首页> 外文期刊>GSA Bulletin >The Arabian continental alkali basalt province: Part II. Evolution of Harrats Khaybar, Ithnayn, and Kura, Kingdom of Saudi Arabia
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The Arabian continental alkali basalt province: Part II. Evolution of Harrats Khaybar, Ithnayn, and Kura, Kingdom of Saudi Arabia

机译:阿拉伯大陆碱玄武岩省:第二部分。沙特阿拉伯王国哈拉巴尔·伊拜恩和库拉的演变

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摘要

Three coalesced basaltic lava fields, Harrats Khaybar, Ithnayn, and Kura, constitute the largest contiguous area of Cenozoic basalt in Saudi Arabia, similar in extent (20,564 km2) and volume (1,850 km3) to Harrat Rahat, which is situated only 25 km to the south. Harrat Kura, with an age range from about 11 to 5 Ma, is the oldest of these harrats; it contains a single stratigraphic unit, the Kura basalt, primarily composed of alkali olivine basalt (AOB) with subordinant basanite and hawaiite and a single cluster of four phonolite domes. In contrast, Harrats Khaybar (5 Ma to Present) and Ithnayn (3 Ma to Present) are composed of more mildly alkaline basalt types. The two oldest units on Harrat Khaybar, the Jarad and Mukrash basalts, are dominated by dictytaxitic-to-ophitic olivine transitional basalt (OTB) flows, which were extruded primarily from major arterial lava tubes to form unusual morphological features, here designated "whaleback lava flows." The lava tubes emanate from a 50-km-long, north-trending fault scarp along the western edge of the central vent zone, which marks the site of voluminous outwelling of OTB lava. The fault scarp ceased to be a major site of extrusion at the end of Mukrash time. Immediately to the east of the fault scarp, a thin (0.7 to 1.0 km), uptilted slab of crust formed the roof of a high-level magma chamber (60 x 25 km) that dominated the eruptive history of the Abyad basalt, the youngest stratigraphic unit on Harrat Khaybar. The Abyad basalt occurs as seven stratigraphic subunits, the two youngest of which (Qb6 and Qb7) are "post-Neolithic" and historical in age. In contrast to the Jarad and Mukrash basalts, the Abyad basalt is dominated by AOB and hawaiite, with only minor OTB. No Abyad differentiated rocks occur on Harrat Ithnayn; however, fractional crystallization in the high-level magma chamber beneath Harrat Khaybar has resulted in an extreme compositional range of rock types, from mugearite to benmoreite, trachyte, and comendite. The vent distribution at Harrat Khaybar shows a distinct zonation indicative of a high-level, compositionally stratified magma chamber. Whole-rock chemistry suggests that even the most primitive basalts are not primary magmas, but rather fractionated melts derived from primary magmas of variable melt fractions generated at differing mantle depths. The more undersaturated Harrat Kura basalts were derived from primary magmas representing the smallest degrees of partial melting, at the greatest depth. Crystal fractionation of most primary magmas appears to have taken place in reservoirs at the crust-mantle boundary. Chemical and petrographic data suggest that open-system magma recharge was an important process in the high-level magma chamber beneath Harrat Khaybar. The chemical and mineralogical heterogeneity of the Harrat Khaybar comendites, their Sr-isotope values, and their Zr/Nb ratios all indicate that they were derived by varying degrees of crystal fractionation (>95%), crustal melting, and halogen complexing. The north-trending volcanic axes of Harrats Rahat, Khaybar, and Ithnayn form a single, 600-km-long linear vent system, designated the Makkah-Madinah-Nafud (MMN)volcanic line. The three transitional-to-mildly alkaline harrats extruded from this volcanic line differ from most Arabian harrats, which like Harrat Kura to the west, are significantly more undersaturated. The relatively large degrees of partial melting evident in Harrats Rahat, Khaybar, and Ithnayn suggest that the MMN volcanic line may overlie a north-south thermal lineation in the mantle. The petrochemical stratigraphic sequence in these three harrats is nearly identical; early voluminous extrusions of OTB were followed by later, less extensive extrusions of minor OTB and abundant AOB, hawaiite, and differentiated lavas. As this petrochemical stratigraphy evolved, it progressed northward along the MMN trend with time, beginning on Harrat Rahat about 10 Ma, on Harrat Khaybar about 5 Ma, and on Harrat Ithnayn about 3 Ma. The interplay of open-system magmatic processes beneath this migrating volcanic line has resulted in a classic example of a strongly fractionated, mildly alkaline basalt series.
机译:三个聚结的玄武岩熔岩田,哈拉特斯·哈伊巴尔,伊斯奈恩和苏拉,构成了沙特阿拉伯新生界最大的玄武岩毗连区,范围相似(20,564 km 2 )和体积 (到1,850 km 3 )到Harrat Rahat,后者距南部的 仅25公里。哈拉特·库拉(Harrat Kura)是年龄最大的哈拉特,年龄在11至5 Ma。它包含一个单一的 地层单元,即Kura玄武岩,主要由碱橄榄石 玄武岩(AOB)与次要的Basanite和hawaiite组成,以及一个 集群四个圆屋顶。相比之下,Harrats Khaybar (5 Ma到现在)和Ithnayn(3 Ma到现在)由 组成,具有更弱的碱性玄武岩类型。 Harrat Khaybar上两个最古老的单元,即Jarad和Mukrash玄武岩,由dictytaxitic到ophitic橄榄石过渡玄武岩(OTB) 为主,它们主要是从主要的动脉熔岩 管中挤出的,形成了异常的形态特征,此处称为“鲸回熔岩流”。熔岩管是从一个50公里长的 北向断裂带沿着中部 带的西边缘喷出的,标志着< sup> OTB熔岩。在穆克拉什(Mukrash)时间结束时,断层陡壁不再是挤压的主要部位。 在断层陡壁的东侧,很薄(0.7至1.0 km),倾斜的地壳板形成了一个高级的 岩浆室(60 x 25 km)的屋顶,该室控制着阿比亚德玄武岩的喷发史 ,是Harrat Khaybar上最年轻的地层单位。阿比亚德玄武岩以七个地层亚基出现,其中两个最年轻的(Qb6和Qb7)是“新石器时代的” ,并且具有历史性。与Jarad和Mukrash 玄武岩相反,Abyad玄武岩由AOB和夏威夷石( )占据主导地位,仅有少量的OTB。在 Harrat Ithnayn上没有Abyad分化的岩石;但是,哈拉特·海巴尔(Harrat Khaybar)下方高空 岩浆室中的分步结晶导致了极端的 岩石组成成分范围,从白云母到膨润土, 曲奇和粉红色。 Harrat Khaybar 处的喷口分布显示出明显的带状分布,指示了一个高层次的,组成上的 层状岩浆室。 最原始的玄武岩 不是原生岩浆,而是由 地幔深度不同而产生的可变熔体分数的原生岩浆衍生的 分馏熔体。较不饱和的Harrat Kura 玄武岩是从原生岩浆中衍生出来的,这些岩浆在最大深度处具有最小的部分熔融度。大多数初级岩浆的晶体分级 似乎发生在地幔幔边界处的储层 中。化学和岩石学数据 暗示开放系统岩浆充注是哈拉特海巴尔(Harrat Khaybar)下方高空岩浆室内的一个重要过程。 Harrat Khaybar 混合物的 化学和矿物异质性,它们的Sr同位素值和Zr / Nb比 都表明它们是衍生的通过不同程度的晶体 分馏(> 95%),地壳融化和卤素络合。 Harrats Rahat,Khaybar,的北向火山轴sup>和Ithnayn形成一个600公里长的单一线性喷口系统,称为 Makkah-Madinah-Nafud(MMN)火山线。从这条火山线挤出的三个过渡至轻度的 碱性哈拉特不同于 大多数阿拉伯哈拉特,如西部的Harrat Kura都是 明显不饱和。在Harrats Rahat,Khaybar和Ithnayn 中明显出现的相对大程度的 暗示MMN火山线可能覆盖南北向 在地幔中。这三个地层中的石油化学地层 序列几乎是相同的。 OTB的早期大体积挤出,随后是较小的OTB和丰富的AOB,夏威夷岩以及分化的 熔岩的较晚,较不广泛的挤出 。随着这一石化地层的发展,它随时间随MMN趋势向北发展,从Harhat Rahat大约10Ma开始,Harrat Khaybar大约5Ma,然后Harrat 开始> Ithnayn大约3 Ma。在这条正在迁移的火山线下,开放系统岩浆过程的相互作用产生了一个强分馏,轻度碱性的玄武岩系列的经典 示例。

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  • 来源
    《GSA Bulletin》 |1991年第3期|363-391|共29页
  • 作者单位

    Directorate General of Mineral Resources, P. O. Box 345, Jiddah 21191 Saudi Arabia;

    Directorate General of Mineral Resources, P. O. Box 345, Jiddah 21191 Saudi Arabia;

    Department of Geology, Washington State University, Pullman, Washington 99164-2812;

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