| 2007 GSA Denver Annual Meeting (28–31 October 2007) | |
| Paper No. 72-8 | |
| Presentation Time: 9:45 AM-10:00 AM | ||
LEAD ISOTOPE DATA FROM PRECIOUS-METAL MINERALS: IMPLICATIONS FOR THE GENESIS OF BONANZA EPITHERMAL AU-AG-SE DEPOSITS OF THE NORTHERN GREAT BASIN, USA | ||
|
SAUNDERS, James A., Department of Geology and Geography, Auburn University, 210 Petrie Hall, Auburn, AL 36849, saundja@auburn.edu, KAMENOV, George D., Department of Geology, Univ of Florida, Gainesville, FL 32611, HAMES, Willis E., Department of Geology and Geography, Auburn Univ, Auburn, AL 36830, and UNGER, Derick L., Geology & Geography, Auburn University, 210 Petrie Hall, Auburn, AL 36849 New high-precision Pb-isotope analyses using MC-ICP-MS and 40Ar/39Ar geochronologic studies of Mid-Miocene bonanza epithermal Au-Ag(Se) ores of the northern Great Basin (NGB) add further support to the proposal that these ores are genetically related to the emergence of the Yellowstone hotspot (YHS). Our 40Ar/39Ar geochronology of adularia intergrown with precious-metal minerals in these ores indicates most of the NGB epithermal ores formed between ~16.5 and 15.5 Ma, approximately coeval with bimodal basaltic volcanism at Steens Mountain (OR) and rhyolites of the McDermitt caldera (NV) that are interpreted by many to have been formed by the initial emergence of the YHS. Lead isotope ratios measured directly on electrum and naumannite (Ag2Se) grains physically separated from vein samples were very similar in the four deposits investigated in our preliminary investigations (Sleeper, National, Jumbo, Seven Troughs). Pb-isotope signatures of electrum and naumannite did not match that of vein adularia, the latter of which was similar to the signature of closely associated host rocks (rhyolites, metasediments). Instead, Pb-isotopic signatures of precious-metal minerals match closely Mid-Miocene basaltic units in the region, as well as regionally extensive basalts of Steens Mountain and the Columbia River flood basalts. Thus we interpret our results to support the concept that primitive, mantle-derived mafic magma at depth contributed Au, Ag, and Se, (and at least some S) to the shallow epithermal environment dominated by meteoric water that leached principal major elements (e.g., K, Al, Na, silica) from the surrounding country rocks. It has been widely proposed that precious metals in epithermal ores are leached from host rocks, but our data casts serious doubt on this hypothesis. We propose that a mantle plume in conjunction with thin crust, deep structures (Northern Nevada Rift+Basin and Range faulting?), likely were important in the genesis of the Mid-Miocene epithermal deposits of the NGB. If so, then perhaps their genesis is not too different than low-temperature Tertiary Au-Ag-Te deposits associated with Rio Grande Rift (e.g., Cripple Creek, Ortiz) and Colorado Mineral Belt of Colorado. | ||
|
2007 GSA Denver Annual Meeting (28–31 October 2007)
General Information for this Meeting | ||
| Session No. 72 Au-Ag-Te-Se Deposits and Other Precious Metal Deposits Colorado Convention Center: 504 8:00 AM-12:00 PM, Monday, 29 October 2007 Geological Society of America Abstracts with Programs, Vol. 39, No. 6, p. 197 | ||
© Copyright 2007 The Geological Society of America (GSA), all rights reserved. Permission is hereby granted to the author(s) of this abstract to reproduce and distribute it freely, for noncommercial purposes. Permission is hereby granted to any individual scientist to download a single copy of this electronic file and reproduce up to 20 paper copies for noncommercial purposes advancing science and education, including classroom use, providing all reproductions include the complete content shown here, including the author information. All other forms of reproduction and/or transmittal are prohibited without written permission from GSA Copyright Permissions. | ||