Dolomitization, Recrystallization, and Cementation in Carbonate Sedimentary Rocks

A special issue of Minerals (ISSN 2075-163X). This special issue belongs to the section "Mineral Geochemistry and Geochronology".

Deadline for manuscript submissions: 20 June 2024 | Viewed by 1327

Special Issue Editors


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Guest Editor
PetroChina Hangzhou Research Institute of Geology, Hangzhou 310023, China
Interests: carbonate sequence stratigraphy and deposition; dolomitization; karstification; reservoir characterization
Key Laboratory of Petroleum Resources Research, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing 100029, China
Interests: diagenesis; petroleum geology; carbonate and evaporite
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Guest Editor
Shandong Provincial Key Laboratory of Deep Oil & Gas, China University of Petroleum (East China), Qingdao 266580, China
Interests: diagenesis; dolomitization; porosity evolution; TSR

Special Issue Information

Dear Colleagues,

Dolomitization, recrystallization and cementation are the most commonly occurring types of diagenetic modification for carbonate rock. They can develop in a variety of situations, conditions, and stages, impacting the pore evolution of carbonate rock reservoirs.

In recent years, remarkable advances have been made in experimental analysis techniques, such as laser U-Pb dating, clumped isotopes, and surface scanning of rare earth elements. These developments have offered an opportunity to understand the stages, diagenetic environments, and related geofluid properties of dolomitization, recrystallization, and cementation.

Different modes of diagenesis, taking place under different conditions, tend to make different contributions to the formation and maintenance of pores in carbonate rock reservoirs during the burial stage, especially during dolomitization. Understanding their contributions to the evolution of reservoir pores can help to promote efforts to predict the distribution and heterogeneity of carbonate reservoirs.

This Special Issue aims to contribute to disseminating advances in the understanding of dolomitization, recrystallization, and cementation in order to decipher the evolution of the carbonate rock and related reservoir.

Dr. Zhanfeng Qiao
Dr. Lei Jiang
Dr. Guangwei Wang
Guest Editors

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Keywords

  • dolomitization
  • recrystallization
  • cementation
  • carbonate reservoir
  • advances in geochronology

Published Papers (1 paper)

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Research

18 pages, 14029 KiB  
Article
Distribution and Genesis of the Deep Buried, Fractured and Vuggy Dolostone Reservoir in the Lower Ordovician Succession, North Tarim Basin, Northwestern China
by Lijun Gao, Jie Li, Guorong Li, Liyun Fu and Yongli Liu
Minerals 2024, 14(1), 58; https://doi.org/10.3390/min14010058 - 02 Jan 2024
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Abstract
Recently, a series of prolific fracture-vug reservoirs have been discovered in the lower Ordovician dolostone successions of the northern Tarim Basin. However, the genesis of these reservoirs remains unclear. In this study, observations on drilling cores and thin sections identify the pore space [...] Read more.
Recently, a series of prolific fracture-vug reservoirs have been discovered in the lower Ordovician dolostone successions of the northern Tarim Basin. However, the genesis of these reservoirs remains unclear. In this study, observations on drilling cores and thin sections identify the pore space characterized by dissolved fractures, fissures, and vugs. Petrology, cathodoluminescence, and homogenization temperatures of fluid inclusions aid in establishing the diagenetic paragenetic sequence. Dissolving enlargement occurred after chemical compaction of overlying limestone and before the Permian volcanic activity. Breccia pores containing unique fillings of terrestrial materials (quartz sand and allogenic kaolinite) and calcite cements with negative δ18OPDB values (−18.4‰) along with 87Sr/86Sr ratios (up to 0.71026) indicate that the dissolving fluid originated from meteoric freshwater at the surface. The δ18OSMOW values of the calcite precipitating fluid (−2.1‰ to −8.7‰) further suggest freshwater as the source of the dissolving fluid, buffered by the Ordovician wall rocks or formation water. As the distance from the unconformity surface increases, both the homogenization temperature and δ18OPDB values of the breccia pore-filling calcite in the southern study area gradually elevate and deplete, respectively, indicating a rise in temperature during the infiltration of meteoric freshwater with increasing subsurface temperatures. The abnormal reflection bodies identified as reservoirs in seismic profiles along deep-seated strike-slip faults delineate these faults as the channel for the infiltration of meteoric freshwater. The penetrating strata of these faults and the high 87Sr/86Sr values of breccia pore-filling calcite suggest that karstification occurred during the Devonian period. Accordingly, we establish a deep karst model in which the Devonian meteoric freshwater penetrated along the strike-slip faults and dissolved the Ordovician dolostones, resulting in the development of deep buried karstic fault reservoirs in the southern region of the northern Tarim Basin. Full article
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