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Grain Size Distribution of Fault Rock in Dynamic Faulting

In search of information for earthquake faulting, well-known active faults and their components have been investigated by many scientists. The availability of drill holes and cores from some of these faults provided an additional advantage of avoiding near surface effects. The study by Blenkinsop (1991) is one of those earlier studies. Blenkinsop identified grain sizesunder 0.01 mm (Figure 1(a) and (b)) in core samples from faults of the San Andreas Fault system and attributed them to cataclastic and ultracataclastic processes (Figure 1(b). He also suggested that as the grain size decreases, the fractal dimension increases. Also see Sammis et al. (1986) on the fractal nature of rock fragmentation.

(a) Photomicrograph of a granitic core sample from the Cajon Pass drillhole showing fine size particles (<0.01 mm) along with porphyroclasts of larger size. (b) Diagram showing various processes interpreted to be operating in grain size reduction of the fault rocks and their fractal dimension of samples of cores from the Cajon Pass and San Gabriel fault zones of the San Andreas Fault system. From Blenkinsop (1991).Figure 1. (a) Photomicrograph of a granitic core sample from the Cajon Pass drillhole showing fine size particles (<0.01 mm) along with porphyroclasts of larger size. (b) Diagram showing various processes interpreted to be operating in grain size reduction of the fault rocks and their fractal dimension of samples of cores from the Cajon Pass and San Gabriel fault zones of the San Andreas Fault system. From Blenkinsop (1991).

Recently, efforts have been made to identify specific mechanism(s) responsible for extreme fragmentation of fault rock also referred to as pulverization (Reches and Drewers, 2005; Sammis and Ben-Zion, 2008; Doan and Gary, 2009; and Yuan et al., 2011). Figure 2 is from Reches and Drewer showing extreme grain size reduction in two samples; one from the San Andreas at the Tejon Pass, California and the other from a newly formed fault in a South African gold mine. The authors interpreted the extreme grain size reduction or pulverization in terms of the advancing stress field at the tip of a dynamic fault and its spatial and temporal variation from tensile to compression as the rupture front propagates. Similarly, controlled laboratory experiments by Yuan et al. (2011) among others provided laboratory data for loading conditions for favoring deformation mode for pulverization.

Particle size distribution of two fault rock (gouge) samples from the San Andreas Fault (301H, solid squares) and (405A_2, open diamonds). The two curves for each sample represent the initial and final stages with few of the grains smaller than 1 micrometer in the former, while almost only grains smaller than 1 micrometer in the former. From Reches and Drewers (2005).Figure 2. Particle size distribution of two fault rock (gouge) samples from the San Andreas Fault (301H, solid squares) and (405A_2, open diamonds). The two curves for each sample represent the initial and final stages with few of the grains smaller than 1 micrometer in the former, while almost only grains smaller than 1 micrometer in the former. From Reches and Drewers (2005).
Reference:

Blenkinsop, T.G., 1991. Cataclasis and processes of particle size reduction. Pure and Applied Geophysics 136: 59-86.

Doan, M.L., Gary, G., 2009. Rock pulverization at high strain rate near the San Andreas fault. Nature Geoscience 2: 709–712, doi:10.1038/ngeo640.

Reches, Z., Dewers, T.A., 2005. Gouge formation by dynamic pulverization during earthquake rupture. Earth Planetary Science Letters 235: 361–374, doi:10.1016/j.epsl.2005.04.009.

Sammis, C.G., Osborne, R.H., Anderson, J.L., Badert, M., White, P., 1986. Self-similar cataclasis and the formation of fault gouge. Pure and Applied Geophysics 124: 53-78.

Sammis, C.G., Ben-Zion, Y., 2008. Mechanics of grain-size reduction in fault zones. Journal of Geophysical Research 113: B022306, doi:1029/2006JB004892.

Yuan, F., Prakash, V., Tullis, T., 2011. Origin of pulverized rocks during earthquake fault rupture. Journal of Geophysical Research 116: B06309, doi:10.1029/2010JB007721.



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