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rare earth elements in Wyoming

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coarse-gra<strong>in</strong>ed granite (QAP: 30% Q, 40% A, 30%<br />

P) at this location is weakly enriched <strong>in</strong> some of the<br />

HREE (Sample 20120921BG-7).<br />

big creek district<br />

The Big Creek pegmatite district, on the west side<br />

of the Medic<strong>in</strong>e Bow Mounta<strong>in</strong>s, was <strong>in</strong>vestigated<br />

and mapped by Houston (1961) and covers an area<br />

several miles wide and 3.2 to 10 km (2 to 6 mi)<br />

south of the Mullen Creek-Nash Fork shear zone<br />

(fig. 8). The Mullen Creek-Nash Fork shear zone<br />

is part of the Cheyenne belt suture, which represents<br />

a cont<strong>in</strong>ental-arc collision zone (Graff, 1978;<br />

Hills and Houston, 1979) separat<strong>in</strong>g the Wyom<strong>in</strong>g<br />

Prov<strong>in</strong>ce to the north from cratonized (1.7 Ga)<br />

Proterozoic basement of the Colorado Prov<strong>in</strong>ce<br />

to the south. The Colorado Prov<strong>in</strong>ce south of the<br />

Cheyenne belt consists of volcanogenic island-arc<br />

basement rocks, <strong>in</strong>trusive granites, and gabbroic<br />

complexes. The Mullen Creek complex, one of<br />

the larger layered mafic complexes <strong>in</strong> the western<br />

United States, lies along the northern edge of the<br />

Big Creek pegmatite district. The district is <strong>in</strong>cluded<br />

with<strong>in</strong> the Prelim<strong>in</strong>ary Geologic Map of<br />

the Saratoga 30’ x 60’ quadrangle (Sutherland and<br />

Hausel, 2005).<br />

Two types of granite pegmatite were described<br />

by Houston (1961) that cut Early Proterozoic<br />

amphibole gneiss <strong>in</strong> close proximity to both a<br />

medium- to coarse-gra<strong>in</strong>ed, p<strong>in</strong>k to gray foliated<br />

granite <strong>in</strong>trusion, and a well-foliated amphibolite<br />

of the 1778 ± 2 Ma, Mullen Creek layered mafic<br />

igneous complex. In the vic<strong>in</strong>ity of known REE<br />

occurrences, the amphibole gneiss is dom<strong>in</strong>ated by<br />

hornblende gneiss and schist, with lesser, alternat<strong>in</strong>g<br />

layers of feldspar-quartz-biotite gneiss.<br />

The most common pegmatite is an unzoned<br />

feldspar-quartz type that is roughly conformable<br />

<strong>in</strong> direction and attitude to the amphibole gneiss.<br />

These pegmatites tend to be long and narrow, with<br />

widths <strong>rare</strong>ly greater than 3 m (10 ft) and lengths<br />

exceed<strong>in</strong>g 0.8 km (0.5 mi). Their contacts with the<br />

country rock are sharp and exhibit no decrease <strong>in</strong><br />

gra<strong>in</strong> size toward the contacts. M<strong>in</strong>eralogy is simple<br />

and is dom<strong>in</strong>ated by feldspar accompanied by m<strong>in</strong>or<br />

quartz and accessory biotite, muscovite, garnet,<br />

magnetite, and ilmenite (Houston, 1961).<br />

29<br />

The second type of pegmatite may have poorly developed<br />

zon<strong>in</strong>g, has cross-cutt<strong>in</strong>g relationships with<br />

the amphibole gneiss, and tends to be elliptical <strong>in</strong><br />

plan view, with lengths averag<strong>in</strong>g three times their<br />

widths. Similar to the first type, these pegmatites<br />

have sharp contacts and show no decrease <strong>in</strong> gra<strong>in</strong><br />

size toward contact with the country rock. However,<br />

the m<strong>in</strong>eralogy is more complicated, and along<br />

with feldspar and quartz, <strong>in</strong>cludes garnet, biotite,<br />

muscovite, tourmal<strong>in</strong>e, fluorite, and <strong>rare</strong> monazite,<br />

allanite, euxenite, and columbite (Houston, 1961).<br />

Economically, these pegmatites can be described<br />

as either copper-bear<strong>in</strong>g or REE-bear<strong>in</strong>g. Houston<br />

(1961) noted five pegmatites <strong>in</strong> the district that<br />

are known to host one or more of the REE-bear<strong>in</strong>g<br />

m<strong>in</strong>erals, monazite, allanite, and euxenite. However,<br />

only the Platt pegmatite conta<strong>in</strong>ed economic<br />

quantities of these m<strong>in</strong>erals. Numerous other<br />

pegmatites <strong>in</strong> the district were not exam<strong>in</strong>ed and<br />

have the potential to host REE m<strong>in</strong>eralization<br />

(K<strong>in</strong>g and Harris, 2002). The nearby Big Creek<br />

m<strong>in</strong>e hosted copper m<strong>in</strong>eralization, but no primary<br />

REE m<strong>in</strong>erals or columbite. Columbite [(Fe,Mn)<br />

(Nb,Ta) 2 O 6 ] may conta<strong>in</strong> REE and uranium as<br />

accessory constituents (K<strong>in</strong>g and Harris, 2002;<br />

M<strong>in</strong>Dat.org, 2011).<br />

Platt M<strong>in</strong>e (Platt Pegmatite, Uranium K<strong>in</strong>g<br />

M<strong>in</strong>e), SW¼SE¼ sec. 3, T. 13 N., R. 81 W.,<br />

Southeastern Carbon County<br />

The Platt m<strong>in</strong>e was excavated to a depth of 23 m<br />

(75 ft) <strong>in</strong> a zoned, cross-cutt<strong>in</strong>g type pegmatite 21<br />

m wide by 49 m long (70 x 160 ft). The outer part<br />

of the pegmatite is feldspar, and the central part<br />

is quartz-mica-feldspar-<strong>rare</strong> <strong>earth</strong> m<strong>in</strong>erals. Euxenite<br />

is the most abundant REE-bear<strong>in</strong>g m<strong>in</strong>eral<br />

followed by monazite, and the least abundant,<br />

columbite (Houston, 1961). These occur as large<br />

<strong>in</strong>dividual crystals and crystal aggregates both <strong>in</strong><br />

the central pegmatite and <strong>in</strong> gash fractures. Uranium<br />

accounted for most of the production from<br />

the Platt m<strong>in</strong>e <strong>in</strong> 1956 with 12 tonnes (13 tons) of<br />

ore (K<strong>in</strong>g and Harris, 2002). Approximately 4,500<br />

kg (10,000 lbs) of euxenite were reported to be<br />

extracted from the m<strong>in</strong>e between 1956 and 1958<br />

(Houston, 1961; Adams and others, 1980), although<br />

the USBM recorded only 1,413 kg (3,115

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