JANAF Thermochemical Table

TL;DR: In this article, a detailed study of the production of melt and vapor in planetary impact events is carried out with hydrocode simulations, where Sandia's two-dimensional axisymmetric hydrocode CSQ was used to estimate the amount of melting and vapor produced for widely varying initial conditions: 10 to 80 km/sec for impact velocity, 0.2 to 10 km for the projectile radius.

TL;DR: The chemical species containing carbon, nitrogen, and oxygen in the atmospheres of giant planets, brown dwarfs (T and L dwarfs), and low-mass stars (M dwarfs) are identified as part of a comprehensive set of thermochemical equilibrium and kinetic calculations for all elements as discussed by the authors.

TL;DR: Active Thermochemical Tables (ATcT) as discussed by the authors is a new paradigm of how to obtain accurate, reliable, and internally consistent thermochemistry and overcome the limitations that are intrinsic to the traditional sequential approach to thermochemistry.

TL;DR: In this paper, a rigorous and computationally efficient thermodynamic model that estimates the state and composition of atmospheric inorganic species between the gas and aerosol phases is presented, and the estimation of important thermodynamic properties, equilibrium constants, ionic activity coefficients, water activity, and deliquescence points is described.