Magma ocean evolution of the TRAPPIST-1 planets
Recent observations of the potentially habitable planets TRAPPIST-1 e, f, and g suggest that
they possess large water mass fractions of possibly several tens of weight percent of water …
they possess large water mass fractions of possibly several tens of weight percent of water …
Machine-learning inference of the interior structure of low-mass exoplanets
We explore the application of machine-learning based on mixture density neural networks
(MDNs) to the interior characterization of low-mass exoplanets up to 25 Earth masses …
(MDNs) to the interior characterization of low-mass exoplanets up to 25 Earth masses …
Water content of rocky exoplanets in the habitable zone
In this study we investigated the interiors of rocky exoplanets in order to identify those that
may have large quantities of water. We modelled the interiors of 28 rocky exoplanets …
may have large quantities of water. We modelled the interiors of 28 rocky exoplanets …
Tidal dissipation in dual-body, highly eccentric, and nonsynchronously rotating systems: Applications to Pluto–Charon and the exoplanet TRAPPIST-1e
JP Renaud, WG Henning, P Saxena… - The Planetary …, 2021 - iopscience.iop.org
Abstract Using the Andrade-derived Sundberg–Cooper rheology, we apply several
improvements to the secular tidal evolution of TRAPPIST-1e and the early history of Pluto …
improvements to the secular tidal evolution of TRAPPIST-1e and the early history of Pluto …
Solid tides in Io's partially molten interior-Contribution of bulk dissipation
Context. Io's spectacular activity is driven by tidal dissipation within its interior, which may
undergo a large amount of melting. While tidal dissipation models of planetary interiors …
undergo a large amount of melting. While tidal dissipation models of planetary interiors …