FastChem Cond: Equilibrium chemistry with condensation and rainout for cool planetary and stellar environments
Daniel Kitzmann, Joachim W. Stock, A. Beate C. Patzer

TL;DR
FastChem Cond is an advanced equilibrium chemistry code that models condensation and rainout in cool planetary and stellar environments, automatically selecting stable condensates and supporting open-source use with C++ and Python interfaces.
Contribution
It introduces a new version of FastChem that handles equilibrium condensation with automatic stable condensate selection and rainout approximation, expanding its capabilities for astrophysical applications.
Findings
Supports equilibrium condensation and rainout modeling.
Automatically determines stable condensates satisfying phase rule.
Includes approximately 290 new condensate species.
Abstract
Cool astrophysical objects, such as (exo)planets, brown dwarfs, or asymptotic giant branch stars, can be strongly affected by condensation. Condensation does not only directly affect the chemical composition of the gas phase by removing elements but the condensed material also influences other chemical and physical processes in these objects. This includes, for example, the formation of clouds in planetary atmospheres and brown dwarfs or the dust-driven winds of evolved stars. In this study we introduce FastChem Cond, a new version of the FastChem equilibrium chemistry code that adds a treatment of equilibrium condensation. Determining the equilibrium composition under the impact of condensation is complicated by the fact that the number of condensates that can exist in equilibrium with the gas phase is limited by a phase rule. However, this phase rule does not directly provide…
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Taxonomy
TopicsAtmospheric chemistry and aerosols · Astrophysics and Star Formation Studies · Atmospheric Ozone and Climate
