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

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

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concordant to bedd<strong>in</strong>g <strong>of</strong> <strong>the</strong> volcaniclastic sedimentary rocks at <strong>the</strong> surface, crosscut <strong>the</strong> strata <strong>in</strong><br />

underground work<strong>in</strong>gs. The Waterman Hills detachment fault crops out less than one kilometer north<br />

<strong>and</strong> south <strong>of</strong> <strong>the</strong> barite ve<strong>in</strong>s. Projections from surface outcrops <strong>in</strong>dicate <strong>the</strong> fault contact should lie less<br />

than 150 meters below <strong>the</strong> present erosional surface. <strong>M<strong>in</strong>eralization</strong> resembles that <strong>of</strong> <strong>the</strong> Calico<br />

District where<strong>in</strong> coarse-gra<strong>in</strong>ed barite has been brecciated <strong>and</strong> replaced by a matrix <strong>of</strong> iron oxides. Little<br />

is known about <strong>the</strong> silver occurrence <strong>and</strong> no sulfides were observed ei<strong>the</strong>r on <strong>the</strong> dumps or <strong>in</strong><br />

underground work<strong>in</strong>gs.<br />

Mitchel Range<br />

The Waterman Gneiss (lower plate <strong>of</strong> <strong>the</strong> Waterman Hills detachment fault) hosts a group <strong>of</strong> northwest<br />

trend<strong>in</strong>g barite ve<strong>in</strong>s at <strong>the</strong> sou<strong>the</strong>ast end <strong>of</strong> <strong>the</strong> Mitchel Range. The ve<strong>in</strong>s crosscut <strong>the</strong> Waterman<br />

Gneiss at steep angles <strong>and</strong> postdate a prom<strong>in</strong>ent mylonitic fabric. Ve<strong>in</strong> marg<strong>in</strong>s are slickensided,<br />

suggest<strong>in</strong>g emplacement with<strong>in</strong> fault zones. Barite occurs as coarse-gra<strong>in</strong>ed rosette-shaped aggregates,<br />

<strong>of</strong>ten heavily iron sta<strong>in</strong>ed. M<strong>in</strong>or iron oxides are present, as are trace amounts <strong>of</strong> galena. No silver<br />

m<strong>in</strong>eralization was observed <strong>and</strong> <strong>the</strong> limited extent <strong>of</strong> <strong>the</strong> work<strong>in</strong>gs suggests ore grades were subeconomic.<br />

Mt. General<br />

The silver–barite m<strong>in</strong>eralization <strong>of</strong> <strong>the</strong> Mt. General area rema<strong>in</strong>s <strong>the</strong> most enigmatic feature <strong>of</strong> <strong>the</strong><br />

Calico District. Mapp<strong>in</strong>g suggests host rocks are similar to those <strong>in</strong> <strong>the</strong> Waterman Hills. Stratigraphic<br />

position <strong>of</strong> <strong>the</strong>se rocks is uncerta<strong>in</strong>. Perhaps <strong>the</strong> most unusual aspect <strong>of</strong> <strong>the</strong> Mt. General occurrence is<br />

<strong>the</strong> barite. The barite occurs with<strong>in</strong> <strong>in</strong>dist<strong>in</strong>ct northwest-trend<strong>in</strong>g shear zones, which lack cont<strong>in</strong>uity<br />

along strike. <strong>M<strong>in</strong>eralization</strong> has been extensively sheared <strong>and</strong> brecciated. Barite is dark <strong>and</strong> cloudy,<br />

commonly with <strong>in</strong>clusions <strong>of</strong> particulate matter. Microscopic exam<strong>in</strong>ation <strong>in</strong>dicates <strong>the</strong> barite <strong>and</strong> m<strong>in</strong>or<br />

associated calcite have undergone extensive recrystallization. Iron sta<strong>in</strong><strong>in</strong>g is common <strong>in</strong> underground<br />

work<strong>in</strong>gs, but iron oxides occur <strong>in</strong> only trace amounts. The very limited underground work<strong>in</strong>gs <strong>and</strong><br />

scattered prospect pits suggest low silver grades.<br />

Paragenesis<br />

Detailed paragenetic studies <strong>of</strong> <strong>the</strong> Calico ve<strong>in</strong> m<strong>in</strong>eralization (Jessey, 1992) <strong>and</strong> dissem<strong>in</strong>ated ores <strong>in</strong><br />

<strong>the</strong> Barstow Formation (Fletcher, 1986) have shown only m<strong>in</strong>or differences <strong>in</strong> <strong>the</strong> sequence <strong>of</strong> ore<br />

m<strong>in</strong>eral deposition (Fig. 6). Less detailed studies <strong>of</strong> m<strong>in</strong>eralization <strong>in</strong> <strong>the</strong> Waterman Hills, Mitchell Range<br />

<strong>and</strong> Mt. General <strong>in</strong>dicate a similar, albeit less complex, paragenesis.<br />

To generalize, barite <strong>and</strong> chalcedony/quartz were deposited early (Early Barite stage). This was followed<br />

by an episode <strong>of</strong> pervasive silicification (<strong>in</strong>itial stage <strong>of</strong> Silver–Silicification) <strong>and</strong> subsequently by<br />

hematite, magnetite <strong>and</strong> manganese oxides. A variety <strong>of</strong> sulfides followed <strong>the</strong> oxides (late stage Silver–<br />

Silicification). The Late Stage Alteration <strong>in</strong>cluded secondary iron oxides, silver chlorides, <strong>and</strong> calcite<br />

deposited by supergene fluids.<br />

Fletcher (1986) <strong>and</strong> Rosso (1992) attribute <strong>the</strong> observed paragenetic sequence to changes <strong>in</strong> fluid pH.<br />

However, <strong>the</strong> elevated sal<strong>in</strong>ity <strong>of</strong> ore fluids (see Fluid Inclusion Geo<strong>the</strong>rmometry) makes this difficult to<br />

rationalize, as sal<strong>in</strong>e fluids typically buffer reactions <strong>and</strong> resist pH change. Ano<strong>the</strong>r explanation would be<br />

a change <strong>in</strong> Eh. Early oxidiz<strong>in</strong>g ore fluids would deposit sulfates (barite) <strong>and</strong> oxides<br />

(magnetite/hematite). As conditions became more reduc<strong>in</strong>g, pyrite, galena <strong>and</strong> acanthite would form.

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