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The North Makassar Straits: what lies beneath?

机译:北孟加锡海峡:背后是什么?

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It has been accepted for many years that eastern Borneo and western Sulawesi were close together in the Late Cretaceous but the mechanism and age of formation of the Makassar Straits, which now separate them, have been the subjects of much debate. Geological studies on land show that the straits formed by Eocene rifting. However, the nature of the crust beneath the straits remains controversial. The southern parts are likely to be underlain by extended continental crust but, in the northern Makassar Straits, it is more difficult to decide. Water depths are up to 2500 m, there is a very thick sedimentary cover, the basement is not well imaged on seismic lines and there is no way of directly sampling it. Field studies from the Borneo and Sulawesi margins have provided the basis for reconstructing the development of the straits, and suggesting they are underlain by oceanic crust. The rift and its margins are asymmetrical and wide, with up to 400 km of stretched crust on the Borneo side and about 200 km on the Sulawesi side, separated by about 200 km of the deepest crust in the northern Makassar Straits. Gravity data and flexural modelling on the Borneo side suggest a junction between continental and oceanic crust beneath the Mahakam delta. The oceanic crust is inferred to be of Middle Eocene age, similar to the Celebes Sea to the north; apparent conical structures on seismic lines have been interpreted as volcanic edifices. However, the earliest backstripping studies suggested thinned continental crust in the central straits and this has been supported by interpretations of new seismic data from the offshore area west of Sulawesi. Half-graben and graben are interpreted beneath thick sediments, there are low-angle extensional faults, and lineaments crossing basement can be traced into the deepest parts of the straits. These structures suggest an origin by oblique rifting of continental crust in which the apparent conical structures are interpreted as carbonate build-ups on tilted fault blocks.
机译:早在白垩纪末期,婆罗洲东部和苏拉威西西部并列在一起已经被接受了很多年,但是望加锡海峡的形成机理和年代, < / sup>现在将它们分隔开来,一直是许多争论的主题。 陆地地质研究表明,始新世 裂谷形成的海峡。但是,海峡 下的地壳的性质仍存在争议。南部地区可能是被扩展的大陆壳覆盖的 ,但在望加锡海峡的北部,这很难决定。水深达 到2500 m,沉积层非常厚,地下 在地震线上的成像效果不佳,无法直接 < / sup>对其进行采样。婆罗洲和苏拉威西边缘 的野外研究为重建 海峡的发展提供了基础,并暗示了它们处于大洋地壳之下。 裂谷及其边缘是不对称且宽的,婆罗洲一侧的地壳延伸达400 km,苏拉威西一侧的地壳延伸达200 km,相距约200 km望加锡海峡北部最深的 地壳。婆罗洲一侧的重力数据和弯曲 建模表明,Mahakam三角洲下方的大陆 与洋壳之间存在交汇处。推测该洋壳 属于始新世中期,类似于北部的Celebes Sea。 地震线上的明显圆锥形结构已被解释为火山构造。但是,最早的 反冲研究表明 中海峡的大陆壳变薄,这得到了近海新地震数据的解释 的支持。苏拉威西岛以西。 半graben和grapen被解释为在厚厚的沉积物之下, 存在低角度伸展断层,并且穿过 基底的线状构造追溯到海峡最深处。 这些结构通过倾斜地裂大陆 地壳暗示了起源,其中明显的圆锥形结构被解释为 倾斜断块上的碳酸盐堆积。

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  • 来源
    《Petroleum Geoscience》 |2009年第2期|147-158|共12页
  • 作者单位

    SE Asia Research Group, Department of Earth Sciences, Royal Holloway University of London , Egham, Surrey TW20 0EX, UK;

    SE Asia Research Group, Department of Earth Sciences, Royal Holloway University of London , Egham, Surrey TW20 0EX, UK|Tullow South Africa , 7 Coen Steytler Avenue, Cape Town 8001,South Africa;

    SE Asia Research Group, Department of Earth Sciences, Royal Holloway University of London , Egham, Surrey TW20 0EX, UK|ConocoPhillips Indonesia , Jl. Jend. Gatot Subroto Kav 9-11, Jakarta 12930, Indonesia;

    SE Asia Research Group, Department of Earth Sciences, Royal Holloway University of London , Egham, Surrey TW20 0EX, UK|Chevron , Jl. Asia Africa No. 8, Jakarta 10270, Indonesia;

    SE Asia Research Group, Department of Earth Sciences, Royal Holloway University of London , Egham, Surrey TW20 0EX, UK|Marathon Oil Company , Jalan TB Simatupang No. 41, Jakarta 12550, Indonesia;

    SE Asia Research Group, Department of Earth Sciences, Royal Holloway University of London , Egham, Surrey TW20 0EX, UK;

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