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

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 elemental compositions of planet-hosting stars serve as proxies for the primordial
compositions of protoplanetary disks within which the planets form. The temperature profile …

The radial-dependent positions of snowlines of abundant oxygen-and carbon-bearing
molecules in protoplanetary discs will result in systematic radial variations in the carbon-to …

Inside-out planet formation (IOPF) proposes that the abundant systems of close-in Super-
Earths and Mini-Neptunes form in situ at the pressure maximum associated with the dead …

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 …

The chemical composition of planetary atmospheres has long been thought to store
information regarding where and when a planet accretes its material. Predicting this …

To understand the role that planet formation history has on the observable atmospheric
carbon-to-oxygen ratio (C/O) we have produced a population of astrochemically evolving …

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 …

Context. The atmospheres of extrasolar planets are thought to be built largely through
accretion of pebbles and planetesimals. Such pebbles are also the building blocks of …