Fabian Lukas Seidler
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View article: Detectability of oxygen fugacity regimes in the magma ocean world 55 Cancri e at high spectral resolution
Detectability of oxygen fugacity regimes in the magma ocean world 55 Cancri e at high spectral resolution Open
Ultra-short-period exoplanets such as 55 Cancri e (55 Cnc e), hosting dayside magma oceans, present unique opportunities to study surface-atmosphere interactions. The composition of a vaporized mineral atmosphere enveloping the dayside is …
View article: Detectability of oxygen fugacity regimes in the magma ocean world 55 Cancri e at high spectral resolution
Detectability of oxygen fugacity regimes in the magma ocean world 55 Cancri e at high spectral resolution Open
Ultra-short Period exoplanets (USPs) like 55 Cnc e, hosting dayside magma oceans, present unique opportunities to study surface-atmosphere interactions. The composition of a vaporised mineral atmosphere enveloping the dayside is dictated b…
View article: Impact of oxygen fugacity on the atmospheric structure and emission spectra of ultra-hot rocky exoplanets
Impact of oxygen fugacity on the atmospheric structure and emission spectra of ultra-hot rocky exoplanets Open
Context. Atmospheres above lava-ocean planets (LOPs) hold clues related to the properties of their interiors, based on the expectation that the two reservoirs are in chemical equilibrium. Furthermore, such atmospheres are observable with c…
View article: Impact of oxygen fugacity on atmospheric structure and emission spectra of ultra hot rocky exoplanets
Impact of oxygen fugacity on atmospheric structure and emission spectra of ultra hot rocky exoplanets Open
Atmospheres above lava-ocean planets (LOPs) hold clues as to the properties of their interiors, owing to the expectation that the two reservoirs are in chemical equilibrium. Here we consider `mineral' atmospheres produced in equilibrium wi…
View article: Detailed chemical compositions of planet-hosting stars: II. Exploration of the interiors of terrestrial-type exoplanets
Detailed chemical compositions of planet-hosting stars: II. Exploration of the interiors of terrestrial-type exoplanets Open
A major goal in the discovery and characterisation of exoplanets is to identify terrestrial-type worlds that are similar to (or otherwise distinct from) our Earth. Recent results have highlighted the importance of applying devolatilisation…
View article: A python package for fast interior modelling of terrestrial (exo-)planets using a Gibbs free energy minimization
A python package for fast interior modelling of terrestrial (exo-)planets using a Gibbs free energy minimization Open
<p>With increasing capabilities of characterizing small rocky exoplanets beyond our solar system, the question of their chemistry, geology and interior structure arises. Accompanied by observational facilities capabale of giving a de…
View article: A Model Earth-sized Planet in the Habitable Zone of α Centauri A/B
A Model Earth-sized Planet in the Habitable Zone of α Centauri A/B Open
The bulk chemical composition and interior structure of rocky exoplanets are fundamentally important to understand their long-term evolution and potential habitability. Observations of the chemical compositions of solar system rocky bodies…