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

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The overall similarity <strong>of</strong> paragenesis for <strong>the</strong> Pickh<strong>and</strong>le ve<strong>in</strong>s <strong>and</strong> Barstow dissem<strong>in</strong>ated ores is<br />

supported by <strong>the</strong> atypical nature <strong>of</strong> <strong>the</strong> paragenetic sequence (oxides early—sulfides late). Most<br />

epi<strong>the</strong>rmal deposits are characterized by early sulfide m<strong>in</strong>eralization with later deposition <strong>of</strong> oxides <strong>and</strong><br />

carbonates. As both <strong>the</strong> Calico ve<strong>in</strong>s <strong>and</strong> Waterloo/Langtry deposits are paragenetically atypical, it<br />

seems more likely <strong>the</strong>re was a s<strong>in</strong>gle evolv<strong>in</strong>g fluid responsible for ore deposition <strong>and</strong> not two unrelated<br />

events.<br />

Figure 6. Detailed paragenesis for <strong>the</strong> ve<strong>in</strong> m<strong>in</strong>eralization <strong>of</strong> <strong>the</strong> Calico District <strong>and</strong> dissem<strong>in</strong>ated ores <strong>of</strong> <strong>the</strong><br />

Barstow Formation (Waterloo/Langtry paragenesis after Fletcher, 1986).<br />

Fluid Inclusion Geo<strong>the</strong>rmometry<br />

Fluid <strong>in</strong>clusion data are summarized <strong>in</strong> Figure 7. Homogenization temperatures for barite range from<br />

160° to 310° C. Calico District barite fluid <strong>in</strong>clusions are <strong>of</strong>ten large (>50 microns) <strong>and</strong> are restricted to<br />

Type I, <strong>in</strong>dicat<strong>in</strong>g <strong>the</strong> fluids were not boil<strong>in</strong>g at <strong>the</strong> time <strong>of</strong> barite crystallization. Homogenization<br />

temperatures range from 240° to 310° C <strong>and</strong> sal<strong>in</strong>ities from 2–4 wt% NaCl. Utiliz<strong>in</strong>g paragenesis, barite<br />

geo<strong>the</strong>rmometry <strong>and</strong> sal<strong>in</strong>ity, <strong>and</strong> Eh-pH relationships, Rosso (1992) calculated depth <strong>of</strong> barite<br />

emplacement at one to 1.5 kilometers. Limited analysis <strong>of</strong> quartz (not shown) has yielded<br />

homogenization temperatures similar to but slightly higher than those for barite (average 290°C).<br />

Fletcher (1986) analyzed both barite <strong>and</strong> quartz from <strong>the</strong> Waterloo <strong>and</strong> Langtry deposits with<strong>in</strong> <strong>the</strong><br />

Barstow Formation. He reported homogenization temperatures from 140° to 230°C with sal<strong>in</strong>ities <strong>of</strong> 4–6<br />

wt% NaCl. Barite <strong>in</strong>clusions were generally smaller than those from <strong>the</strong> Pickh<strong>and</strong>le ve<strong>in</strong>s <strong>and</strong> Type II<br />

<strong>in</strong>clusions, <strong>in</strong>dicative <strong>of</strong> boil<strong>in</strong>g, were common. Utiliz<strong>in</strong>g similar data <strong>and</strong> logic to that <strong>of</strong> Rosso, Fletcher<br />

(1986) calculated depth <strong>of</strong> emplacement <strong>of</strong> Barstow m<strong>in</strong>eralization at no greater than a few hundred<br />

meters.<br />

Figure 7 comb<strong>in</strong>es data for <strong>the</strong> Waterman Hills <strong>and</strong> Mitchel Range. While homogenization temperatures<br />

show considerable overlap (Waterman Hills 180° to 220° C <strong>and</strong> Mitchel Range 180-270°C) <strong>the</strong>re are<br />

significant differences between <strong>the</strong> two localities (Jessey <strong>and</strong> Tarman, 1994). Waterman Hills barite

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