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Theory for Previous HitQuartzNext Hit Cementation in Structurally Deformed Sandstones

R. H. Lander1, L. M. Bonnell1, S. E. Laubach2, R. E. Larese3, and J. Gale2
1Geocosm LLC
2Bureau of Economic Geology 
3
Consultant

A comprehensive theory for Previous HitquartzNext Hit cementation must account for variations in the abundance and morphologies of cement in undeformed sandstones as well as in fractures of all scales. Our approach toward developing such a theory is to extend existing kinetic models by rigorously simulating the crystal growth anisotropy and nucleation surface area. 
For our analysis we assume that the rate limiting control on Previous HitquartzNext Hit cementation is the crystal precipitation rate (Walderhaug 1994, 1996, 2000). In a strict sense this assumption does not address whether the silica is derived from local diffusion or larger scale fluid advection but instead simply considers that dissolved silica is supplied at a rate that equals or exceeds the rate at which the crystals can precipitate. This assumption is reasonable for Previous HitquartzNext Hit cementation in near neutral pH fluids at temperatures in excess of ~80 °C but is not applicable to Previous HitquartzNext Hit precipitation in highly supersaturated fluids (e.g., in silcretes, saline-alkaline lakes, or in the presence of biogenic opal). 
We assessed the predictive accuracy of a kinetic model for Previous HitquartzNext Hit cement abundance in undeformed sandstones. The model (Touchstone™ version 5.0) considers the temperature effect on precipitation rates, the increase in surface area normalized rates of precipitation with nucleation surface area that have been documented in natural and synthetic Previous HitquartzNext Hit overgrowths (Makowitz and Sibley 2001, Bonnell and Lander in preparation, Lander et al in preparation), and the nucleation surface area and how it varies with sandstone texture, depositional composition, and diagenetic alteration. Previous HitQuartzNext Hit cement abundances are predicted to within four bulk volume percent of the measured values for more than 90% of structurally undeformed sandstone samples from diverse basin settings (rift, wrench, foreland/thrust belt, and cratonic), compositions (quartzarenite to litharenite to subarkose), thermal histories (maximum temperatures ranging from 108 to 244 °C for samples with Ordovician to Miocene depositional ages), and fluid overpressures (from hydrostatic pressure to near fracture gradient fluid overpressures) (Bonnell and Lander in preparation). 
We have extended this Previous HitquartzNext Hit modeling approach to explicitly account for the following effects of particular importance in structurally deformed sandstones: (1) substantially greater growth rates on surfaces that grow parallel to the c-crystallographic axis (pyramidal faces) compared to along the a-crystallographic axes (prismatic faces), (2) the order of magnitude increase in precipitation rate on non-euhedral surfaces compared to euhedral surfaces growing along the same crystallographic orientations (Lander et al in preparation), and (3) the complex interaction of repeated fracturing and cementation on nucleation surface area.
Preliminary results obtained using a 2D model incorporating these effects (Prism™) reproduces Previous HitquartzNext Hit morphologies in fractures of varying scales as well as in pores within undeformed sandstones. Results indicate that the abundance and morphology of Previous HitquartzNext Hit cement within fractures depend on the relative rates of Previous HitquartzNext Hit precipitation and fracture opening, the geometries and sizes of grain surfaces and pores, and the orientations of crystallographic axes with respect to fractures. Pervasive Previous HitquartzNext Hit sealing of fractures occurs in the simulations when the rate of crystal growth on surfaces of the slowest growing type (along the a-crystallographic axis) exceeds the net rate of fracture opening. Euhedral Previous HitquartzNext Hit crystals rim otherwise open fractures when the rate of fracture opening exceeds the fastest rate of Previous HitquartzNext Hit crystal growth (on non-euhedral surfaces that grow parallel to the c-crystallographic axis). Simulations suggest that Previous HitquartzNext Hit bridges form where the following conditions are met: 

  • The c-crystallographic axis is near perpendicular to the fracture plane for monocrystalline grains bisected by the fracture.
  • Increases in fracture apertures are small for individual fracture events (e.g., microns to tens of microns)
  • Integrated over geologic time scales, the rate of kinematic aperture increase is less than the rate of precipitation along the Previous HitquartzNext Hit c-axis on non-euhedral surfaces (the fastest growth rate) but greater than a-axis precipitation rates, and 
  • Fracturing of bridged Previous HitquartzNext Hit crystals periodically creates new non-euhedral nucleation surfaces.

References

Bonnell, L. M. and R. H. Lander, in preparation, Previous HitQuartzNext Hit precipitation kinetics vary with sandstone grain size.

Lander, R. H., R. E. Larese, and L. M. Bonnell, in preparation, Origin of the “grain size” effect for Previous HitquartzNext Hit overgrowth         precipitation kinetics.

Makowitz, A. and Sibley, D.F., 2001, Crystal growth mechanisms of Previous HitquartzNext Hit overgrowths in a Cambrian Previous HitquartzNext Hit arenite: Journal of Sedimentary Research. v. 71, p. 809-816.

Walderhaug, O., 1994, Precipitation rates for Previous HitquartzNext Hit cement in sandstones determined by fluid-inclusion microthermometry and temperature-history modeling: Journal of Sedimentary Research, v. A64, p. 324-333.

Walderhaug, O., 1996, Kinetic modelling of Previous HitquartzNext Hit cementation and porosity loss in deeply buried sandstone reservoirs: American Association of Petroleum Geologists Bulletin, v. 80, p. 731–745.

Walderhaug, O., 2000, Modeling Previous HitquartzTop cementation and porosity loss in Middle Jurassic Brent Group Sandstones of the Kvitebjørn Field, Northern North Sea: American Association of Petroleum Geologists Bulletin, v. 84, p. 1325-1339.

 

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