Re-assessment of depositional conditions of Cretaceous deposits around the Amfilochia and Arta areas

N. Dimopoulos, E. Georgoulas, Savvas Peridis, G. Iliopoulos, Nikolina Bourli, P. Antoniou, A. Zelilidis
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Abstract

Sedimentological studies of the Cretaceous limestones in the central Ionian basin (Amfilochia, Arta as well as Kerasonas areas) indicate that these deposits are composed of calciturbidites interbedded with breccia-microbreccia deposits. In the Amfilochia new cross-section, with a NNW-SSE direction, the lower Cretaceous Vigla limestones and Vigla shales were outcropped for the first time. This section is directed parallel to the paleo Ionian basin axis and the fact of the lateral discontinuity of Vigla limestones and Vigla shales indicate that during the sedimentation of these two Formations there was a restriction along the paleo basin axis, probably due to synsedimentary transfer fault activity. Forty-two (42) samples from Vigla shales were analyzed for their content in CaCO 3 and TOC, showed that these sediments present poor to fair hydrocarbon potential. In the Arta new cross-section, with a NE-SW direction, the Upper Cretaceous Senonian deposits showed strong deformation that took place during the compressional regime that affected the Ionian basin after sedimentation. This deformation appears stronger in the western part being close to a major thrust, and thus it is possible that this deformation could be responsible for the high secondary porosity of Upper Cretaceous deposits. Microfacies analysis of these deposits showed in general that deep-sea depositional environments prevailed, nevertheless in a few cases indications for the presence of environments with a shallow character imply the existence of isolated carbonate platforms close to the studied sections. In the studied sections with an E-W direction, no lateral changes were observed in the depositional conditions within the same Formation introducing standard depositional conditions across the paleo basin.
Amfilochia和Arta地区白垩系沉积条件的再评价
对爱奥尼亚盆地中部(Amfilochia、Arta和Kerasonas地区)白垩系灰岩的沉积学研究表明,这些沉积是由角砾岩-微角砾岩互层组成的。在Amfilochia新剖面,NNW-SSE方向,首次出露下白垩统Vigla灰岩和Vigla页岩。该剖面平行于古伊奥尼亚盆地轴线,而维格拉灰岩和维格拉页岩的横向不连续表明,在这两个组的沉积过程中,可能由于同沉积转移断层的活动,沿古盆地轴线存在一个限制。对42个Vigla页岩样品的caco3和TOC含量进行了分析,结果表明,这些沉积物具有较差至一般的油气潜力。在阿尔塔新剖面上,上白垩统Senonian沉积表现出NE-SW方向的强烈变形,这种变形发生在沉积后影响伊奥尼亚盆地的挤压期。这种变形在靠近主逆冲的西部表现得更为强烈,因此这种变形可能是导致上白垩统矿床次生孔隙度高的原因。这些矿床的微相分析表明,总的来说,深海沉积环境占主导地位,但在少数情况下,浅层环境的存在表明,在研究剖面附近存在孤立的碳酸盐台地。在东西向的研究剖面中,同一组内的沉积条件未发生横向变化,导致整个古盆地的标准沉积条件。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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