Abstract
Molecular-level Monte Carlo simulations are performed to validate equation of state approaches for the description of the N2/CH4/C2H6 vapour–liquid equilibria under conditions relevant to Titan’s lower atmosphere. The Monte Carlo simulations confirm the validity of the equation of state approaches, so that both provide a reliable description of the unknown composition of cloud droplets in this region of Titan’s atmosphere. Furthermore, the models are compared with experimental data from laboratory studies of aerosol droplets that contain N2, CH4 and C2H6. Good agreement is also found here.
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