Modeling Binary Mixtures of Water + Light Hydrocarbon Using the Perturbed-Chain Statistical Associating Fluid Theory with Induced Association: Improvement in Describing All Equilibrium Phases

Author:

Tan Sugata P.1ORCID,Kargel Jeffrey S.1,Vance Steven D.2,Lopes Rosaly M.2

Affiliation:

1. Planetary Science Institute, Tucson, Arizona 85719, United States

2. Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California 91109, United States

Funder

NASA Astrobiology Institute

Publisher

American Chemical Society (ACS)

Subject

Space and Planetary Science,Atmospheric Science,Geochemistry and Petrology

Reference66 articles.

1. Vance, S.; Sotin, C.; Choukroun, M.; Mitchell, K. Titan’s subsurface alkanology. Proceedings of the 43rd Lunar and Planetary Science Conference; The Woodlands, TX, March 19–23, 2012; Abstract 2939.

2. Contributions from Accreted Organics to Titan’s Atmosphere: New Insights from Cometary and Chondritic Data

3. Is Titan's shape caused by its meteorology and carbon cycle?

4. Corrigendum to “Revised solubility data and modeling of water in the gas phase of the methane/water binary system at temperatures from 283.08 to 318.12 K and pressures up to 34.5 MPa”

5. Hayduk, W. IUPAC Solubility Data Series; Pergamon Press: Oxford, U.K., 1982; Vol. 8: Ethane, p 16.

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