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巴西桑托斯盆地下白垩统Barra Velha组微生物碳酸盐岩储层特征及主控因素
朱奕璇, 张忠民, 胡宗全, 鲍志东, 张淘
海相油气地质 ›› 2025, Vol. 30 ›› Issue (5) : 435-446.
PDF(61813 KB)
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巴西桑托斯盆地下白垩统Barra Velha组微生物碳酸盐岩储层特征及主控因素
Characteristics and main controlling factors of microbial carbonate reservoirs of the Lower Cretaceous Barra Velha Formation in the Santos Basin, Brazil
巴西桑托斯盆地下白垩统Barra Velha组微生物碳酸盐岩主要形成于高盐碱沉积环境,是近年深水领域油气勘探开发的热点。然而对于这种特殊环境及成因形成的微生物碳酸盐岩储层特征及其发育主控因素的研究相对薄弱。通过岩心、薄片、测井和物性测试等资料,系统研究了盆地微生物碳酸盐岩的岩相、储集空间类型和物性,明确了储层成岩序列以及孔隙演化特征,并探讨优质储层发育的主控因素与模式。研究表明:①桑托斯盆地下白垩统Barra Velha组微生物碳酸盐岩储层主要岩石类型包括叠层石灰岩、球粒微生物岩、层纹岩、砂屑灰岩、砾屑灰岩和角砾灰岩。纵向上可划分为2个三级层序,主要发育微生物礁、颗粒滩、微生物球粒滩、滩间等4种沉积微相。②储集空间主要为生物格架孔及生物格架溶孔、粒间孔及粒间溶孔、粒内溶孔、晶间孔以及溶蚀缝,孔隙度和渗透率整体呈正相关关系,以孔隙型储层为主。微生物礁和颗粒滩沉积微相的储层物性较好,微生物球粒滩和滩间沉积微相的储层物性相对较差。③明确了微生物碳酸盐岩储层成岩序列及孔隙演化。早成岩阶段,大气水溶蚀、白云石化对储层演化起到建设性作用;中—晚期热液作用下,断裂附近储层孔隙被硅质充填,对储层起到破坏性作用的同时也增加了储层的非均质性。④古气候、古水介质、层序及沉积微相类型是控制微生物碳酸盐岩优质储层发育和分布的主要因素;结合成岩演化,建立了微生物碳酸盐岩储层发育模式。
The microbial carbonates of the Lower Cretaceous Barra Velha Formation in the Santos Basin, Brazil, primarily formed in a high-salinity alkaline depositional environment, and have recently become a hotspot for hydrocarbon exploration and development in deep-water areas. However, research on the characteristics of microbial carbonate reservoirs formed in such unique environment is relatively limited and controlling factors of reservoir formation remains poorly understood. Based on integrated core samples, thin sections, well logs, and petrophysical test data, this study systematically investigates the lithofacies, reservoir space types, and physical properties of microbial carbonates in the basin. It clarifies the diagenetic sequence and pore evolution of the reservoirs and explores the main controlling factors and models for the development of high-quality reservoirs. The research results show that: (1) The main rock types of microbial carbonate reservoirs of the Lower Cretaceous Barra Velha Formation in the Santos Basin include stromatolite, spherulitite, laminite, rudstone, grainstone and breccia. The formation can be divided into two third-order sequences, primarily consisting of four microfacies types: microbial reef, grain shoal, microbial spherulitic shoal, and inter-shoal deposits. (2) The reservoir space is mainly composed of biological framework pore, framework dissolution pore, intergranular pore, intergranular dissolution pore, intragranular dissolution pore, intercrystalline pore, and dissolution fracture. Porosity and permeability generally exhibit a positive correlation, indicating the dominance of pore-type reservoirs. Statistics show that the microbial reef and grain shoal microfacies have better reservoir properties, while the microbial spherulitic shoal and inter-shoal microfacies show relatively poorer reservoir quality. (3) The diagenetic sequence and pore evolution of microbial carbonate reservoirs have been clarified. In the early diagenetic stage, meteoric water dissolution and dolomitization played constructive roles in reservoir evolution. In contrast, mid-to-late hydrothermal activity led to silica filling of reservoir pores particularly in areas adjacent to faults, which not only damaged the reservoir but also increased reservoir heterogeneity. (4) Paleoclimate, paleo-water condition, sequence stratigraphy, and sedimentary microfacies types are the main factors controlling the development and distribution of high-quality microbial carbonate reservoirs. Combined with diagenetic evolution, an evolution model of microbial carbonate reservoirs has been established in this study.
微生物碳酸盐岩 / 储层特征 / 成岩作用 / 储层发育模式 / 桑托斯盆地 / 巴西
microbial carbonates / reservoir characteristics / diagenesis / reservoir development model / Santos Basin / Brazil
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朱奕璇, 张忠民, 张德民. 巴西桑托斯盆地早白垩世微生物碳酸盐岩沉积环境与成因[J]. 岩石学报, 2022, 38(9): 2619-2633.
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This study aims to provide a better understanding of the genesis and diagenetic evolution of the rift pre-salt deposits of the Santos Basin, in the context of evolution of the lake system in which the sediments were deposited. The study of the syngenetic and early diagenetic constituents and their paragenetic relations allowed reconstruction of the evolution of lacustrine environmental conditions during the rift stage in the central area of the basin. A petrological study was performed on cores and sidewall samples of a well drilled through the pre-salt rift section in the Lower Cretaceous of the central Santos Basin, eastern Brazilian coast. The studied rocks consist of carbonate and non-carbonate intrabasinal components, with extrabasinal non-carbonate contribution. During Barremian early rift sedimentation, intense syngenetic precipitation of magnesian clay minerals under highly alkaline conditions deposited arenites constituted by stevensite ooids and peloids, as well as hybrid, resedimented deposits of the Piçarras Formation. Freshening of the lacustrine environment provided the conditions required for the proliferation of bivalves and sedimentation of the coquinas of the Itapema Formation. The massive structure of the deposits, poor sorting, chaotic to concave-up orientation of the bioclasts, and mixing of bivalves with stevensite particles indicate redeposition by gravity flows. The main diagenetic processes in rift stevensite and hybrid rocks are the cementation and replacement of grains by calcite, dolomite, and subordinately, silica and smectite. Siliciclastic-volcaniclastic mudrocks present intense replacement by dolomite. In the bivalve rudstones, the main diagenetic processes were dissolution of the shells and cementation of the intraparticle and interparticle pores by calcite and, subordinately, dolomite and silica.
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Since the discovery of giant Aptian pre-salt reservoirs in Brazilian margin basins, the study of lacustrine carbonates has drawn great attention from the scientific community. Comparatively, minor attention was given to the characterization and genesis of the Mg-silicates (e.g., stevensite, kerolite) which are commonly associated with these carbonates. A systematic petrological study was performed in the Aptian Barra Velha Formation (BVF) within distinct structural compartments of the giant Lula Field in the Santos Basin, in order to recognize the patterns of primary formation and diagenetic alteration of these Mg-silicates. Mg-silicates occur as peloids, ooids, intraclasts, and fine-grained laminated deposits, either mixed in variable proportions with other particles, such as carbonate bioclasts and volcanic rock fragments, or constituting specific intrabasinal deposits. In the BVF interval, clay peloids and laminated deposits are associated with spherulitic and fascicular calcite aggregates, as substrate and hosts for these precipitates. Ooids are interpreted as formed at the sediment–water interface by the nucleation of concentric envelopes on the surface of particles (heterogeneous nucleation), through repeated rolling under gentle wave and current action. Laminated deposits, interpreted as precipitated directly from the water column (homogeneous nucleation) in highly supersaturated and low-hydrodynamic-energy environments, constitute extensive deposits in the BVF. Peloids were probably formed in intermediate energy conditions. Some ooidal arenites show porosity from the dehydration and contraction, and/or the dissolution of ooids. In some rocks, these pores are filled with fibrous calcite, while the remaining Mg-silicates are replaced by dolomite, calcite, or silica. A similar diagenetic pattern occurs in the laminated deposits, where magnesite and dolomite fill shrinkage pores formed along their characteristic wavy laminae. Owing to their elevated solubility, most of the Mg-silicates were dissolved, or intensely replaced by calcite, dolomite, or silica. The detailed petrologic analysis indicates that the original volumes of Mg-silicates were substantially larger, and that their deposition was widespread in the basin, including on structurally high areas. The types and intensity of diagenetic alteration of the Mg-silicate deposits are distinct for each structural compartment, being more intense towards the highs and closer to the overlying evaporites, which imposed a strong influence on reservoir quality.
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康洪全, 吕杰, 程涛, 等. 巴西桑托斯盆地盐下湖相碳酸盐岩储层特征[J]. 海洋地质与第四纪地质, 2018, 38(4): 170-178.
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商志垒, 武静, 尚凡杰, 等. 巴西桑托斯盆地盐下碳酸盐岩油藏硅化作用成因及其对储层的影响[J]. 油气地质与采收率, 2020, 27(6): 20-29.
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贾怀存, 康洪全, 梁建设, 等. 桑托斯盆地湖相碳酸盐岩储层特征及控制因素[J]. 西南石油大学学报(自然科学版), 2021, 43(2): 1-9.
巴西桑托斯盆地盐下湖相碳酸盐岩领域油气资源十分丰富,是世界油气勘探的热点地区。利用桑托斯盆地41口井的岩芯、薄片等资料,明确了盐下湖相碳酸盐岩包括以微生物作用为主的微生物礁叠层石灰岩和以机械成因为主的生屑滩贝壳灰岩两种类型。盐下湖相碳酸盐岩储层整体上属于孔隙型灰岩储层,孔隙度整体上属于中等-好,渗透率中等。储层孔隙类型以原生孔隙为主,并受后期溶蚀改造。根据碳氧同位素地球化学资料、介形虫古生物等资料分析,总结出桑托斯盆地湖相碳酸盐岩储层发育主要受湖水古盐度、古构造格局和沉积相带3种因素控制。其中,湖水古盐度控制储层成因类型,古构造格局控制储层宏观分布,沉积相带控制储层物性特征。预测了桑托斯盆地东部隆起带和中央拗陷带的低凸起是湖相碳酸盐岩储层发育有利区带,对该地区油气勘探具有实践指导意义。
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Deposits produced by microbial growth and metabolism have been important components of carbonate sediments since the Archaean. Geologically best known in seas and lakes, microbial carbonates are also important at the present day in fluviatile, spring, cave and soil environments. The principal organisms involved are bacteria, particularly cyanobacteria, small algae and fungi, that participate in the growth of microbial biofilms and mats. Grain‐trapping is locally important, but the key process is precipitation, producing reefal accumulations of calcified microbes and enhancing mat accretion and preservation. Various metabolic processes, such as photosynthetic uptake of CO2and/or HCO3–by cyanobacteria, and ammonification, denitrification and sulphate reduction by other bacteria, can increase alkalinity and stimulate carbonate precipitation. Extracellular polymeric substances, widely produced by microbes for attachment and protection, are important in providing nucleation sites and facilitating sediment trapping.
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Transgressive–regressive (T–R) sequence analysis has been applied to the Jurassic succession of the Sverdrup Basin with sequence boundaries drawn at subaerial unconformities or the correlative transgressive surfaces. A hierarchal system of sequence order that reflects the different nature of the boundaries has been formulated on the basis of boundary characteristics. Second- through fifth-order sequences have been recognized in the Jurassic succession, which itself is part of a first-order sequence of mid-Permian – Early Cretaceous age.The Jurassic strata occur within four second-order sequences. The boundaries of these sequences are characterized by widespread subaerial unconformities across which major changes in depositional and subsidence regimes occur. These boundaries are earliest Rhaetian, earliest Pliensbachian, earliest Bajocian, earliest Oxfordian, and Hauterivian in age.Each second-order sequence is divisible into a number of third-order sequences bounded mainly by basin-wide transgressive surfaces with subaerial unconformities present on the basin margins. The ages of the 10 Jurassic third-order sequences are Rhaetian – Hettangian, Sinemurian, Pliensbachian – Toarcian, late Toarcian – Aalenian, Bajocian, Bathonian, Callovian, Oxfordian – early Kimmeridgian, late Kimmeridgian – early Tithonian, and late Tithonian. The third-order sequences commonly contain three to six fourth-order sequences. These sequences are bound entirely by transgressive surfaces that can be correlated only over a portion of the basin.A good correlation between the second- and third-order transgressive events of the Sverdrup Basin and proposed global events is observed. This worldwide occurrence suggests that the events in part reflect eustatic sea-level changes. The characteristics of the second- and third-order boundaries also indicate that each had a tectonic influence that resulted in a rapid relative sea-level fall (uplift) followed by a rapid rise (subsidence). Given the apparent combination of tectonic and eustatic influence on the generation of the second- and third-order sequence boundaries, they are interpreted to reflect significant plate-tectonic reorganizations that affected the intraplate stress regimes of the oceanic (eustatic) and continental (tectonic) portions of each lithospheric plate.
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