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ERIKA Project
Guerrero State, Mexico
SEM and Gold deportment study
Prepared for:
Tarsis Resources Ltd
1103-750 W Pender St
Vancouver, BC
Canada, V6C 2T8
Tel: +1 (604) 689 7644
Fax: +1 (604) 689 7645
By:
Venessa Bennett (Ph.D)
Consulting Geologist
33 Roundel Rd
Whitehorse, YT
Canada, Y1A 3H4
Tel: +1 (867) 335 5245
Email: [email protected]
Key Point Summary
Polished thin sections were prepared for 6 samples from the 2011 drill program completed on the
Erika project of Tarsis Resources Ltd. Standard binocular and petrographic microscopy was carried out
on these polished thin sections and subsequently prepared for Scanning electron microscopy (SEM)
modal mapping and mineral analysis.
SEM mineral mapping completed on 6 polished thin sections from Au mineralized samples
demonstrates the presence of several ore fluid processes that are analogous to Carlin‐style
mineralization including decalcification, decarbonatization, argillization and associated silicification of
calcareous siltstone.
Decalcification (removal of Ca) and formation of dolomite occurs in samples more distal to higher
grade Au mineralization. Samples more proximal are devoid of dolomite. Decarbonatization (complete
removal of carbonate) is associated with the influx of illite, quartz and pyrite.
Pyrite grains within zones of intense decarbonatization are distinct in the occurrence of 'fuzzy'
arsenian rich pyrite growth either as fine‐grained disseminated grains or as thin micron scale rims on
different generations of pre‐existing pyrite. Arsenian rich pyrite is interpreted to be associated with Au
mineralization.
Arsenic rich clay is associated with the growth of arseniosiderite in samples that are devoid of
arsenic sulphides and pyrite. Micron scale native gold is observed within arseniosiderite grains and
disseminated within the matrix of As rich clay.
Pathfinder elements, As‐Hg‐Sb‐Tl are either highy anomalous or show moderate to strong
correlation within gold. The elements were observed to have mineral hosts of orpiment, realgar, As‐clay,
arseniosiderite and arsenian pyrite, cinnabar and stibnite, respectively. The mineral host for Tl was not
observed.
Two types of structures were observed to be associated with sediment hosted Au‐mineralization at
Erika including, (ii) high‐angle brittle, normal and dilational faults and calcite vein faults that occur within
the peripheral calcite vein halo and (ii) bedding parallel to subparallel shear zones that postdate high
angle structures and locally preserve reidel shear geometries.
Collectively, the macro and microscale datasets available for the Erika property support the
interpretation of a sediment‐hosted gold target (Carlin‐style) as opposed to a high‐sulphidation
epithermal target.
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1.0 Introduction
Sediment‐hosted gold mineralization was recently discovered on Erika property, Guerrero state,
Mexico, 2011 (Fig. 1) by Tarsis Resources Ltd. Previous exploration programs, that included geological
mapping, soil and silt geochemical sampling and an 8‐hole drill program, were conducted by Almaden
Minerals and focussed on delineation of high sulphidation Au‐Ag epithermal mineralization. The Coacoyula
area, which is known for historical epithermal mercury deposits, also exhibits intense clay alteration
consisting of kaolinite‐alunite‐dickite‐svanbergite‐gypsum associated with opaline and massive silicification,
and local dolomitization of limestone host rocks (Fonseca, 2007). Drill results yielded no significant high
sulphidation Au‐Ag mineralization, however, one of the 8 drill holes (97‐EK‐03) intersected 1,078 ppb Au,
immediately above a fault intersection.
In 2010, Tarsis Resources Ltd initiated a drill program to test the source of a central As‐Hg‐Sb soil
geochemical anomaly (Drill Transect 1). Eight drill holes were completed along an E‐W transect, immediately
south of the town of Coacoyula. Despite intense clay, Hg and iron oxide mineralization in the host limestone,
no significant gold mineralization was intersected. After review of both the 1997 and 2010 drill core, a
second E‐W drill transect was designed to assess potential extension of Au mineralization that had been
intersected in DDH 97‐EK‐03. Au mineralization was intersected in 4 of 5 holes, with best interval 1.14g/t
over 10.28m.
Mineralization encountered did not share characteristics of typical high‐sulphidation epithermal
targets, but rather exhibited many features consistent with sediment‐hosted gold mineralization. In order to
verify the style of alteration and mineralization intersected in the 2011, transect B drill program, a suite of
samples were collected from several mineralized intervals to complete petrographic and Scanning Electron
Microscope (SEM) studies. The core objectives of the study included:
(1) Documentation of the location and intensity of decarbonatization within the mineralized
intervals and assessment of the relationship to gold mineralization.
(2) Assessment of which minerals hosted key pathfinder elements As‐Hg‐Tl‐Sb within the
mineralized intervals sampled.
(3) A Au deportment study to define the mode of gold occurrence within the mineralized intervals.
The main purpose of this work was to assess the veracity of the application of a sediment‐hosted
gold deposit model and more specifically, a Carlin‐style deposit model. If this could be verified, then any
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future exploration programs would require modification to successfully delineate this style of mineralization
which manifests in entirely different modes than high‐sulphidation epithermal deposits.
A suite of 6 samples were selected for polished thin section preparation from diamond drill holes
11‐ER‐09, 11‐ER‐14 and 11‐ER‐15. A standard petrographic and binocular microscopy review was completed
on these samples, which were subsequently prepared for analysis on the scanning electron microscopy
(SEM). All six samples were mapped using Mineral Liberation Analysis software on the Scanning Electron
Microscope (MLA‐SEM) at Memorial University of Newfoundland.
2.0 Geological Setting
The Erika Property lies on Guerrero‐Morelos Platform, which consists of a thickness of over 2,000 m
of Mesozoic carbonate rocks unconformably overlaying Early Cretaceous to Late Jurassic island arc
sequences of Guerrero Terrane. Guerrero‐Morelos Platform is bound to the south by the Xolapa
metamorphic core complex, and to the north it is covered by Trans Mexican Volcanic Belt magmatic rocks
(Figure 2; Fonseca, 2007). The sedimentary rocks of Guerrero‐Morelos Platform were folded during Late
Cretaceous to Early Tertiary Laramide deformation. Guerrero‐Morelos Platform has three units: Morelos
Formation (Albian to Cenomanian limestones and dolostones; Cuautla Formation (Turonian calcareous
shales and limestones); and Mezcala Formation (Coniancian to Campanian, calcareous shales with
interbeded sandstones; Fonseca, 2007).
The Coacoyula epithermal district lies at the northern flanks of the Sierra Madre del Sur
physiographic and geologic provinces, where Tertiary plutonic rocks of adakitic composition occur
associated with large gold‐skarn deposits approximately 15 kilometres south of Erika (Fonseca, 2007).
Lithologies underlying the Erika Property include a Cretaceous sedimentary sequence that includes the
Morelos Formation limestone and overlying calcareous siltstone and mudstone of the Mezcala Formation.
The Mesozoic sedimentary sequence is partially covered by Tertiary felsic volcanic flows, breccias and
volcaniclastic accumulations (Fig. 3).
The Mesozoic sedimentary package strikes generally to the north, and is overlain by a thin package
of Tertiary felsic volcanic rocks. The felsic volcanic unit consists of brecciated volcaniclastics containing fine‐
grained, angular to sub‐rounded lithic fragments, quartz phenocrysts, rare pumice fragments. The property
includes several areas of intense clay alteration, from which clay has been mined for industrial applications
(Fonseca, 2007). A compilation of interpreted lineaments, faults, and dikes from air photos of Erika Property
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by Leach and Corbett (1996; Fig. 3) demonstrates that important structural trends are north‐northwest and
northeast. The property is located along a major north‐ to north‐northwest trending structural zone that
extends over 45 km north to the Taxco silver veins deposit, and 15‐20 km south to the Au‐skarn deposits of
Mezcala district (Fonseca, 2007).
3.0 Alteration/Mineralization and Au Pathfinders
Alteration associated with gold mineralization occurring at the Erika property includes:
1. Peripheral calcite veining that formed in response to early‐stage decalcification of host calcareous
sedimentary rocks (Fig. 4a,b).
2. Calcite + orpiment and/or realgar veining associated with low grade (<0.1g/t) Au mineralization
(Fig. 4c).
3. Disseminated orpiment mineralization associated with zones of decalcification (Fig. 4d).
4. Partial to complete decarbonatization (removal of carbonate) associated with disseminated
arsenic sulphides, pyrite and gold mineralization (Fig. 4e‐g).
Gold mineralization is associated with zones of intense decarbonatization, increased SiO2 and
anomalous Tl‐Hg‐As‐Sb. Dissolution collapse breccias occur in both intensely decarbonatized calcareous
siltstone (Mescala Formation; Fig. 4h) and limestone (Morelos Limestone; Fig. 4j). Additionally, a distinct
yellow‐green clay phase hosts mineralization (Fig. 4i).
4.0 MLA‐SEM Modal Mapping
Six polished thin sections were selected for scanning electron microscopy analysis using the FEITM
Quanta 650 field emission Scanning Electron Microscope (SEM). Samples chosen for the analysis are listed
with associated assay data in Table 1 and illustrated in Figure 5.
The purpose of the SEM study was to utilize the automated Mineral Liberation Analysis (MLA)
software to map the mineralogy of each polished surface. The data generated were subsequently used to
calculate mineral modes (wt %) and characterize the mineral associations present. The end goal of this
mapping process was to establish generalized ore and alteration mineral relationships and to use the semi‐
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Sample FROM TO Au_ppm Ag_ppm As_ppm Hg_ppm Sb_ppm Tl_ppm Mo_ppm Ba_ppm Se_ppm Te_ppm W_ppm S_% Fe_% Ca_% Cu_ppm Pb_ppm Zn_ppm
ER‐11‐09_306.66‐307.05m 306.66 307.05 0.459 7.56 >10,000 20.4 616 78.6 58.1 80 12.2 0.33 0.61 4.27 2.46 4.62 18.4 10.4 76
ER‐11‐09_307.43‐307.58m 307.43 307.58 0.89 6.65 451 24.1 73.1 44.3 24.4 80 4.9 0.38 0.34 2.63 1.88 5.41 10.3 7.6 317
ER‐11‐14_274.50‐274.56m 274.29 274.83 2.07 0.79 9040 38.5 75 230 1.4 80 3.2 0.69 0.5 3.64 2.29 10.85 19.6 8.3 54
ER‐11‐14_274.90m 274.83 275.05 4.17 1.6 1200 56.8 9.3 40.4 1.27 50 2.5 0.77 0.33 2.67 1.81 12.95 15.1 6.6 15
ER‐11‐15_297.52‐297.58m 296.42 297.82 1.775 1.81 >10,000 25.4 3570 53.9 52.6 800 0.6 2.71 0.65 0.01 2.35 3.77 19.9 10.3 90
ER‐11‐15_298.03‐298.08m 297.82 299.1 0.53 3.72 >10,000 15.75 3070 510 206 70 56.6 1.39 0.28 6.88 0.84 19.15 8.4 3.8 36
Table 1: Geochemical assay data for samples presented in SEM study. Samples underwent partial digestion and may values for some elements may be an underestimate
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quantitative analytical capability of the SEM to determine which mineral phases hosted both Au and main
Au pathfinder elements.
Modal Mapping ‐ Methodology
Modal mapping using the automated MLA‐SEM technique involves collection of back‐scattered
electron and X‐ray spectra data across an entire offcut surface. The SEM sample‐stage is programmed to
systematically move the sample at equal increments in both the X and Y directions to allow collection of the
two datasets. For BSE data collection the entire range of mineral brightness values (i.e. mean atomic
number) is acquired. Data acquisition occurs in a series of mosaic images which are subsequently merged
together into one image of the polished surface (Figs. 6‐11).
Additionally, a uniformly spaced point grid is created across the entire thin section and at each point
location x‐ray spectra are collected. Each of these point x‐ray spectra are subsequently matched to a
reference x‐ray spectra mineral list created for the project. Any minerals that do not match the mineral
reference list are classified as unknown, which are reviewed and identified after the automated analysis is
complete (post‐processing). Once all mineral phases present are identified and assigned a representative X‐
ray spectra and mineral formula, a final colourized mineral map is produced (Fig 6‐11) and modal
abundances are calculated by both wt% (Table 2). In the case of the Erika sample suite, an X‐ray sampling
strategy was developed to overcome data point collection problems caused by the fine grained matrix that
occurs in all 6 samples. Rather than reduce the sampling distance between X ray points to a few microns, X‐
ray spectra for a sampling area (100x100microns) was collected and stored. Thus, a matrix X‐ray library was
generated that represented a composite X‐ray spectra of all minerals that occurred within the 100x100
micron averaging window. Five separate matrix types were identified:
i) Ca‐rich matrix: Quartz‐Albite‐Calcite and unidentified Ca‐rich clays
ii) Moderate abundance Ca‐matrix: Quartz‐Albite‐Calcite‐minor Ca‐clays
iii) Ca‐poor matrix A: Illite‐quartz‐pyrite
iv) Ca‐poor matrix B: Quartz‐illite‐pyrite (distinct from (iii) due to different proportions of minerals).
v) As‐rich clay: Quartz‐illite‐As rich clay.
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ER‐11‐09 ER‐11‐09 ER‐11‐14 ER‐11‐14 ER‐11‐15 ER‐11‐15
306.66‐307.05m 307.43‐307.58m 274.50‐274.56m 274.90m 297.52‐297.58m 298.03‐298.08m
Mineral Wt% Wt% Wt% Wt% Wt% Wt%
Apatite 0.05 0.19 0.06 0.06 0.07 0.09
Quartz 12.84 11.27 6.45 3.65 5.59 9.68
White‐mica 0.11 0.03 0.13 0.23 0 0.02
Illite 1.28 6.74 2.29 5.96 7.86 16.18
Ca Rich Matrix: Quartz‐Albite‐Calcite‐Ca Clay 5.55 13.52 21.96 24.66 5.76 3.06
Moderate Ca Matrix: Quartz‐Albite‐Calcite 23.5 11.48 11.57 6.36 11.05 8.22
Ca Poor Matrix‐A: Quartz‐Illite 42.13 26.85 21.78 16.61 18.22 31.69
Ca Poor Matrix‐B: Quartz‐Illite 2.69 5.11 3.02 6.55 8.57 5.29
As‐Rich Clay‐Quartz‐Illite Matrix 3.49 5.74 2.17 3.71 37.42 3.23
Rutile 0.02 0.03 0.01 0.01 0.01 0.01
Dolomite 3.04 12.32 0.04 0.01 0 0
Calcite 0.32 2.13 26.56 28.52 0.04 2.28
Sericite 0.13 0.12 0.13 0.14 0.09 0.09
Muscovite 0.03 0.01 0.02 0.01 0.01 0.01
As‐Ca_Fe siderite 0.03 0.05 0 0 0.71 0
Diagenetic_Kaolinite 0.05 0.01 0.19 0.37 0 0.01
Barite 0.02 0.1 0.01 0 0 0.02
Gypsum 0 0 0.19 0.03 0 16.63
Pyrite 0.86 1.32 0.91 1.4 0 1.13
Pyrite‐altrd 1.21 1.42 1.34 1.42 0 1.54
Orpiment‐Qtz_illite 0.11 0.07 0.26 0.08 0.01 0.22
Orpiment 1.89 0 0.69 0 0 0.43
Altd_Arseniosiderite 0.63 1.44 0.18 0.2 4.55 0.16
Total 100 100 100 100 100 100
Table 2: Modal calculations by weight %.
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Modal Mapping ‐ Results per sample
ER‐11‐09_306.66‐307.05m is a strongly decalcified and decarbonatized siltstone crosscut by several high
angle minor structures and several quartz veins. Both the minor faults and calcite veins terminate before a
horizon of intense decarbonatization associated with orpiment‐illite‐quartz‐pyrite growth (Fig. 6a‐d).
Dolomite locally replaces calcite adjacent to zones of decalcification (Fig. 6e). Total clay rich matrix material
comprises 77.4 wt% of the sample, with Ca‐rich matrix representing only 5.5wt%. Illite and quartz represent
1.28 and 12.8 wt%, respectively. Dolomite, which replaces calcite constitutes 3.04wt%, pyrite and altered
pyrite comprise approximately 2wt% and disseminated orpiment represents 1.9wt% of the mode. Accessory
phases include apatite, rutile, barite, kaolinite and sericite.
ER‐11‐09_307.43‐307.58m is a deformed tectonic breccia that is has undergone decalcification and less
intense decarbonatization (Fig. 7a‐d). Siltstone breccia clasts are strongly flattened and preserve evidence of
rotation. Coarse‐grained calcite formed in a low strain window adjacent to the largest siltstone clast present
in the slide. Dolomite replaces calcite throughout the slide. The deformed breccia matrix is more pervasively
decarbonatized than siltstone clasts (Fig. 7e). Total clay rich matrix material comprises 62.7 wt% of the
sample, with Ca‐rich matrix representing 13.5wt%. Illite and Quartz represent 6.74 and 11.3 wt%,
respectively, calcite and dolomite comprise 2.13 and 12.3wt%, respectively. Pyrite and altered pyrite
comprise approximately 2.7wt% and disseminated orpiment represents 1.9wt% of the mode. Accessory
phases include apatite, rutile, barite, kaolinite and sericite.
ER‐11‐14_274.50‐274.56m is a moderately deformed dissolution collapse breccia that has undergone
intense decarbonatization in the matrix enclosing the limestone and siltstone breccia clasts (Fig. 8a‐e).
Breccia clasts have undergone variable decalcification and locally contain coarse‐grained disseminated
orpiment. Total clay rich matrix material comprises 60.5 wt% of the sample, with Ca‐rich matrix
representing 21.96 wt%. Illite and quartz represent 2.29 and 6.45 wt%, respectively. Dolomite was not
recognized in this sample, whereas calcite comprised 26.56wt% of the estimated mode. Pyrite and altered
pyrite represent 2.25wt% and disseminated orpiment comprises 0.7wt%. Accessory phases include apatite,
rutile, gypsum, kaolinite and sericite.
ER‐11‐14_274.90m is a dissolution collapse breccia that is has undergone intense decarbonatization in the
matrix enclosing the limestone and siltstone breccia clasts (Fig. 9a‐e). Rounded breccia clasts have
undergone variable decalcification. Total clay rich matrix material comprises 57.9 wt% of the sample, with
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Ca‐rich matrix representing 26.66 wt%. Illite and quartz represent 5.59 and 3.65 wt%, respectively.
Dolomite was not recognized in this sample, whereas calcite comprised 28.52wt% of the estimated mode.
Pyrite and altered pyrite represent 2.82 wt% Accessory phases include apatite, rutile, gypsum, kaolinite and
sericite.
ER‐11‐15_297.52‐297.58m is a heterogeneous, compositionally banded clay rich sample. Banding is defined
by a late‐stage As rich clay that pervasively has infiltrated a quartz‐illite dominant clay (Fig. 10a‐e). The As‐
rich clay species within the sample is associated locally with a distinct As‐Fe mineral (arseniosiderite). Total
clay rich matrix material comprises 81.02 wt% of the sample, with Ca‐rich matrix representing 5.76 wt%.
Illite and quartz represent 7.86 and 5.59 wt%, respectively. Dolomite was not recognized and calcite was
only observed in trace abundances. Additionally, orpiment and pyrite were not identified. Arseniosiderite
comprised 4.55 wt%. Accessory phases include apatite and sericite.
ER‐11‐15_298.03‐298.08m is a variably decalcified and decarbonatized siltstone with coarse grained gypsum
laths that are intergrown with orpiment and spatially associated with concentrations of illite (Fig. 11a‐e).
Total clay rich matrix material comprises 51.49 wt% of the sample, with Ca‐rich matrix representing 3.06
wt%. Illite and quartz represent 16.18 and 9.68 wt%, respectively. Dolomite was not recognized in this
sample, whereas calcite comprised 2.28wt% of the estimated mode. Pyrite and altered pyrite represent
2.67wt% and disseminated orpiment comprises 0.4wt%. Accessory phases include apatite, rutile, barite,
kaolinite and sericite.
Mineral mapping of the Erika sample suite illustrates the occurrence of both decalcification and
decarbonatization in Au‐bearing rocks. Apart from the Au‐bearing clay sample, ER‐11‐15_297.52‐297.58m,
pyrite abundances range from 2 ‐ 2.8 wt% in all samples. Importantly, the occurrence of dolomite in
samples from ER‐11‐09 (and absence from ER‐11‐14 and 15) implies this drill hole intersected a more distal
component of the Au mineralizing system, which is consistent with the higher gold grades that were
intersected in holes ER‐11‐14 and 15 (i.e. more proximal).
5.0 Gold Deportment and Pathfinder Mineral Hosts
A examination of the sites of gold deposition was carried out on samples ER‐11‐14‐274.5‐274.56m
and ER‐11‐15‐297.52‐207.58m. Carlin‐style gold mineralization is typically associated with the occurrence of
submicron, invisible Au in trace element‐rich pyrite and marcasite. Gold‐bearing pyrite
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and marcasite occur as discrete grains, generally less than a few micrometers in diameter, or as arsenian rich
narrow rims on earlier formed pyrite grains (Cline et al., 2005). An important objective of SEM examination
of the Erika sample suite was to assess whether arsenian pyrite was present in samples that correlated with
elevated gold concentrations. Figure 12a presents the mineral map for sample ER‐11‐14‐274.5‐274.56m and
associated SEM images for various locations across the sample surface. Irregular, arsenian pyrite rims and
disseminated arsenian pyrite grains were identified within strongly decarbonatized material that formed a
breccia matrix enclosing dissolution collapse breccia clasts. A cursory review of pyrite grains in other
samples (Fig. 12b‐e), demonstrated the ubiquitous presence of 'fuzzy' arsenian rich pyrite rims on several
different pre‐existing pyrite generations. Framboidal pyrite, euhedral pyrite and inclusion‐rich pyrite grains
that occurred in decarbonatized zones were all associated with the growth of thin arsenian pyrite rims up to
5 microns wide.
Sample ER‐11‐15‐297.52‐207.58m is a heterogeneous dominantly clay‐bearing sample that is
associated with elevated Au values (up to 1.775g/t; Fig. 13a). No pyrite or arsenic sulphide minerals were
identified in this sample, however two distinct clay matrix types were mapped out including (i) an early
stage Ca‐poor quartz‐illite clay matrix, similar in composition to the clay matrix compositions comprising
strong zones of decarbonatization in the other samples examined in the study, and (ii) and a late stage As
rich clay phase that post‐dates the Ca‐poor clay matrix (Fig. 13c). A distinctive Ca‐Fe‐As oxide species,
arseniosiderite, is directly associated with the As rich clay matrix (Fig. 13b‐d). Micron size native gold was
identified within both arseniosiderite grains and disseminated with the As rich clay matrix, implying a second
gold bearing event post‐dating the decarbonatization and arsenian pyrite rim growth event. The two gold
events likely represent a continuum of one gold bearing fluid phase. The Au rich clay intervals appear to be
associated with infilling of voids (kharsts) below the siltstone/limestone contact, whereas the arsenian
pyrite gold bearing event is exclusively within decarbonatized siltstone.
Several pathfinder elements were identified to have a moderate to strong correlation with gold (Hg‐
Sb‐Tl or were extremely anomalous (As). Binocular and SEM observations identified:
1. Arsenic occurred as orpiment, realgar, As‐rich clay, As rich pyrite and arseniosiderite. In one
sample, orpiment was observed associated with gypsum, where gypsum laths grew at the expense
of orpiment. Alternatively, orpiment grains represented a nucleation point from which the gypsum
laths grew (Fig. 14a‐c).
2. Hg was locally observed to form as small grains of cinnabar at the outermost margins of pre‐
existing pyrite grains (Fig. 14d).
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3. Rare radiating stibnite grains were observed replacing a fine‐grain siltstone matrix (Fig. 14e)
The mineral host for Tl was not identified.
6.0 Structural Observations
Qualitative lineament analysis of the Erika property (Fig. 3) indicate that high‐angle NNW and NE
structural orientations prevail. On a regional scale, these structures represent part of an extensive north‐ to
north‐northwest trending structural zones that extends over 45 km north to the Taxco silver veins deposit,
and 15‐20 km south to the Au‐skarn deposits of Mezcala district (Fonseca, 2007). The nature and geometry
of fault structures controlling sediment‐hosted gold mineralization at Erika are currently not well
understood, but are tentatively correlated to N‐trending regional faults. Examination of drill core indicates
that two types of structures related to both alteration and mineralization are present, including:
1. High angle to core‐axis and bedding brittle faults and dilational calcite vein faults (Fig. 15). High
angle brittle faulting is typically associated with brecciation and focussed decarbonatization (Fig.
15c‐e). Kinematic observations indicate normal and dilatant displacement (Fig. 15a, b). Dilatant
calcite vein faultings is particularly well developed in the peripheral calcite vein halo (to Au
mineralization).
2. Bedding parallel to subparallel shear zone development that truncates high‐angle to core‐
axis/bedding structures and is associated with intense decarbonatization, local orpiment and pyrite
formation (Fig. 16). In rare instances, the preserved array of fault and fractures in these bedding
plane shears zones is consistent with riedel shear geometry. These structures are interpreted to be
associated with gold deposition and represent reactivation of zones of weakness parallel to bedding
planes.
SUMMARY
Scanning electron microscopy mineral mapping completed on 6 polished thin sections of Au
mineralized samples demonstrates the presence of several ore fluid processes that are analogous to Carlin‐
style mineralization including decalcification, decarbonatization, argillization and associated silicification of
calcareous siltstone. Arsenian fuzzy pyrite and disseminated arsenian pyrite in zones of decarbonatization
are likely a host of Au in siltstone‐hosted mineralization. Collectively, the data presented support the
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interpretation of Au mineralization at the Erika property to be a Carlin‐style target. Future work should focus
on delineating the location and orientation of controlling mineralizing structures in order to more effectively
assess the scope of Au bearing zones identified to date.
References
Cline, J.S., Hofstra, A.H., Muntean, J.L., Tosdal, R.M and Hickey, K.A. 2005. Carlin‐type gold deposits in
Nevada: Critical geological characteristics and viable models. Economic Geology, Vol. 100, 451 ‐ 484.
Fonseca, A., 2007. Technical report on exploration results for the Erika high sulphidation gold property,
Guerrero State, Mexico, 45p.
Leach, T.M., and Corlett, G., 1996, Interim field report on the Erika Prospect, Guerrero State,
Mexico, Internal report for Almaden Resources, 8 p.
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