Eocene Challis Magmatism in the Western Part of the Thunder Mountain Volcanic Field and Adjacent Stibnite-Yellow Pine Au-Sb-W-Hg Mining District, Central Idaho

Abstract The Stibnite-Yellow Pine gold-antimony-tungsten-mercury (Au-Sb-W-Hg) mining district, an important source of antimony (Sb) and tungsten (W) in World War II with a major (~7 Moz) Au resource, is located a few kilometers west of the Thunder Mountain volcanic field on the northwestern edge of the Eocene Challis magmatic complex in west-central Idaho. Using new field studies,40Ar/39Ar and U/Pb geochronology, and major and trace element and isotope geochemistry, we document the stratigraphy of the western part of the Thunder Mountain volcanic field and the ages of related dikes in the Stibnite-Yellow Pine mining district and Pistol Creek dike swarm. The volcanic succession is divisible into a lower section of dacitic tuffs and lavas (ca. 49.5–48.0 Ma) and an upper section of rhyolitic lavas and tuffs (ca. 47.6–46.5 Ma), locally capped by trachyandesite flows (ca. 42.6 Ma). Dikes in the Stibnite-Yellow Pine mining district similarly range from basaltic andesite to rhyolite. Dike ages range from dacitic dikes as old as ca. 49.3 Ma to rhyolitic dikes as young as ca. 46.9 Ma; the emplacement age of basaltic andesite dikes has not been determined. Geochemical and isotopic compositions of igneous rock units of the western Challis magmatic complex indicate they can be clustered into four petrologic groups, which differ in source characteristics and/or in fractionation history. Although Challis magmatism was synchronous with extensional tectonism and detachment faulting, the broader tectonic setting of Challis magmatism is controversial. Despite exhibiting the geochemical hallmarks of subduction-related magmatism, most authors interpret these igneous rocks to have been derived by partial melting of the previously subduction-modified lithospheric mantle that was heated by upwelling asthenosphere in the Eocene. Epithermal Au-Ag mineralization in the Thunder Mountain mining district, located centrally in the Thunder Mountain volcanic field about 15 km northeast of Stibnite, is dated here at 46.0 ± 0.4 Ma. This age postdates the episodes of Au and W mineralization in the nearby Stibnite-Yellow Pine mining district but overlaps in age with its youngest mineralization episode of Sb-Hg ores.

Authors

Institutions

Publication Details

Journal
Economic Geology
Published
2025-12-01
DOI
https://doi.org/10.5382/econgeo.5050
Citations
3
Primary Topic
Geological and Geochemical Analysis
Type
article
Field-Weighted Citation Impact
5.60
Controls
|||
ALL TIME
JAN
FEB
MAR
APR
MAY
JUN
JUL
AUG
SEP
OCT
article

Eocene Challis Magmatism in the Western Part of the Thunder Mountain Volcanic Field and Adjacent Stibnite-Yellow Pine Au-Sb-W-Hg Mining District, Central Idaho

J.V. Box, David A. John, Leah E. Morgan, Jorge A. Vázquez et al.
3 citations
Economic Geology
Geological and Geochemical Analysis
5.60
article

Eocene Challis Magmatism in the Western Part of the Thunder Mountain Volcanic Field and Adjacent Stibnite-Yellow Pine Au-Sb-W-Hg Mining District, Central Idaho

J.V. Box, David A. John, Leah E. Morgan, Jorge A. Vázquez, Michael A. Cosca, Christopher S. Holm-Denoma, Wayne R. Premo
article en
3 citations

Abstract

Abstract The Stibnite-Yellow Pine gold-antimony-tungsten-mercury (Au-Sb-W-Hg) mining district, an important source of antimony (Sb) and tungsten (W) in World War II with a major (~7 Moz) Au resource, is located a few kilometers west of the Thunder Mountain volcanic field on the northwestern edge of the Eocene Challis magmatic complex in west-central Idaho. Using new field studies,40Ar/39Ar and U/Pb geochronology, and major and trace element and isotope geochemistry, we document the stratigraphy of the western part of the Thunder Mountain volcanic field and the ages of related dikes in the Stibnite-Yellow Pine mining district and Pistol Creek dike swarm. The volcanic succession is divisible into a lower section of dacitic tuffs and lavas (ca. 49.5–48.0 Ma) and an upper section of rhyolitic lavas and tuffs (ca. 47.6–46.5 Ma), locally capped by trachyandesite flows (ca. 42.6 Ma). Dikes in the Stibnite-Yellow Pine mining district similarly range from basaltic andesite to rhyolite. Dike ages range from dacitic dikes as old as ca. 49.3 Ma to rhyolitic dikes as young as ca. 46.9 Ma; the emplacement age of basaltic andesite dikes has not been determined. Geochemical and isotopic compositions of igneous rock units of the western Challis magmatic complex indicate they can be clustered into four petrologic groups, which differ in source characteristics and/or in fractionation history. Although Challis magmatism was synchronous with extensional tectonism and detachment faulting, the broader tectonic setting of Challis magmatism is controversial. Despite exhibiting the geochemical hallmarks of subduction-related magmatism, most authors interpret these igneous rocks to have been derived by partial melting of the previously subduction-modified lithospheric mantle that was heated by upwelling asthenosphere in the Eocene. Epithermal Au-Ag mineralization in the Thunder Mountain mining district, located centrally in the Thunder Mountain volcanic field about 15 km northeast of Stibnite, is dated here at 46.0 ± 0.4 Ma. This age postdates the episodes of Au and W mineralization in the nearby Stibnite-Yellow Pine mining district but overlaps in age with its youngest mineralization episode of Sb-Hg ores.

Economic GeologyVol. 120(8)
United States Geological Survey (US), Denver Federal Center (US)
Openalex Percentile: Top 4%
Geological and Geochemical Analysis
5.60
AI Navigator

Ask Laika to Summarize, Analyze, and Connect papers live on the map.

Summarize Papers & Methodologies

Extract key findings, datasets, and comparative methods across publications.

Benchmark Rankings & Visual Analytics

Rank top research institutions, authors, funders, topics, and journals by Field-Weighted Citation Impact (FWCI) and paper volume with instant charts.

Connect Distant Disciplines

Bridge topological clusters on the map to find hidden collaborative intersections.