Eloro Resources Intersects 198.00 g Ag eq/t (67.79 g Ag/t, 1.44% Zn and 1.04% Pb) over 134.47m in Silver-Rich Area of High-Grade Feeder Zone in Santa Barbara Target Area at the Iska Iska Silver-Tin Polymetallic Project, Potosi Department, Bolivia
This intersection in hole DSB-31, drilled 200m southeast of the Santa Barbara adit, includes a higher-grade portion grading 566.36 g Ag eq/t (246.26 g Ag/t, 3.72% Zn and 3.88% Pb) over 25.51m. Additional significant intersections in this hole include: 161.54 g Ag eq/t (32.14 g Ag/t, 1.94% Zn and 0.76% Pb) over 82.12m, 123.24 g Ag eq/t (9.23 g Ag/t, 1.44% Zn, 0.26% Pb and 0.07% Sn) over 62.23m, and 126.21 g Ag eq/t (6.05 g Ag/t, 1.58% Zn and 0.52% Pb) over 81.12m Overall, 51% of the overall length of this 987.99m long hole yielded reportable intersections, which collectively average 139.44 g Ag eq/t. The high-grade silver zone intersected in hole DSB-31 appears to be in the same structural-mineralized corridor as the silver-rich zone in the Santa Barbara adit. As previously reported channel sampling along the adit returned 441.98 g Ag eq/t (164.96 g Ag/t, 0.23 g Au/t, 3.46% Pb and 0.46% Sn) over 165.89m. Adjusted to prices used in this current release, the overall Ag eq/t value is 493.61 g Ag eq/t. Hole DSB-33 drilled at an azimuth of 2250 with a dip of -600 to test the southwest limit of the high-grade feeder zone in the vicinity of the Central Breccia intersected 18 reportable intersections including a very high tin intersection grading 1.41% Sn over 21.25m which included a 9.04m section that graded 3.08% Sn. A total of 26% of this hole contained reportable intersections which collectively averaged 123.39 g Ag eq/t.Eloro Resources Ltd. (TSX-V: ELO; OTCQX: ELRRF; FSE: P2QM) (“Eloro”, or the “Company”) is pleased to announce assay results from two (2) additional diamond drill holes from its on-going drilling program at the Iska Iska silver-tin polymetallic project in the Potosi Department, southern Bolivia. One drill hole, DSB-31, tested the potential south-southeastern extension of the high-grade feeder zone at Santa Barbara while the second hole, DSB-33, tested the southwest limit of the zone in the vicinity of the Central Breccia, as shown in Figure 1.