Abstract
Carbon monoxide occurs in abundance throughout the cosmos, potentially in clathrate form, whereas on Earth, it forms a notable constituent of industrial flue gases. It has been proposed that hydrate technology could be used in CO2 separation from flue gases, and in subsea flue gas CO2 disposal. This - and the likely widespread occurrence of CO clathrates in the cosmos - means it is important that the phase behavior of CO hydrates is known. Here, we present experimental H-L-V (hydrate-liquid-vapor) equilibrium data for CO, CO-CO2, and CO-C3H8 (propane) clathrate hydrates. Data were generated by a reliable step-heating technique validated using measured data for CO2 and CH4 hydrates. Data for CO and CO-C3H8 clathrates have been used in the optimization of Kihara potential parameters for CO, reported here, facilitating the extension of a thermodynamic model to the prediction of CO hydrate equilibria. Model predictions are validated against independent experimental data for CO-CO 2 (structure I) systems, with good agreement being observed. © 2005 American Institute of Chemical Engineers'.
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Mohammadi, A. H., Anderson, R., & Tohidi, B. (2005). Carbon monoxide clathrate hydrates: Equilibrium data and thermodynamic modeling. AIChE Journal, 51(10), 2825–2833. https://doi.org/10.1002/aic.10526
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