Introduction and BackgroundCarbon dioxide clathrate hydrate (CO 2 •nH 2 O) and methane clathrate hydrate (CH 4 •nH 2 O), both with n ≥ 5.75, are ice-like crystalline substances with hydrogen-bonded water molecules that form polyhedral cage-like structures stabilized by "guest" molecules of appropriate size. CO 2 hydrate and CH 4 hydrate are stable over a wide range of elevated pressure and low temperature conditions relevant to both terrestrial and planetary conditions (e.g., Sloan & Koh, 2007, and references therein); on Earth, natural gas hydrate-most commonly methane hydrate-forms in continental shelves below roughly 500 m depth, given sufficient gas availability, as well as in Arctic permafrost environments below ∼200 m (Ruppel & Kessler, 2017, and references therein).Pure CO 2 hydrate and CH 4 hydrate typically form as cubic structure I (sI), space group Pm3n, with a unit cell composed of 46 water molecules forming two small (pentagonal dodecahedral, 5 12 ) and six large (tetrakaidekahedral, 5 12 6 2 ) cavities. Formation, structural properties, and crystallographic characteristics of laboratory-formed CO 2 hydrate have been investigated by a variety of diffraction and spectroscopic methods (