Startseite Structural characterization of the Zalm district, West Saudi Arabia, using aeromagnetic data: An approach for gold mineral exploration
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Structural characterization of the Zalm district, West Saudi Arabia, using aeromagnetic data: An approach for gold mineral exploration

  • Hassan Alzahrani und Elkhedr Ibrahim EMAIL logo
Veröffentlicht/Copyright: 10. Februar 2025
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Abstract

The Zalm district in western Saudi Arabia has drawn significant attention from those interested in exploring for gold mineralization. In the present study, the structural framework and major structural trends that most likely control the distribution of the gold mineral deposits in the Zalm district are interpreted using aeromagnetic data. For this purpose, the aeromagnetic data were subjected to enhancement filters to make the structural interpretation of the data easier. In this respect, the data were reduced to the north magnetic pole and processed through two enhancement filters: the analytical signal (AS) and the first vertical derivative (1VD). Lineament analysis of aeromagnetic maps suggests that three major fault sets dissected the Zalm district trending in the northwest (NW), northeast (NE), and north-south (NS) directions. These faults likely affected the mineralization occurrences in the Zalm district and could serve as important structural conduits for hydrothermal fluid channeling. Based on the current results, four localities were identified as promising for additional mineral resource investigation. These localities are delimited and dissected by the NW, NE, and NS faulting and are intruded by a series of felsic and mafic–ultramafic intrusions. It is likely that, in similar to Bi'r Tawilah where the location is structurally controlled by NW and NS faulting, the interpreted felsic and mafic served as sources of mineralizing fluids which remobilized the ore in the district by channeling through the faults. Three of the suggested localities, one lying in close proximity to Zalm city and two along the Rada and Nabitah fault zones, are characterized by high magnetic anomalies, indicating the presence of ultramafic and volcanic rocks that most likely host mineralization. The fourth locality situated in the central part of the district is marked by an elongated N–S low magnetic anomaly, interpreted as felsic diorite and granite rocks delimited by N–S faulting. To accurately detect mineral resources in the selected zones, additional comprehensive and in-depth geological and geophysical research are recommended.

1 Introduction

The Arabian Shield is home to numerous gold occurrences, some of which are significant economically (e.g., Mahd Ad Dahab, Ad Duwayhi, and Bi'r Tawilah). In western Saudi Arabia, the Zalm district has drawn special attention for gold deposit exploration and mining. The Saudi Mining Company (Ma’aden) has initiated a comprehensive gold exploration campaign in this district. A number of studies have examined the lithology and mineral occurrences in the Zalm district [1,2,3,4,5,6,7,8].

Current and future investigations into gold mineralization in the Zalm area will greatly benefit from a closer examination of the link between tectonics and ore genesis. In this field, aeromagnetic data effectively aid in defining the favorable mineral localization structures, including rock properties, faults, lineaments, and shear zones [9,10,11,12]. Gobashy et al. [13] applied a combination of digital magnetic filters to a well-known Au mineralization zone to delineate gold mineralization sites enhancing the identification of gold prospects using magnetic data. Eldougdoug et al. [14] employed geophysical techniques to link gold mineralization with the altered ultramafic rocks associated with faulting. In the present study, aeromagnetic data and applied filtering techniques are used to delineate favorable areas of mineral deposits and potential pathways for ascending hydrothermal fluids focusing particularly on structural lineaments, faults, and shear zones in the Zalm region. This region is located east of the Nabitah suture belt and west of the Afif terrane, between Latitude 22°00′ N and 23°00′ N and Longitude 42°00′ and 43°30′E (Figure 1). The ongoing and future exploration of gold mineralization in Zalm district will benefit greatly from this study.

Figure 1 
               The Arabian Shield geologic map showing the tectonic terranes and their boundaries [15].
Figure 1

The Arabian Shield geologic map showing the tectonic terranes and their boundaries [15].

2 Geological overview

The formation of the 40–100 km thick lithosphere of the Arabian Shield was driven by the division of the Arabian Shield into distinct tectonostratigraphic terranes (Figure 1) composed of Tonian (1,000–850 Ma) and Cryogenian (850–650 Ma) volcanic and plutonic rocks [16,17]. Ophiolite-lined sutures (e.g., Yanbu, Bi'r Umq, Nabitah, and Al Amar) divide these terranes (Figure 1), which were joined by accretionary process [16,18,19,20]. According to Stoeser and Camp [19], the Afif terrane is a complex assemblage of volcanic-arc periods overlain by 710 Ma volcano-sedimentary stages in deep basins. The Zalm region (Figure 2) is situated on the western side of the Afif terrane [21]. This region has drawn the interest of numerous earth scientists due to its historic gold and tungsten mine workings and gold mineralization, particularly near the Nabitah suture zone [21,22,23,24,25,26,27,28,29,30,31,32,33]. Based on the host rocks and structural setting, primary gold mineralization can be divided into three basic categories, according to Harbi et al. [25]. The first category is connected with sedimentary sequences formed by volcanics, and includes significant sulfide deposits [26,27,28,34]. The second category as stated by Al Shanti [34] is spatially connected with carbonatized ophiolitic ultramafic rocks. The third category is widespread east of the Nabitah suture zone and west of the Afif terrane, where late- to post-tectonic (640–610 Ma) diorite–granite plutons are found [21,29,30,31,32]. Gold deposits in the Zalm district are controlled by intraplate structural and/or magnetic activity [33]. The Nabitah suture belt, near the Zalm area, is characterized by prominent NS and NW structural trends [35]. The main NW-oriented faults are associated with the Najd fault system, which was active during the most recent tectonic event of the Pan-African orogeny that affected the Arabian Shield [35]. According to previous studies, the Najd fault system was crucial in the formation of the gold deposits in the Arabian Shield as well as those in the Zalm area [1,36,37,38]. The importance of Najd faulting in the genesis of gold ores in the Zalm region was confirmed by the structural data obtained by Agar [1], who analyzed the movement vectors of the Najd fault system at the Zalm district, including the Bi'r Tawilah deposit area. The main shear components of the regional fault system in this area are thick, barren quartz veins trending in the NW and NE directions.

Figure 2 
               A generalized geologic map of Zalm district [1].
Figure 2

A generalized geologic map of Zalm district [1].

3 Data and methods

The aeromagnetic data of the Zalm district was collected as part of government-sponsored aeromagnetic survey that covered central and western Saudi Arabia between 1962 and 1983. A line spacing of 800 m and an altitude of 150–300 m above ground level was used for most of the Arabian Shield data collection. To create the total magnetic intensity (TMI) map for the entire region, the surveys were fully re-leveled using specialized techniques, combined, and gridded at 200 m intervals. Since the processing eliminated almost all leveling errors, resulting in only slight discontinuities at the survey boundaries, no upward continuation was used [39,40,41].

The obtained TMI gridded datasets (Figure 3) were further processed by reducing them to the magnetic pole using the estimated magnetic inclination and declination (32.294° and 2.297°, respectively) for the study area (Figure 4). Reduced to the magnetic Pole (RTP) transformation was conducted using Fourier Domain filtering provided by MAGMAP, Geosoft 8.3.3 package [42] after which the residual field was produced. Thereafter, other forms of processing and enhancement filtering techniques were applied. The RTP grid was subjected to two enhancement filters; the first vertical derivative (1VD, Figure 5) and the analytical signal (AS, Figure 6). Nabighian [43] proposed the 1VD to enhance shallow features with their boundaries and associated lineaments by using 3D Hilbert transforms in the x and y directions. This approach highlights and maps shallower sources by emphasizing short-wavelength anomalies over large ones. By combining the vertical and horizontal gradients of the magnetic anomaly, the AS [44] produces a maximum directly over source bodies and their edges [45]. This filter emphasizes short-wavelength anomalies and is used to highlight discontinuities and reveal the anomaly texture [46]. Thus, to identify that the litho-structural features are related anomalous zones that may be useful in delineating the mineralization occurrences, this study employed first-order vertical derivatives and AS techniques.

Figure 3 
               TMI map of the Zalm district, west Saudi Arabia.
Figure 3

TMI map of the Zalm district, west Saudi Arabia.

Figure 4 
               RTP map of the Zalm district, west Saudi Arabia.
Figure 4

RTP map of the Zalm district, west Saudi Arabia.

Figure 5 
               1VD map of the Zalm district, west Saudi Arabia.
Figure 5

1VD map of the Zalm district, west Saudi Arabia.

Figure 6 
               AS map of the Zalm district, west Saudi Arabia.
Figure 6

AS map of the Zalm district, west Saudi Arabia.

In this study, the minimum curvature method as described by Briggs and Swain [47,48] was used for data gridding. This method interpolates the data by fitting a two-dimensional surface to the raw XYZ data in a way that minimizes the surface curvature.

4 Results and discussion

In the current study, 1VD and AS filtering techniques were applied to process and evaluate aeromagnetic data (Figure 4) of the Zalm district in order to facilitate structural interpretation. The near-surface structures, such as faults, are well-represented by the 1VD map (Figure 5), where the filter accentuates short-wavelength anomalies responsible for shallow sources while suppressing long-wavelength ones. Additionally the AS map (Figure 6) draws attention to the variance in the magnetization of the magnetic sources in the study area. Unlike the 1VD map (Figure 5), the AS map allows for the accurate identification and mapping of various rock units, considering both their mineralogical compositions and depths.

According to Telford et al. [49], strong magnetic anomalies are typically associated with rocks rich in ferromagnetic minerals and low in felsic minerals. Consequently, high magnetic anomaly areas around the Zalm city, the Rada fault zone and the Nabitah fault zone, as shown in the interpreted RTP map (Figure 7), can be correlated to the ultramafic and volcanic rocks that contain mineralization sources [50,51,52,53,54]. According to previous literature [22,23,24,34], gold deposits are located near the ultramafic rocks of the Zalm district which are associated with the Nabitah and Rada suture zones. However, the central zone of the study is characterized by N–S trending low magnetic anomalies (Figure 7) that may correlate with felsic diorite, granodiorite, and granite zones bounded by the N–S faulting [8]. According to Surour et al. [8], these felsic rocks hosting sulfide gold ores with the intrusion-related Bi'r Tawilah gold mineralization is a notable example of these deposits [30,53].

Figure 7 
               RTP map with delineated structural lineaments of the Zalm district, west Saudi Arabia.
Figure 7

RTP map with delineated structural lineaments of the Zalm district, west Saudi Arabia.

A structural lineament map was constructed (Figure 8), based on the examination of aeromagnetic maps (Figures 7, 9, and 10). Using the several filtering techniques, especially the 1VD (Figure 9) and AS (Figure 10), numerous faults were delineated. The three dominant faulting systems in the area – the NW, NE, and NS faulting systems – are represented by lineaments traced from RTP, 1VD, and AS maps (Figure 10). This result is consistent with the structural data from the study by Agar [1] who analyzed the fault system at the Zalm district and with Surour et al. [8], who hypothesized that the N-S faulting system serves as a significant conduit for channeling hydrothermal fluids, based on mineralogical and microstructural data. Surour et al. [8] concluded that the major NW-Najd faulting system, which significantly affects the Zalm district [5557], is responsible for all shears and conjugate fractures at the mineralization zone. Surour et al. [8] further concluded that the mineralization occurrences in the Zalm region appear clearly associated with the NW-trending shears and the NS slip faulting.

Figure 8 
               A map of the vectorization structural lineaments of the Zalm district, west Saudi Arabia.
Figure 8

A map of the vectorization structural lineaments of the Zalm district, west Saudi Arabia.

Figure 9 
               1VD map of magnetic data with mapped structural lineaments of the Zalm district, west Saudi Arabia.
Figure 9

1VD map of magnetic data with mapped structural lineaments of the Zalm district, west Saudi Arabia.

Figure 10 
               AS map of magnetic data with mapped structural lineaments of the Zalm district, west Saudi Arabia.
Figure 10

AS map of magnetic data with mapped structural lineaments of the Zalm district, west Saudi Arabia.

According to Surour et al. [8], the interpreted NW and NS lineament zones act as channels for hydrothermal fluids migrating and reacting with the rock formation, resulting in subsequent alteration. The interpreted lineaments with high complexity trending in the NS and NW directions indicate a strong potential for gold mineralization similar to other structurally controlled locations such as Bi'r Tawailah and Zalm district which are in hydrothermally altered zones that offer favorable conditions for gold occurrence [8]. Consequently, four prospective locations are delineated by interpreting structural trends in respect to the recognized mineralized zones. These likely locations (designated as PMZ-1, PMZ-2, PMZ-3, and PMZ-4) are suggested for further investigation of gold mineralization (Figure 11). However, a detailed, more thorough geological and geophysical study is required to accurately detect ore deposits in the proposed localities.

Figure 11 
               Proposed localities (labeled by PMZ-1, PMZ-2, PMZ-3, and PMZ-4) for future gold mineralization exploration in the study area.
Figure 11

Proposed localities (labeled by PMZ-1, PMZ-2, PMZ-3, and PMZ-4) for future gold mineralization exploration in the study area.

5 Conclusion

The Zalm district, located in western Saudi Arabia, is in high demand for additional research due to its notable gold potential and the presence of abandoned gold mine workings. The gold deposit in the Zalm district is an example of Pan-African gold mineralization. Magnetic mapping of the lithology and structural faulting in the district was conducted using enhancement techniques, namely, RTP, 1VD, and AS, to identify probable gold mineralization zones. According to interpretations of the aeromagnetic maps, the primary structural faulting systems affecting the Zalm district are the NW, NE, and NS faulting systems. Based on the pattern and intensity of the magnetic anomalies in the region, the maps show two distinct magnetic anomalies. The NS trending fault zone and areas of low magnetic anomalies, which indicate the dominance of felsic diorite, granodiorite, and granite intrusions, constitute the “Nabitah orogenic zone.” High magnetic anomalies are associated with the gabbro-granite and ultramafic intrusions in the Nabitah suture zone which formed during terrane amalgamation. Massive intrusions of felsic diorite, granodiorite, and granite, as well as mafic-ultramafic intrusions, are thought to be the sources of the host mineralization. Conversely these felsic and mafic intrusions are likely the source of the mineralizing fluids that moved through the NW and NS faults, acting as crucial conduits for the hydrothermal fluids that generally led to ore remobilization in the region. It is hypothesized that the heat from these hydrothermal fluids triggered convection of meteoric water facilitating the leaching of gold from the surrounding rocks [8].

Acknowledgements

This research was supported by Researchers supporting Project number (RSP2025R425), King Saud University, Riyadh, Saudi Arabia.

  1. Author contributions: Hassan Alzahrani contributed to the conception of the manuscript and revised it. Elkhedr Ibrahim contributed importantly to the analysis, review, and editing. Two authors have read and agreed to the published version of the manuscript.

  2. Conflict of interest: All authors declare that there is no conflict of interest.

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Received: 2024-08-13
Revised: 2024-11-03
Accepted: 2024-12-22
Published Online: 2025-02-10

© 2025 the author(s), published by De Gruyter

This work is licensed under the Creative Commons Attribution 4.0 International License.

Artikel in diesem Heft

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Heruntergeladen am 20.10.2025 von https://www.degruyterbrill.com/document/doi/10.1515/geo-2022-0764/html
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