Computational Recreation of Carbon Dioxide Hydrates at Habitable Planetary Conditions

Gas clathrate hydrates are proposed as constituents of the icy moons of the giant planets in the Solar System [1]. Carbon dioxide has been detected on the surface of the moons of Jupiter, supposedly originated by internal degasification. In Ganymede, an aqueous ocean is proposed to exist under a thick ice crust in coexistence with several forms of ice, with pressure reaching up to 1.3 GPa [2]. Due to the limited available data on these systems under these conditions, we propose a combination of computational and experimental studies to describe microscopically and macroscopically the structural and chemical behavior of CO2@H2O polymorphs. This will allow us to understand how their presence affects the geophysical structure and activity and their impact on the habitability of the icy moon. A transition from the sI cubic structure to a high pressure phase at around 0.7 GPa has been found for CO2@H2O. In spite of different attempts to characterize the new structure, a definite answer has not been provided yet. A MH-III Filled Ice Structure type was proposed after neutron diffraction experiments in contrast with an alternative structure similar to the hexagonal C0 type for H2 hydrates [3]. It has an estimated hydration level ratio up to 2H2O:1CO2 and 6 water molecules per unit cell. In the figure below, our optimized unit cell based on this hexagonal C0 structure is displayed. Ab initio calculations using the XDM approximation to include van der Waals effects are performed in our search for the pressure evolution of the equilibrium geometries of the C0-CO2@H2O phase and those of a close related structure to this one called Ih-C0, with 8 water molecules per unit cell. We obtain occupation energies at different hydration ratios, densities, equations of state parameters, and stability energies with respect to decomposition. Raman and IR frequencies are also computed in the 0-2 GPa range. High pressure experiments are also being done in a newly designed chamber able to reach 1 GPa. It is equipped with a sapphire window to allow the measurements of Raman spectra. We believe that these results may throw light into gas hydrates of the habitable bodies of our Solar System. [1] Buffet B. A., Ann. Rev. Earth Plan. Sci. 28, 477, 2010. [2] Bland, M.T. et al. Icarus 200, 207, 2009. [3] Smirnov G. S. et al., J. Phys. Chem. Lett., 2013, 4, 3560