2019年希腊和阿尔巴尼亚侏罗系Posidonia页岩连续油气资源评价

Q4 Environmental Science
C. J. Schenk, T. Mercier, M. Tennyson, T. Finn, Cheryl A. Woodall, M. Brownfield, K. Marra, Heidi M. Leathers-Miller, P. Le, R. M. Drake
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引用次数: 0

摘要

美国地质调查局(USGS)定量评估了希腊西部和阿尔巴尼亚南部的侏罗系Posidonia页岩全油气系统(TPS)中未被发现的、技术上可开采的连续油气资源潜力(图1)。从晚三叠世到早侏罗世,希腊西部和阿尔巴尼亚南部的这一地区是在阿普利安板块上及其周围发育的一个区域广泛的碳酸盐岩台地的一部分(Karakitsios, 1995;2013)。在此期间,沿被动边缘沉积了长达1000米的潘托克拉托石灰岩台地碳酸盐。侏罗纪的伸展和裂谷作用与新特提斯洋的张开有关,导致沿阿普利亚板块边缘形成了许多地堑和半地堑(Karakitsios, 1995;Karakitsios and Rigakis, 2007)。深地堑和半地堑底部水体缺氧,形成了侏罗系Posidonia页岩富有机质烃源岩的沉积和保存。这些伸展构造持续了整个侏罗纪,最终被区域性广泛的白垩纪后滑脱期维格拉灰岩所掩埋。从白垩纪到古近纪,阿普利安板块相对来说没有变形,并被可能数百米的碳酸盐沉积物所掩埋。始新世起至中新世止,阿普利亚板块与欧亚板块碰撞,形成了迪纳里德和希腊里德褶皱和冲断带,造成了中生代岩石的挤压变形。与普利亚碰撞有关的是造山碎屑楔的进积,厚度可达数公里(Gonzalez-Bonorino, 1996;Karakitsios, 2013)。这些造山碎屑的新近纪埋藏导致热成熟进入侏罗纪Posidonia烃源岩的油气生窗(Rigakis and Karakitsios, 1998;Karakitsios and Rigakis, 2007)。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Assessment of continuous oil and gas resources in Jurassic Posidonia Shales of Greece and Albania, 2019
The U.S. Geological Survey (USGS) quantitatively assessed the potential for undiscovered, technically recoverable continuous oil and gas resources in the Jurassic Posidonia Shale Total Petroleum System (TPS) of western Greece and southern Albania (fig. 1). From the Late Triassic to Early Jurassic, this area of western Greece and southern Albania was part of a regionally extensive carbonate platform that developed on and around the Apulian Plate (Karakitsios, 1995; 2013). Deposited along the passive margin during this time were as much as 1,000 meters of platform carbonates of the Pantokrator Limestone. Jurassic extension and rifting associated with the opening of the neo-Tethys Ocean led to the formation of numerous grabens and half-grabens along the margin of the Apulian Plate (Karakitsios, 1995; Karakitsios and Rigakis, 2007). The bottom waters of the deeper grabens and half-grabens were anoxic, resulting in the deposition and preservation of organic-rich petroleum source rocks of the Jurassic Posidonia Shale. These extensional structures persisted through the Jurassic and eventually were buried by the regionally extensive, postrift Cretaceous Vigla Limestone. From the Cretaceous through the Paleogene, the Apulian Plate was relatively undeformed and buried by perhaps hundreds of meters of carbonate deposits. Beginning in the Eocene and ending in the Miocene, the Apulian Plate collided with the Eurasian Plate, forming the Dinaride and Hellenide fold and thrust belts, resulting in compressional deformation of Mesozoic rocks. Associated with the collision of Apulia was the progradation of orogenic clastic wedges up to several kilometers thick (Gonzalez-Bonorino, 1996; Karakitsios, 2013). Neogene burial by these orogenic clastics resulted in the thermal maturation into the oiland gas-generation windows of the Jurassic Posidonia source rocks (Rigakis and Karakitsios, 1998; Karakitsios and Rigakis, 2007).
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来源期刊
U.S. Geological Survey Fact Sheet
U.S. Geological Survey Fact Sheet Environmental Science-Water Science and Technology
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