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Research about north-central Nevada

Source-linked reports with geographic coverage including north-central Nevada.

3 recordsLinked to original sources
USGS2003

Geophysical and isotopic constraints on crustal structure related to mineral trends in north-central Nevada and implications for tectonic history

We combined information from Sr and Pb isotope data and magnetotelluric models to develop a new magnetic and gravity interpretation of the crustal structure of north - central Nevada to better understand the origin of mineral trends . The new interpretation suggests a crustal structure that is composed of Precambrian continental crust, transitional crust, and primarily oceanic crust that are separated by northwest- and northeast-striking fault zones. The magnetic expression of the buried Precambrian continental crust is recognized for the first time. Low magnetic values primarily reflect magnetite-poor crystalline crust rather than elevated temperatures at depth. Northwest- and northeast-striking crustal boundaries are defined by isotopic data and abrupt gradients in gravity and magnetic data. The Carlin and Battle Mountain-Eureka mineral trends are associated with two of three northwest-striking boundaries. The Carlin boundary is primarily defined by a change in density and isotopic character of the lower to middle crust. The Battle Mountain-Eureka boundary coincides with a density contrast in the upper crust and a change in isotopic character in the lower to middle crust. Magnetotelluric models suggest that the Battle Mountain-Eureka boundary represents a crustal fault zone for most of its extent, but that deep-rooted faulting is more complex near and northwest of Battle Mountain. Crustal fault zones inferred from the magnetotelluric models near the Carlin trend are oblique to it, suggesting that they may not have been controlled by the deep boundary seen in the gravity and isotopic data. The third northwest-trending boundary is related to the western edge of the buried Precambrian continent in west- central Nevada , but lacks an associated mineral trend . A northeast-striking boundary forms the northern limit of Precambrian continental and transitional crust. The boundaries may have originated as rift or transform faults during Precambrian breakup of Rodinia or as faults accommodating lateral movements or accretion during later Paleozoic tectonic events. Comparing the crustal structure to tectonic elements produced by successively younger events shows that it had a profound influence on subsequent sedimentation, deformation, magmatism, extension, and most important, mineralization.

Nevada↗
USGS2003

Geologic setting and genesis of the Mule Canyon low-sulfidation epithermal gold-silver deposit, north-central Nevada

The Mule Canyon mine exploited shallow, low - sulfidation , epithermal Au-Ag deposits that lie near the west side of the Northern Nevada rift in northern Lander County, Nevada . Mule Canyon consists of six small deposits that contained premining reserves of about 8.2 Mt at an average grade of 3.81 g Au/tonne. It is an uncommon mafic end member of low - sulfidation Au-Ag deposits associated with tholeiitic bimodal basalt-rhyolite magmatism. The ore is hosted by a basalt-andesite eruptive center that formed between about 16.4 to 15.8 Ma during early mafic eruptions related to regionally extensive bimodal magmatism. Hydrothermal alteration and Au-Ag ores formed at about 15.6 Ma and were tightly controlled by north -northwest- to north -striking high-angle fault and breccia zones developed during rifting, emplacement of mafic dikes, and eruption of mafic lava flows. Hydrothermal alteration assemblages are zoned outward from fluid conduits in the sequence silica-adularia, adularia-smectite, smectite (intermediate argillic), and smectite-carbonate (propylitic). All alteration types contain abundant pyrite and/or marcasite ± arsenopyrite. Field relations indicate that silica-adularia alteration is superimposed on argillic and propylitic alteration. Little or no steam-heated acid-sulfate alteration is present, probably the result of a near-surface water table during hydrothermal alteration and ore deposition. Two distinct ore types are present at Mule Canyon : early replacement and later open-space filling. Replacement ores consist of disseminated and vesicle-filling pyrite, marcasite, and arsenopyrite in argillically altered or weakly silicified rocks. Ore minerals consist of Au-bearing arsenopyrite and arsenian pyrite overgrowths on earlier-formed pyrite and marcasite. Open-space filling ores include narrow stockwork quartz-adularia veins, banded and crustiform opaline and chalcedonic silica-adularia veins, silica-adularia cemented breccias, and sparse carbonate-pyrite and/or marcasite veins. Ore minerals consist mostly of electrum and Ag sulfide and selenide minerals, with minor to major amounts of pyrite, marcasite, and arsenopyrite, and local stibnite. Both types of ores have similar geochemical signatures, characterized by high Au, Ag, As, Sb, and Se contents, locally high Hg, Mo, Tl, and W contents, and low Cu, Pb, and Zn contents. Stable isotope data indicate that ore fluids consisted dominantly of meteoric water that evolved by deep circulation through Paleozoic sedimentary rocks at low water/rock ratios (about 1) and high temperatures (>200°C). Calculated isotopic compositions of ore fluids are δ 18 O H2O = -3 to -7 per mil, δD H2O = -107 to -124 per mil, δ 13 C CO2 = 0 to -6 per mil, and δ 34 S H2S = -3 to +8 per mil. The ore fluids obtained much of their H 2 S and CO 2 and probably scavenged ore metals and trace elements from the Paleozoic sedimentary rocks. Some H 2 S and CO 2 may have been derived from degassing Miocene magmas. Mule Canyon formed at shallow depths, probably about 100 m below the paleosurface. Ore fluids were dilute, nearly neutral in pH, reduced, H 2 S-rich, and CO 2 -bearing. Peak temperatures in ore zones reached 230° to 265°C at nearly lithostatic pressures when some crystalline quartz ± adularia precipitated, but most ore formed at temperatures <200°C at near hydrostatic pressures and was accompanied by precipitation of opaline and chalcedonic silica ± adularia ± calcite and dolomite. Deposition of gold in As-rich overgrowths on pyrite and/or marcasite in disseminated ores occurred owing to decreasing H 2 S in the ore fluids resulting from sulfidation reactions. Later electrum and Ag selenide precipitation in open spaces occurred owing to boiling, loss of H 2 S to the vapor phase, and cooling. Mule Canyon is similar to most other low - sulfidation Au-Ag deposits associated with Miocene tholeiitic bimodal basalt-rhyolite magmatism in the Great Basin, such as Sleeper, Midas, and Buckhorn. Major differences at Mule Canyon are the high Fe sulfide contents of some ores and altered wall rocks, the paucity of silicification, and the presence of only narrow and discontinuous gold -bearing siliceous veins. These differences primarily are due to the mafic composition of the host rocks. Mule Canyon differs from low - sulfidation deposits associated with subduction-related calc-alkaline porphyry intrusions, such as the Comstock lode, in that a much smaller proportion of water, salts, and metals was derived from crystallizing magmas.

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