One of the best-known uses of methanol is as antifreeze. Methanol is used in large quantities in industrial applications to prevent methane clathrate hydrate blockages from forming in oil and gas pipelines. Methanol is also assigned a major role as antifreeze in giving icy planetary bodies (e.g., Titan) a liquid subsurface ocean and/or an atmosphere containing significant quantities of methane. In this work, we reveal a previously unverified role for methanol as a guest in clathrate hydrate cages. X-ray diffraction (XRD) and NMR experiments showed that at temperatures near 273 K, methanol is incorporated in the hydrate lattice along with other guest molecules. The amount of included methanol depends on the preparative method used. For instance, single-crystal XRD shows that at low temperatures, the methanol molecules are hydrogen-bonded in 4.4% of the small cages of tetrahydrofuran cubic structure II hydrate. At higher temperatures, NMR spectroscopy reveals a number of methanol species incorporated in hydrocarbon hydrate lattices. At temperatures characteristic of icy planetary bodies, vapor deposits of methanol, water, and methane or xenon show that the presence of methanol accelerates hydrate formation on annealing and that there is unusually complex phase behavior as revealed by powder XRD and NMR spectroscopy. The presence of cubic structure I hydrate was confirmed and a unique hydrate phase was postulated to account for the data. Molecular dynamics calculations confirmed the possibility of methanol incorporation into the hydrate lattice and show that methanol can favorably replace a number of methane guests.flow assurance | outer planets | X-ray crystallography | NMR spectra | molecular dynamics simulation M ethanol is the quintessential antifreeze. It works by altering thermodynamic conditions of aqueous solution to suppress or delay the formation of icy phases when the temperature is reduced to below the normal freezing point of water. The action in aqueous solution is readily understood by considering strong hydrogen-bonding interactions between water and methanol that lower the chemical potential of the aqueous phase, leading to strongly nonideal solution behavior (1). The low-temperature phase diagram of water-methanol is well known (2), with a single solid 1:1 methanol hydrate compound identified (3) in addition to the pure solid phases. The eutectic in the water-methanol system occurs at rather low temperatures (between 155 and 160 K), which has led to speculations that liquid aqueous oceans may exist on icy planetary bodies, such as Titan and Enceladus (2-5). For the formation of clathrate hydrates, which are ice-like host lattices composed of water molecules so as to form cages that encapsulate guest molecules, the behavior of methanol as an antifreeze has always been assumed to parallel that in watermethanol solutions. Even after some 70 y of applied research of hydrate inhibition by methanol as part of gas-pipeline flow assurance programs in the oil and gas industry (6) and, more recently, applie...