Abstract
This study examines the geochemical and petrographic characteristics of seven bituminite shales from the Kapurdi mine in the Rajasthan, NW India, in order to assess their organic matter inputs and evaluate the oil-prone potentials. These bituminite shale samples exhibit high total organic carbon (TOC) content (up to 45.11 wt.%). The high TOC contents were correlated with low total sulfur content of less than 1 wt.% and suggest that these bituminite shales were deposited in a fresh lacustrine environment. The dominance of such lacustrine environmental setting was confirmed by the presence of the Botryococcus algae. The analyzed bituminite shales are characterized by a bimodal distribution of normal alkanes and relatively low isoprenoid Pr/Ph, Pr/n-C17 and Ph/n-C18 ratios. These characteristics suggest that these bituminite shales contain a blend of organic matter that was derived primarily from algal lacustrine and other aquatic organic matter, with terrigenous land plants and deposited under suboxic to anoxic environmental conditions. Such findings of the organic matter (OM) input and environmental conditions are consistent with mainly Types I and II kerogen and small amounts of Type II/III kerogen, thus yielding both oil and gas prone to higher concentrations of oil generation potential. The dominance of hydrogen-rich kerogen and oil generation potential is in agreement with the findings of high hydrogen index (HI = 240–425 mg HC/g TOC) and H/C atomic ratio of more than 1.20. The abundance of n-alkene and n-alkane doublets in the pyrolysis–gas chromatography (Py–GC) also indicates that these bituminite shales have potential to generate high concentrations of paraffinic waxy oil. Most of the maturity indicators show that the bituminite shales from the Kapurdi mine have not yet entered the main stage of oil generation window, exhibiting a range of immature stages. Therefore, as highlighted in this study, these bituminite shales can be considered as a good candidate for oil shale reoterting processes to release commercial amounts of oil upon using artificial heating techniques such as hydrothermal conversion.
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Introduction
The Kapurdi mine is located in the northern Barmer Basin, along 25° 56′ 44″ N latitude and 71°21′ 17″ E longitude (Fig. 1). The Barmer Basin is associated with the intracratonic tectonic during the early Archean to Holocene period (Bhowmick 2008; Mathews et al. 2020). The Barmer Basin includes sedimentary successions, ranging in age between Mesozoic and Recent (Fig. 2) along with three significant unconformities (Mukherjee et al. 1992). The basin is also filled with thick organic-rich succession, including lignite and organic-rich shales (Fig. 3), with major distributions in the Cenozoic successions (Rana et al. 2005; Aggarwal et al. 2011; Raju and Mathur 2013; Paul and Dutta 2016; Shivanna and Singh 2016; Singh et al. 2020). The lignite deposits of the Eocene succession have received unprecedented attention from numerous researchers (Ambwani and Singh 1996; Kar and Sharma 2001; Shukla et al. 2014; Singh et al., 2017; Singh and Kumar 2018; Mathews et al. 2020). As a result, the genesis, paleodepositional, climatic conditions and the petroleum generation potential of these lignite deposits were investigated based on organic and inorganic geochemistry analyses together with microscopic observations. However, limited works focused on the other organic-rich sediments of bituminite and carbonaceous shales in the Cenozoic successions. In this regard, the current study is focusing on the bituminite shale deposits within the Cenozoic succession from the Kapurdi mine, northern Barmer Basin, south western Rajasthan (Fig. 1).
In the Kapurdi mine, the Cenozoic succession consists of siltstone, sandstone, conglomerate, fullers’ earth, bentonite, bituminite shale, and lignite (Mukherjee et al. 1992; Shivanna et al. 2017). The entire bituminite shales were obtained from the parting present within the lignite deposits of the Early Eocene succession (Fig. 3). These black shales (bituminite shale) were studied as an attempt to expand our knowledge on highlighting the characteristics of organic matter and evaluate its potential for conventional and unconventional resources for further petroleum exploration.
The objective of this study was to investigate the organic matter characteristics, including organic matter content, quality of organic matter (quantitatively and qualitatively), assess the thermal maturity level, and evaluate the petroleum generation potential by applying multiply geochemical techniques coupled with microscopic examinations. In addition, the n-alkane and isoprenoid distributions in the aliphatic hydrocarbon fraction of the extracted shale rocks together with other geochemical and petrological results were discussed and used to assess the nature of organic matter input and environmental conditions at the time of deposition.
Geological background
Barmer Basin is an active rift basin, with a 200 km long and 40 km wide (Farrimond et al. 2015). It was formed as a result of the rapid separation of India plate from Africa plate during the Late Jurassic to Cretaceous (Dolson et al. 2015).
The lithostratigraphic column of the Barmer Basin is presented in Fig. 3. This basin contains clastic sediments ranging from the Mesozoic (Early Jurassic-Late Cretaceous) to Cenozoic (Early Paleocene to Mid Miocene), with the Cenozoic sedimentary succession having the greatest thickness (Fig. 3).
The Mesozoic sequence comprises Jurassic and Cretaceous formations, i.e., Lathi and Ghagga–Hakra (Fig. 3). The Early Jurassic Lathi sediments are mainly sandstones and subordinate shales and were deposited unconformably above the basement rocks of the Precambrian age (Fig. 3). The sandstone of the Lathi Formation is considered good quality reservoir in the Barmer Basin (Dolson et al. 2015).
The Lower Cretaceous Ghagga-Hakra Formation lies unconformably on the Lathi sediments comprising mainly non-marine (fluvial and lacustrine) sandstones (Fig. 3). The Ghagga-Hakra Formation also exhibits organic-rich shales and is considered as a potential source rock in the Barmer Basin (Dolson et al. 2015). The Ghagga–Hakra Formation overlies by the Deccan Trap volcanics (Upper Cretaceous–Lower Paleocene). The Deccan volcanics make a conformable contact with the Mesozoic (Late Cretaceous) and Cenozoic (Early Paleocene) sequences. The Cenozoic (Early Paleocene-Mid Miocene) sequence in the basin comprises many formations, namely Fatehgarh, Barmer Hill, Dharvi/Dungar, Thumbli, Akli Nagarka, Jagadia, and Uttarlai (Fig. 3).
The Fatehgarh Formation is dominated by organic-rich shale and sandstone intervals accumulated in braided to meandering channels (Dolson et al. 2015). These sandstone intervals are regarded as important reservoir rocks in the Barmer Basin, with porosity and permeability values ranging from 17 to 33% and 200 to 20,000 mD, respectively (Dolson et al. 2015). During the Late Paleocene, mainly lacustrine shale and sandstone sediments of the Barmer Hill Formation were deposited conformably above the Fatehgarh Formation (Fig. 3). The Barmer Hill Formation is followed by the Early Eocene Dharvi/Dungar and Thumbli formations, which consists of black shale intercalated with lignite (Fig. 4). The black shale unit of the Early Eocene Dharvi/Dungar and Thumbli formations was deposited in lacustrine environmental setting (Dolson et al. 2015). The Late Eocene Akli Formation follows the early Eocene Dharvi/Dungar and Thumbli formations, with unconformable contact (Fig. 3). It contains of lacustrine black shale intervals with interbedded swamp lignites (Dolson et al. 2015). It is followed by the Mid Miocene formations (Nagarka, Jagadia, and Uttarlai) (Fig. 3). This young geologic sequence lies unconformably on the Akli sediments (Fig. 3) and mainly composed of cross-bedded sandstone intervals (Dolson et al. 2015).
Dataset and methods
A total number of seven outcrop samples were taken from the Kapurdi mine site (Fig. 1). These outcrop samples exhibit the bituminite shales that were mainly collected from the lignite rock unit (Fig. 1). The samples were cleaned before geochemical and petrological analyses to eliminate impurities such as weathering and oxidation.
The bituminite shale samples were subjected to multi-geochemical analyses, utilizing total organic carbon (TOC) and sulfur (TS) contents, Rock–Eval programmed pyrolysis analysis, ultimate analysis, pyrolysis–gas chromatography (Py–GC), bitumen extraction and gas chromatography–mass spectrometry (GC–MS), along with microscopic examinations of the maceral types and reflectance measurements of huminite/vitrinite (VRo %).
Total organic carbon content (TOC), programmed pyrolysis (Rock–Eval-6) analysis
The seven shale samples were ground to generate standardized powder for the source rock geochemical analyses such as TOC content and programmed pyrolysis.
A 100 mg powdered (< 200 mesh size) was utilized to evaluate TOC content using a LECO CS244 Carbon/Sulfur Analyzer instrument, and the results were primarily expressed as weight percentages (TOC wt.%).
The seven shale samples also underwent programmed pyrolysis with a programmed oven temperature between 300 and 600 °C. Rock–Eval 6 instrument was used to measure the bulk pyrolysis on the powdered samples according to the procedure outlined by Espitalie et al. (1977) and Lafargue et al. (1998).
This instrument was used to evaluate the petroleum yields such as free petroleum (S1, mg HC/g rock) and hydrocarbon yield from kerogen cracking (S2, mg HC/g rock) at a temperature between 300 and 600 °C. The S3 peak also released during programmed pyrolysis, which represents the quantity of CO2 formed by pyrolysis of the organic matter and expressed in milligrams of CO2 per gram of rock (mg/g).
The maximum temperature (Tmax) of S2 peak was also measured during pyrolysis analysis (Table 1). Because Tmax refers to the temperature at which the maximum S2 peak yield is most reliable when the S2 values surpass 1 mg/g rock, it is employed for samples with S2 values above 1 mg HC/g TOC (Jarvie et al. 2001; Katz and Lin 2021).
Furthermore, the geochemical parameters like hydrogen index (HI), oxygen index (OI) and production index (PI) were also determined (Shown in Table 1), following the studies of Peters and Cassa (1994).
Ultimate elemental analysis
The ultimate analysis was also performed on the bituminite shale samples following the standards of ASTM D3176-09 (2009). The whole fine grounded samples were analyzed using an elemental analyzer to measure carbon, hydrogen, nitrogen and sulfur (CHNS) contents in percentage. Subsequently, the oxygen content was calculated based on the difference in the percentages of the CHNS contents. The atomic ratios of H/C and O/C were then calculated following the procedure of ASTM D3176-09 (2009).
Open pyrolysis–gas chromatography (Py–GC)
The seven shale samples were subsequently subjected to open pyrolysis–gas chromatography (Py–GC) and used to obtain information on kerogen characteristics and compositions (Dembicki et al. 1983; Horsfield 1989; Dembicki 1993; Abbassi et al. 2016).
The Py–GC examines ~ 2 mg of each sample, applying a Frontier Lab Pyrolyzer System in thermal desorption (40–330 °C) and pyrolysis (600 °C) as outlined by Larter (1984).The Py–GC analysis was programmed from 40 to 300 °C before pyrolyzate flowed through the GC column between 300 and 600 °C. The chromatography of the pyrolyzates at 600 °C shows a methane spike followed by a set of n-alkane and n-alkene double spikes, along with a few aromatic peaks occurring among them.
Bitumen extraction and gas chromatography–mass spectrometry (GC–MS)
Representative three shale samples were subjected to the extraction process and gas chromatography–mass spectrometry (GC–MS) analysis.
The soluble bitumen was extracted using an azeotropic mixture of dichloromethane (DCM) with methanol (CH3OH) with a ratio of 93:7 for approximately 72 h. The extracted bitumen in these shale rocks was fractionated into three fractions aliphatic and aromatic hydrocarbons and polar (NSO) compounds using liquid column chromatography with silica gel.
In addition, the aliphatic fraction was analyzed by applying Agilent 5975B inert MSD gas chromatography-mass spectrometry (GC–MS) using a HP-5MS column, with temperature ranging from 40 to 340 °C at a rate of 4 °C/min and a holding time of 30 min at 300 °C. The GC–MS analysis was employed to assess the lipid biomarkers in the saturate hydrocarbon fraction such as n-alkanes and isoprenoids applying specific ions, e.g., m/z 85, and their proportions and parameters were measured from their peak heights.
Organic petrology
The seven shale bituminite samples also underwent microscopic examinations comprising maceral types and reflectance measurements of huminite/vitrinite (VRo) under plane-polarized reflected white and ultraviolet (UV) lights.
The polished sample blocks were investigated under microscope for the identification of organic facies. In this case, entire whole shale samples were broken into pea-sized fragments (~ 2–3 mm) and placed in molds through a mixture of Serifix resin and cold-mount hardener. Being hardened, the blocks were grounded to expose the sample surfaces using silicon carbide papers with varying grit sizes; then, they were singly polished using alumina powder and oxide-polishing suspension solution.
The polished blocks then underwent examination using oil immersion under both reflected white and ultraviolet (UV) light using a LEICA DM 2700P optical microscope coupled with fluorescence illuminators photometry microscope. The quantitative and qualitative analyses of maceral types, including huminite, liptinite, and inertinite, were carried out following ICCP (2001), Sýkorová et al. (2005), Hower and Wagner (2012), and Pickel et al. (2017). In this case, reflected UV lights were used to discriminate maceral types for each sample.
In addition, the reflectance of huminite/vitrinite (VRo) measurements was also performed on the polished blocks using reflected white light. The huminite/vitrinite (VRo %) reflectance was measured after calibration using a reflectance standard value of 0.42% under oil immersion, in a white plane-polarized reflected light using a DM 2700P Leica Microsystems, and the mean of reflectance values was calculated for 25 measurements per sample.
Results and interpretation
Organofacies characterization (organic petrology)
Microscopic examinations were carried out to identify maceral types in the analyzed bituminite shales. The overall composition of the macerals was determined on the basis of mineral matter and mineral matter free with the observations is presented in Table 1. The results show that these bituminite shale samples are entirely dominated by mineral matter between 61.38 and 83.18% (Table 1). The shale samples have a high abundance of the huminite and liptinitic macerals that were derived from terrestrial organic matter, ranging from 33.60 to 70.50% and 25.03 to 64.18%, respectively (Table 1). The occurrence of inertinite macerals of the terrestrial organic matter is also commonly present in the studied samples in the range of 1.09–9.86% (Table 1).
The results of the optical observations under the UV-light excitation show that most of the hydrogen-rich liptinite macerals are structured and unstructured organic matter and are characterized by fluorescence intensities ranging from orange to yellow (Fig. 4). Most of the structured organic matter includes suberinite, sporinite, cutinite and alginite (Fig. 4). Sporinite occurs as a ring-agglomerated form and is commonly associated with cutinite maceral. Both sporinite and cutinite macerals are characterized by yellow to orange-yellow fluorescence (Fig. 4a and b). Suberinite maceral is also represented and characterized by cell-wall tissue and has fluorescence intensities ranging from brownish-yellow to yellow (Fig. 4c). Hydrogen-rich liptinite, i.e., alginate, is also obtained in some samples, which was primarily presented as Botryococcus (Fig. 4d).
In addition, resinite and bituminite are also found as unstructured liptinite macerals in the studied bituminite shale samples (Fig. 4e and f). Resinite mainly takes the form of isolated globular bodies with various shapes and is characterized by high fluorescence intensities ranging from greenish-yellow orange to bright yellow (Fig. 4e). A small portion of bituminite was also found with an irregular surface and characterized by an orange to brownish-yellow fluorescence (Fig. 4f).
Total organic carbon (TOC) and total sulfur (TS) contents
The organic carbon content (TOC) is commonly inferring the presence of organic matter richness (Bissada 1982; Jarvie 1991; Peters 1986; Peters and Cassa 1994; Katz and Lin 2014).
In this study, the TOC content measurements are conducted for all the bituminite shale samples and as expected the studied samples have high TOC content between 9.44 and 45.11 wt.% (Table 1). Majority of the measurements indicate high TOC > 20 wt.% (21.39–45.11%); meanwhile, two samples exhibit less TOC content between 9.4 and 16.73% (Table 1). The TOC contents of the studied shale samples, overall, indicate organic matter richness.
The total sulfur (S) content in the studied bituminite shale samples was found to be in its lowest amounts, between 0.34 and 0.91 wt.% (Table 1). However, the S content is usually employed to investigate the depositional environments of marine versus non-marine (e.g., Berner and Raiswell 1983). A high S content of more than 1 wt.% implies a marine environment (Hakimi et al. 2016), while a low S content of less than 0.5 wt.% suggests a non-marine environment (freshwater) (Berner and Raiswell 1983; Makeen et al. 2015). Accordingly, the low S content of < 1 wt.% demonstrates that the analyzed samples were deposited in a freshwater environmental setting (i.e., lacustrine).
Programmed pyrolysis (RE) and ultimate elemental
Table 1 also summarizes the S1, S2, S3, HI, OI and PI values obtained by Rock–Eval pyrolysis of the seven bituminite shale samples. The results show that the petroleum generated by the thermal cracking of kerogen (S2) yield is high and found to be the range of 22.74–182.69 mg HC/g rock. Most of the samples (n = 5) have S2 values greater than 70 mg hydrocarbon/g rock (range 73.93–182.69 mg hydrocarbon/g rock), while two samples have S2 yields ranging from 22.74 to 46.46 mg hydrocarbon/g rock (Table 1). The pyrolysis data, on other hand, revealed that the free petroleum (S1) yield in most of the examined samples (n = 5) is substantial, ranging from 1.57 to 7.59 mg hydrocarbon/g rock (Table 1). Two samples show the lowest values of S1 of less than 1 mg hydrocarbon/g rock (Table 1).
In addition, the Tmax, values based on the S2 generation of the analyzed shale samples were found to be more than 1 (22.74–182.69 mg HC/g rock) as shown in Table 1. Therefore, the most reliable Rock–Eval Tmax data were attained between values of 420–429 °C (Table 1).
The HI and OI parameters were calculated utilizing the compatibility of pyrolysis S2 and S3 yields with TOC content, respectively (Table 1). The HI values of the analyzed samples are substantial, ranging from 240 to 425 mg hydrocarbon/g TOC (Table 1). Most of the analyzed samples (n = 5) have HI values of more than 300 mg HC/g TOC, with values ranging from 344 to 425 mg HC/g TOC (Table 1). However, two samples show the lowest HI values between 240 and 277 mg HC/g TOC (Table 1). In terms of OI values, most of the samples have values of ˂ 50 mg CO2/g TOC (14–40 mg CO2/g TOC; Table 1).
The H/C and O/C atomic ratios were also obtained in addition to the HI and OI data (Table 1). The H/C atomic values are substantial and found to be in the range between 1.21 and 1.58 (Table 1). In contrast, the analyzed samples have low O/C atomic values of less than 1, ranging from 0.42 to 0.76 (Table 1).
Open pyrolysis–gas chromatography (Py–GC)
The Py–GC method which employs the distributions of n-alkene and n-alkane doublets coupled within light aromatic hydrocarbon of the pyrolyzate S2 provides a critical insight about the kerogen composition and petroleum-generating facies in the investigated samples (Dembicki 1993, 2009; Horsfield 1989; Dembicki et al. 1983; Abbassi et al. 2016). In this study, the Py–GCs of pyrolyzate S2 in the representative four samples are shown in Fig. 5. The chromatograms show bimodal distributions of the carbon peaks, ranging from C5 to beyond C30 of n-alkene and n-alkane aliphatic compounds. The n-alkane and n-alkene compounds in most of the samples are highly concentrated in low and high molecular carbon fractions. The aromatic hydrocarbons are also present in low concentrations and are mainly toluene, xylene, and benzene alkylbenzenes. Besides aliphatic and aromatic hydrocarbons, the pyrolyzates also include low amounts of 2, 3-dimethylthiophene (Fig. 5).
Normal alkane and isoprenoid distributions
In the current study, the hydrocarbon distributions of n-alkane along with acyclic isoprenoids (i.e., pristane and phytane) in the saturated HC fraction of the representative three extracted shale rocks were examined and are shown in chromatograms of GC (Fig. 6), and their ratios and parameters are presented in Table 1. In the chromatograms of the samples, the normal alkanes and isoprenoids display bimodal distribution of low to high molecular weight compounds, ranging from n-C8 to n-C36 (Fig. 6). The carbon preference index (CPI) values were calculated using the distributions of normal alkane by the following equation: CPI = [2(C23 + C25 + C27 + C29)/(C22 + 2(C24 + C26 + C28] + C30)]; and range from 1.98 to 2.30 (Table 1).
In addition to n-alkanes, the chromatograms of most of the samples are also the presence of the pristane (Pr) and phytane (Ph) isoprenoid hydrocarbons (Fig. 6). For most of the samples, the predominance of Pr over Ph (Fig. 6) results in a Pr/Ph ratio of more than 1 (1.17–2.70) as shown in Table 1. Additionally, isoprenoid ratios relative to n-alkane concentrations (C17-C18) were also determined as Pr/n-C17 and Ph/n-C18 ratios and found to be in the range of 0.20–0.69 and 0.20–0.31, respectively (Table 1).
Discussion
Organic matter input and environmental conditions
The organic matter input, its origin and the depositional environment of the analyzed bituminite shales were primarily investigated by applying normal alkane and isoprenoid in the saturated hydrocarbon together with microscopic results as previously described.
Normal alkanes and isoprenoids can permit postulating logical interpretations related to the nature of organic matter and its environmental conditions during deposition (Waples and Machihara 1991; Hadad et al. 2021).
In the present study, the normal alkanes and isoprenoids in the saturated HC fraction are portrayed by a bimodal distribution of low-medium molecular weight (n-C8–n-C25) and notable amounts of waxy alkanes (+ n-C25) as shown in Fig. 6. As a result, this distribution of n-alkanes suggests a mixture of organic matter of aquatic and terrestrial organic matter input (Alias et al. 2012; Sarki Yandoka et al. 2015).
The higher contributions from the aquatic organic matter and terrestrial source inputs into these shale sediments are compatible with isoprenoids and their Pr/Ph, Pr/n-C17 and Ph/n-C18 ratios. Such isoprenoid ratios can also aid interpretation of the paleodepositional environment as an indicator of redox conditions (e.g., Didyk et al. 1978; Ten Haven et al. 1987; Chandra et al. 1994; Peters et al. 2005; Tserolas et al. 2019). Generally, a low Pr/Ph ratio of less than 1.0 indicates strongly anoxic conditions commonly associated with a stratified water column, whereas a high Pr/Ph ratio of more than 3.0 is related to more terrestrial organic matter input under oxic environmental conditions (Didyk et al. 1978). In this regard, the studied bituminite shale samples with Pr/Ph values between 1.17 and 2.70 suggest suboxic environmental conditions during deposition. The isoprenoid Pr/n-C17 and Ph/n-C18 ratios further indicate high contributions of mixed organic matter inputs that were most likely deposited in suboxic to relatively anoxic environmental conditions (Fig. 7A). The combination between the isoprenoid ratios of Pr/Ph and Pr/n-C17 can also be used to provide information on organic matter input (e.g., Hughes et al. 1995; Williams et al. 1995; Hakimi et al. 2012; Alias et al. 2012; Sarki Yandoka et al. 2015). Marine organic matter usually has Pr/Ph ratios of less than 1 (Hakimi et al. 2012; Gharib et al. 2021; Hadad et al. 2021), while terrestrial organic matter has ratios of greater than 3.0 (Alias et al. 2012; Sarki Yandoka et al. 2015). The relationship between Pr/Ph and Pr/n-C17 ratios suggests a mainly lacustrine organic matter input (Fig. 8B). This interpretation of the organic matter input and the depositional environment of the analyzed bituminite shales are compatible with the geochemical proxies and maceral types that were observed under light microscopy.
The high TOC of up to 45.11 wt.% confirms the presence of the relatively reducing (suboxic-relatively anoxic) conditions that consequently enhanced the enrichment of organic matter during the deposition of the bituminite shale. However, the high TOC content is also correlated with low sulfur content and further shows that these bituminite shales being deposited in a non-marine environment (i.e., lacustrine), as shown in Fig. 8. The presence of the Botryococcus algae in some of the studied samples (Fig. 4d) is evident that the shales were deposited in freshwater lacustrine environments (e.g., Makeen et al. 2015).
Organic matter characterization and implications on source rock effectiveness and petroleum generation potential
This section discusses the potential of petroleum generation based on the characteristics of organic matter in the analyzed bituminite shales using integration multi-geochemical results and microscopic features of the organic facies.
The main factors controlling the amount of and type of petroleum generation in the source rocks are the organic richness and composition of the organic matter input (Dow 1977; Peters and Cassa 1994; Ardakani et al. 2017; Abdullah et al. 2017; Makeen et al. 2019; Aziz et al. 2020; Ahmad et al. 2022; Sohail et al. 2022).
The presence of adequate volumes of organic matter in the source rocks is the critical factor for controlling their generative potential once thermal maturity is attained (Peters 1986; Bordenave 1993; Peters and Cassa 1994; Aziz et al. 2020).This study presents high TOC contents from the investigated bituminite shale, overall, highlighting organic matter richness capable of generating hydrocarbons. The highest TOC content is correlated with high S1 and S2 yields and indicates that most of the analyzed bituminite shale samples have very good to excellent petroleum generative potential (Fig. 9).
The quality of organic matter in terms of kerogen typing is another critical factor in predicting the petroleum generation potential from source rocks (e.g., Espitalie et al. 1985; Peters and Cassa 1994; Mukhopadhyay et al. 1995; Aziz et al. 2020).
The presented Rock–Eval pyrolysis (i.e., the HI and OI) results show that most of the examined samples contain mainly Type II kerogen, with small contributions of mixed II/III kerogen as indicated from the van Krevelen diagram of HI against OI (Fig. 10a). The modified van Krevelen diagram of programmed pyrolysis HI and Tmax values also confirms the predominance of Type II kerogen, with mixed Type II/III kerogen and all fall within the immature zone (Fig. 10b).
In addition, the H/C and O/C atomic ratio is used to corroborate the kerogen characteristics (Hunt 1996; Erik 2011). The high ratios of H/C atomic indicate rich oil-prone Type I and II kerogens, while high O/C atomic indicates gas-prone Type III kerogen (Peters and Cassa 1994; Hunt 1996). Accordingly, the kerogen type in the analyzed bituminite shale samples is mainly oil-prone kerogen and classified as Types I and II based on their high ratio of H/C atomic in the range of 1.21–1.59 and low O/C atomic between 0.42 and 0.76 (Table 1). In this regard, four samples have Type II kerogen, while other three samples have Type I, as implied from the Van Krevelen’s diagram of H/C and O/C atomic ratios (Fig. 10c).
The dominant presence of high n-alkene and n-alkane doublets with low amounts of light aromatic hydrocarbon (Fig. 5) suggests that the studied bituminite shales are likely to be oil-prone kerogen (e.g., Hasiah 1999; Harry 2008; Hakimi et al. 2013, 2015; Makeen et al. 2019). This interpretation of kerogen type is strongly demonstrated by a ternary plot modified by Eglinton et al. (1990), which used relative percentages of three pyrolyzate compounds, i.e., 2,3-dimethylthiophene, ortho-xylene, and carbon 9 (Fig. 11A).
This is further confirmed by the maceral types under microscope. However, when the results of the maceral composition in the analyzed samples (Table 1) were plotted on the Cornford (1979) ternary diagram, it was observed that the dominating organic matter is largely Type II kerogen, with small amounts of mixed Type II/III kerogen, as shown in Fig. 11B. The Type II kerogen is mainly consistent with hydrogen-rich liptinitic terrestrial organic matter, including alginite, sporinite, cutinite, resinite and bituminite (Fig. 4). Other samples with more than 60% and less than 80% of huminite macerals were likely to be Type II/III kerogen (Fig. 11B).
By evaluating the maceral composition and organic geochemical data, it is evident that these distributions of mainly Type II and II/III kerogen in the bituminite shale rocks are both oil- and gas-prone resources, with strong oil generation potential, as implied from the cross-plots of the TOC, HI, and S2/S3 geochemical data (Fig. 12A, B). The high contribution of oil generation potential from these bituminite shale rocks is confirmed by the high proportion of liptinitic materials (Fig. 13A). However, most of the hydrogen-rich liptinite macerals (i.e., sporinite, resinite, cutinite and suberinite) can generate paraffinic oil with a high waxy characteristic as reported by previously published works of Taylor et al. (1998) and Petersen et al. (2013) (Fig. 6). The high waxy characteristic of the expected oil to be generated from the analyzed samples is also consistent with the distributions of n-alkene and n-alkane doublets in the Py–GC results (Fig. 5). The relative percentages of pyrolyzate compounds, i.e., total resolved C1 to C5 hydrocarbons, the sum C6 to C14, and C+15 of the n-alkenes/n-alkane ranges (Table 1) were plotted on the ternary diagram of Horsfield (1989) and indicate that the expected oil generating potential from the studied bituminite shale samples is mainly paraffinic oil, with high wax content (Fig. 13B).
Besides, the oil generation capacity of the analyzed bituminite shale samples was further assessed from the thermal maturation of the organic matter. The thermal maturity level of the analyzed bituminite shale samples was primarily evaluated using huminite/vitrinite reflectance (VRo %) data. These measurements are the best indicators in providing valuable information about the organic maturation and evolution of the petroleum generation capacity (Sweeney and Burnham 1990; Teichmüller et al. 1998). In this regard, the reflectance of the huminite/vitrinite in the studied samples was measured and found to be in low range between 0.29 and 0.35% (Table 1). This indicates that these bituminite shale rocks are still in immature stage and have not yet generated oil. The temperature of the maximum pyrolysis rate (Tmax) is also commonly used to estimate the maturity of kerogens; as they mature, their Tmax values increased (Bordenave 1993; Peters 1986; Tissot et al. 1987; Tissot and Welte 1984). However, the Tmax is affected by several parameters, including migrated HCs, oil-based mud, and low pyrolysis response (Espitalie et al. 1985; Ahmed et al. 2022). The Tmax values depend on the S2 measurements, and the best Tmax values were observed in samples with S2 > 1 mg/g rock (Jarvie et al. 2001; Katz and Lin 2021). The analyzed samples of this study have S2 of more than 70 mg/g rock (Table 1); hence, the maturation of the organic matter could be estimated through the measured Tmax values. The Tmax values of the samples range from 420 to 423 °C (Table 1), which indicates immature sources. This confirms the previously obtained VRo that agrees that most of the analyzed shales fall within the immature stage of the oil generation window (Fig. 14A).
The state of thermal maturity is further supported by the PI values obtained via the Rock–Eval pyrolysis. Low PI value of < 0.10 indicates immature organic matter, whereas a PI value between 0.10 and 0.40 suggests mature source rock (Peters 1986; Hazra et al., 2019). In agreement with the previously obtained VRo and Tmax maturity data, the calculated PI values of less than 0.10 (Table 1) confirm that most of the studied shale samples are thermally immature source rocks (Fig. 14B). As a result, the organic matter of the bituminite shales collected from the Kapurdi mine has not yet reached the sufficient maturity levels to generate oil but can be recommended for oil shale retorting processes to release commercial amounts of oil upon using artificial heating techniques such as hydrothermal conversion.
Conclusions
The bituminite shale rocks from the Kapurdi mine in the northern Barmer Basin, NW India, were subjected to extensive organic geochemical and petrological analyses to investigate the characteristics of organic matter and the potential for oil generation. The conclusions from the results of this study are highlighted below.
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The analyzed bituminite shales have high TOC content of up to 45.11 wt.% and petroleum potential of up to 190.28 mg hydrocarbon/g rock, making them excellent source rocks for petroleum generation.
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The high TOC contents were correlated with low total sulfur content of < 1 wt. % and suggest a non-marine environment (i.e., lacustrine) during the deposition of these bituminite shale sediments. The dominant liptinitic terrestrial macerals with the presence of the Botryococcus algae confirm lacustrine environmental setting.
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The major portion of the analyzed bituminite shales is plotted along the hydrogen-rich kerogen (i.e. Types I, II and II/III), with high hydrogen index values (240 and 425 mg HC/g TOC) and high H/C atomic ratio of more than 1.20 as well as the dominant aliphatic n-alkene and n-alkane doublets with relatively minimal light aromatic components. This indicates that they are mainly oil-prone source rocks, with waxy paraffinic oil potential.
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The maturity-related indicators such as VRo (< 40%) and Tmax of < 430 °C show that the studied bituminite shale samples in the Kapurdi mine are still in an immature stage for oil generation. As a result, the attainment of the low thermal maturation level is not critical for converting the hydrogen-rich kerogen to the oil needed for commercial production.
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This study has shown that the bituminite shales in the Kapurdi mine are prospective unconventional petroleum resources. It can therefore be recommended for oil shale retorting processes to produce commercial amounts of oil using artificial heating techniques such as hydrothermal conversion.
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Funding
The authors Alok Kumar and Alok K. Singh would like to express their gratitude to the Rajiv Gandhi Institute of Petroleum Technology for providing the facilities for organic geochemical investigations. The authors are grateful to the Researchers Supporting Project number (RSP2023R92) at King Saud University in Riyadh, Saudi Arabia, for their support. This work was also supported by the Ministry of Science and Higher Education of the Russian Federation under agreement No. 075-15-2022-299 within the framework of the development program for a world-class Research Center “Efficient development of the global liquid hydrocarbon reserves.” The constructive comments by six anonymous reviewers have improved the original and revised manuscripts and are gratefully acknowledged.Authors, Alok Kumar and Khairul Azlan Mustapha also acknowledge the University of Malaya Post-Doctoral Research Fellowship scheme (associated with grant number IF064-2019). Author, Alok Kumar and Khairul Azlan Mustapha also acknowledge the University of Malaya Post-Doctoral Research Fellowship scheme (associated with grant number IF064-2019).
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Hakimi, M.H., Kumar, A., Singh, A.K. et al. Geochemistry and organic petrology of the bituminite shales from the Kapurdi mine, Rajasthan of NW India: implications for waxy oil generation potential. J Petrol Explor Prod Technol 13, 505–521 (2023). https://doi.org/10.1007/s13202-022-01597-9
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DOI: https://doi.org/10.1007/s13202-022-01597-9