Mixed-230Th/U formation ages and secondary uranium concentrations of above-water carbonates, and primary uranium concentrations of continuously submerged calcite at Devils Hole, Nevada
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For more than a half million years, dense vein calcite has been precipitating in Devils Hole, located about 115 km northwest of Las Vegas, Nevada. This process also occurs in Devils Hole Cave 2, which is hydrologically connected and situated about 200 meters north of the original Devils Hole cave. Calcite has been precipitating in this natural laboratory in oxygen isotopic equilibrium at constant temperature to a depth of at least 140 meters. This vein calcite, also called mammillary calcite because of its morphology, is suitable for high-accuracy uranium-series dating. Continuously submerged calcite contains an unbroken record of the sequential variation of the oxygen isotopic composition of water recharging this well-mixed environment. A record of stable oxygen isotopes in the continuously submerged calcite provides climate variations spanning 563 thousand years. This record displays warm and cold climate cycles. Paleoclimate modelers use the Devils Hole oxygen-isotope record to validate climate models. Model prediction is particularly relevant for the parched southwestern United States. This high-accuracy oxygen-isotope time series was used to correct published uranium-series ages of non-continuously formed calcite in two cores (see Table S1 and Figure S1), cyclically exposed by water-table decline during glacial-interglacial transitions. This method relies on the premise that the oxygen isotopic compositions of coevally precipitated calcite are identical, allowing matching calcite oxygen isotopic composition values to establish formation ages. Uranium-series ages (based on matching oxygen-isotope values) differ by thousands of years because of mobility of uranium in samples from cores collected at or above the modern water table (Table S1). As a part of this project, samples of bat guano and soil samples were analyzed for uranium concentration (see Table S2 and Figure S2). The mean uranium-238 concentration of original formation uranium within continuously submerged vein calcite (termed primary uranium) can be estimated from uranium-238 concentrations of vein calcite within samples collected from cores deeper than 20 meters below the modern water table. The mean uranium-238 mass fraction within these deep samples (Table S3) is 456 ± 100 nanograms per gram (2 sigma uncertainty, n = 45). Uranium added to calcite samples after their formation is termed secondary uranium. Secondary uranium in a calcite sample can decrease the apparent uranium-series age of that sample if its secondary uranium concentration is not accounted for. The estimated mass fraction of secondary uranium-238 within 46 samples from nine cores collected at or above the modern water table having uranium-series ages less than 296,000 years ranges from 30 to 37,046 nanograms per gram (Table S4). The estimated secondary uranium-238 concentrations within 14 samples from six cores having uranium-series ages greater than 296,000 years is shown in Table S5. Nineteen samples from eight cores (Table S6) have uranium-238 concentrations substantially lower than that of primary uranium (Table S3). Based on an evaluation of oxygen isotopic compositions of samples from core DH2-D (Table S1), the uranium-series ages between approximately 140 and 120 thousand years ago need to be increased by between 4 and 8 kyr as shown in Figure S3. Based on a comparison of oxygen isotopic compositions of folia, flowstone, and calcite from Brown’s Room, a subaerial room in Devils Hole, with those of cores DHC2-8 or DH-2 (Table S1), many formation ages of Brown’s Room samples are as much as 11,600 years too young (Table S7 and Figure S4). Figure S5 is a cross-sectional sketch of Devils Hole Cave 2 showing the estimated minimum zone of cessation of precipitation of vein (mammillary) calcite since approximately 18 to 20 thousand years ago.
Elemental Concentrations and Carbon and Oxygen Isotope Ratios in Mammillary Calcite from Devils Hole and Devils Hole II, Nevada, USA
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Elemental concentrations and stable oxygen and carbon isotope ratios are reported for five mammillary calcite specimens collected from the groundwater-filled fissures Devils Hole and Devils Hole II in the southern Amargosa Desert, south-western Nevada. Previous studies of these specimens yielded oxygen and carbon isotope chronologies of paleoclimatic and paleo hydrologic conditions over an approximately 500,000-year time period as defined by uranium series dates (Winograd and others, 1992, 2006; Landwehr and others, 1997, 2011). The elemental concentration measurements reveal additional chronologies in the mammillary calcite. The specimens were sampled by milling contiguous 0.050-inch-thick layers (1.27 millimeters) oriented approximately parallel to the free, wetted growth faces of the specimens. For three of the five specimens (cores DH-10 and DH-11, hand specimen DH-7), the oxygen and carbon isotope measurements reproduce measurements of the same milled samples made by Landwehr and others (1997) and Coplen and others (2021). For the remaining specimens (hand specimens DHC2-3 and DHC2-8), the oxygen and carbon isotope measurements reproduce isotopic records published by Coplen and others (2021) but at a coarser resolution because Coplen and others (2021) analyzed milled layers of 0.010-inch thickness (0.25 millimeters). The elemental chronologies can be dated by referring to prior studies. For DH-11, uranium series dates and interpolated ages are given by Landwehr and others (1997). For DH-7 and DH-10, ages obtained by matching oxygen and carbon isotope chronologies to the dated chronologies of DH-11 are given by Coplen and others (2021). For DHC2-3 and DHC2-8, ages can be obtained by matching the oxygen and carbon isotope chronologies presented here to the higher-resolution dated chronologies provided by Coplen and others (2021). However, age assignments should be made with caution (see, for example, Moseley and others, 2016). Devils Hole and Devils Hole II are extensional tectonic fissures that open to the land surface adjacent to the major Ash Meadows ground-water discharge area. Devils Hole II is approximately 200 meters north of Devils Hole. The fissures intersect the regional groundwater table at about 17 meters and 36 meters below land surface at Devils Hole and Devils Hole II, respectively. These localities have long been important in paleoclimate research because mammillary calcite phreatically precipitated on the fissure walls has yielded a dated continuous paleotemperature proxy record that spans several glacial cycles (Winograd and others, 1988, 1992, 2006; Ludwig and others, 1992; Coplen and others, 1994; Riggs and others, 1994; Szabo and others, 1994; Plummer and others, 2000; Kolesar and Riggs, 2004; Moseley and others, 2016; Coplen and others, 2021). References listed chronologically: Winograd, I.J., Szabo, B.J., Coplen, T.B., and Riggs, A.C., 1988, A 250,000-year climatic record from Great Basin vein calcite: implications for Milankovitch theory: Science, v. 242, p. 1275-1280, doi: 10.1126/science.242.4883.1275. Ludwig, K.R., Simmons, K.R., Szabo, B.J., Winograd, I.J., Landwehr, J.M., Riggs, A.C., and Hoffman, R.J., 1992, Mass-spectrometric Th-230-U-234-U-238 dating of the Devils Hole calcite vein: Science, v. 258, p. 284-287, doi: 10.1126/science.258.5080.284. Winograd, I.J., Coplen, T.B., Landwehr, J.M., Riggs, A.C., Ludwig, K.R., Szabo, B.J., Kolesar, P.T., and Revesz, K.M., 1992, Continuous 500,000-year climate record from vein calcite in Devils Hole, Nevada: Science, v. 258, p. 255-260, doi: 10.1126/science.258.5080.255. Coplen, T.B., Winograd, I.J., Landwehr, J.M., and Riggs, A.C., 1994, 500,000-year stable carbon isotope record from Devils Hole, Nevada: Science, v. 263, p. 361-365, doi: 10.1126/science.263.5145.361. Szabo, B.J., Kolesar, P.T., Riggs, A.C., Winograd, I.J., and Ludwig, K.R., 1994, Paleoclimatic inferences from a 120,000-year calcite record of water-table fluctuation in Browns Room of
Elemental Concentrations and Carbon and Oxygen Isotope Ratios in Mammillary Calcite from Devils Hole and Devils Hole II, Nevada, USA
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Elemental concentrations and stable oxygen and carbon isotope ratios are reported for five mammillary calcite specimens collected from the groundwater-filled fissures Devils Hole and Devils Hole II in the southern Amargosa Desert, south-western Nevada. Previous studies of these specimens yielded oxygen and carbon isotope chronologies of paleoclimatic and paleo hydrologic conditions over an approximately 500,000-year time period as defined by uranium series dates (Winograd and others, 1992, 2006; Landwehr and others, 1997, 2011). The elemental concentration measurements reveal additional chronologies in the mammillary calcite. The specimens were sampled by milling contiguous 0.050-inch-thick layers (1.27 millimeters) oriented approximately parallel to the free, wetted growth faces of the specimens. For three of the five specimens (cores DH-10 and DH-11, hand specimen DH-7), the oxygen and carbon isotope measurements reproduce measurements of the same milled samples made by Landwehr and others (1997) and Coplen and others (2021). For the remaining specimens (hand specimens DHC2-3 and DHC2-8), the oxygen and carbon isotope measurements reproduce isotopic records published by Coplen and others (2021) but at a coarser resolution because Coplen and others (2021) analyzed milled layers of 0.010-inch thickness (0.25 millimeters). The elemental chronologies can be dated by referring to prior studies. For DH-11, uranium series dates and interpolated ages are given by Landwehr and others (1997). For DH-7 and DH-10, ages obtained by matching oxygen and carbon isotope chronologies to the dated chronologies of DH-11 are given by Coplen and others (2021). For DHC2-3 and DHC2-8, ages can be obtained by matching the oxygen and carbon isotope chronologies presented here to the higher-resolution dated chronologies provided by Coplen and others (2021). However, age assignments should be made with caution (see, for example, Moseley and others, 2016). Devils Hole and Devils Hole II are extensional tectonic fissures that open to the land surface adjacent to the major Ash Meadows ground-water discharge area. Devils Hole II is approximately 200 meters north of Devils Hole. The fissures intersect the regional groundwater table at about 17 meters and 36 meters below land surface at Devils Hole and Devils Hole II, respectively. These localities have long been important in paleoclimate research because mammillary calcite phreatically precipitated on the fissure walls has yielded a dated continuous paleotemperature proxy record that spans several glacial cycles (Winograd and others, 1988, 1992, 2006; Ludwig and others, 1992; Coplen and others, 1994; Riggs and others, 1994; Szabo and others, 1994; Plummer and others, 2000; Kolesar and Riggs, 2004; Moseley and others, 2016; Coplen and others, 2021). References listed chronologically: Winograd, I.J., Szabo, B.J., Coplen, T.B., and Riggs, A.C., 1988, A 250,000-year climatic record from Great Basin vein calcite: implications for Milankovitch theory: Science, v. 242, p. 1275-1280, doi: 10.1126/science.242.4883.1275. Ludwig, K.R., Simmons, K.R., Szabo, B.J., Winograd, I.J., Landwehr, J.M., Riggs, A.C., and Hoffman, R.J., 1992, Mass-spectrometric Th-230-U-234-U-238 dating of the Devils Hole calcite vein: Science, v. 258, p. 284-287, doi: 10.1126/science.258.5080.284. Winograd, I.J., Coplen, T.B., Landwehr, J.M., Riggs, A.C., Ludwig, K.R., Szabo, B.J., Kolesar, P.T., and Revesz, K.M., 1992, Continuous 500,000-year climate record from vein calcite in Devils Hole, Nevada: Science, v. 258, p. 255-260, doi: 10.1126/science.258.5080.255. Coplen, T.B., Winograd, I.J., Landwehr, J.M., and Riggs, A.C., 1994, 500,000-year stable carbon isotope record from Devils Hole, Nevada: Science, v. 263, p. 361-365, doi: 10.1126/science.263.5145.361. Szabo, B.J., Kolesar, P.T., Riggs, A.C., Winograd, I.J., and Ludwig, K.R., 1994, Paleoclimatic inferences from a 120,000-year calcite record of water-table fluctuation in Browns Room of
U-Pb age determinations of uraninite by electron microprobe analyses of ore samples from two solution-collapse breccia pipe uranium deposits, Grand Canyon region, northwest Arizona, USA
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This data release compiles the electron microprobe spot analyses of U, Th, and Pb concentrations in uraninite (U oxide) particles, and corresponding calculated age determinations, measured in samples of ore from two uranium-copper breccia pipe ore bodies, the Canyon (Pinyon Plain) and Hack II deposits. The U-rich samples that were analyzed typify the deposits hosted by solution-collapse breccia pipes in the Grand Canyon region of northwestern Arizona. Applying procedures outlined by Bowles (1990), the U, Pb, and Th measurements from each spot analysis were used to calculate a model age for the formation of each uraninite particle. The U, Pb, and Th analyses and calculated age determinations are provided as additional information on the timing and origin of the uranium deposition within the unusual breccia pipe deposits of northwestern Arizona. One of the analyzed samples (CMCH-053-21A) was selected from drill core of a U-Cu ore body of the Canyon deposit, hosted in a solution-collapse breccia pipe. This deposit lies about 750 to 2,000 ft (230 to 610 m) below the surface about 6.1 miles (10 km) south-southeast of Tusayan, Arizona, at latitude 35.88333 North, longitude -112.09583 West (datum WGS 1984). Energy Fuels Inc., owner and operator of the property, conducted extensive drilling into the Canyon deposit, delineating the extent and uranium and copper content of the ore bodies (Mathisen and others, 2017). Mining facilities, including a shaft, have been developed by Energy Fuels at the deposit. The company renamed the Canyon mine as the “Pinyon Plain mine” in 2021. As of October 2021, they await favorable economic conditions to resume mining operations and recover the ore. An earlier-published data release (Van Gosen and others, 2020a) provides the geochemical analyses of 63 elements for 35 drill core samples of the Canyon deposit that were collected by the USGS. X-ray diffraction (XRD) analyses were performed on 28 of these samples to examine their mineralogy; the raw XRD data are provided in Van Gosen and others (2020a). In addition to the XRD analyses, ore mineralogy was also determined by examinations of thin sections of 21 of the ore samples using a scanning electron microscope equipped with an energy dispersive spectrometer (SEM-EDS). The mineralogical analyses are published in Van Gosen and others (2020c). The bulk geochemistry and mineralogy of Canyon deposit sample CHCH-053-21A, analyzed in this study, is provided in Van Gosen and others (2020a, 2020b). The geochemical and mineralogical analysis of ore samples collected from the Hack II deposit, also hosted by a solution-collapse breccia pipe, are published in another data release (Van Gosen and others, 2020b). That data release includes the bulk geochemistry and mineralogy of samples 84-HJW-12 and 84-HJW-3A, which were examined by this study. The Hack II deposit is one of four breccia pipes mined in Hack Canyon near its intersection with Robinson Canyon, approximately 30 miles (48 km) southwest of Fredonia and 9 miles (14.5 km) north-northwest of Kanab Creek, at latitude 36.58219 north, longitude -112.81059 west (datum of WGS84). Mining began at Hack II in 1981 and ended in May 1987. The USGS collected the samples from the Hack II mine in 1984 from underground exposures during active mining. The Canyon and Hack II deposits are representative of numerous other uranium deposits hosted by solution-collapse breccia pipes in the Grand Canyon region of northwest Arizona. These U-Cu deposits occur within matrix-supported, vertical columns of breccia (a "breccia pipe") that formed by solution and collapse of sedimentary strata (Wenrich, 1985; Alpine, 2010). The breccia pipes average about 300 ft (90 m) in diameter and can extend vertically for as much as 3,000 ft (900 m), from their base in the Mississippian Redwall Limestone to as stratigraphically high as the Triassic Chinle Formation. The regions north, south, and east of the Grand Canyon host hundreds of
U-Pb age determinations of uraninite by electron microprobe analyses of ore samples from two solution-collapse breccia pipe uranium deposits, Grand Canyon region, northwest Arizona, USA
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This data release compiles the electron microprobe spot analyses of U, Th, and Pb concentrations in uraninite (U oxide) particles, and corresponding calculated age determinations, measured in samples of ore from two uranium-copper breccia pipe ore bodies, the Canyon (Pinyon Plain) and Hack II deposits. The U-rich samples that were analyzed typify the deposits hosted by solution-collapse breccia pipes in the Grand Canyon region of northwestern Arizona. Applying procedures outlined by Bowles (1990), the U, Pb, and Th measurements from each spot analysis were used to calculate a model age for the formation of each uraninite particle. The U, Pb, and Th analyses and calculated age determinations are provided as additional information on the timing and origin of the uranium deposition within the unusual breccia pipe deposits of northwestern Arizona. One of the analyzed samples (CMCH-053-21A) was selected from drill core of a U-Cu ore body of the Canyon deposit, hosted in a solution-collapse breccia pipe. This deposit lies about 750 to 2,000 ft (230 to 610 m) below the surface about 6.1 miles (10 km) south-southeast of Tusayan, Arizona, at latitude 35.88333 North, longitude -112.09583 West (datum WGS 1984). Energy Fuels Inc., owner and operator of the property, conducted extensive drilling into the Canyon deposit, delineating the extent and uranium and copper content of the ore bodies (Mathisen and others, 2017). Mining facilities, including a shaft, have been developed by Energy Fuels at the deposit. The company renamed the Canyon mine as the “Pinyon Plain mine” in 2021. As of October 2021, they await favorable economic conditions to resume mining operations and recover the ore. An earlier-published data release (Van Gosen and others, 2020a) provides the geochemical analyses of 63 elements for 35 drill core samples of the Canyon deposit that were collected by the USGS. X-ray diffraction (XRD) analyses were performed on 28 of these samples to examine their mineralogy; the raw XRD data are provided in Van Gosen and others (2020a). In addition to the XRD analyses, ore mineralogy was also determined by examinations of thin sections of 21 of the ore samples using a scanning electron microscope equipped with an energy dispersive spectrometer (SEM-EDS). The mineralogical analyses are published in Van Gosen and others (2020c). The bulk geochemistry and mineralogy of Canyon deposit sample CHCH-053-21A, analyzed in this study, is provided in Van Gosen and others (2020a, 2020b). The geochemical and mineralogical analysis of ore samples collected from the Hack II deposit, also hosted by a solution-collapse breccia pipe, are published in another data release (Van Gosen and others, 2020b). That data release includes the bulk geochemistry and mineralogy of samples 84-HJW-12 and 84-HJW-3A, which were examined by this study. The Hack II deposit is one of four breccia pipes mined in Hack Canyon near its intersection with Robinson Canyon, approximately 30 miles (48 km) southwest of Fredonia and 9 miles (14.5 km) north-northwest of Kanab Creek, at latitude 36.58219 north, longitude -112.81059 west (datum of WGS84). Mining began at Hack II in 1981 and ended in May 1987. The USGS collected the samples from the Hack II mine in 1984 from underground exposures during active mining. The Canyon and Hack II deposits are representative of numerous other uranium deposits hosted by solution-collapse breccia pipes in the Grand Canyon region of northwest Arizona. These U-Cu deposits occur within matrix-supported, vertical columns of breccia (a "breccia pipe") that formed by solution and collapse of sedimentary strata (Wenrich, 1985; Alpine, 2010). The breccia pipes average about 300 ft (90 m) in diameter and can extend vertically for as much as 3,000 ft (900 m), from their base in the Mississippian Redwall Limestone to as stratigraphically high as the Triassic Chinle Formation. The regions north, south, and east of the Grand Canyon host hundreds of
Water-Quality and Borehole Geophysical Data Associated with Uranium Background Concentrations at the Homestake Superfund Site near Milan, New Mexico: 2016 (ver. 1.2)
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The datasets contained herein were collected as part of a cooperative U.S. Geological Survey (USGS) and U.S. Environmental Protection Agency (EPA) project entitled "Field Investigations to Help Support the Assessment of Background Concentrations for Uranium at the Homestake Mining Company, Superfund Site near Milan, New Mexico, July 2016." Groundwater samples were collected from pre-selected wells and analyzed for metals (including uranium), alkalinity, ammonia, common ions, nitrogen, gross alpha/beta, radium isotopes, Radon-22, uranium isotopes, stable isotopes, sulfur isotopes, nitrogen isotopes, helium-4, dissolved gases, tritium/helium-3, carbon-14 and chlorofluorocarbons. Groundwater samples were collected using micropurge, volumetric, and passive samplers. Seven different laboratories analyzed the samples; separate datasets containing the results from each laboratory are provided in this data release. Microsoft excel .xlsx, xml, and tab-delimited text files are included for most dataset. A subset of the files are in .csv format.
Data for Uranium-Lead Geochronology, Carbon and Sulfur Stable Isotopes, and Raman Spectroscopy from Graphite Creek, Alaska
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This data release supports the paper titled, "Insights into the metamorphic history and origin of flake graphite mineralization at the Graphite Creek graphite deposit, Seward Peninsula, Alaska, USA", published in the journal Mineralium Deposita. The data release includes zircon and titanite U-Pb-Thisotope and age data, monazite U-Pb-Th isotope, trace element and age data, carbon and sulfur stableisotope data, and graphite Raman spectroscopy data, from samples collected at the Graphite Creek deposit, Alaska. Sample location information and descriptions are in table "sample_descriptions.csv". The raw numerical data are presented in tabular format. Additionally, plots of select zircon data – conventional discordia, U/Th vs age, U (ppm) vs age, and percent discordance vs age – are included in PDF format (zircon_plots.pdf), along with scanning electron microscope cathodoluminescence images of zircon in TIFF format. Folder "zircon_data" contains all zircon numerical data, plots, and images. Table "raman_peak_fits.csv" contains all raw Raman spectra peak fit data. Table "monazite_isotopic_data.csv" contains all monazite data. Table "carbon_sulfur_isotopic_data.csv" contains all carbon and sulfur data. Interpretations of the data are presented in the aforementioned journal paper.
Water-Quality and Borehole Geophysical Data Associated with Uranium Background Concentrations at the Homestake Superfund Site near Milan, New Mexico: 2016 (ver. 1.2)
공공데이터포털
The datasets contained herein were collected as part of a cooperative U.S. Geological Survey (USGS) and U.S. Environmental Protection Agency (EPA) project entitled "Field Investigations to Help Support the Assessment of Background Concentrations for Uranium at the Homestake Mining Company, Superfund Site near Milan, New Mexico, July 2016." Groundwater samples were collected from pre-selected wells and analyzed for metals (including uranium), alkalinity, ammonia, common ions, nitrogen, gross alpha/beta, radium isotopes, Radon-22, uranium isotopes, stable isotopes, sulfur isotopes, nitrogen isotopes, helium-4, dissolved gases, tritium/helium-3, carbon-14 and chlorofluorocarbons. Groundwater samples were collected using micropurge, volumetric, and passive samplers. Seven different laboratories analyzed the samples; separate datasets containing the results from each laboratory are provided in this data release. Microsoft excel .xlsx, xml, and tab-delimited text files are included for most dataset. A subset of the files are in .csv format.
Water-Quality and Borehole Geophysical Data Associated with Uranium Background Concentrations at the Homestake Superfund Site near Milan, New Mexico: 2016 (ver. 1.2)
공공데이터포털
The datasets contained herein were collected as part of a cooperative U.S. Geological Survey (USGS) and U.S. Environmental Protection Agency (EPA) project entitled "Field Investigations to Help Support the Assessment of Background Concentrations for Uranium at the Homestake Mining Company, Superfund Site near Milan, New Mexico, July 2016." Groundwater samples were collected from pre-selected wells and analyzed for metals (including uranium), alkalinity, ammonia, common ions, nitrogen, gross alpha/beta, radium isotopes, Radon-22, uranium isotopes, stable isotopes, sulfur isotopes, nitrogen isotopes, helium-4, dissolved gases, tritium/helium-3, carbon-14 and chlorofluorocarbons. Groundwater samples were collected using micropurge, volumetric, and passive samplers. Seven different laboratories analyzed the samples; separate datasets containing the results from each laboratory are provided in this data release. Microsoft excel .xlsx, xml, and tab-delimited text files are included for most dataset. A subset of the files are in .csv format.