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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 direcdy 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:早在白垩纪晚期,婆罗洲东部和苏拉威西岛就连在一起已经被接受了很多年,但现在将它们分开的望加锡海峡的形成机理和年代已经成为许多争论的主题。陆地地质研究表明,始新世裂谷形成了海峡。然而,海峡两岸地壳的性质仍存在争议。南部地区可能被扩大的大陆壳所覆盖,但在望加锡海峡北部,则很难决定。水深达2500 m,沉积覆盖层很厚,地下室在地震线上的成像不佳,无法直接取样。来自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,并表明它们被大洋地壳所掩盖。裂谷及其边缘是不对称且宽阔的,婆罗洲一侧的绵延地壳长达400公里,苏拉威西一侧的绵延约200公里,相距北部望加锡海峡最深的外壳约200公里。婆罗洲一侧的重力数据和弯曲模型表明,马哈卡姆三角洲下方的大陆壳和海洋壳之间存在交汇处。推测该洋壳为始新世中期,类似于北部的西里伯斯海。地震线上的明显圆锥形结构已被解释为火山构造。但是,最早的回抽研究表明中部海峡的大陆壳变薄,这一点得到了苏拉威西以西近海地区新的地震数据解释的支持。半粗部和grab部被解释为在较厚的沉积物之下,存在低角度的伸展断层,并且穿过基底的线可以追溯到海峡最深的部分。这些结构通过陆壳的斜裂表明了其起源,其中明显的圆锥形结构被解释为倾斜断层块上的碳酸盐堆积。

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