Physics
Scientific paper
Sep 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000georl..27.2929k&link_type=abstract
Geophysical Research Letters, Volume 27, Issue 18, p. 2929-2932
Physics
13
Hydrology: Frozen Ground, Mineral Physics: Surfaces And Interfaces, Planetology: Solid Surface Planets: Polar Regions, Planetology: Solar System Objects: Comets
Scientific paper
We present results of experimental studies on the formation of gas hydrates (clathrates) at conditions of geophysical interest. Clathrate hydrates formed by a reaction of gas at ice Ih surfaces are always found to be mesoporous to macroporous with pores sizes between 100 to 400 nm and pore volumes of approximately 25-40% for CH4, Ar and N2 hydrate, and smaller pores of 20 to 100 nm with a porosity of approximately 10-20% for CO2 hydrate. The three-dimensional sponge-like microstructure occurs in single crystalline grains of typically a few μm size and was observed by field-emission scanning electron microscopy. It forms over a wide range of p-T conditions below the ice Ih melting. The porous microstructure is stable for at least several months, even close to the clathrate decomposition, and is proposed to be formed by local differences in the energy balance between hydrate formation and ice decomposition. The results presented are considered of potential major importance for the understanding of the behavior of natural gas hydrates found e.g. in polar ice sheets and permafrost regions, and also in some celestial bodies.
Gotthardt Frank
Heinrichs Till
Klapproth Alice
Kuhs Werner F.
Techmer Kirsten
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