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Magma Contamination And Sulfide Immiscibility Of The Meteoric Impact Zone

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MAGMA CONTAMINATION AND SULFIDE IMMISCIBILITY OF THE METEORIC IMPACT ZONE IN THE SUDBURY NI-CU DEPOSITS: ONTARIO, CANADA
WILLIAMS, Jane B. (University of Wisconsin-Eau Claire, willijan@uwec.edu)

Sudbury, Canada is the location of a world class Ni-Cu deposit phenomena. Numerous studies have produced an explanation for the complex evolution of its deposition and enrichment thanks to the impaction of a meteorite 1.85 million years ago. The impact of the meteorite is thought to have caused fracturing that led to the generation of magma from deep in the crust that helped in later filling the crater and producing the igneous complex (Faggart et. al., 1985). The igneous complex (Figure 1a) has an elongated shape (60 km long and 27 km wide) with circular deposits surrounding it similar to a bulls-eye. Evidence of the meteoric impact includes brecciation located in the center of the basin (Onaping Formation), deformation of the margin of the intrusive complex (Huronian Group), shatter cones, and pseudotachylite. The meteor is thought to have flash melted the crust which proceeded to differentiate into a granophyre and a leuconorite to norite composition. The granophyre makes up 60% of the complex and the leuconorite and norite make up the remaining 40% (Figure 1b)(Barnes et. al., 2005). About 50% of the ore is found in the sublayer norite and the breccia that is associated with the norite. This ore is mainly disseminated sulphides. The massive sulphides are located in the center

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