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The AAPG/Datapages Combined Publications Database
West Texas Geological Society
Abstract
Diverse Origins and
Facies
of
Carbonate
Microporosity
Abstract
Carbonate
microporosity has reached new significance with the modern focus on the exploration for natural gas reservoirs. Because microporosity does not permit good fluid flow, microporous
carbonate
facies
and diagenetic systems received limited study in the oil-focused exploration programs of the 20th century. However, because microporosity is effective for gas flow, there is growing interest in the distribution and origins of microporous
carbonate
facies
as potential gas reservoirs. Microporous
carbonate
reservoir rocks occur throughout the geologic column, and vary greatly in both their
facies
distributions and origins. Microporous
carbonate
reservoir examples given here vary from peritidal dolomites, to shallow-water packstone-grainstone banks, to deeper water mud-rich and cherty
carbonate
facies
.
Ordovician peritidal
facies
of the updip Bromide dolomite reservoirs in the Arkoma Basin of Oklahoma are dominated by micro-intercrystalline dolomite porosity resulting from rapid early diagenetic reflux dolomitization. Lower Devonian mid-to-lower slope gas reservoirs in the Thirtyone Formation in the Permian Basin of West Texas rely on cherty microporosity in spiculitic packstones, accompanied by spicule-moldic porosity, and sometimes fracture porosity. Middle Pennsylvanian (Strawn, Desmoinesian) gas reservoirs in Komia packstone-grainstone banks of the Val Verde basin in West Texas are characterized by intraskeletal microporosity within the small branching fossils. And Late Jurassic Cotton Valley deep-water microbial-sponge mound gas reservoirs of the East Texas Basin have microporosity developed in the recrystallized originally high-Mg calcite microbialites.
Microporous
carbonate
rocks commonly require an associated macroporosity type in order to be good primary exploration targets, but
carbonate
rocks with only microporosity can be good secondary producing horizons. The growing interest in tight
carbonate
gas reservoirs, and the increased exploration into deeper and higher temperature horizons, provide impetus to learn more about micro-porous
carbonate
facies
and diagenetic systems, which should enable better predictability.
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