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2009-05-19_REVISION - M1977285 (28)
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2009-05-19_REVISION - M1977285 (28)
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Last modified
6/15/2021 5:39:02 PM
Creation date
5/28/2009 7:42:30 AM
Metadata
Fields
Template:
DRMS Permit Index
Permit No
M1977285
IBM Index Class Name
REVISION
Doc Date
5/19/2009
Doc Name
EPP amendment (AM-03) Hydrogeologic Evaluation Attachment O (part 9)
From
Denison Mines
To
DRMS
Type & Sequence
AM3
Email Name
RCO
Media Type
D
Archive
No
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Hydrogeological Evaluation of Sunday Mines Group <br />Geologic and Hydrologic Conditions <br />¦ Cretaceous Mancos Shale; and <br />¦ Unconsolidated Quaternary deposits. <br />The Permian Cutler Formation directly overlies the Hermosa Formation, and consists <br />predominantly of arkosic sandstone and conglomerate. Small quantities of sandy <br />shale are present within the formation. The formation has an estimated thickness that <br />approaches 3,000 ft. <br />The Culter Formation is overlain by the Upper Triassic Chinle Formation. This unit <br />consists primarily of siltstone interbedded with fine grained sandstone, shale and <br />conglomerate. The individual lithological units within the formation are lenticular <br />and discontinuous. This unit is commonly 500 to 600 ft. thick, but the unit thins along <br />the flanks of the Gypsum Valley Anticline. <br />The Chinle Formation is overlain by the Jurassic Glen Canyon Group, which consists of <br />three formations: the Wingate Sandstone, the Kayenta Formation, and the Navajo <br />Sandstone. The Wingate Sandstone overlies the Chinle Formation. This formation <br />consists of massive, fine grained sandstone composed of clean well-sorted quartz <br />sand grains. The unit contains vertical joints that extend the entire thickness of the <br />formation, which contributes to cliff formation in the project area. The Wingate <br />sandstone forms the large cliffs present on the north side of Big Gypsum Valley. <br />The Kayenta Formation overlies the Wingate Sandstone and consists of interbedded <br />sandstone, siltstone and shale. The sandstone is thin bedded, flaggy to massive, and <br />occurs in discontinuous beds that interfinger with siltstone and shale. The thickness of <br />the Kayenta Formation ranges from 180 ft. to 210 ft. <br />The Navajo Sandstone is massive fine-grained clean quartz sandstone, which overlies <br />the Kayenta Formation. This unit is eolian in origin as evidenced by very large <br />tangential cross-bedding. The formation is approximately 400 ft. thick in the project <br />area. <br />The Glenn Canyon Group is overlain by the Jurassic San Rafael Group, which includes <br />three formations: The Carmel Formation, the Entrada Sandstone, and the Summerville <br />Formation. The Carmel Formation overlies the Navajo Sandstone and consists of a <br />variety of clastic sedimentary rocks including siltstone, shale, and sandstone. This <br />unit is relatively thin with an estimated thickness of 10 to 25 ft. <br />The Entrada Sandstone overlies the Carmel Formation. This formation consists of a <br />combination of horizontally bedded and eolian-type cross bedded sandstones with a <br />bimodal grain size distribution including very fine grained sandstone (<0.0001 inches <br />(in.) grain size) and medium grained sandstone (0.02 to 0.03 in. grain size). The <br />Entrada Sandstone is 110 to 120 feet thick. <br />• <br />cm 2-3 <br />T:\64986-Denison Mines\Task Order 3 - DMO Sampling and Analysis Plan\Task 3.14 - Hydrogeology ReportVinal Sunday hydro reporNeXITINAL Sunday Hydrogeology Reporl.doc
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