The CHONS elements that constitute the outgassed atmosphere and exosphere have likely
been delivered by chondritic materials to the Earth during planetary accretion and …

Since the first discovery of planets in another solar system of our galaxy in the early 90s and
the discovery of 51 Pegassi b, a Jovian-type planet around a Sun-like star in 1995 (Mayor …

Earth's core is likely the largest reservoir of carbon (C) in the planet, but its C abundance has
been poorly constrained because measurements of carbon's preference for core versus …

Massive steam and CO 2 atmospheres have been proposed for magma ocean outgassing of
Earth and terrestrial planets. Yet formation of such atmospheres depends on volatile …

Extracting atmospheric moisture for freshwater production is an appealing way to mitigate
the global water crisis. However, the low moisture sorption capacity and high desorption …

Atmospheres are products of time-integrated mass exchange between the surface of a
planet and its interior. On Earth and other planetary bodies, magma oceans likely marked …

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 …

Volatiles are important for planetary geodynamics, climate, and habitability. The C/N ratio of
the bulk silicate Earth (BSE) is superchondritic, which provides a useful tool for …

The composition of atmospheres and the resulting potential for planetary habitability in the
rocky bodies of our Solar System and beyond is strongly controlled by the volatile exchange …

Abstract Knowledge of N solubility in silicate melts is key for understanding the origin of
terrestrial N and the distribution and exchanges of N between the atmosphere, the silicate …