Cloud Formation above Magma Oceans in Sub-Neptune Atmospheres
The potential presence of a magma surface below a thick atmosphere primarily composed of hydrogen in some sub-Neptune exoplanets suggests a strong link between the interior composition and atmosphere through chemical coupling of volatile and refractory ...
Elspeth K. H. Lee +2 more
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THE IMPACT OF NON-UNIFORM THERMAL STRUCTURE ON THE INTERPRETATION OF EXOPLANET EMISSION SPECTRA [PDF]
Y. Katherina Feng +6 more
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Increasingly precise space-based photometry uncovers higher-order effects in transits, eclipses, and phase curves that can be used to characterize exoplanets in novel ways.
Shashank Dholakia +2 more
doaj +1 more source
Machine-learning Inferences of the Interior Structure of Rocky Exoplanets from Bulk Observational Constraints [PDF]
Yong Zhao, Dongdong Ni, Zibo Liu
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Temperature Structures Associated with Different Components of the Atmospheric Circulation on Tidally Locked Exoplanets [PDF]
Neil T. Lewis, Mark Hammond
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Structure and evolution of super-Earth to super-Jupiter exoplanets [PDF]
I. Baraffe, G. Chabrier, Travis Barman
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Fundamentals of Interior Modelling and Challenges in the Interpretation of Observed Rocky Exoplanets. [PDF]
Baumeister P +9 more
europepmc +1 more source
Impact of oxygen fugacity on atmospheric structure and emission spectra of ultra hot rocky exoplanets [PDF]
Fabian L. Seidler +2 more
openalex +1 more source
Exo-Geoscience Perspectives Beyond Habitability. [PDF]
Spohn T +7 more
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