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Unusual lithospheric structure and evolutionary pattern of the cratonic segments of the South Indian shield

机译:南印度盾构克拉通地层异常的岩石圈结构和演化模式

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摘要

The southern Indian shield, characterised by several prominent geological and geophysical features, can be divided into three distinct tectonic segments: Western Dharwar craton (WDC), Eastern Dharwar craton (EDC) and Southern Granulite terrain (SGT). With the exception of WDC, the entire crust beneath EDC and SGT has been remobilized several times since their formation during the mid- to late Archeans (3.0-2.5 Ga). In order to understand the evolutionary history of these segments, a multiparametric geological and geophysical study has been made which indicates that the south Indian shield, characterized by a reduced heat flow of 23-38 mW/m2 has a much thinner (88-163 km) lithosphere compared to ~200-450 km found in other global shields. In the EDC-SGT terrain, high velocity upper crust is underlain by considerably low mantle velocity with a thick high conductive/low velocity zone sandwiched at mid crustal level. Our study reveals that the entire EDC region is underlain by granulite facies rocks with a density of about 2.85 to 3.16 g/cm3 at a shallow depth of about 8 km in the southern part and at even shallower depth of about 1 to 2 km below the Hyderabad granitic region in the north. Cratonic mantle lithosphere beneath EDC may contain a highly conductive, anisotropic and hydrous metasomatic zone between the depth of 90 and 105 km where estimated temperatures are in the range of 850-975°C. It is likely that before the early Proterozoic, the entire south Indian shield was a coherent crustal block which subsequently got segmented due to persistent plume-induced episodic thermal reactivations during the last 2.7 Ga. These reactivations led to self destruction of cratonic roots giving rise to negative buoyancy at deeper levels which may have been responsible for crustal remobilisations, followed by regional uplifting and erosion of once substantially thick greenstone belts. Consequently, the crustal column beneath the EDC has become highly evolved and now corresponds closely to SGT at depth.
机译:印度南部盾构具有几个突出的地质和地球物理特征,可以分为三个不同的构造部分:西部Dharwar克拉通(WDC),East Dharwar克拉通(EDC)和Southern Granulite地形(SGT)。除了WDC之外,EDC和SGT之下的整个地壳自它们在太古宙斯中晚期(3.0-2.5 Ga)形成以来已经动了好几次。为了了解这些部分的演化历史,已进行了多参数地质和地球物理研究,结果表明,以23-38 mW / m2的热流减少为特征的南印度盾构要薄得多(88-163 km )岩石圈,而在其他全球盾构中则可找到约200-450公里。在EDC-SGT地形中,高速上地壳被相当低的地幔速度所覆盖,地壳中部水平夹有厚厚的高导电/低速区域。我们的研究表明,整个EDC区域都由花岗石相岩石包裹着,密度大约为2.85至3.16 g / cm3,在南部的浅层深度约为8 km,而在岩石的下方甚至更浅的深度约为1-2 km。北部的海得拉巴花岗岩区。 EDC下方的克拉通地幔岩石圈可能在90至105 km深度之间包含一个高度导电,各向异性和含水的交代带,估计温度在850-975°C之间。可能是在元古代以前,整个南印度盾构是一个完整的地壳块,随后由于在最后2.7 Ga内持续的羽流诱发的偶发性热活化而被分段。这些活化导致克拉通根的自毁,从而导致较深层的负浮力可能是造成地壳运动的原因,其次是区域抬升和侵蚀曾经很厚的绿岩带。因此,EDC下方的地壳柱已经高度演化,现在与深部的SGT紧密对应。

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