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To: LoneClone who wrote (173268)8/24/2023 3:59:51 PM
From: LoneClone  Read Replies (1) | Respond to of 192522
 
Archer Exploration Down Hole EM Surveys Yield Strong Conductors at Grasset

newswire.ca

Archer Exploration Corp. 17 Aug, 2023, 08:30 ET

VANCOUVER, BC, Aug. 17, 2023 /CNW/ - Archer Exploration Corp. (CSE: RCHR) (OTCQB: RCHRF) (FSE: 6YR0) (the "Company" or "Archer") is pleased to announce that it has received very encouraging results from down hole electromagnetic (DHEM) surveys recently completed on its 100%-owned Grasset Ni-Cu-Co PGE project located in the Abitibi Greenstone Belt of Quebec, Canada.

Highlights








Figure 1: H1 Horizon Contour Long Section with DHEM Conductive Plates (CNW Group/Archer Exploration Corp.)



Figure 2: Grasset Deposit Planview and 2023 Drilling (CNW Group/Archer Exploration Corp.)





  • Recently completed DHEM surveys yielded three new highly conductive plates within the H1 Horizon at Grasset
  • The newly modeled plates begin 360 metres below surface and have not yet been drill tested
  • Conductivity measurements suggest semi-massive to massive pyrrhotite (± pentlandite) is likely the source of the conductive anomalies


  • Jack Gauthier, VP Exploration, commented: "Conductive plates modelled from geophysical surveys indicate the potential for the presence of mineralization such as nickel. The strong and sizeable off-hole anomalies below hole GR23-03 support our view of the untested potential at Grasset and it confirms the potential for discovering greater volumes of high-grade nickel mineralization at depth. Additional drilling is warranted to test these strong conductors."

    The downhole surveys were conducted by Abitibi Geophysics using the InfiniTEM® XL dual loop system and totaled 3,085 metres in five boreholes. The surveys defined several deep-seated, strongly conductive targets along the H1 Horizon.

    Of particular interest are three strong and deep DHEM anomalous plates (Figure 1) best defined by the survey in hole GR-23-03. This hole, drilled in May 2023, yielded the best intersection to date within the H1 Horizon with 1.82% Ni over 4.60 metres, including 5.75% Ni over 0.60 metres (see news release dated June 15, 2023).

    The three large conductors contain known mineralized intercepts in their periphery but remain largely untested. The size of the three modeled DHEM anomalies suggests a much better continuity at depth when compared to the numerous small plates detected closer to surface (PA and P15 plates in Figure 1).

    Figure 1 shows the longitudinal view of the modelled DHEM conductive plates over nickel metal factor values (% nickel X estimated thickness).

    Table 1: Summary of DHEM Survey Results



    DHEM Plates

    Area
    (m2)


    Conductance
    (S)


    Depth
    (m)


    P23-03C

    5,800

    1,370

    360

    P23-03D1

    42,000

    1,500

    365

    P23-03D2

    22,500

    750

    690




    Average conductivity measurements of drill core that was near the conductive plates:

  • Mudstone: 12 S/m
  • Massive pyrite: 58.6 S/m
  • Massive pyrrhotite + pentlandite (H1 in GR23-03): 38,026 S/m


  • This suggests that semi-massive to massive pyrrhotite (± pentlandite) is the most likely source of the highly conductive DHEM anomalies. The three newly modeled conductive plates identified begin 360 metres below surface and have not been previously drill tested.

    Physical property measurements were taken on drilling core near the target plates with a TerraPlus KT-10 Magnetic Susceptibility and Conductivity meter. The measurements were done on potentially conductive lithologies close to the northern contact of the main ultramafics around the expected location of the extension of the H1 Zone. The average of 42 measurements on mudstone with disseminated graphite (mudstone) gave 12 S/m, with the highest being 248 S/m (holes GR23-02, GR23-05). Two measurements on the barren massive sulfides (60-80% pyrite) in hole GR23-02W1 gave 16.8 and 99.6 (average 58.6). The conductivity value obtained on the massive pyrrhotite with pentlandite that assayed 5.75% nickel over 0.60 metres in hole GR23-03 was 38,026 S/m. This indicates that the mudstone and the massive pyrite are relatively poor conductors and unlikely sources of the strong DHEM anomalies at depth. Comparing those measurements to the conductivity of the DHEM plates (Table 1) suggests that that the most likely source of the conductive plates is massive pyrrhotite +/- pentlandite.

    It should be noted that small lenses of barren pyrrhotite have also been identified in the mudstone in some holes. It is thought that these may not be as extensive compared to nickel-bearing pyrrhotite in the ultramafics and could be filtered out by their location in the stratigraphy.

    Table 2: Detailed DHEM Conductive Plate Characteristics



    Hole ID

    DHEM Plate

    X

    (m)

    Y

    (m)

    Z

    (m)

    Dip

    (°)

    Dir

    (°)

    Length

    (m)

    Depth
    Extension


    (m)

    Conductivity

    (S)

    GR-15-74

    P15-74A

    679713

    5540064

    50

    90

    233

    50

    50

    200

    GR-15-74

    P15-74B1

    679745

    5540045

    125

    80

    233

    50

    100

    1,859

    GR-15-74

    P15-74B2

    679760

    5540010

    75

    85

    240

    50

    100

    1,859

    GR-15-74

    P15-74B3

    679755

    5540005

    -45

    80

    238

    25

    25

    500

    GR-15-77

    P15-77A

    679807

    5539978

    25

    90

    228

    50

    50

    2,000

    GR-15-80

    P15-80A

    679844

    5539934

    40

    90

    45

    45

    75

    2,500

    GR-23-03

    P23-03A

    680029

    5539685

    -38

    90

    225

    25

    40

    300

    GR-23-03

    P23-03B

    680027

    5539688

    -47

    90

    225

    25

    10

    20,000

    GR-23-03

    P23-03C

    680088

    5539639

    -70

    90

    223

    93

    62

    1,370

    GR-23-03

    P23-03D1

    679901

    5539863

    -75

    80

    225

    140

    300

    1,500

    GR-23-03

    P23-03D2

    679865

    5539835

    -400

    80

    225

    150

    150

    750

    GRA-01

    PA-01A

    679834

    5539913

    190

    75

    233

    40

    50

    2,500

    GRA-01

    PA-01B

    679795

    5539980

    100

    80

    215

    25

    25

    1,000

    GRA-01

    PA-01C

    679851

    5539879

    160

    90

    233

    15

    15

    2,500

    GRA-01

    PA-01D

    679851

    5539858

    145

    90

    53

    30

    50

    2,500

    GRA-02

    PA-02

    679539

    5540167

    150

    75

    190

    50

    150

    500

    GRA-03

    PA-03A

    680115

    5539710

    250

    90

    228

    75

    50

    500

    GRA-03

    PA-03B

    680100

    5539665

    150

    90

    228

    100

    100

    1,000

    GRA-06

    PA-06

    679655

    5540100

    110

    75

    190

    25

    25

    500




    Conductance over 500 Siemens (S) are of interest for massive to semi-massive pyrrhotite +/- pentlandite especially given the high tenor of the mineralization at Grasset. Plate P23-03B is a very conductive in-hole anomaly that fits with the 0.60 metres of massive pyrrhotite/pentlandite that assayed 5.75% in hole GR23-03 (see news release dated June 15, 2023).

    2023 Drill Holes Completed
    Holes GR23-04 and GR23-05 were completed with disseminated sulfides intersected within the extensions of H3 and H1 zones. Assays are currently pending. Hole GR23-06 is underway and nearing completion, testing a deep-seated 3D magnetic anomaly at the north-west limit of the mineralized zones.

    Table 3: Drillhole Collar Coordinates



    Hole ID

    Easting

    (UTM)

    Northing

    (UTM)

    Elevation

    (m)

    Azimuth

    (°)

    Dip

    (°)

    Hole Length

    (m)

    GR23-01

    679759

    5539876

    291

    21

    -90

    446

    GR23-02

    679859

    5539783

    291

    322

    -88

    759

    GR23-02W1

    679859

    5539783

    291

    322

    -88

    874

    GR23-03

    679939

    5539491

    291

    30

    -60

    576

    GR23-04

    679374

    5537683

    291

    45

    -55

    885

    GR23-05

    679323

    5539538

    291

    50

    -70

    1,152






    Collar coordinates are UTM Zone 17N
    Azimuths and dips are taken from survey record at collar unless otherwise noted




    Table 4: Summary of Assay Results – Ni-Cu-Co-PGE



    Hole ID

    From

    (m)

    To

    (m)

    Length

    (m)

    Ni

    (%)

    Cu

    (%)

    Co

    (%)

    Pt

    (g/t)

    Pd

    (g/t)

    GR23-01

    No significant mineralization observed

    GR23-02

    514.5

    515.0

    0.50

    0.67

    0.03

    0.02

    0.17

    0.39

    GR23-03

    358.0

    358.5

    0.50

    0.53

    0.04

    0.01

    0.08

    0.17

    GR23-03

    403.0

    408.8

    5.80

    1.55

    0.18

    0.04

    0.35

    0.82

    Including

    404.2

    408.8

    4.60

    1.82

    0.22

    0.04

    0.40

    0.95

    Including

    408.2

    408.8

    0.60

    5.75

    0.24

    0.13

    1.68

    3.85

    GR23-04

    Assays pending

    GR23-04

    Assays pending






    All lengths are downhole lengths and true widths are expected to be greater than or equal to 60-70% of downhole lengths




    Table 5: Summary of Assay Results – Gold



    Hole ID

    From

    (m)

    To

    (m)

    Length

    (m)

    Au

    (g/t)

    GR23-03

    98.0

    98.5

    0.50

    1.39

    GR23-03

    110.0

    111.0

    1.00

    0.90

    Including

    110.0

    110.5

    0.50

    1.28

    GR23-03

    265.8

    266.6

    0.80

    16.19

    Including

    265.8

    266.1

    0.30

    49.10




    Qualified Person
    The scientific and technical content of this press release has been reviewed and approved by Mr. Jacquelin Gauthier, P.Geo, Vice President, Exploration, who is a "Qualified Person" as defined by National Instrument 43-101 - Standards of Disclosure for Mineral Projects. Mr. Gauthier is satisfied that the analytical and testing procedures used are standard industry operating procedures and methodologies, including sampling, analytical and test data underlying the technical information disclosed in this news release.

    About Abitibi Geophysics
    Abitibi Geophysics has built a 30 year reputation internationally with safe, efficient, reliable high quality geophysical data acquisition, processing and interpretation services to help our clients find a variety of mineral resources and expand their exploration programs. Our products also include data compilation, modeling/inversion and interpretation services.

    Abitibi Geophysics' InfiniTEM® XL dual loop system generates a large primary electromagnetic field that couples with deep, steeply dipping conductors while minimizing the response from conductive overburden. The secondary field induced in the conductor is detected by a sensor located on the surface or inside a borehole. The downhole surveys were completed using a DigiAtlantis system at a low base frequency (1Hz).

    About Archer
    Archer Exploration is a Canadian Ni-Cu-Co-PGE focused exploration and development company with an extensive portfolio of assets in Quebec and Ontario, Canada. The Company's flagship asset is the Grasset Project, located within the Abitibi Greenstone Belt, with an Indicated Resource of 5.5 Mt @ 1.53% NiEq. In addition, the Company holds a portfolio of 37 properties and over 300 km2 in the world-class mining district of Sudbury, Ontario.

    The Company's growth strategy is focused on the exploration and development of its nickel sulphide properties within its portfolio. Archer's vision is to be a responsible nickel sulphide developer in stable pro-mining jurisdictions. Archer is committed to socially responsible exploration and development, working safely, ethically, and with integrity. For more information, please visit www.archerexploration.com.

    Cautionary Note Regarding Forward-Looking Statements
    Neither the CSE nor its Market Regulator (as that term is defined in policies of the CSE) accepts responsibility for the adequacy or accuracy of this release.

    The information contained herein contains "forward-looking statements" within the meaning of applicable securities legislation. "Forward-looking information" includes, but is not limited to, statements with respect to the activities, events or developments that Archer expects or anticipates will or may occur in the future. Generally, but not always, forward-looking information and statements can be identified by the use of words such as "plans", "expects", "is expected", "budget", "scheduled", "estimates", "forecasts", "intends", "anticipates", or "believes" or the negative connotation thereof or variations of such words and phrases or statements that certain actions, events or results "may", "could", "would", "might" or "will be taken", "occur" or "be achieved" or the negative connotation thereof.

    Such forward-looking information and statements are based on numerous assumptions, including among others, that the results of planned exploration activities are as anticipated, the anticipated cost of planned exploration activities, that general business and economic conditions will not change in a material adverse manner, that financing will be available if and when needed and on reasonable terms, that third party contractors, equipment and supplies and governmental and other approvals required to conduct Archer's planned exploration activities will be available on reasonable terms and in a timely manner. Although the assumptions made by Archer in providing forward-looking information or making forward-looking statements are considered reasonable by management at the time, there can be no assurance that such assumptions will prove to be accurate.

    By their nature, forward-looking statements involve known and unknown risks, uncertainties and other factors which may cause our actual results, performance or achievements, or other future events, to be materially different from any future results, performance or achievements expressed or implied by such forward-looking statements. Such factors and risks include, among others: risks associated with the conduct of the Company's mining activities; regulatory, consent or permitting delays; risks relating to reliance on the Company's management team and outside contractors; risks relating to project financing and equity issuances; risks and unknowns inherent in all mining projects; laws and regulations governing the environment, health and safety; the ability of the communities in which the Company operates to manage and cope with the implications of COVID-19; the economic and financial implications of COVID-19 to the Company; operating or technical difficulties in connection with mining or development activities; employee relations, labour unrest or unavailability; the Company's interactions with surrounding communities; the Company's ability to successfully integrate acquired assets; the speculative nature of exploration and development; stock market volatility; conflicts of interest among certain directors and officers; lack of liquidity for shareholders of the Company; litigation risk; the ongoing military conflict in Ukraine; general economic factors (including inflationary pressure); the price of commodities; and the factors identified under the caption "Risk Factors" in the Company's public disclosure documents.

    The forward-looking information contained in this news release represents the expectations of Archer as of the date of this news release and, accordingly, is subject to change after such date. Readers should not place undue importance on forward-looking information and should not rely upon this information as of any other date. Archer does not undertake any obligation to update these forward-looking statements in the event that management's beliefs, estimates or opinions, or other factors, should change.

    SOURCE Archer Exploration Corp.

    For further information: Tom Meyer, President & Chief Executive Officer, Tel: +1 866.899.7247 (RCHR), Email: tom@archerexploration.com