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The AAPG/Datapages Combined Publications Database

Houston Geological Society Bulletin

Abstract


Houston Geological Society Bulletin, Volume 36, No. 5, January 1994. Pages 11-11.

Abstract: Previous HitApatiteNext Hit Previous HitFissionNext Hit Previous HitTrackNext Hit Previous HitAnalysisNext Hit Applied To The Margins Of The Gulf Coast Basin

By

Raymond A. Donelick and Jeff Corigan

Trace quantities of radioactive uranium occur in Previous HitapatiteNext Hit grains. When one of these uranium nuclei decays by nuclear Previous HitfissionNext Hit, the tm, resultant nuclear fragments repel each other and tear a damage trail through their host Previous HitapatiteNext Hit crystal lattice. Damage trails of this type are called Previous HitfissionNext Hit tracks, and they can be made visible using conventional light microscopes by immersion in acid solution. The measurable characteristics of the Previous HitfissionNext Hit tracks in Previous HitapatiteNext Hit (i.e., their number, length, width) contain a wealth of information regarding the thermal history that the host rock has experienced during its geological evolution.

Previous HitApatiteNext Hit Previous HitfissionNext Hit Previous HittrackNext Hit ages from 12 Precambrian granitic samples from the Llano Uplift vary from 182+50 Ma to 425+72 Ma (95% confidence intervals) , with mean Previous HittrackNext Hit lengths varying from 11.2+0.1 µm for the same samples. While not systematic, ages generally increase from cart to west Zircons from these samples are metamict, indicating that rocks presently exposed in the Llano Uplift did not experience temperatures greater than ~225+25°C since Precambrian time. A single sample from a Pennsylvanian sandstone (Smithwick Formation), located just east of the Llano Uplift, gives an Previous HitapatiteNext Hit Previous HitfissionNext Hit Previous HittrackNext Hit age of 241+18 Ma, and a mean length of 11.9+0.2 µm. Using available stratigraphic constraints, it is inferred that the Llano basement samples were at temperatures of <70°C prior to initiation of the Ouachita orogeny during Pennsylvanian time. Subsequent heating of the Llano basement samples associated with the Ouachita orogeny is evident in the Previous HitapatiteNext Hit Previous HitfissionNext Hit Previous HittrackNext Hit data. The ages and Previous HittrackNext Hit length distributions are all consistent with the Llano basement samples having been heated to temperatures of ~90-120°C due to burial of the Llano by a 1-2 km thick Pennsylvanian to Permian molasse sequence (Strawn to Cisco Groups) derived from the Ouachita orogeny. Based on numerical modeling of the Previous HitapatiteNext Hit Previous HitfissionNext Hit Previous HittrackNext Hit data, we interpret the variability in ages and mean Previous HittrackTop lengths to reflect small magnitude (<1 km) differential loading of the Llano Uplift due to westward thinning of this molasse sequence. From late Permian (?) through Julassic time, samples cooled from ~90-120°C, based on model results, to <40°C, based on stratigraphic constraints. This early Mesozoic stage of cooling is attributed to erosional unroofing associated with extensional collapse of the Ouachita orogen during initial opening of the Gulf of Mexico. Mild reheating of these samples to >60°C due to deposition of -1 km of Cretaceous to Early Tertiary (?) strata across the Llano region is needed to explain the low percentage of tracks in the 14-16 µm range. Final cooling of these samples below ~60°C did not occur until post- Paleogene (?) time. This late stage cooling is interpreted in terms of regional Tertiary erosion along the outer rim of the Gulf of Mexico basin due to flexural upwarping associated with basinward loading of the crust.

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