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Geology and Ore Genesis of Silver–Barite Mineralization in the ...

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ve<strong>in</strong>s are hosted by upper plate rocks correlative to <strong>the</strong> Miocene Pickh<strong>and</strong>le Formation (upper plate<br />

WHDF). Inclusions were <strong>the</strong> smallest observed <strong>in</strong> <strong>the</strong> central Mojave Desert (average diameter 10-15<br />

microns) <strong>and</strong> evidence for boil<strong>in</strong>g <strong>the</strong> most widespread. Although sal<strong>in</strong>ity could not be determ<strong>in</strong>ed, field<br />

observation suggests barite was emplaced at shallow depths. Mitchel Range barite was deposited <strong>in</strong><br />

ve<strong>in</strong>s cutt<strong>in</strong>g basement rocks (Waterman Gneiss) <strong>in</strong> <strong>the</strong> lower plate <strong>of</strong> <strong>the</strong> WHDF. Barite occurs as<br />

coarse-gra<strong>in</strong>ed rosette-shaped aggregates, <strong>of</strong>ten heavily iron sta<strong>in</strong>ed. Crystals are water-clear <strong>and</strong><br />

conta<strong>in</strong> large <strong>in</strong>clusions (>100 microns). There is no evidence <strong>of</strong> fluid boil<strong>in</strong>g.<br />

Figure 7. Fluid <strong>in</strong>clusion homogenization temperatures for central Mojave Desert barite occurrences (data for<br />

Waterloo/Langtry from Fletcher, 1986).<br />

Mt. General barite (not shown <strong>in</strong> Figure 7) is dark, cloudy, <strong>and</strong> yields few usable <strong>in</strong>clusions. Fur<strong>the</strong>rmore,<br />

upon heat<strong>in</strong>g <strong>the</strong> <strong>in</strong>clusions <strong>of</strong>ten fracture mak<strong>in</strong>g homogenization temperature difficult to measure.<br />

Data from a small number <strong>of</strong> observations (12) suggests <strong>the</strong> average homogenization temperature is<br />

approximately 210°C.<br />

Discussion<br />

Any model for <strong>the</strong> genesis <strong>of</strong> silver–barite m<strong>in</strong>eralization must take <strong>in</strong>to account structural <strong>and</strong><br />

stratigraphic relationships, as well as m<strong>in</strong>eral paragenesis <strong>and</strong> fluid <strong>in</strong>clusion geo<strong>the</strong>rmometry <strong>and</strong><br />

geobarometry. The first question that must be addressed is <strong>the</strong> age <strong>of</strong> m<strong>in</strong>eralization. Fletcher (1986)<br />

states that two samples <strong>of</strong> potassically altered Barstow Formation yielded K/Ar dates <strong>of</strong> 17.1 <strong>and</strong> 17.5<br />

Ma respectively. This is consistent with tim<strong>in</strong>g <strong>of</strong> deposition <strong>of</strong> <strong>the</strong> Barstow Formation.<br />

The relationship <strong>of</strong> <strong>the</strong> m<strong>in</strong>eralization to structural evolution is more problematic. S<strong>in</strong>gleton <strong>and</strong> Gans<br />

(2008) argue that unro<strong>of</strong><strong>in</strong>g <strong>of</strong> <strong>the</strong> Waterman Hills core complex occurred between 25 Ma <strong>and</strong> 19 Ma.<br />

Bartley et al. (1990) place <strong>the</strong> onset <strong>of</strong> dextral shear <strong>in</strong> <strong>the</strong> central Mojave at 19 Ma, although it is<br />

unclear if this <strong>in</strong>cludes <strong>the</strong> Calico fault. S<strong>in</strong>gleton <strong>and</strong> Gans (2008) state, however, that active dacitic

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