|
|
|
|||||||||||||||||
| JOURNAL HOME | HELP | CONTACT PUBLISHER | SUBSCRIBE | ARCHIVE | SEARCH | TABLE OF CONTENTS |

U. S. Geological Survey, Mail Stop 905, P. O. Box 25046, Denver, Colorado 80225
Corresponding author: email, cnutt{at}usgs.gov, ahofstra@usgs.gov
Carlin-type deposits in the Alligator Ridge mining district are present
sporadically for 40 km along the north-striking Mooney Basin fault system but
are restricted to a 250-m interval of Devonian to Mississippian strata. Their
age is bracketed between silicified ca. 45 Ma sedimentary rocks and unaltered
36.5 to 34 Ma volcanic rocks. The silicification is linked to the deposits by
its continuity with ore-grade silicification in Devonian-Mississippian strata
and by its similar
18O
values (~17
) and trace element signature (As, Sb, Tl, Hg). Eocene
reconstruction indicates that the deposits formed at depths of <300 to 800 m.
In comparison to most Carlin-type gold deposits, they have lower Au/Ag, Au
grades, and contained Au, more abundant jasperoid, and textural evidence for
deposition of an amorphous silica precursor in jasperoid. These differences most
likely result from their shallow depth of formation.
The peak fluid temperature (~230°C) and large
18OH2O
value shift from the meteroric water line (~20
) suggest that ore fluids were
derived from depths of 8 km or more. A magnetotelluric survey indicates that the
Mooney Basin fault system penetrates to mid-crustal depths. Deep circulation of
meteoric water along the Mooney Basin fault system may have been in response to
initial uplift of the East Humboldt-Ruby Mountains metamorphic core complex;
convection also may have been promoted by increased heat flow associated with
large magnitude extension in the core complex and regional magmatism. Ore fluids
ascended along the fault system until they encountered impermeable Devonian and
Mississippian shales, at which point they moved laterally through permeable
strata in the Devonian Guilmette Formation, Devonian-Mississippian Pilot Shale,
Mississippian Joana Limestone, and Mississippian Chainman Shale toward erosional
windows where they ascended into Eocene fluvial conglomerates and lake
sediments. Most gold precipitated by sulfidation of host-rock Fe and mixing with
local ground water in zones of lateral fluid flow in reactive strata, such as
the Lower Devonian-Mississippian Pilot Shale.
This article has been cited by other articles:
![]() |
B. W. Rockwell and A. H. Hofstra Identification of quartz and carbonate minerals across northern Nevada using ASTER thermal infrared emissivity data--Implications for geologic mapping and mineral resource investigations in well-studied and frontier areas Geosphere, February 1, 2008; 4(1): 218 - 246. [Abstract] [Full Text] [PDF] |
||||
![]() |
C. J. Nutt and A. H. Hofstra Bald Mountain Gold Mining District, Nevada: A Jurassic Reduced Intrusion-Related Gold System Economic Geology, September 1, 2007; 102(6): 1129 - 1155. [Abstract] [Full Text] [PDF] |
||||
![]() |
A. H. Hofstra, A. H. Hofstra, D. A. John, and T. G. Theodore A Special Issue Devoted to Gold Deposits in Northern Nevada: Part 2. Carlin-Type Deposits Economic Geology, September 1, 2003; 98(6): 1063 - 1067. [Full Text] [PDF] |
||||
| JOURNAL HOME | HELP | CONTACT PUBLISHER | SUBSCRIBE | ARCHIVE | SEARCH | TABLE OF CONTENTS |