We discuss the chemical pre-conditions for planet formation, in terms of gas and ice
abundances in a protoplanetary disk, as function of time and position, and the resulting …

Giant planets can interact with multiple and chemically diverse environments in
protoplanetary disks while they form and migrate to their final orbits. The way this interaction …

We present the next step in a series of papers devoted to connecting the composition of the
atmospheres of forming planets with the chemistry of their natal evolving protoplanetary …

The composition of planets is largely determined by the chemical and dynamical evolution of
the disk during planetesimal formation and growth. To predict the diversity of exoplanet …

We present a model of the early chemical composition and elemental abundances of
planetary atmospheres based on the cumulative gaseous chemical species that are …

Agreement about planetary formation processes deteriorates sharply with distance from the
Sun. While the terrestrial planets are widely believed to have formed from the collisional …

Context. The composition of exoplanet atmospheres provides us with vital insight into their
formation scenario. Conversely, planet formation processes shape the composition of …

Recently, gas disks have been discovered around main-sequence stars well beyond the
usual protoplanetary disk lifetimes (that is,≳ 10 Myr), when planets have already formed …

The compositions of nascent planets depend on the compositions of their birth disks. In
particular, the elemental compositions of gas giant gaseous envelopes depend on the …

Context. Exoplanet atmospheres are thought be built up from accretion of gas as well as
pebbles and planetesimals in the midplanes of planet-forming disks. The chemical …