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首页> 外文期刊>Geological Society of America Bulletin >Large-scale sedimentary recycling of tectonic melange in a forearc setting: The Ionian basin (Oligocene-Quaternary, southern Italy)
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Large-scale sedimentary recycling of tectonic melange in a forearc setting: The Ionian basin (Oligocene-Quaternary, southern Italy)

机译:前肢环境中构造混杂岩的大规模沉积物再循环:爱奥尼亚盆地(渐新世-第四纪,意大利南部)

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Distinctive horizons of melange—ranging in maximum thickness from a few tens to several hundreds of meters—are conformably interbedded with the regularly stratified, Oligocene-to-Quaternary, predominantly marine deposits of the Ionian forearc basin along the leading edge of the Calabria-Peloritani microplate of southern Italy. These melange horizons were emplaced from the late-early to the late Miocene during collision of the southern and northern margins of the microplate with the passive margins of northern Africa and the Apulian Platform, respectively. Collisional deformation induced uplift of parts of the accretion-ary prism and ensuing sedimentary recycling of melange into the adjacent Ionian forearc basin. The thickest melange horizon can be traced for a distance >80 km with a consistent stratigraphic position within the forearc basin fill, and ranges in thickness from ~1 km near the collision zone to zero away from it. It was emplaced in the late Burdigalian and records oblique collision of the Calabria-Peloritani microplate with the northern continental margin of Africa. In this context, portions of the melange of the accretion-ary prism were extruded tectonically and gravitationally mobilized from southwest to northeast in the remaining, undeformed parts of the forearc basin. This interpretation is supported by (1) the overall geometry of the melange horizon pinching out away from the collision zone, (2) its conformable contacts and chronostratigraphic relationships with the underlying and overlying stratigraphic units, (3) its composition, and (4) the absence of tectonic deformation at base and top of the horizon. Younger and thinner melange horizons are interbedded within the latest Tortonian-Messinian succession and resulted from the erosion of thrust tip areas within the inner portion of the ac-cretionary prism following incipient collision of the northern end of the microplate with the Apulian Platform. Integration of the results of this and other studies indicate that sedimentary recycling of large volumes of melange from accretionary prisms into forearc basins is an important process along both collisional and noncollisional active plate margins.
机译:混杂的独特层位(最大厚度范围从几十到几百米)与沿着卡拉布里亚-佩洛里塔尼前缘的爱奥尼亚前陆盆地的规则分层,渐新世至第四纪主要为海洋沉积物相交。意大利南部的微孔板。这些混杂层位从微板的南缘和北缘与北非被动缘和阿普利亚平台的被动缘碰撞时,分别从中晚期晚期到中新世。碰撞变形引起吸积棱镜的部分隆起,并导致混杂岩的沉积物再循环到相邻的爱奥尼亚前臂盆地。可以追踪到最厚的混杂层地平线,其距离> 80 km,并且前臂盆地填充物中的地层位置一致,厚度范围从碰撞区附近的〜1 km到碰撞区附近的零。它放置在Burdigalian晚期,记录了Calabria-Peloritani微孔板与非洲北部大陆边缘的倾斜碰撞。在这种情况下,在前陆盆地剩余的未变形部分中,吸积棱镜的混杂部分从西南向东北以构造和重力的方式运动。这种解释得到以下方面的支持:(1)混杂层地平线从碰撞区中伸出的总体几何形状;(2)其与下伏地层和上覆地层单元的顺应性接触和年代地层关系;(3)其组成;以及(4)在地平线的底部和顶部没有构造变形。在最新的Tortonian-Messinian演替中夹杂着更年轻,更薄的混杂层,这是由于微孔板北端与Apulian平台开始碰撞后,在增生棱镜内部内部的逆冲尖端区域受到侵蚀而导致的。这项研究和其他研究结果的整合表明,从混杂棱柱到前臂盆地的大量混杂物的沉积物再循环是沿着碰撞和非碰撞活动板块边缘的重要过程。

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