Page 112 - Introduction to Mineral Exploration
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5: FROM PROSPECT TO PREFEASIBILITY  95


                 pit and the underground accesses. In addition  detected, probably because of the use of a wider
                 the company investigated the potential of the  sampling spacing. BGS also drilled two holes
                 area around the open pit and particularly its  (Fig. 5.19) to check the subsurface extension of
                 strike extensions by taking soil samples for  the western end of the Wheal Prosper system as
                 geochemical analysis along E–W lines (Hosking  well as a copper anomaly adjacent to the old
                 1971). These suggested that the deposit contin-  pit. Limited assays gave similar results (up to
                 ued to the south into the calc flintas. CGF then  0.3% Sn) to surface samples.
                 undertook a drilling program to test the poten-  The third commercial program was a more
                 tial of the deposit at depth (Fig. 5.16). Drilling  exhaustive attempt from 1979 to 1982 by Cen-
                 over the period 1964–66 confirmed that the    tral Mining and Finance Ltd (CMF), a subsi-
                 mineralisation continued at roughly the width  diary of Charter Consolidated Ltd, themselves
                 of the open pit but that the cassiterite was con-  an associate company of the Anglo American
                 tained in thin erratic stringers. Drilling to the  group. Charter Consolidated had substantial
                 north of the open pit showed a sharp cut-off  interests in tin and wolfram mining, including
                 whereas drilling to the south showed that tin  an interest in the South Crofty Mine and an
                 values continued from the slate host into a calc  interest in Tehidy Minerals, the main mineral
                 flinta host where mineralisation became much  rights owners in the area. CMF’s approach
                 more diffuse. Although the grades intersected  included a re-evaluation of the Mulberry pit
                 were similar to those in the open pit, the size  and a search for extensions, as well as a search
                 and grade were not considered economic, espe-  for extensions of the Wheal Prosper system
                 cially when compared with Wheal Jane (even-  and an attempt to identify any buried granite
                 tually a producing mine) which CGF was also  cupolas with their associated mineralisation.
                 investigating, and the lease was terminated.  Their program contained four phases. In the
                   The next phase of exploration was from     first phase the Mulberry pit was resampled and
                 1971 to 1972 when the area was investigated  regional soil geochemistry and gravity surveys
                 by Noranda–Kerr Ltd, a subsidiary of the Cana-  were undertaken. The gravity survey identified
                 dian mining group Noranda Inc. This explora-  a perturbation in the regional gravity field
                 tion built on the work of CGF and investigated  along the Mulberry trend (Fig. 5.18). Regional
                 the possibility that the diffuse mineralisation  shallow soil geochemistry samples were taken
                 within the calc silicates might be stratabound  on 100 m centers and analysed for Sn, Cu,
                 and more extensive than previously suspected.  As, Mo, and W. They showed an ill-defined
                 Noranda conducted another soil survey (Fig.  southern continuation of the Mulberry system
                 5.17) that showed strong Sn and Cu anomalies  in Cu data and a large Cu and As anomaly to
                 over the calc silicates. Four drillholes were  the southwest of the Wheal Prosper system.
                 then sited to test these anomalies after pits  Resampling of the Mulberry pit led to a re-
                 were dug to confirm mineralisation in bedrock.  estimation of the resource to 1.1 Mt at 0.44%
                 The drillholes intersected the calc silicates but  Sn using a 0.2% Sn cut off. This would form
                 the structure was unclear and not as predicted  part of the resource for any mine.
                 from the surface. In addition although exten-  The Phase 2 program in 1980 consisted of a
                 sive (>20 m thick) mineralisation was inter-  detailed geochemical soil survey follow-up of
                 sected it was weak (mainly 0.2– 0.5% Sn) with  anomalous areas identified in phase 1, as well
                 few high grade (>1% Sn) intersections. The   as the planning of two holes to test the geo-
                 program therefore confirmed the exploration   physical anomaly. The first hole (CMF1, Fig.
                 model but was terminated.                    5.19) was a 540 m deep diamond-cored bore-
                   As part of an effort to encourage mineral  hole that failed to find any indication of granite
                 exploration in the UK, the British Geological  or associated contact metamorphism, although
                 Survey investigated the southern part of the  it did cut vein mineralisation of 0.51% Sn over
                 area (Bennett et al. 1981). Their surveys also  3.1 m at 206.5 m depth. Because of the lack of
                 defined the southern geochemical anomaly to   granite the planned second hole was cancelled.
                 the SW of Wheal Prosper, as well as an area of  The results of the soil geochemistry survey
                 alluvial tin in the west of the area. The exten-  encouraged CMF to progress to phase 3 with
                 sion of the Mulberry trend was not as clearly  a deep overburden sampling program to the
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