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首页> 外文期刊>GSA Bulletin >Tectonic Development and Metallogeny of Madagascar with Reference to the Fracture Pattern of the Indian Ocean
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Tectonic Development and Metallogeny of Madagascar with Reference to the Fracture Pattern of the Indian Ocean

机译:马达加斯加的构造发育和成矿作用-以印度洋断裂模式为例

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摘要

Madagascar is apparently a large block of continental crust intermittently uplifted as a complex horst between two subsiding depressions within the system of north-northeast–trending fractures of the Indian Ocean floor. A set of major east-trending fractures intersect the Precambrian basement rocks. These fractures are probably of Precambrian age, but later movements occurred along them. Because of the continuing movement, these fracture zones are topographically detectable as a system of evenly spaced low areas followed by river valleys that cut the sedimentary cover of western Madagascar. The Mahanoro-Tsiribihina fracture zone in the middle of the island is the most significant. Its latitude roughly corresponds to that of a segment of the east-trending Rodriguez fracture zone which intersects the crest of the Mid–Indian Ocean (Mid-Oceanic) Ridge east of long. 63° E. An axis of magmatic reactivation in central Madagascar corresponds to a deep-seated Precambrian fracture zone along which magmatic processes occurred at different times. Endogenous ore deposits of Precambrian and Paleozoic age are related to the intersection of the east-trending fracture zones with the axis of magmatic reactivation and lines parallel to this axis. The mineralization associated with Cretaceous intrusive rocks exhibits another pattern of distribution. Madagascar essentially occupies its original place. Furthermore, India was not derived from the western Indian Ocean by continental drift. Instead, a continuous landmass, referred to as the "Malagasy-Mascarene subcontinent," existed in the region between the eastern coast of present-day Africa and the Mid-Oceanic Ridge. This interpretation does not contradict the derivation of India from the central part of the Indian Ocean between 75 and 55 m.y. B.P. as suggested by McKenzie and Sclater. If the above two interpretations are correct, disintegration of a continental mass as well as continental drift have contributed to the origin of the Indian Ocean. Key Words: structural geology • economic geology • Madagascar • Malagasy-Mascarene subcontinent • sea-floor spreading • continental disintegration
机译:马达加斯加显然是由北-北-东向 断裂系统中的两个沉降 凹陷之间的复杂地壳而间歇性地抬升的大块地壳 印度洋海底。一组主要的东向断裂 断裂与前寒武纪基底岩相交。这些骨折 可能是前寒武纪,但后来发生了移动 。由于不断的运动,这些裂缝 带在地形上可以检测为一个均匀分布的 低洼区域的系统,随后是切开沉积物 cover的河谷马达加斯加西部。岛中部的Mahanoro-Tsiribihina断裂 带最为明显。它的 纬度大致对应于东趋势的 Rodriguez断裂带的一段,该断裂带与印度中部 海洋的波峰相交。 -海洋)脊长东。 63°E。马达加斯加中部 岩浆活化的轴对应于一个 深层前寒武纪断裂带,沿该岩浆带在不同时间发生岩浆作用 。前寒武纪 和古生代的内生矿床与东趋 断裂带与岩浆活化轴线和线 平行的交点有关到这个轴。与白垩纪 侵入岩有关的矿化表现出另一种分布模式。 马达加斯加基本上占据了其原始位置。此外, 印度不是通过大陆 漂移从印度洋西部获得的。取而代之的是,在当今非洲东部海岸 和大洋中脊之间的区域中存在一个连续的陆块,称为“马尔加斯-马斯卡林 次大陆。这种解释 与印度从印度洋中部75至55 m。的中部 的派生没有矛盾。 B.P.如McKenzie和Sclater所建议的 如果以上两种解释是正确的,则大陆质量的崩解 和大陆漂移都对 到印度洋的起源。 关键词:结构地质•经济地质•马达加斯加•马达加斯加-马斯卡林次大陆•海底扩散•大陆解体

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  • 来源
    《GSA Bulletin》 |1975年第4期|582-592|共11页
  • 作者

    JAN KUTINA;

  • 作者单位

    Institute of Mineral Raw Materials, Sedlec 425, Kutná Hora, Czechoslovakia|Present address: School of Marine and Atmospheric Science, University of Miami, Miami, Florida 33149.;

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