This paper is concerned with the development of magmatic, mechanical instabilities in Tuolumne Batholith (TB), Sierra Nevada , California , USA (Figure 1) and the resulting physical accumulation and concentration of K-feldspar megacrysts (phenocrysts).
Evidence for physical accumulation of megacrysts in the TB was presented long ago by Gilbert (1906), but a recent suggestion by Higgins (1999) that megacryst concentrations are due to in situ crystallization during open-system conditions has prompted us to re-examine the existing evidence and search for new evidence. We conclude that K-feldspar megacrysts grew from a melt and that a number of processes led to their physical accumulation . In some places, these accumulations in turn were positively buoyant and continued to rise in the magma chamber while concentrating additional megacrysts. These accumulations formed prior to the development of a late magmatic foliation/lineation (Figure 2), that is before final crystallization of magma in the chamber.
After briefly summarizing the main characteristics of the TB, we provide a review of the evidence for the magmatic origin of K-feldspar megacrysts, mainly because some authors still favor a metasomatic origin [e.g., Dickson, 1996], and then discuss the cause of the large size of the megacrysts — nucleation and growth versus "Ostwald ripening." We then present evidence for megacryst movement and accumulation in granitic magma, and conclude with a discussion of the timing of megacryst growth in the TB, the lack of evidence for grain coarsening or concentration by in situ growth of megacrysts by precipitation from K-rich solutions, and of the physical processes by which the megacrysts were accumulated in the TB.