斯里兰卡近海Mannar盆地古新世洪水玄武岩层序与层间沉积序列的岩石成因(印度洋北赤道缘)

S. Karunarathne , P.L. Dharmapriya , W.M.H.M. Wijesinghe , M. Hellers , A.U. Wijenayake , H.M.T.G.A. Pitawala , E.K.C.W. Kularathna
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引用次数: 0

摘要

马纳尔盆地是冈瓦纳断裂期间形成的裂谷盆地,由多个旋回沉积组成。油气勘探发现了分布在整个盆地沉积层序中的火成岩层序。这些层序具有地球化学特征,是60 ~ 62 Ma一系列喷发期间形成的洪水玄武岩的典型特征。以往的研究主要集中在含油气系统、构造地层学、岩石地层学和古环境背景等方面,对该泛流玄武岩层序的岩石成因知之甚少。本文研究了洪水玄武岩层序的岩石成因,重点研究了结晶温度、源岩浆特征和岩浆分馏结晶性质。此外,它还研究了层间沉积层的矿物学特征,包括粘土矿物,以解释它们的起源——这是一个以前没有深入研究过的领域。从Barracuda石油勘探井4000-4200米深度的未洗钻屑中制备了岩石薄片。对这些样品进行了详细的岩石学研究,探讨了岩石成因。此外,利用电子探针微量分析(EPMA)测定了玄武岩和层间沉积岩样品的矿物化学成分。玄武岩主要由斜长石(An62-82)和斜辉石(主要是辉石)组成,少量有正辉石(En54-67)和ulvöspinel。只有最下面的玄武岩层(4200-4210 m)含有橄榄石(Fo56-71)。在较浅层序中观察到高铝正映石。矿物分带和矿物化学变化记录了基性岩浆的分异结晶。这些矿物共同反映了一个复杂的岩浆演化过程,在这个过程中,最初是高温条件占优势,随后是分异和分异结晶;从原始状态到更进化状态的过渡。地热计算表明,玄武岩的结晶温度在1330 ~ 1340℃之间,与幔源岩浆有关,代表了高温岩浆过程。玄武岩层间沉积岩呈深色,由风化长石和斜辉石组成,少量石英和方解石。粉末x射线衍射(XRD)分析显示,在这些沉积岩中存在粘土矿物,如蒙脱石、反长晶石、凹凹土和绿泥石。虽然未发表的报告表明,层间岩石是砂岩和页岩(基于伽马射线测井数据),但这些分析表明,它们是火山碎屑沉积物,是洪水玄武岩序列中单个层在喷发后风化的结果。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Petrogenesis of paleocene flood basalt sequence and interlayered sedimentary successions in the Mannar Basin – Offshore Sri Lanka (Northern Equatorial margin of the Indian Ocean)
The Mannar Basin is a rift basin formed during the breakup of Gondwana, comprising sedimentary deposits from multiple cycles. Exploration for hydrocarbons has uncovered igneous sequences distributed throughout the basin's sedimentary sequences. These sequences exhibit geochemical characteristics, typical for flood basalts formed during a series of eruptions from 60 to 62 Ma. Previous studies have focused on the petroleum system, tectonostratigraphy, lithostratigraphy, and the paleo-environmental setting, therefore, little was known about the petrogenesis of this flood basalt sequence. This study investigates the petrogenesis of the flood basalt sequence, focusing on crystallization temperature, source magma characteristics, and the nature of magma fractional crystallization. Additionally, it examines the mineralogical characteristics, including clay minerals, of the interstratified sedimentary layers to interpret their origins—an area that has not been previously studied in depth. Petrographic thin sections were prepared from unwashed drill cuttings taken from a depth of 4000–4200 m in the Barracuda petroleum exploration well. A detailed petrographic study was conducted on these samples to investigate the petrogenesis. Additionally, electron probe microanalysis (EPMA) was performed to determine the mineral chemistry of the basalt and interstratified sedimentary rock samples. The basalts are primarily composed of plagioclase (An62-82) and clinopyroxene (mostly augite), with minor occurrences of orthopyroxene (En54-67) and ulvöspinel. Only the lower-most basalt layers (4200–4210 m) contain olivine (Fo56-71). High-Al orthopyroxenes were observed in the shallower sequence. Mineral zoning and mineral chemical variations record fractional crystallization of the mafic magma. Together, these minerals reflect a complex magmatic evolution, where, initially, high-temperature conditions prevailed, followed by differentiation and fractional crystallization; a transition from primitive to more evolved conditions. Geothermometric calculations indicate crystallization temperatures of the basalt varying from 1330 to 1340 °C, typically associated with mantle-derived magmas and representing high-temperature magmatic processes.
The interlayered sedimentary rocks within the basalt sequence are dark-coloured and consist of weathered feldspar and clinopyroxenes, with minor quartz and calcite. Powder x-ray diffraction (XRD) analyses reveal the presence of clay minerals such as smectite, antigorite, attapulgite, and chlorite in these sedimentary rocks. While unpublished reports suggest that the interlayered rocks are sandstones and shales (based on gamma-ray log data), these analyses indicate that they are volcaniclastic sediments resulting from the weathering of individual layers of the flood basalt sequence after their eruption.
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