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sgr ms thesis - University of Maine

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achieve supersolidus temperatures. For example, volcanic tuff, quartzite, or calcsilicate<br />

layers would not melt with the pelitic layers, leaving a preference to<br />

preserve the clasts produced from the higher melting temperature layers. This<br />

means that not all clasts would follow the same trend <strong>of</strong> melting, and could<br />

explain why not all Bar Harbor Formation clasts completely melted in Type 3<br />

Shatter Zone.<br />

For the 900°C intrusion model, the clasts and matrix reach equilibrium at a<br />

temperature well above Cadillac Mountain Granite feldspar crystallization<br />

temperatures (Wiebe et al., 1997a), but the 800°C intrusion model is well below<br />

the 825°C feldspar crystallization <strong>of</strong> the Cadillac mountain Granite (Wiebe et al.,<br />

1997). Although the temperature remains above the Bar Harbor Formation<br />

solidus for a relatively long time, feldspar crystallization would significantly<br />

increase viscosity (e.g. Baker, 1996; Bea, 2010). If magma partially solidifies<br />

around a clast, there is a reduced chance for disaggregation (e.g. Beard and<br />

Ragland, 2005). For the 900°C intrusion model, the equilibrium temperature is<br />

too high for a viscosity increase, but for the 800°C intrusion model, magma<br />

crystallization may have been able to protect clasts from disaggregation with an<br />

envelope <strong>of</strong> more viscous material.<br />

The initial temperature and volume fraction <strong>of</strong> wall rock and magma<br />

determine the equilibrium temperature. As seen in Figure 7.4, a lower magma<br />

matrix percent by volume would cause less clast melting. Several initial intrusion<br />

and clast temperatures are used to replicate potential magma temperatures and<br />

wall rock temperatures with distance from the reservoir. Type 1 and 2 Shatter<br />

105

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