Controle estrutural dos pegmatitos ricos em ETR associados ao depósito Madeira (Sn-Nb-Ta), mina Pitinga, Amazonas, Brasil

Q4 Earth and Planetary Sciences Pesquisas em Geociencias Pub Date : 2019-06-07 DOI:10.22456/1807-9806.93249
Fernanda Claas Ronchi, F. Althoff, A. B. Neto
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Abstract

We have studied the structural control of pegmatites (F-REE-Li vein-type granite pegmatite) associated with the albite-enriched granite facies (AEG) of the Madeira A-type granite (~1.83 Ga). This facies corresponds to the Madeira world-class Sn-Nb-Ta-F (cryolite) deposit at the Pitinga mine. These REE-rich pegmatites [xenotime-(Y) and gagarinite-(Y)], presently exploited together with the disseminated ore, have potential to exploitation by selective mining. They have a common geometric arrangement and share the same mineralogy, therefore they all originated from the same source. They have the same mineralogical composition of the host rock and their emplacement occurred in the parental rock itself. The geometric arrangement of the pegmatites is settled by contractional brittle structures (reverse faults, imbrication fans and horses). The reverse fault planes (~N320/60SW) were essentially the conduits for the fluid. The preferential sites for the pegmatites bodies were horizontal tensile fractures. The well-marked geometric arrangement of the tectonic structures and the fact that there are also reverse faults planes without pegmatites show that the fractures that host the pegmatites were not formed by the fluid pressure. The orientation of the contractional structures in the AEG indicates a transport from SW to NE. With reduced dimensions, the AEG cooled fast, however its location in the cold upper crust and the low solidus temperature allowed pegmatites formation. The pegmatites were formed with the AEG emplaced in a structural level above the critical crustal depth, where minimum normal stress is vertical.
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巴西亚马逊Pitinga矿马德拉矿床(Sn-Nb-Ta)富ETR伟晶岩的结构控制
本文研究了马德拉a型花岗岩(~1.83 Ga)富钠长石花岗岩相(AEG)伴生的伟晶岩(F-REE-Li脉状花岗岩伟晶岩)的构造控制作用。该相对应于Pitinga矿马德拉世界级Sn-Nb-Ta-F(冰晶石)矿床。这些富稀土伟晶岩[xenotime-(Y)和gagarinite-(Y)]目前与浸染的矿石一起开采,具有选择性开采的潜力。它们具有共同的几何排列和相同的矿物学,因此它们都起源于同一来源。它们具有与寄主岩相同的矿物组成,它们的侵位发生在母岩本身。伟晶岩的几何排列是由收缩脆性构造(逆断层、瓦叠扇和马)决定的。逆断面(~N320/60SW)主要是流体的输送通道。伟晶岩体的优先发育部位为水平张性裂缝。构造构造的几何排列和无伟晶岩的逆断面表明,含伟晶岩的裂缝不是由流体压力形成的。在AEG中收缩结构的方向表明从西南向东北的转移。随着尺寸的减小,AEG冷却得很快,然而它在寒冷的上地壳中的位置和较低的固相温度使得伟晶岩的形成成为可能。伟晶岩形成时,AEG侵位在临界地壳深度以上的构造水平上,此处的最小法向应力是垂直的。
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来源期刊
Pesquisas em Geociencias
Pesquisas em Geociencias Earth and Planetary Sciences-Earth and Planetary Sciences (all)
CiteScore
0.70
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发文量
6
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