Zhaolin Qi
Yalin Li2*- 1Department of Geological Engineering, Qinghai University, Xining, China
- 2School of Earth Science and Resources, China University of Geosciences, Beijing, China
The Qamdo Basin in eastern Tibet has significant petroleum potential and previous studies indicate that the basin contains thick potential source rocks of the Late Permian and the Late Triassic ages. In this paper, the petroleum potential of samples from measured the Upper Permian and Upper Triassic outcrop sections were evaluated on the basis of sedimentological, organic petrographic and geochemical analyses. Initial evaluations of total organic carbon contents indicated that shale samples from the Upper Permian Tuoba Formation and the Upper Triassic Adula and Duogala Formations have major source rock potential, while carbonate rocks from the Upper Triassic Bolila Formation are comparatively lean in organic matter More detailed analyses of OM-rich shale samples from the Tuoba, Adula and Duogala Formations included Rock-eval, elemental analyses, gas chromatography and organic petrography. Maceral compositions and plots of atomic O/C versus H/C indicate that the organic matter present in the samples is primarily Type II with a mixed source. Analyses of acyclic isoprenoid biomarkers indicate the organic matter was deposited under reducing and sub-to anoxic conditions. Based on the high vitrinite reflectance (Ro>1.3%) and Rock-eval data, the samples are classified as highly to over-mature, suggesting that the Tuoba, Adula and Duogaila Formation shales may generate thermogenic gas. Source rock intervals in the three formations are interpreted to have been deposited in marginal-marine environment during transgressions and under a warm and moist climatic condition.
Introduction
Tibet is located in the eastern part of the petroliferous Tethyan realm (Klemme and Ulmishek, 1991). However, compared to analogous areas to the west such as the Persian Gulf and the Caucasus, petroleum exploration in Tibet has not been successful due mainly to the complexity of the tectonic history (Yin and Harrison, 2000; DeCelles et al., 2002; Wang et al., 2014). Nevertheless, oil shows have been recorded in the Qiangtang Basin which is believed to have significant exploration potential (Fu et al., 2009; Yang et al., 2015). Over 200 surface seeps of solid petroleum have been found at outcrop and five potential petroleum systems have been identified within the Mesozoic succession (Tan et al., 2002; Wang et al., 2009; Zeng et al., 2013). In addition, the Tertiary continental basins, such as the Lunpola Basin, have been received attention as they have the most promising source rocks (Wang et al., 2011a). It was reported that the ‘industrial’’ oil flow was discovered at two wells of the Lunpoa Basin in 1990s (Gu et al., 1999). The Tibetan Plateau is therefore considered be an exploration Frontier with numerous under-explored marine and continental petroliferous basins (Taner and Meyerhoff, 1990a; Wang and Zhang, 1996; Wang et al., 2006).
The Qamdo Basin in eastern Tibet covers an area of more than 10,000 km2 and is similar to the Qiangtang Basin in terms of age, stratigraphy and tectonic setting. Preliminary field surveys (Sichuan BGMR [Sichuan Bureau of Geology and Mineral Resources], 2007; Tibet BGMR [Tibet Bureau of Geology and Mineral Resources], 2007) indicate that thick black shales are exposed at outcrop over large areas of the basin and may have significant hydrocarbon potential. Chen et al. (2010) proposed that the paleo-oil reservoirs in Qamdo area charged with four events during foreland basin stage from the early Jurassic to the early Cretaceous, which had been destroyed or cracked during the strike-slip basin stage of the Cenozoic. The presence of oil-saturated sandstones (Xu et al., 2004) and seepages (Taner and Meyerhoff, 1990b) together with evidence from fluid inclusions in Mesozoic reservoir rocks (Chen et al., 2010; Wu et al., 2010) indicate that hydrocarbon generation, migration and accumulation have taken place in the basin. Moreover, previous study (Du et al., 1997; Peng et al., 2005) of the Late Palaeozoic sequence stratigraphy in the Qamdo Basin unveiled the sea level change of the Qamdo block.
However, detailed studies of source rocks and its linkage with the sea level change have not yet been undertaken. In this study, we investigate the Upper Permian and the Upper Triassic organic rich shales at five outcrop locations in the Qamdo Basin. The purpose of the paper is to analyse the samples’ sedimentological and organic geochemical characteristics and to evaluate their hydrocarbon potential. Factors controlling source rock deposition including sea level changes, climatic variations and regional tectonics, are briefly reviewed.
Geological Setting
The Tibetan Plateau is composed of a series of continental terranes which were accreted to the margin of the Eurasian Plate during the Palaeozoic and Mesozoic (Chang et al., 1986; Yin and Harrison, 2000; Pan et al., 2012). The NW-SE elongated Qamdo Basin in eastern Tibet, the focus of this study, is located on the Precambrian crystalline basement of the Qiangtang-Qamdo terrane (Du et al., 1998). From stratigraphic and structural data, the Qiangtang Terrane can be divided from west to east into the Qiangtang Block in central Tibet and the Qamdo Block to the SE (Chang et al., 1989; Huang et al., 1992), which is sandwiched between the Jinshajiang and Bangong-Nujiang suture zones (Figure 1). The former suture marks the boundary between the Yidun Arc complex and the Qiangtang Terrane which formed during closure of the PalaeoTethys, while the latter separates the Lhasa and Qiangtang Terranes which formed during closure of the MesoTethys (Yin and Harrison, 2000).
FIGURE 1. Simplified structural map of eastern Tibet showing the major suture zones and rivers (modified from Deng et al., 2014). Abbreviations: AKMS, Anyimaqin-Kunlun-Muztagh suture; JS, Jinshajiang suture; BNS, Bangong-Nujiang suture; ITS, Indus-Tsangpo suture.
After the amalgamation of continental blocks and terranes during the Palaeozoic and Mesozoic, regional tectonism during the Cenozoic including the India-Asia collision reshaped the lithospheric structure of the Tibet region (Deng et al., 2014). Late Cenozoic to Recent deformation across the SE portion of the Tibet Plateau is localized on a series of strike-slip faults which accommodate the clockwise rotation of the SE Tibetan Plateau around the Eastern Himalayan Syntaxis (Burchfiel et al., 1995; Hoke et al., 2014).
The Qamdo Basin has therefore had a complex structural history since the Palaeozoic. At present the basin is bounded by the Lancangjiang Fault to the west/SW and the Zixia-Deqing Fault to the east/NE (Figure 2). The surface geology of the basin is characterized by widespread Upper Triassic to Cretaceous sedimentary and volcanogenic strata with local exposures of Palaeozoic to Lower Triassic sedimentary and metasedimentary rocks (Figure 2).
FIGURE 2. Geological map of the Qamdo Basin showing the location of the measured sections (modified form Tibet BGMR [Tibet Bureau of Geology and Mineral Resources], 2007).
The sedimentary succession is over 12,000 m thick and the local stratigraphic nomenclature is summarised in Figure 3 according to geological report (Tibet BGMR [Tibet Bureau of Geology and Mineral Resources], 2007). The cover succession above Precambrian basement begins with Ordovician to Permian units dominated by marine carbonates with deltaic sandstones, mudstones and coal seams. The Upper Permian Tuoba Formation includes organic-rich shales, coals and sandstones, as well as minor bioclastic limestones at the top of the unit.
FIGURE 3. Stratigraphic column and regional stratigraphic nomenclature for the Qamdo Basin (based on Tibet BGMR [Tibet Bureau of Geology and Mineral Resources], 2007).
Above a stratigraphic hiatus, a thick Upper Triassic to Cretaceous section occurs throughout the basin (Figure 3). The lower Upper Triassic Jiapila Formation includes coarse-grained alluvial, fluvial, lacustrine (evaporite), and marine (shale) deposits. Platform carbonates in the overlying middle Upper Triassic Bolila Formation are overlain by the Upper Triassic Adula and Duogaila Formations which comprise organic-rich shales, sandstones and coals deposited in a marginal marine to deltaic setting. A prominent change in colour marks the boundary between the Duogala Formation and the overlying Lower Jurassic Wangbu Formation which is composed of red-coloured sandstones. Jurassic-Cretaceous deposits are exposed in the SW of the basin between the Qamdo and Mangkang (Figure 1B) and are mainly composed of fluvial-lacustrine siliciclastics; the Middle Jurassic Dongdaqiao Formation is composed of transgressive black shales (Figure 3).
Materials and Methods
Materials
This study focuses on organic-rich shale strata in four formations in the Qamdo Basin and aims to evaluate their hydrocarbon potential. Stratigraphic sections were chosen on the basis of stratigraphic data, accessibility via roads and well-exposed conditions. Five stratigraphic sections (TB, BLL, ADL, DGL-E and DGL-W: Figure 2) were measured at outcrops alone the established roads.
At the TB section, about 489 m of the upper part of the Upper Permian Tuoba Formation is exposed, which is composed here of organic-rich shales, fine quartzose sandstones and bioclastic limestones (Figures 4, 5A). Palaeofusulina was found in the limestones, indicating that the formation is of Changhsingian (latest Permian) age (Sheng and Wang, 1981). The cumulative thickness of dark shale on the section is over120m, which is the potential source rock of this group. Eight source rock samples were collected within a 45 m thick organic-rich shale interval in the lowermost part of the measured section (Figure 3).
FIGURE 4. Stratigraphic columns for the measured sections in the Qamdo Basin showing the locations of the studied samples. Abbreviations: P3t, Upper Permian Tuoba Formation; T1x, Lower Triassic Xiayacun Formation; T3j, Upper Triassic Jiapila Formation; T3b, Upper Triassic Bolila Formation; T3a, Upper Triassic Adula Formation; T3d, Upper Triassic Duogaila Formation.
FIGURE 5. Outcrop photographs showing: (A) brown sandstones, black shales and bioclastic limestones in the upper part of the Tuoba Formation; inset shows a fusulinid found in the limestone interval. (B) Dark grey mudstones of the Adula Formation; a pen (15 cm) for scale. (C) Black mudstones and sandstones of the Duogaila Formation outcropping at the DGL-W section. (D) Coal seam in the upper part of the DGL-W section; a hammer (30 cm) for scale.
At the BLL outcrop section, the Upper Triassic Bolila Formation is > 480 m thick and mainly consists of limestones, dolomites and bioclastic limestones. Six dark limestone samples were collected for further analysis from the upper part of the formation (Figure 4). The carbonates consisted of fine-grained micrite and coarse sparry calcite in the pore spaces between grains and in larger cavity structures.
The ADL section spans the entire Upper Triassic Adula Formation with a thickness of approximately 635 m and the cumulative thickness of black shale over 290 m (Figures 4, 5B). The stratigraphically overlying DGL-W section (Figures 4, 5C) is dominated by Upper Truiassic Duogala Formation sandstones and shales with thin coal intervals, suggesting that facies pass from prodelta to delta-plain deposits corresponding to a drop of sea level. A total of 14 samples were collection from these two sections. Another outcrop section (Figure 5D) of the Duogala Formation was measured to the SE (the DGL-E section) where eight samples were collected.
Methods
For laboratory investigations, the samples were cleaned and weathered surfaces were removed. They were ground to analytical grain sizes (approximately 100 mg and 120 μm) and dried prior to further treatment. After the removal of carbonates using hydrochloric acid (HCl), a Leco CS-200 carbon–sulphur elemental analyzer was used to determine the total organic carbon (TOC) and total sulphur (TS) contents. The samples were also analysed by a Rock–Eval II instrument following the guidelines of Peters (1986).
A total of 29 samples were selected for further analysis as they contained abundant organic matter. The crushed samples were extracted with chloroform in a Soxhlet apparatus for 72 h. The extracted organic matter was further separated by a silica gel alumina column chromatography into saturated hydrocarbons, aromatic hydrocarbons and NSO (nitrogen, sulfur, and oxygen bearing compounds) compounds (Petersen et al., 2005). The saturated hydrocarbon fractions in the extracts were analysed by gas chromatography using an Agilent 6890N (GC) instrument with an injector temperature of 310°C. The GC was equipped with a 30 m × 0.20 mm internal diameter fused silica column (0.2 μm film) using helium as the carrier gas. The oven was gradually heated from 70 to 300°C at a rate of 8°C/min and followed by an isothermal period of 20 min.
To prepare kerogen material, carbonates were first removed using HCl. Then samples were washed several times with distilled water and treated with hydrofluoric acid (HF) for 12 h to remove silicates; this step was repeated until pure kerogens were isolated (c.f. Guthrie and Pratt, 1994; Ma et al., 2015). Strew-mounted kerogen slides were then prepared and used for further identification. A visual estimation of the relative abundance of macerals was conducted using an Axioskop2 plus microscope and a Swift point counter. To determine the relative abundance of macerals, at least 300 components were counted (Petersen et al., 2005). The vitrinite reflectance (% Ro) was determined using a MPM-80 microphotometer.
Elemental analyses were performed on a FLASH EA-1112 Series elemental analyzer according to National Standard of P.R. China (GB/T 19,143–2003).
Experimental work was performed at the Organic Geochemistry Laboratory, Institute of Exploration and Development, Huabei Oilfield Branch Company of the China National Petroleum Corporation (CNPC).
Results
Total Organic Carbon and Rock-Eval
TOC, TS and Rock-eval data of the outcrop samples from the measured sections are presented in Table 1. The TOC content of the eight Tuoba Formation samples from the TB section varies between 1.66 wt% and 3.01 wt%, with an average of 2.33 wt%. The S1 and S2 values are in the range of 0.–0.22 mg HC/g rock and 0.29–4.29 mg HC/g rock, respectively. Low TOCs (<0.30 wt%) were recorded in the Bolila Formation limestone samples from the BLL section, and the Adula Formation samples (ADL section) also have relatively low TOC (0.43–0.75% wt%). The samples of the Duogaila Formation from the DGL-W section have TOC contents ranging from 0.48 to 3.47 wt%, with the exception of the coaly samples DGL-W-S6 (TOC = 25.60 wt%). In the DGL-E section, the TOC contents of the Duogaila Formation samples are 0.47–1.04 wt% (average: 0.70 wt%).
TABLE 1. The results of TOC, TS, Roc-eval data, vitrinite reflectance (%Ro) and maceral compositon (vol%) of the kerogen.
The average S1, S2, potential yield (PY) values are 0.12, 0.32 and 0.44 mgHC/g rock for samples from the Tuoba Formation, 0.04, 0.11 and 0.15 mgHC/g rock for samples from the Adula Formation, and 0.06, 0.33, and 0.39 mgHC/g rock for samples from the Duogaila Formation, respectively (Table 1). The Tmax values fall within the range of 424–538°C and an average of 492°C.
Maceral Composition and Vitrinite Reflectance
The maceral composition (vol%) and vitrinite reflectance (Ro) values for selected samples from the Tuoba, Adula and Duogaila Formations are shown in Table 1. About 47–53 vol% of the total organic matter (OM) in the Tuoba Formation samples from the TB section is composed of amorphous organic matter (AOM). Vitrinite and inertinite account for about 20–38 vol% and 14–30 vol% of the kerogen assemblages, respectively (Figure 6A).
FIGURE 6. Photomicrographs (intransmitted light) of macerals in samples from the Tuoba and Duogaila Formations (AMO: amorphous organic matter) (A) Photomicrograph showing dominant AMO together with minor inertinite (sample No. TB-S2: Tuoba Formation); (B) Photomicrograph showing dominant AMO relative to inertinite and vitrinite (sample No. DGL-E-S7: Duogaila Formation). (C) Photomicrograph showing abundant AMO compared to inertinite and vitrinite (sample No. DGL-E-S9: Duogaila Formation). (D) Photomicrograph showing mostly inertinite (coal sample from DGL-W section: Duogaila Formation).
In Adula Formation samples from the ADL section, AOM dominates the maceral composition with proportions of more than 65 vol% of total OM. Inertinite group macerals accounts for 28%-31 vol% of the kerogen, and vitrinite up to 4 vol%.
In the DGL-E section samples, AOM is present as 40–64 vol%, whereas vitrinite and inertinite range from 15 to 35 vol% and 17 to 30 vol%, respectively (Figures 6B,C).
Within the eight Duogaila Formation samples from the DGL-W location, the samples from lower part of the section are dominated by AOM (65–68 vol%), followed by 28–32 vol% inertinite and 0–5 vol% vitrinite. Samples DGL-W-S5 and DGL-W-S6 have a different maceral composition which is dominated by inertinite and vitrinite. Coal seam occurs in the upper part of the DGL-W section and the photomicrograph showing an inertinite dominated composition (Figure 6D).
Vitrinite reflectance (Ro) values for samples from the four measured sections are listed in Table 1, including the number of points measured for each sample. All of the samples have Ro values > 1.3%, and some have Ro > 2.0%.
Elemental Analysis and Gas Chromatography
Elemental analysis provides a measure of the bulk chemical properties of isolated kerogen (Katz, 1988; Wang et al., 2011b) and data are summarized in Table 2. In general proportions of major elements are similar in all samples. Atomic O/C ratios and H/C ratios range from 0.05 to 0.16 and 0.48 to 1.38, respectively (Table 2).
TABLE 2. Elemental analysis results and molecular geochemical data.
Gas chromatograms of saturated hydrocarbon fractions in extracts of the samples are shown in Figure 7, and calculated parameters are given in Table 2. The chromatograms display a wide range of n-alkanes and isoprenoids between n-C15 and n-C35. The n-alkane distribution shows a bimodal pattern with a predominance of high molecular weight compounds (n-C23 -- n-C35); most of the samples have a peak at n-C25 or n-C33. In addition, all samples show odd-over-even predominance with a moderate carbon preference index (1.09 < CPI <1.72). These results indicate a high input of terrigenous organic matter.
FIGURE 7. Gas chromatograms of the saturated fractions for extracts from four samples (sample No. TB-S6, ADL-S1, DGL-W-S5, DGL-E-S6) showing the distribution of the n-alkanes and isoprenoids.
Discussion
Kerogen Type and Maturity
The maceral composition can be interpreted to indicate the origin and type of kerogen. Previous studies (e.g., Hutton et al., 1994; Petersen et al., 2005; Bechtel et al., 2014; Ma et al., 2015) have suggested that alginate, liptinite, and inertinite and vitrinite can be correlated to Types I, II and III kerogens, respectively. For most of the samples, AOM derived from lipid-rich precursors accounts for the largest proportion (nearly 50 vol%) of OM relative to vitrinite and inertinite macerals, suggesting that samples from all of the measured sections contain mostly Type II kerogen with smaller proportions of Type III kerogen. A cross-plot (Figure 8) shows that the organic matter in the samples is mainly Type II with the exceptions of two Duogaila Formation samples from the DGL-W section which contain Type III OM. The results are consistent with the relative proportions of the maceral groups.
FIGURE 8. Cross-plot of H/C versus O/C ratios for the analysed samples.
Vitrinite reflectance (Ro) is the most reliable parameter for measuring the thermal maturity of sedimentary organic matter (Tissot and Welte, 1978; Grassmann et al., 2005; Opera et al., 2013). In general, Ro values of 1.3 and 2.0% are accepted as the threshold values for highly mature and over-mature Type II kerogen (Killops and Killops, 2005). Therefore, the thermal maturity of the measured samples is high-to overmature (i.e., wet gas to dry gas zone). The results are consistent with the high Tmax value.
Hydrocarbon Potential
Overall, the samples collected from Tuoba Formation exhibit the best hydrocarbon potential of the formations investigated with TOC >1.0 wt%. By contrast, the samples from the BLL section have TOC <0.3 wt%. Samples from the Adula and Duogala Formations have poor to medium organic contents, with the exception of a few coaly samples of the latter formation from the DGL-W section. PY (PY = S1 + S2) represents the potential yield and a quantity of the transformation potential of the total organic matter (Demaison and Huizinga, 1991; Tissot and Welte, 1978). According to evaluation criterion of the hydrocarbon source rock established by the China National Petroleum Corporation (Wang et al., 2009; Ding et al., 2013), PI value over 0.25 is classified as good source rock, and 0.15 to 0.25 for medium source rock.
The proneness towards oil or gas generation is indicated by the kerogen type and the maceral composition. Fluorescent macerals of the liptinite group are here considered as the oil-prone fraction, and the sum of inertinite and vitrinite group macerals are the gas-prone fraction (Killops and Killops, 2005; Furmann et al., 2015; Hakimi and Ahmed, 2016). The analysed samples contain mainly Type II OM with nearly equal oil- and gas-prone fractions. However, all the samples are highly to over-mature in terms of Ro, as discussed above. The maturity stage of studied samples (high to over mature) is high enough to generate and expel large amount of hydrocarbons and cracked into dry gas (Killops and Killops, 2005; Liang et al., 2017), this reveals that the measured strata were underwent deep burial after deposition. Therefore, the combined evidence suggests that gas generation can be expected in the Tuoba, Adula and Duogaila Formations.
Controls on Source Rocks Deposition
Total sulphur is considered to be a good measure of the degree of marine influence (Sykes, 2004; Sykes et al., 2014; Sarki Yandoka et al., 2015). In samples from the Tuoba Formation, TS contents varied between 0.60 and 1.12 wt%; values for samples from the ADL, DGL-W and DGL-E sections (Adula and Duogaila Formations) were much lower (0.10–0.40 wt%). Thus, compared to the Tuoba Formation, the samples from the Adula and Duogaila Formations are interpreted to have been deposited under more freshwater-influenced conditions which consistent with delta facies.
Pristane (Pr) and phytane (Ph) occur in significant amounts in all the studied samples (Figure 7). The most abundant source of pristane and phytane is the phytyl side-chain of chlorophyll a in phototrophic organisms, and bacterio chlorophyll a and b in purple sulphur bacteria (Powell and McKirdy, 1973). The phytyl side-chain is prone to be converted into phytane in reducing or anoxic conditions, whereas oxic conditions favour pristane (Peters et al., 2005). Therefore, the value of the Pr/Ph ratio is considered to indicate the redox conditions during sedimentation and diagenesis (Didyk, 1978; Chandra et al., 1994; Escobar et al., 2011). High Pr/Ph (>3.0) indicates oxic conditions often associated with terrigenous organic matter input, while low values (<0.8) typify anoxic, commonly hypersaline or carbonate environments (Peters et al., 2005; El Diasty and Moldowan, 2012). Phytane occurs in high relative concentrations in the analyzed samples, resulting in Pr/Ph ratios in the range of 0.44–0.85 (Table 2), indicating a suboxic to relatively anoxic depositional setting. Furthermore, Pr/n-C17 and Ph/n-C18 ratios are in the range of 0.64–0.94 and 0.58–2.54, respectively. A cross-plot of Pr/n-C17 versus Ph/n-C18 (Figure 9) also suggests that marine-derived organic matter was an important input to the source rock and was preserved under a reducing environment.
FIGURE 9. Cross-plot of phytane/n-C18 alkane (Ph/n-C18) versus pristane/n-C17 alkane (Pr/n-C17) for analysed samples howing depositional conditions and source of organic matter (after Hunt, 1995; Riboulleau et al., 2007; El Diasty and Moldowan, 2012).
The Qamdo Basin experienced frequent sea-level fluctuations, especially in the Late Triassic, and four transgressive-regressive cycles have been recognized according to the sedimentary record (Du et al., 1997; Du et al., 1998). Based on sequence stratigraphy analyses for the outcrops in the Qamdo area, Peng et al. (2005) constructed a curve of sea level change for the Late Triassic (Figure 10). Compared with the eustatic cycle of Haq et al. (1988), the curve in the Qamdo area contains more low-amplitude signals relating to short-term sea-level change. Figure 10 shows that the source rock intervals in the Adula and Duogala Formations were deposited during transgressive episodes. Instead, peat deposits (coal beds of Duogaila Formation) and coarse-grained clastic deposits may be preserved in response to relative sea-level fluctuations (Diessel, 1992; Lv and Chen, 2014).
FIGURE 10. Upper Triassic lithology of the Qamdo Basin and sea level curve showing that two source rock intervals correspond to transgressive episodes. Sea-level curve based on 1 Peng et al., 2005 and 2 Haq et al., 1988.
Various reasons have been proposed to account for the positive association between transgressions and the deposition of organic-rich facies (Klemme and Ulmishek, 1991; Arthur and Sageman, 1994; Arthur, 2005). including: 1) transgressive periods may enhance seasonal or longer-term water-column stratification and development of anoxia; 2) rising sea levels may promotes near-shore trapping of terrigenous clastic material, creating condensed intervals which are characterized by enrichment in organic carbon (Arthur, 2005); and 3) land-derived nutrients give rise to surface plankton booms, resulting in high biological productivity (Hao et al., 2011; Li et al., 2016).
The transgressive episodes in the Jiapila and Bilila Formations have quite different sedimentary characteristics. During Jiapila Formation deposition, intense tectonism resulted in widespread conglomerates which are have little source rock potential (Du et al., 1997; Du et al., 1998). In addition, evidence for an arid palaeoclimate in the Qamdo basin area is provided by evaporitic lacustrine deposits (Du et al., 1997; Du et al., 1998). By contrast, the Bolila Formation is characterised by the development thick platform carbonates during a period of tectonic and volcanic quiescence, during which terrigenous input was greatly reduced (Peng et al., 2005). Consequently, the accumulation of organic matter just depended on the productivity of the ocean with the insufficient nutrients.
Clearly, the development of source rock is governed by a variety of factors, such as a warm and moist climate, profitable regional tectonics and eustasy. Among them, sea level fluctuations have important implications for organic productivity of the oceans and sediment distribution patterns for the Qamdo Basin. The rise of sea level usually results in a reduced environment, and indicators of redox (such as Pr/Ph ratio) in accord with these samples were deposited in an anoxic and reducing environment.
Conclusion
Sedimentary characteristic and organic properties of Tuoba, Bolila, Adula and Duogala Formations were analysed to investigate the formations’ geochemical characteristics, hydrocarbon potential, and the controls on organic matter input. The following major conclusions were reached:
1) Outcrop samples of the Tuoba Formation has relatively high TOC contents averaging 2.33%, while the Adula and Duogala Formations have poor to medium organic richness with exception of a few coaly samples from the DGL-W section. However, the Bolila Formation shows very low TOC contents lower than 0.3%, indicating that the Bolila carbonates have barely hydrocarbon generation potential.
2) Elemental analysis and maceral composition indicate that the organic matter in shale samples from the Tuoba, Adula and Duogala Formations are characterized by Type II kerogen with a mixed sources of organic matter input.
3) All of the samples analysed have high vitrinite reflectance (Ro > 1.3%) and most of the samples show a high Tmax (424–538°C). Maturity estimates based on vitrinite reflectance and Rock-eval parameters indicate that all of the samples analysed are thermally highly-to overmature.
4) According to the organic matter abundance and kerogen type evaluation for the samples of the Qamdo Basin, it seems that the Late Permian Tuoba Formation is considered to be the best candidate of effective source rock. The Late Triassic Source Rocks (Adula and Duogaila Formations) shows considerable hydrocarbon potential as well. Combined with results of maturity indicators, the analysed formations have reached thermogenic dry gas window and gas generation can be expected from the Late Permian Tuoba Formation, the Late Triassic Adula and the Late Triassic Duogaila Formations.
5) Enrichment of organic carbon in the analysed formations was probably controlled by eustatic sea level changes, regional tectonics and climatic variations. Organic-rich facies accumulated during major transgressive episodes.
Data Availability Statement
The original contributions presented in the study are included in the article/Supplementary Material, further inquiries can be directed to the corresponding authors.
Author Contributions
ZQ wrote the manuscript, organized the database and performed the statistical analysis. YL and CW contributed to conception and design of the study. All authors contributed to manuscript revision, read, and approved the submitted version.
Funding
This research is financially supported by the Strategic Priority Research Program of Chinese Academy of Sciences (Grant Nos. XDA20070303) and the Science and Technology Department of Qinghai Province- Qinghai Natural Science Foundation (Youth Project: 2019-ZJ-964Q).
Conflict of Interest
The authors declare that the research was conducted in the absence of any commercial or financial relationships that could be construed as a potential conflict of interest.
Publisher’s Note
All claims expressed in this article are solely those of the authors and do not necessarily represent those of their affiliated organizations, or those of the publisher, the editors and the reviewers. Any product that may be evaluated in this article, or claim that may be made by its manufacturer, is not guaranteed or endorsed by the publisher.
Acknowledgments
We thank Xiaohan Li, Sheng Wei, Bo Wang, Jinghua Dai, Haiyang He, Yajuan Wang and Yaoyao Duan for the fieldwork, and Shunping Ma for assistance in the laboratory.
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Keywords: Qamdo Basin, eastern Tibet, organic geochemistry, source rock, shale
Citation: Qi Z, Li Y and Wang C (2021) Hydrocarbon Potential of the Late Permian and the Late Triassic Source Rocks from the Qamdo (Changdu) Basin, Eastern Tibet and Its Linkage with the Sea Level Change. Front. Earth Sci. 9:778025. doi: 10.3389/feart.2021.778025
Received: 16 September 2021; Accepted: 22 November 2021;
Published: 07 December 2021.
Edited by:
Ziqi Feng, China University of Petroleum, Huadong (UPC), ChinaReviewed by:
Pengfei Ma, Tongji University, ChinaTian Dong, China University of Geosciences Wuhan, China
Copyright © 2021 Qi, Li and Wang. This is an open-access article distributed under the terms of the Creative Commons Attribution License (CC BY). The use, distribution or reproduction in other forums is permitted, provided the original author(s) and the copyright owner(s) are credited and that the original publication in this journal is cited, in accordance with accepted academic practice. No use, distribution or reproduction is permitted which does not comply with these terms.
*Correspondence: Zhaolin Qi, emhscWlfcWh1QDE2My5jb20=; Yalin Li, bGl5YWxpbkBjdWdiLmVkdS5jbg==