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K. Lund
    ... RR—Ramey Ridge suite; AB—Acorn Butte suite; RC—Rush Creek Point suite; Y—Yellowjacket suite; D—Deep Creek suite; A—Arnett Creek suite; DG—Daugherty Gulch drill site; BH—Beaverhead pluton. ... SEDIMENTARY UNITS OF DAUGHERTY GULCH. ...
    ... Although earlier workers thought these deposits were Cretaceous (Lindgren, 1904; Thompson and Ballard, 1924; Beckwith, 1928; Ross, 1931; Shenon and Reed, 1934), Anderson (1951) thought the Cretaceous plu-tons of the Idaho batholith... more
    ... Although earlier workers thought these deposits were Cretaceous (Lindgren, 1904; Thompson and Ballard, 1924; Beckwith, 1928; Ross, 1931; Shenon and Reed, 1934), Anderson (1951) thought the Cretaceous plu-tons of the Idaho batholith were the barren host rocks of ...
    ABSTRACT The Late Cretaceous Boulder batholith, southwestern MT, is composed of the Butte Granite and at least a dozen smaller granodiorite to syenogranite plutons. These plutons (81-73 Ma) were dated by zircon U-Pb geochronology using... more
    ABSTRACT The Late Cretaceous Boulder batholith, southwestern MT, is composed of the Butte Granite and at least a dozen smaller granodiorite to syenogranite plutons. These plutons (81-73 Ma) were dated by zircon U-Pb geochronology using the SHRIMP. Typically for SIMS analysis of igneous zircon, the analytical spot is located midway between core and rim on an area that displays fine oscillatory zoning, thus sampling a ~25-30 µm area of vertically oriented zones to a depth of 1-2 µm. For this study, preliminary LA-ICP-MS analysis of Hf isotopes in zircons from several plutons suggested that some grains show significant variation (>5 εHf units) between inner and outer zones. This finding instigated a detailed investigation in which data for multiple isotopic systems (U-Pb, trace elements, O, and Hf ) were collected from horizontally oriented zones. Zircons were mounted in epoxy but not ground or polished. Reflected light, profilometer, and CL images were used to select homogeneous crystal faces. The outermost parts of 12-15 grains each from 12 plutons were analyzed consecutively for O and U-Pb isotope ratios, and trace element concentrations using an ion microprobe. The grains were then ground to half-thickness and O, U-Pb, and trace elements were measured at the centers of previously analyzed grains. The final step was Hf isotopic analysis by LA-ICP-MS which ablated a hole completely through the remaining half-grains. Although measurements of these isotopes from the outsides and insides of selected zircons is a limited form of depth-profiling, it enables acquisition of a very large, more precise data set than typical depth profiling. For all samples, U-Pb ages of zircon from interior and exterior zones are not resolvably different at ± 1% (2-sigma). However, in several samples a few outliers were identified, suggesting that interior parts in some grains formed later, during or after growth of the exterior parts of other grains. Thus, zircon growth was not an episodic process, but was semi-continuous, and probably controlled by inclusion in major rock-forming phases that isolated zircon from residual melt, local chemical gradients, and magma mixing. These processes are important for proper interpretation of isotopic and trace element data; the presumption that all zircon growth was initiated simultaneously could lead to misinterpretation of data arrays. Values of delta18O show variations between interior and exterior parts of grains both within a single sample and between samples. Hf isotopic data reveal that many grains in several samples are composed of two components that have resolvable differences in εHf suggesting multiple contributions to magmas. Trace element data suggest that some magmas followed systematic fractionation trends, whereas others were also influenced by magma mixing. Despite caveats pertaining to relative ages, analysis of trace elements and isotope ratios within discrete thin zones of individual zircons can be a powerful tool for understanding the details of magma evolution.
    ABSTRACT The Cu-Co ± Au (± Ag ± Ni ± REE) ore deposits of the Blackbird district, east-central Idaho, have previously been classified as Besshi-type VMS, sedex, and IOCG deposits within an intact stratigraphic section. New studies... more
    ABSTRACT The Cu-Co ± Au (± Ag ± Ni ± REE) ore deposits of the Blackbird district, east-central Idaho, have previously been classified as Besshi-type VMS, sedex, and IOCG deposits within an intact stratigraphic section. New studies indicate that, across the district, mineralization was introduced into the country rocks as a series of structurally controlled vein and alteration systems. Quartz-rich and biotite-rich veins (and alteration zones) and minor albite and siderite veinlets maintain consistent order and sulfide mineral associations across the district. Both early and late quartz veins contain chalcopyrite and pyrite, whereas intermediate-stage tourmaline-biotite veins host the cobaltite. Barren early and late albite and late carbonate (generally siderite) form veins or are included in the quartz veins. REE minerals, principally monazite, allanite, and xenotime, are associated with both tourmaline-biotite and late quartz veins. The veins are in mineralized intervals along axial planar cleavage, intrafolial foliation, and shears. Mineralized intervals are hosted by a variety of metasedimentary rocks, including three phyllitic units of Mesoproterozoic age and two schistose units. All of these units are S-tectonites in the footwall of a regional thrust fault. Specifically, the district lies within an oblique thrust ramp containing a series of structural horses (three domains) in a duplex system. The deposits span the three domains and are hosted by metamorphic rocks that range from lower amphibolite facies in the structurally upper domain to lower-middle greenschist facies in the lower domain (an inverted metamorphic sequence). Early quartz and biotite veins were introduced during progressive folding and prolonged peak metamorphic conditions and they underwent late-tectonic retrograde recrystallization and metamorphic mineral growth, to the same extent as the country rocks in each domain. Where little subsequent deformation occurred, early veins are discordant to bedding but, where folding was polyphase and fabrics are penetrative, mineralized zones are concordant with metamorphic compositional layering. Late quartz veins in the zones are associated with retrograde minerals and textures and are only locally deformed. 40Ar/39Ar dating of unoriented muscovite from the selvage of a late quartz vein yields a Late Cretaceous age of about 83 Ma, the time of retrograde metamorphism associated with introduction of late quartz veins. Textural data at all scales indicate that the host sites for veins and the tectonic evolution of both host rocks and mineral deposits were kinematically linked to Late Cretaceous regional thrust faulting. Heat, fluids, and conduits for generation and circulation of fluids were part of the regional crustal thickening. The faulting also juxtaposed metaevaporite layers in the Mesoproterozoic Yellowjacket Formation over Blackbird district host rocks. We conclude that this facilitated chemical exchange between juxtaposed units resulting in leaching of critical elements (Cl, K, B, Na) from metaevaporites to produce brines, scavenging of metals (Co, Cu, etc) from rocks in the region, and, finally, concentrating metals in the lower-plate ramp structures. Although the ultimate source of the metals remains undetermined, the present Cu-Co ± Au (± Ag ± Ni ± REE) Blackbird ore deposits formed during Late Cretaceous compressional deformation.
    ABSTRACT The Blackbird district, east-central Idaho, contains the largest known Co reserves in the United States. The origin of strata-hosted Co-Cu ± Au mineralization at Blackbird has been a matter of controversy for decades. In order to... more
    ABSTRACT The Blackbird district, east-central Idaho, contains the largest known Co reserves in the United States. The origin of strata-hosted Co-Cu ± Au mineralization at Blackbird has been a matter of controversy for decades. In order to differentiate among possible genetic models for the deposits, including various combinations of volcanic, sedimentary, magmatic, and metamorphic processes, we used U-Pb geochronology of xenotime, monazite, and zircon to establish time constraints for ore formation. New age data reported here were obtained using sensitive high resolution ion microprobe (SHRIMP) microanalysis of (1) detrital zircons from a sample of Mesoproterozoic siliciclastic metasedimentary country rock in the Blackbird district, (2) igneous zircons from Mesoproterozoic intrusions, and (3) xenotime and monazite from the Merle and Sunshine prospects at Blackbird. Detrital zircon from metasandstone of the biotite phyllite-schist unit has ages mostly in the range of 1900 to 1600 Ma, plus a few Neoarchean and Paleoproterozoic grains. Age data for the six youngest grains form a coherent group at 1409 ± 10 Ma, regarded as the maximum age of deposition of metasedimentary country rocks of the central structural domain. Igneous zircons from nine samples of megacrystic granite, granite augen gneiss, and granodiorite augen gneiss that crop out north and east of the Blackbird district yield ages between 1383 ± 4 and 1359 ± 7 Ma. Emplacement of the Big Deer Creek megacrystic granite (1377 ± 4 Ma), structurally juxtaposed with host rocks in the Late Cretaceous ca. 5 km north of Blackbird, may have been involved in initial deposition of rare earth elements (REE) minerals and, possibly, sulfides. In situ SHRIMP ages of xenotime and monazite in Co-rich samples from the Merle and Sunshine prospects, plus backscattered electron imagery and SHRIMP analyses of trace elements, indicate a complex sequence of Mesoproterozoic and Cretaceous events. On the basis of textural relationships observed in thin section, xenotime and cobaltite formed during multiple episodes. The oldest age for xenotime (1370 ± 4 Ma), determined on oscillatory-zoned cores, may date the time of initial cobaltite formation, and provides a minimum age for the host metasedimentary rocks. Additional Proterozoic xenotime growth events occurred at 1315 to 1270 Ma and ca. 1050 Ma. Other xenotime grains and rims grew in conjunction with cobaltite during Cretaceous metamorphism. However, ages of these growth episodes cannot be precisely determined due to matrix effects on 206Pb/238U data for xenotime. Monazite, some of which encloses cobaltite, uniformly has Cretaceous ages that mainly are 110 ± 3 and 92 ± 5 Ma. These data indicate that xenotime, monazite, and cobaltite were extensively mobilized and precipitated during Middle to Late Cretaceous metamorphic events.