Abstract
The Mamu Formation source rocks in the Anambra Basin are targets for shale gas reservoir. However, fundamental data on the critical pore structures for assessing the shale reservoir capabilities are lacking. In this study, the source rocks were investigated for their mineralogical compositions and pore structure characteristics by X-ray diffraction, accelerated surface area and porosimetry and field emission scanning electron microscopy (FE-SEM). The bulk mineralogy of the samples is dominated by kaolinite and quartz with average percentage composition of 52.0 and 41.5, respectively, suggesting that the rocks are potential candidates for fracking. The total average pore volume and specific surface area in the samples are 0.0421 cm3/g and 22.43 m2/g, respectively. The shale samples show higher amounts of total pore volumes relative to the sub-bituminous coals. No obvious organic pore is observed in the shale samples, but some inherited primary organic matter pores of plant origin exist in the sub-bituminous coals. Therefore, inorganic minerals pores are the major contributors to the pore development in the immature shales. The FE-SEM results reveal that the pore network in the shales is dominated by intraparticle pores and fractures. The observed well-developed fractures within the Mamu shales that may have resulted from tectonic events are capable of positively influencing the petrophysical properties of shales in the basin and by extension assist in shale gas exploration and development in the entire Lower Benue Trough.
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1 Introduction
The understanding of the petrophysical properties such as the porosity, permeability, mineralogy, specific surface area and pore volume of shales, especially the nanopore arrangement is significant in characterising the shale pore structure [1,2,3,4,5] and in providing a practical implication when evaluating the adsorption, desorption, diffusion and gas flow in shales [1, 6]. Shales are complex in nature with heterogeneous porous media [2]; thus, the complex pore network of shale is constrained by several geologic features such as the sedimentary processes, tectonic [7, 8], mineralogy, total organic carbon (TOC) content, thermal maturity [9] and organic matter type [3, 10].
Unlike the conventional hydrocarbon system, the shale gas reservoir is a steady self-contained source-reservoir petroleum system [2], with the nanometre-scale pore system significantly controlling the shale gas storage capacities [11]. Based on the classification published by the International Union of Pure and Applied Chemistry (IUPAC) [12], pores in shale can be categorised into 3 based on their sizes: micropores (pore width < 2 nm), mesopores (pore width between 2 and 50 nm) and macropores (pore width > 50 nm). While taking into account of the different pore types, 3 divisions have been made, namely interparticle (interP) pores, intraparticle (intraP) pores and organic matter pores [4]. Shale gas could be derived from biogenic and/or thermogenic process [13, 14] and in situ accumulated as adsorbed dry gas in the fine micropores and mesopores of the organic matter and clays and also as free gas in the crevices and macropores [9, 13, 14].
The Mamu Formation in the Anambra Basin contains organic matter with confirmed hydrocarbon generation potential [15,16,17]. The formation is composed of alternating shales, sandstones and coal seams [18]. The lower parts of the formation consist of several intervals of shale coexisting with coal, particularly in the middle section of the basin where its depth attains over 300 m [18], thereby positioning the formation as hot spot for possible unconventional shale gas generation. Studies on Mamu Formation have been limited to paleoenvironmental [16, 18,19,20,21] and hydrocarbons generative studies [15,16,17, 22].
As the demand for clean energy source increases, the Mamu Formation remains a target for shale gas resource. However, fundamental data on the pore structure of its source rock are practically not available and these are significant in resource potential evaluation [23]. The occurrence of shale gas depends mainly on the distribution and connectivity of pores for accumulating and forming the flow path network for gas flow [6]. As shales are combinations of minerals and organic-rich rock, the mineralogical compositions also play a major role in controlling the economics of shale gas plays. The different mineral compositions influence the different microscopic pore characteristics of shales [24]. This in turn is controlled by the different depositional environments. Marine shales are considered to be relatively enriched with higher amounts of brittle minerals as compared to shales deposited in lacustrine and fluvial environments [25]. The present study was conducted to investigate the mineralogical compositions, pore characteristics and factors controlling the pores development in the early Maastrichtian Mamu Formation, Anambra Basin. This work is expected to provide useful information and implications for fracturing, pores networks and shale gas potential of organic-rich source rocks in Mamu Formation.
2 Geological background
The geologic and stratigraphic settings of the Anambra basin have been adequately described in the literatures [15, 16, 26, 27]. The basin traverses an area of about 40,000 km2 with roughly 6000 m thick Cretaceous and Tertiary sediments. The Anambra Basin was formed during the Santonian tectonism that affected the entire Benue Trough [28] (Fig. 1). The event was marked with folding, faulting, volcanic extrusion, uplift and exhumation of pre-Santonian sedimentary fill [29]. The Anambra Basin is adjoined to the west by the Precambrian basement complex rocks of the western Nigeria, while Southern Benue Trough and Niger Delta basins restricted it to the east and south, respectively (Fig. 1). Sedimentation began in the basin during the transgressive cycle (Campanian–Maastrichtian) and invariably led to the deposition of the oldest formation (Enugu/Nkporo shales) in the late Campanian. The Early Maastrichtian Mamu Formation overlies the Enugu/Nkporo shale with alternating sandstones, mudstones and shales. This unit also consists of coal seams in the lower parts of the formation at several intervals [18]. The Middle Maastrichtian Ajali Sandstone overlies the Mamu Formation and consists of unconsolidated coarse- and fine-grained siltstone and weakly cemented mudstone [26, 27]. The Ajali sandstone is overlain by Nsukka Formation, which is also referred to as upper coal measure dated Maastrichtian–Danian [26, 30]. The Imo shale (Paleocene) comprising shale with intermittent ironstone and thin sandstone overlies the Nsukka Formation [26, 27, 31]. The youngest strata in the basin are the Ameki Group (Eocene) consisting sandstones, shale, limestone, ironstone and siltstones [30, 32].
3 Materials and methods
3.1 Samples
Twelve core source rocks samples obtained from shallow boreholes ONP1 (7°27′39.0″ N, 7.45′27.0″ E) and ONP4 (7°27′13.9″ N, 7o45′53.5″ E) situated at Onupi, Kogi State, Nigeria (Fig. 1) were collected from depths ranging from 7.65 to 50.5 m. The samples were taken from the Mamu Formation (Early Maastrichtian) in the Anambra Basin. The basic geochemical characteristics of the source rocks have been earlier described [17]. The TOC ranges from 1.30 to 7.37, 14.87 to 24.61 and 57.71 to 58.28% for shale, carbonaceous shale and sub-bituminous coal, respectively. The shale and carbonaceous shale/sub-bituminous coal contain organic matter Type II/III and Type III, respectively. The samples are immature with an average Tmax of 419 °C. The study location and the lithostratigraphy of Anambra Basin are shown in Fig. 1. The generalised stratigraphic chat of the Lower Benue Trough showing the basin and the lithologies of the sampled boreholes is illustrated in Fig. 2.
3.2 Mineral composition and petrophysical analyses
Each sample was pulverized (200 mesh) and oven dried at 80 °C prior to mineral analysis. The mineral analysis was performed using a Bruker D8 Advance X-ray diffractometer with Cu kα radiation (λ = 1.54066 used for CuKα1) operated at 40 kV and 30 mA and scanned step-wisely at 4° min−1 from 3° to 85° (2Ɵ). The relative percentage compositions of the minerals were determined semi-quantitatively by employing area under the curve for the main peaks of every mineral, with adjustment for Lorentz polarization [33]. The instrument’s analytical precision for the results was ± 3%.
Prior to the pore-sizes distribution (PSD) analysis of the rock samples, an approximately 3 g of each rock sample was crushed to 60–120 mesh. The samples were dried at 80 °C and degassed under high vacuum until constant weights were obtained for at least 24 h using a degassing system. Briefly, the PSD was determined using liquid nitrogen (N2) at − 195.8 °C and carbon dioxide (CO2) at 0 °C by employing a micromeritics ASAP 2460 instrument. The glass tube enclosing the degassed rock samples were then lowered into − 195.8 °C liquid nitrogen Dewar. The N2 adsorption measurements of the rock samples at different relative pressures were performed using N2 (purity = 99.999%) as the adsorbate. The equilibrium intervals were 30 s and 45 s for N2 and CO2, respectively. The free spaces were examined independently and inputted manually during the CO2 adsorption measurements [34]. The instrument automatically merged the N2 and CO2 adsorption isotherms.
The FE-SEM imaging of the nanopores was achieved on sample chips after being treated with argon ion-beam milling (IM4000, Hitachi High-Tech). The topographic variation was documented using secondary electron (SE) images, while backscattered electron (BSE) images were used to delineate the compositional variation using both the Hitachi S4800 and Field Electron and Ion Company Helios NanoLab™ 600 systems [24].
4 Results and discussion
4.1 Mineralogical composition
The mineral compositions of the source rocks are listed in Table 1. The Mamu rock samples consist mainly of kaolinite and quartz minerals. The kaolinite and quartz contents vary from 23.7 to 80.9% (av. 52%) and 17.3 to 76.3% (av. 41.5%), respectively. The amount of other minerals present are generally low and include feldspar, illite and pyrite with values ranging from 0 to 11.9% (av. 4.5%), 0 to 6.6% (av. 0.9%), and 0 to 4.4% (av. 0.6%), respectively. The low amount of illite may indicate lower conversion of the clay minerals to illite form due to shallow burial [36]. The presence of kaolinite as predominant clay in the rocks (Table 1) indicates intensive chemical weathering process, which corresponds to the tropical conditions prevailing in the area that resulted in excessive leaching [20, 37]. This idea is supported by Maastrichtian paleoclimatic reconstruction [20, 38] that grouped Nigeria (including Anambra Basin) within the tropical climate zone.
The comparison of the mineralogical compositions of the source rock samples from the Mamu Formation with other shale gas reservoirs source rocks from the United States and China is depicted in Fig. 3. The mineral composition is similar to other shale gas reservoirs from the United States and China [39, 40]. The feldspar content in Mamu source rocks is comparable to that of Barnett shale, while the pyrite content is similar to that of Marcellus shale. Most of the samples are clay mineral (kaolinite)-rich ( > 40%), but also with relatively good amounts of quartz mineral ( > 30%). The high clay mineral contents could reduce the effectiveness of fracturing. However, the appreciable amounts of brittle mineral (quartz) in the samples may negate this effect and preserve the brittleness for fracturing which is a significant factor for the development of shale gas [8, 41]. The clay-rich source rocks in the Mamu Formation would also provide large surface areas that could positively influence the gas sorption capacity [42].
4.2 FE-SEM observations and pore types
The FE-SEM images for the immature shales and sub-bituminous coals are shown in Fig. 4. Fractures and intraparticle pore within the clay mineral platelets are the major pore types in the shale samples along with a few interparticle pores (Fig. 4a–c). No obvious organic matter pore is observed in the shale samples. However, the sub-bituminous coal samples display quite high amounts of organic matter domains and with associated inherited primary organic matter pores of vascular plant origin (illustrated with parallel lines and a cycle in Fig. 4e–f). These primary organic matter pores have been considered important in the distribution and morphology of pores even in late oil maturity to gas maturity samples [43]. Such primary organic pores have also been reported for immature marine Woodford shale in the United States (Ro < 0.35%) and marine-continental coals and Qinshui shale in China [43, 44]. The natural fractures observed in the immature shale samples [Fig. 4b, c] may have emanated from the effect of strong tectonic activities that pervaded the entire Benue Trough during the Santonian period that led to the development of the Anambra Basin [28] (Fig. 1). The plasticity nature of coal may have shielded it from cracking during the tectonic events and as such, no obvious fracture is observed in the sub-bituminous coal samples [Fig. 4].
4.3 Pore characterisation of the samples
4.3.1 Gas adsorption characteristics
The nitrogen adsorption and desorption isotherms for the Mamu source rocks are shown in Fig. 5. The curves generally show an increasing adsorption of nitrogen with increasing pressure in all the samples. All the samples demonstrate some level of adsorption at relative low pressure (P/Po < 0.01), signifying micropores existence [45, 46]. A critical look at the hysteresis loops of the samples reveals that the samples have Type H3 with non-appearance of plateaus at relative high pressure (P/Po > 0.95) [47]. This pattern of hysteresis loops has been linked to conglomeration of plate-shaped particles leading to slit-shaped pores [45, 47, 48]. The primary textural control of mudrock nanostructure had been attributed to clay hosted porosity [45]. Consequently, the high clay mineral (kaolinite) content as indicated by the XRD and FE-SEM analyses (Table 1; Fig. 4) in the Mamu shales and sub-bituminous coals might have spurred the slit-shaped pores observed in the adsorption–desorption isotherms. The CO2 adsorption isotherms for all the samples indicate Type I (Fig. 6a), confirming the existence of pores diameter less than 2 nm [47]. The capacity for adsorption by the samples generally increases with increasing relative pressure with most of the samples showing relatively strong adsorption capacity (1.12–16.2 cm3/g at a relative pressure P/Po = 0.03) (Fig. 6a). The carbonaceous shale and sub-bituminous coal samples with higher TOC contents (TOC > 10%) obviously indicate stronger adsorption capacity even at very low relative pressure (P/Po < 0.005), suggesting more micropores (Fig. 6A), than the shale samples having TOC < 10%. A strong positive correlation (R2 = 0.947) exists between the average quantities of CO2 adsorbed and the total organic content in all the studies samples (Fig. 6b).
4.3.2 Pore volume
The nonlocal density functional theory (NLDFT) technique was employed to determine the pore parameters of the samples based on the CO2 and N2 composited adsorption. This method has proved to be more suitable for exploring a broad pore size range (0.33–100 nm) for organic-rich shale [47, 49]. The values obtained for the pore parameters from the samples are presented in Table 2. The total average pore volume obtained for all the samples is 0.0421 cm3/g. This value is reasonably higher than the values reported from shale gas reservoirs in both Rhuddianian (av. 0.0268 cm3/g) and lower Aeronian (av. 0.0226 cm3/g) sections of Longmaxi Formation, in the Sanquan town, China [49]. The total average values of micropore, mesopore and macropore volumes in the samples are 0.0033 cm3/g, 0.0330 cm3/g and 0.0058 cm3/g (Table 2) amounting to 7.6%, 78.3% and 13.6% of the total pore volumes, respectively. This shows that over 70% of the micropores–macropores volume in the Mamu source rocks is contained within the mesopores, with little contributions from micropores and macropores. The total pore volume of the shale, carbonaceous shale and sub-bituminous coal ranges from 0.0245 to 0.0806 cm3/g (av. 0.0455 cm3/g), 0.0259 to 0.0553 cm3/g (av. 0.0464 cm3/g), and 0.0181 to 0.028 cm3/g (av. 0.0231 cm3/g), respectively. This clearly shows that the average values of the total pore volume of the shales samples are comparatively higher than that of the sub-bituminous coal.
It is instructive to note from the N2 adsorption isotherm (Fig. 7), that samples with higher TOC contents do not normally show stronger N2 adsorption capacity as observed from the CO2 adsorption isotherm (Fig. 6). For example, the shale sample ONP1-45 (TOC = 5.85%) has the highest N2 adsorption up to 56.45 cm3/g (Fig. 7A) as compared to the sub-bituminous coal sample ONP1-39 (TOC = 58.28%), that displays the lowest N2 adsorption capacity (13.64 cm3/g) (Fig. 7B). This suggests that the micropores may be largely associated with organic matter in the samples while mineral compositions and fracture might be accountable for the larger pores.
4.3.3 Pore specific surface area
The total average specific surface area derived for the samples is 22.43 m2/g. This value is relatively lower than the average value reported from Rhuddianian (av. 24.8 m2/g), but higher than the average value from lower Aeronian (av. 18.5 m2/g) sections of Longmaxi Formation, in the Sanquan town, China [49]. The total average values of micropore, mesopore and macropore specific surface areas in the samples are 17.43 m2/g, 4.86 m2/g and 0.14 m2/g (Table 2) amounting to 77.7%, 21.7% and 0.6% of the total pore specific surface areas, respectively. This implies that over 70% of the micropores–macropores surface area in the samples is enclosed within the micropores. The total pore specific surface area of the shale, carbonaceous shale and sub-bituminous coal range from 5.42 to 34.82 m2/g (av. 15.55 m2/g), 11.4 to 38.16 m2/g (av. 29.33 m2/g), and 28.97 to 29.62 m2/g (av. 29.30 m2/g), respectively. This clearly shows that carbonaceous shale and sub-bituminous coal have similar pore surface areas which almost double that of the shale, probably resulting from the large number of micropores in carbonaceous shale and sub-bituminous coal samples. In general, large pore surface areas observed for all the samples along with high amount of clay mineral (kaolinite) suggest excellent gas holding potential [46].
4.4 Constraints on pore development
4.4.1 Constraint of TOC
Previous authors have shown that pore development and porosity of shale gas reservoirs are controlled by the TOC content [9, 50]. In the present study, the TOC content reveals a weak positive correlation with the pore structure parameters (specific surface areas and pore volumes) in the rock samples with TOC < 10% (Fig. 8a–b), but an obvious general negative relationship is observed with pore structure parameters in samples having TOC > 10% (Fig. 8c–d). It is believed that a more dominant factor such as the mineral content could play a more influential role in the pore system development of the samples. Pan et al. [45] have suggested that a fragile relationship exists between TOC contents and the pore structure parameters in source rocks having high clay mineral content. This may have resulted from compaction effects between the soft organic matter pores and clay minerals in the rocks during the burial [2]. However, the observed weak positive association between the pore structure parameters and TOC content in the shales with TOC < 10%, shows that TOC contents remain a contributing factor in the nanopore development of immature shale in Mamu Formation.
4.4.2 Constraint of minerals
The plots between the pore volumes and pore specific surface areas of the samples with TOC < 10% (Fig. 9a and b), indicate a very strong correlation between the pore structure parameters and the clay mineral (kaolinite) with R2 values greater than 0.9 (Fig. 9a and b). This suggests that clay mineral (kaolinite) strongly controlled the pore development of the source rocks samples from Mamu Formation. This is also true for samples with TOC > 10% where the influence of kaolinite on the pore structure parameters shows a positive correlation, except for the micropore pore volume and micropore specific surface area (Fig. 9c and d).
In the contrary, quartz displays a strong negative relationship with pore structure parameters in all the studied samples (Fig. 10). This suggests the terrigenous origin of the quartz in the source rocks where pore development is hindered by secondary growth of pores that occur during diagenesis [46]. Therefore, inorganic minerals are the major contributing factors of pore development in immature deltaic source rocks in Mamu Formation.
4.4.3 Constraint of fractures
Tectonism may appreciably influences the pore type and pore structure evolution of organic-rich shale [8]. The FE-SEM images indicate that fractures are well developed in the immature shales. This is believed to have resulted from tectonic movements. The mesopore and macropore volumes in the shale samples are significantly higher than the sub-bituminous coal (Table 2) and consequently with higher total pore volumes. This may partly be attributed to contributions from fractures which are non-existent in the sub-bituminous coal. Many authors had previously attributed the enhanced total pore volume to the increase in mesopores and macropores caused by the development of cracks and microcracks [49, 50]. These pores and cracks could favour gas release from the shale matrix [49, 51], improve storage space [8], as well as capable of increasing the connectivity of the shale pore network and providing lateral migration conduits for shale gas on a regional scale [49]. Therefore, pore structure of shales in the basin may be largely influenced by fractures resulting from tectonic activities.
4.4.4 Implications for shale gas accumulation and exploration
Although, the samples under study are immature, the deeper parts of the formation contain mature source rocks [16], and more importantly, the more mature source rocks in the pre-Santonian (Cross River Group—Eze-Aku and Awgu Formations) successions of the Lower Benue Trough that are capable of generating oil and gas [15]. The gas generated could migrate up-dip through faults, fractures originated from the effect of strong tectonic activities and even along the Santonian boundary and store within the Mamu Formation due to the large storage space within its shale pore structure. The well-developed natural fractures would save shale gas developmental cost and water resource [7]. Thus, the Mamu Formation is a potential target for shale gas exploration and development for the entire Lower Benue Trough.
5 Conclusions
The reservoir quality of deltaic source rocks from the Mamu Formation in the Anambra Basin, Nigeria was investigated within the context of the mineralogical composition and pore structure characterisation. The bulk mineralogy of the samples is dominated by kaolinite and quartz. The clay-rich source rocks would provide large surface areas that could positively influence the gas sorption capacity, and the relatively high brittle mineral would be favourable to the hydraulic fracturing process. The pore volumes and specific surface areas in the samples are significantly related to the mineral compositions. The FE-SEM images indicate that inroganic mineral pores (intraP pores) and fractures are the dominant pore types in the immature shales. The well-developed fractures that may have originated from tectonic movements will greatly compensate for the intraP pores and improve connectivity, storage space and gas migration pathways in the basin. The pore distribution patterns obtained in this work are critical for further research in shale gas exploration and exploitation in this basin. Owing to the immature and limited numbers of studied samples, further works are required from mature sections in the Basin and by extension, other formations in the Lower Benue with proven potential for economic hydrocarbon accumulation to improve our present knowledge on the pore structural evolution of the source rock with increasing reservoir depths.
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Acknowledgements
This work was supported by the CAS President’s International Fellowship Initiative for Postdoctoral Researchers (grant no. 2018PM0058) and the National Natural Science Foundation of China (grant no. 41772117).
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Faboya, O.L., Sonibare, O.O., Xu, J. et al. Mineralogical and pore structure of organic-rich deltaic shales and sub-bituminous coals from early Maastrichtian Mamu Formation, Anambra Basin, Nigeria. SN Appl. Sci. 2, 2057 (2020). https://doi.org/10.1007/s42452-020-03899-1
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DOI: https://doi.org/10.1007/s42452-020-03899-1