首页> 外文期刊>Contributions to Mineralogy and Petrology >Origin of Meso-Proterozoic post-collisional leucogranite suites (Kaokoveld, Namibia): constraints from geochronology and Nd, Sr, Hf, and Pb isotopes
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Origin of Meso-Proterozoic post-collisional leucogranite suites (Kaokoveld, Namibia): constraints from geochronology and Nd, Sr, Hf, and Pb isotopes

机译:中元古代碰撞后白云石套件的起源(纳米比亚考科维尔德):年代学和Nd,Sr,Hf和Pb同位素的限制

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Leucocratic granites of the Proterozoic Kaoko Belt, northern Namibia, now preserved as meta-granites, define a rock suite that is distinct from the surrounding granitoids based on their chemical and isotopic characteristics. Least evolved members of this ~ 1.5-1.6-Ga-old leucogranite suite can be distinguished from ordinary calc-alkaline granites that occur elsewhere in the Kaoko Belt by higher abundances of Zr, Y, and REE, more radiogenic initial ε_(Nd) values and unradiogenic initial ~(87)Sr/~(86)Sr. The leucogranites have high calculated zircon saturation temperatures (mostly > 920°C for least fractionated samples), suggesting that they represent high-temperature melts originating from deep crustal levels. Isotope data (i.e., ε_(Ndi): +2.3 to -4.2) demonstrate that the granites formed from different sources and differentiated by a variety of processes including partial melting of mantle-derived meta-igneous rocks followed by crystal fractionation and interaction with older crustal material. Most fractionation-corrected Nd model ages (T_(DM)) are between 1.7 and 1.8 Ga and only slightly older than the inferred intrusion age of ca. 1.6 Ga, indicating that the precursor rocks must have been dominated by juvenile material. Epsilon Hf values of zircon separated from two granite samples are positive (+11 and +13), and Hf model ages (1.5 and 1.6 Ga) are similar to the U-Pb zircon ages, again supporting the dominance of juvenile material. In contrast, the Hf model ages of the respective whole rock samples are 2.3 and 2.4 Ga, demonstrating the involvement of older material in the generation of the granites. The last major tectonothermal event in the Kaoko Belt in the Proterozoic occurred at ca. 2.0 Ga and led to reworking of mostly 2.6-Ga-old rocks. However, the presence of 1.6 Ga "post-collisional" granites reflects addition of some juvenile mantle-derived material after the last major tectonic event. The results suggest that similar A-type leucogranites are potentially more abundant in crustal terranes but are masked by AFC processes. In the case of the Kaoko Belt, it is suggested that this rock suite indicates a yet unidentified period of mantle-derived crustal growth in the Proterozoic of South Western Africa.
机译:纳米比亚北部元古生界高科带的白云岩花岗岩,现已保存为超花岗岩,根据其化学和同位素特征,形成了与周围花岗岩不同的岩石组。这个〜1.5-1.6-Ga老的白云石组中演化最少的成员可以通过较高的Zr,Y和REE丰度,更多的放射成因的初始ε_(Nd)值来区别于Kaoko带其他地方的普通钙碱性花岗岩和非放射源的初始〜(87)Sr /〜(86)Sr。无色花岗岩具有较高的计算锆石饱和温度(对于最少分级的样品,大多数温度> 920°C),这表明它们代表了来自深地壳水平的高温熔体。同位素数据(即ε_(Ndi):+ 2.3至-4.2)表明,花岗岩是由不同来源形成的,并通过多种过程加以区分,包括地幔衍生的亚火成岩的部分熔融,随后的晶体分级分离以及与较老的相互作用。地壳物质。大多数经分馏校正的Nd模型年龄(T_(DM))在1.7至1.8 Ga之间,并且仅比推断的ca年龄稍大。 1.6 Ga,表明前体岩石一定是由幼年物质主导的。从两个花岗岩样品中分离出的锆石的Epsilon Hf值为正(+11和+13),并且Hf模型年龄(1.5和1.6 Ga)与U-Pb锆石年龄相似,再次证明了幼年材料的优势。相反,整个岩石样品的Hf模型年龄分别为2.3 Ga和2.4 Ga,这表明较老的材料参与了花岗岩的生成。最后一次主要的构造热事件发生在元古代的高科带。 2.0 Ga导致大部分2.6 Ga老的岩石重新加工。但是,存在1.6 Ga的“碰撞后”花岗岩反映了在最后一次重大构造事件之后添加了一些来自幼小地幔的物质。结果表明,相似的A型无色花岗岩在地壳中可能更丰富,但被AFC过程掩盖了。对于高科带来说,这套岩石表明在西南元古代的一个地幔衍生的地壳生长时期尚未确定。

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