We demonstrate that the deep volatile storage capacity of magma oceans has significant
implications for the bulk composition, interior, and climate state inferred from exoplanet mass …

The geology of Earth and super‐Earth sized planets will, in many cases, only be observable
via their atmospheres. Here, we investigate secondary volcanic atmospheres as a key base …

Context. Stellar elemental abundances are generally used to constrain the interiors of rocky
exoplanets by assuming planet's relative abundances of major refractory elements (Fe, Mg …

Context. Earth-sized exoplanets have been discovered and characterized thanks to new
developments in observational techniques, particularly those planets that may have a rocky …

Exoplanets orbiting distant stars have revealed to us that no one could have predicted Earth.
Many stars host planets which appear to be made of rock and iron like Earth, but sit at …

The study of the atmospheric composition and evolution of rocky planet atmospheres is key
to understanding both the conditions required to develop a habitable planet, and to analyse …

During the last decade, a wealth of new large-scale surveys have come online across the
world. These huge spectral, astrometric and photometric surveys are providing astronomers …

K2-18 b is a super-earth exoplanet revolving around an M-dwarf star K2-18 in constellation
Leo. Here we have analysed the internal structure of exoplanet K2-18 b for mass and radius …

Earth remains our only reference point for an inhabited world. The field of astrobiology,
however, seeks to differentiate between the specific requirements for life on Earth (terran life; …