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2008 annual meeting – Spruce Pine Mining District: Little Switzerland, North <strong>Carolina</strong><br />
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structure. Euhedral epidote is fine to medium-grained and is included in coarse-grained<br />
muscovite. Experiments show epidote is a stable ph<strong>as</strong>e in granitic magm<strong>as</strong> at high<br />
pressures (e.g., Naney, 1983). The occurrence of epidote in the Spruce Pine granite<br />
suggests a high pressure for crystallization of the Spruce Pine magm<strong>as</strong>.<br />
DISCUSSION<br />
The LUF1 pegmatite provides a re<strong>as</strong>onable model for crystallization and recrystallization<br />
of the Spruce Pine granitic rocks. The mineralogy and texture of the LUF1 pegmatite is<br />
identical to that of other Spruce Pine granitic rocks and pegmatites. Many early workers<br />
suggested a similar origin for the granitic rocks and pegmatites of the Spruce Pine<br />
District (Olson, 1944; Brobst, 1962). However, the most compelling argument to use the<br />
LUF crystallization model for the Spruce Pine system is the garnet compositional data.<br />
Garnet is the most refractory ph<strong>as</strong>e in the Spruce Pine granitic rocks and shows a similar<br />
range of compositional variation in the LUF1 pegmatite <strong>as</strong> in a suite of Spruce Pine<br />
granitic rocks (Figure 6). Compositions of muscovite and feldspar from LUF1 are also<br />
similar to the compositional variation of these ph<strong>as</strong>es in the Spruce Pine plutonic suite,<br />
but the range in the LUF pegmatite is more restricted that the range in the Spruce Pine<br />
plutonic suite (Swanson, 1998). It appears that the recommendation of Jahns (personal<br />
communication, 1978) is correct, small Spruce Pine pegmatites are good models for<br />
crystallization in the larger Spruce Pine system.<br />
Compositions of coexisting feldspars allow an estimate of temperature of crystallization.<br />
Following the method of Whitney and Stormer (1977), P-T paths for crystallization of<br />
coexisting feldspars are calculated b<strong>as</strong>ed on the structural state of the K-feldspar. For<br />
most granitic rocks the authors suggest (Whitney and Stormer, 1977) K-feldspar probably<br />
crystallizes from the magma <strong>as</strong> orthocl<strong>as</strong>e and they use a combination of sanidine<br />
(Stormer, 1975) and microcline models for feldspar geothermometry. This approach w<strong>as</strong><br />
adopted in the current study.<br />
P-T paths for the magmatic crystallization of LUF1 feldspars were calculated using the<br />
estimates of pre-exsolution compositions of feldspars in Table 1. Results of those<br />
calculations are shown on Figure 7. The feldspar P-T models intersect the experimentally<br />
determined solidus for Spruce Pine granitoids (Vaughn, 1963; Fenn, 1986, and<br />
unpublished) between 8 and 12 kilobars at a temperature of 650-700 degrees C (Figure<br />
7). These pressure estimates translate to a depth of 25 to 40 km, suggesting a mid- to<br />
lower crust site for crystallization of the Spruce Pine magm<strong>as</strong>. These conditions<br />
correspond to the estimates of regional metamorphism in the Spruce Pine thrust sheet<br />
(Adams and Trupe, 1997) and are near the upper limits of regional metamorphism<br />
estimated by Abbott and Raymond (1984) and McSween (et al., 1987) for the Spruce<br />
Pine thrust sheet northe<strong>as</strong>t of the Spruce Pine area. Goldberg and Dallmeyer (1997)<br />
reported Sm-Nd and Rb-Sr ages for hornblende from amphibolites with ages of 379-472<br />
Ma and this age is consistent the 377 Ma age for solidification of the Spruce Pine magma<br />
(Johnson et al., 2001).<br />
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Page 13<br />
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