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Geologic Studies in Alaska by the U.S. Geological Survey, 1992

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192<br />

GEOLOGIC STUDIES IN ALASKA BY THE U.S. GEOLOGICAL SURVEY, <strong>1992</strong><br />

estimated several percent of iron <strong>in</strong>dicated for this phase<br />

would be most unusual for albite, especially a presumed<br />

low-temperature albite, <strong>in</strong>asmuch as pegmatitic albites<br />

typically have less than 0.01 percent iron (Smith, 1983).<br />

Possibly <strong>the</strong> phase is a quenched iron-bear<strong>in</strong>g glass, but<br />

<strong>the</strong>n its lack of potassium might seem puzzl<strong>in</strong>g.<br />

In fact, a potassic m<strong>in</strong>eral is present on <strong>the</strong> smooth<br />

areas on <strong>the</strong> natural fracture surface of CM rock sample<br />

92DB-05C where it occurs as (light gray) hexagonal plates<br />

(fig. 9A). It is even more apparent <strong>in</strong> <strong>the</strong> gray area at <strong>the</strong><br />

lower left of figure 9A. The area, shown enlarged <strong>in</strong> <strong>the</strong><br />

upper right of figure 9B, can be seen to consist of two<br />

phases. The darker areas show<strong>in</strong>g between <strong>the</strong> hexagons<br />

<strong>in</strong> figure 9B are of (iron-free) albite composition (ab). The<br />

lighter phase (kim) conta<strong>in</strong>s abundant potassium (fig. 11).<br />

Over a range of a factor of five <strong>in</strong> potassium peak <strong>in</strong>ten-<br />

sity, FeK is acceptably <strong>in</strong>variant (3 to 3.6) for 9 of 12<br />

analyses. Similarly, eight analyses gave MoK peak <strong>in</strong>ten-<br />

sities from 2.1 to 3.1. In contrast, SiIK <strong>in</strong>tensities ranged<br />

from 1 to 27 and Si/Al <strong>in</strong>tensities are close to those for<br />

albite. We conclude that <strong>the</strong> spectrum shown <strong>in</strong> figure 11<br />

likely represents a mixture of albite and a non-silicate m<strong>in</strong>-<br />

eral conta<strong>in</strong><strong>in</strong>g potassium, iron, and molybdenum. Be-<br />

cause <strong>the</strong> readily observed X-ray peaks for molybdenum<br />

and sulfur have overlapp<strong>in</strong>g energies that cannot be easily<br />

dist<strong>in</strong>guished, <strong>the</strong> m<strong>in</strong>eral could be a sulfide. It also could<br />

be an oxide or hydroxide among o<strong>the</strong>r possibilities.<br />

Ferrimolybdite is a known wea<strong>the</strong>r<strong>in</strong>g product, and <strong>the</strong>re<br />

are several potassic molybdates. This raises <strong>the</strong> question<br />

of <strong>the</strong> orig<strong>in</strong> of thls hexagonal phase. Because we are ana-<br />

lyz<strong>in</strong>g a natural, unpolished surface, <strong>the</strong> phase almost cer-<br />

ta<strong>in</strong>ly represents some k<strong>in</strong>d of surficial deposit or reaction.<br />

The hexagons appear to be oriented parallel to <strong>the</strong> surface<br />

and nucleation appears to have dom<strong>in</strong>ated crystal growth<br />

k<strong>in</strong>etics (that is, <strong>the</strong>re are numerous small crystals). If<br />

<strong>the</strong>y are wea<strong>the</strong>r<strong>in</strong>g products, a source of potassium would<br />

be required, and this could be <strong>the</strong> potassium feldspar con-<br />

ta<strong>in</strong>ed <strong>in</strong> <strong>the</strong> bulk rock. Ano<strong>the</strong>r possibility is that this<br />

potassium-iron-molybdenum phase may have crystallized<br />

(perhaps subsolidus) as part of a system quenched <strong>in</strong> a<br />

manner similar to that ascribed above to <strong>the</strong> conjectured<br />

iron-albite glass.<br />

DISCUSSION<br />

The Dora Bay molybdenite occurrences are only<br />

show<strong>in</strong>gs, but molybdenite occurs here <strong>in</strong> similar sett<strong>in</strong>gs<br />

at two localities that are 3 km apart; readily visible molyb-<br />

denite occurs over a width of about 5 m <strong>in</strong> <strong>the</strong> HM pit<br />

face; and analyses of two bulk HM samples yielded 0.5<br />

and 1.2 percent molybdenum, respectively. These discov-<br />

eries offer at least some prospect of a molybdenite deposit<br />

<strong>in</strong> <strong>the</strong> vic<strong>in</strong>ity. At our current level of understand<strong>in</strong>g, <strong>the</strong><br />

Figure 6. Scann<strong>in</strong>g electron microscope backscattered-electron Figure 7. Scann<strong>in</strong>g electron microscope backscattered-electron<br />

image of HM rock sample CDP-92-29. A gra<strong>in</strong> of scapolite (sc) is image of HM rock sample CDP-92-29. Molybdenite (mo)<br />

ve<strong>in</strong>ed <strong>by</strong> calcite (ca) and potassium feldspar (or). Molybdenite lenses and ve<strong>in</strong>s occur <strong>in</strong> potassium feldspar (or) and albite (ab).<br />

(mo) occurs with<strong>in</strong> a calcite ve<strong>in</strong> <strong>in</strong> <strong>the</strong> upper left comer of <strong>the</strong> Mottled m<strong>in</strong>eral at <strong>the</strong> top of <strong>the</strong> photograph is scapolite (sc),<br />

scapolite gra<strong>in</strong>. Accessory m<strong>in</strong>erals <strong>in</strong>cl~ide sphene (sph), apatite which is adjacent to a gra<strong>in</strong> of biotite (bt). Field of view is<br />

(ap), and zircon (zr). Field of view is approximately 2 mm. approximately 8 mm.

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