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Ishmas - Nabitah Region

Ishmas-Nabitah Regional Summary

Arabian Gold Licences

Detailed descriptions of the licences to follow.

Regional Geology

The Ishmas-Nabitah geological district includes two terranes, the eastern and western, which are separated by the north-trending Nabitah Fault Zone (NFZ). The eastern terrane, constituting part of the Malahah-Najran terrane, is composed of amphibolite and mylonite schist, originally a sequence of volcanic and volcaniclastic rocks of Halaban age (785 - 746 Ma), and an intrusion of monzogranite. The western terrane, constituting part of the Asir terrane, comprises Halaban age formations which include mafic volcanic rocks, ferruginous chert, carbonates and volcanic wacke. Some fine grained amphibolites is also present along with older plutonic rocks which include an extensive diabase sill complex and several gabbro intrusive.

Post-Nabitah plutonic rocks in the western terrane include quartz-diorite plutons, tonalite masses, dacite porphyry and quartz monzodiorite.

Three phases of faulting have been identified in the regional and can be defined as follows:

Economic Geology

There are over 30 gold occurrences within the district. These occurrences range in size from isolated surface exposures to large ancient workings with extensive tailings. Several phases of work have investigated these occurrences in the past (Worl, 1979; Doebrich et al., 1988) with several locations having resource potential. More critically the area as a whole has yet to be thoroughly investigated by modern exploration technologies giving great upside-potential for the discovery of significant resources.

Mineralisation occurrences in the Ishmas-Nabitah geological district can be generally grouped chronologically in association with the first and third phases of deformation described in the previous section:

Owing to the fact that faulting occurs through both Transitional and Post-Nabitah ages, it is possible to conclude that the fluids are from a shallow origin although available literature questions the requirement for a proximal igneous intrusion (White et al., 1988).

Regardless of the fluid origin, the basic elements of the ore-forming process are generally thought to be the same in the faults of both ages, with fluids leaching constituents from surrounding country rock, concentrating in permeable fracture zones and then precipitating quartz, gold and associated sulphides. The quartz body was dependent on the host rock and structure type (strike-slip or open) and gold precipitation was predominantly concentrated in the quartz with subsequent remobilisation and recrystallisation to adjacent fractured and sheared footwall and hanging wall contacts as a result of weathering (supported by iron-oxide-coated fracture surfaces, White et al., 1988).

References:

Doebrich, J.L., White, W.H., 1988, Geology of the Ishmas Gold District, Kingdom of Saudi Arabia: Saudi Arabian Directorate General of Mineral Resources Technical Report USGS-TR-08-1, 40p.

Moore, J.Mc., Al-Shanti, A.M., 1979, Structure and mineralization in the Najd Fault System, Saudi Arabia, Volume 2, Bulletin No.3 - Evolution and Mineralization of the Arabian-Nubian Shield, Institute of Applied Geology, King Abdulaziz University, Jeddah, pp17-28.

White, W.H., Doebrich, J.L., 1988, Gold deposits of the Ishmas district, Kingdom of Saudi Arabia: Saudi Arabian Directorate General of Mineral Resources Technical Report USGS-TR-07-5, 73p.

Worl, R.G., 1979, Gold deposits associated with the Jabal Ishmas-Wadi Tathlith Fault Zone, Volume 2, Bulletin No.3 - Evolution and Mineralization of the Arabian-Nubian Shield, Institute of Applied Geology, King Abdulaziz University, Jeddah, pp61-69.
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