SAME SOURCE, DIFFERENT TEXTURES: THE CACHE AND QUANAH GRANITES, SOUTHWESTERN OKLAHOMA
The Quanah’s typical facies is coarse and subequigranular, dominated by strongly exsolved perthite with overgrowths that form an intercumulus with glomerocrystic medium-grained equant Qz and smaller Arf + Fe-Ti oxides. Qz exhibits a low-intensity CL core mantled by two higher–intensity zones, with a ~60 micron, low-intensity rim that joins glomerocrystic grains. Including small inclusions, sections contain roughly 250 Qz particles per cm2. The Quanah’s medium-grained Craterville facies is perthitic Ksp and equant glomerocrystic Qz with oxides ± Bt, surrounded by variable amounts of dense granophyre. Qz phenocryst cores have relatively elevated CL intensity, with ~60 micron rims that match the low CL intensity of the granophyric Qz. Sections contain 1050-1575 Qz particles per cm2. In contrast, the type facies of the Cache Granite exhibits the strongly porphyritic microstructure more typical of the WGG. The medium-grained phenocrysts of perthitic Ksp and glomerocrystic equant quartz with oxides is surrounded by intense, very fine granophyre. These glomerocrysts display subtle CL zoning with lower intensity cores; their skeletal rim intensity is largely the same as the surrounding granophyre. Sections contain greater than 2300 Qz particles per cm2.
Field relationships and high-precision dating show that the Quanah magma intruded the Cache Granite 110 to 650 Kyr after Cache crystallization. Their near-identical composition suggests separate pulses arising from the same source. Over this interval, emplacement conditions progressed from severe undercooling to those permitting the persistence of near-solidus temperatures.