阿根廷Potrerillos花岗岩内La Elsa NYF伟晶岩中的铋矿物:从岩浆到热液阶段流体演化的监测

IF 1.1 4区 地球科学 Q3 MINERALOGY Canadian Mineralogist Pub Date : 2021-01-28 DOI:10.3749/CANMIN.2000011
R. Škoda, M. Novak, R. Čopjaková, M. A. Galliski, M. F. Márquez-Zavalía, J. Sejkora
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引用次数: 2

摘要

NYF La Elsa伟晶岩形成了一个约30米长、约20米宽的亚圆形体,包裹在阿根廷Las chacras - potrerilllos岩基的母岩potrerilllos花岗岩中。伟晶岩具有典型的带状内部构造,具有体积显著的石英芯和岩浆萤石荚体。与黑云母一起,主要在外层单元中,电气石(榴辉石,氟榴辉石)在大多数伟晶岩单元中常见到丰富。辅助矿物包括常见的强赤铁矿和罕见的铋辉石自晶体晶体,长可达2厘米,出现在块状带和石英岩心之间的过渡处。根据Bi2S3(s) + CO2(aq) + 6O2(aq) + 3H2O(l) = Bi2CO3O2(s) + 3H2SO4(aq)的反应,铋酸铋矿被铋酸铋矿I明显取代。随后,铋矿I被铋矿II和钾钠矿所取代。前者需要Ca和F的流入,其形成可以用反应Bi2CO3O2(s) + 2Ca2+(aq) + 2F - (aq) + CO32 - (aq) = 2CaBiCO3OF(s)来表征。在热液后期,随着V的流入,铋辉石被斜辉石/水辉石取代,反应过程为Bi2CO3O2s + 2H3VO4(aq) = 2BiVO4(s)+ CO2(aq) + 3H2O(l)。铋矿及其次生产物中只有微量的Pb和±Cu,所有Bi矿物均接近理想配方。铋矿物的结晶顺序为岩浆铋辉石(S2 -)→早期热液铋辉石I (CO32 -)→中期铋辉石II +钾辉石(CO32 -, F -)→晚期辉石、水辉石(VO43 -)。石英流体包裹体的共聚焦拉曼显微光谱证实,伟晶岩衍生的早期亚固体流体富含CO2,并导致铋辉石分解为铋辉石。岩浆萤石在酸性条件下蚀变过程中释放出形成钾辉石所必需的钙和F。钒由富含蚀变岩浆矿物(黑云母、钛铁矿)元素的陨石H2O提供,这些元素要么来自伟晶岩,要么来自宿主花岗岩。
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Bismuth minerals from the intragranitic La Elsa NYF pegmatite, Potrerillos granite, Argentina: Monitors of fluid evolution from magmatic to hydrothermal stage
The NYF La Elsa pegmatite forms a subcircular, ∼30 m long, ∼20 m wide body enclosed in the parental Potrerillos granite, Las Chacras-Potrerillos batholith, Argentina. The pegmatite has a typical zonal internal structure with a volumetrically significant quartz core and pods of magmatic fluorite. Along with biotite, mostly in the outer units, tourmaline (schorl, fluor-schorl) is common to abundant in most pegmatite units. Accessory minerals include common strongly hematitized ilmenite and rare euhedral crystals of bismuthinite, up to 2 cm long, occurring at the transition between the blocky zone and the quartz core. The bismuthinite was significantly replaced by bismutite I according to the reaction Bi2S3(s) + CO2(aq) + 6O2(aq) + 3H2O(l) = Bi2CO3O2(s) + 3H2SO4(aq). Subsequently, bismutite I was replaced by bismutite II and kettnerite. The former requires an influx of Ca and F and its formation can be characterized by the reaction Bi2CO3O2(s) + 2Ca2+(aq) + 2F–(aq) + CO32–(aq) = 2CaBiCO3OF(s). At the late hydrothermal stages bismutite was replaced by clinobisvanite/pucherite during influx of V according to the reaction Bi2CO3O2s + 2H3VO4(aq) = 2BiVO4(s)+ CO2(aq) + 3H2O(l). All Bi minerals are close to the ideal formulae with only minor Pb and ±Cu in bismuthinite and its secondary products. The crystallization sequence of Bi minerals is magmatic bismuthinite (S2–) → early hydrothermal bismutite I (CO32–) → medium stage bismutite II + kettnerite (CO32–, F–) → late stage clinobisvanite, pucherite (VO43–). Pegmatite-derived early subsolidus fluids were enriched in CO2, which was confirmed by confocal Raman microspectroscopy of fluid inclusions in quartz and caused breakdown of bismuthinite to bismutite. Calcium and F, necessary for kettnerite formation, were released during alteration of magmatic fluorite at acidic conditions. Vanadium was supplied by meteoritic H2O enriched in elements from altered magmatic minerals (biotite, ilmenite), either from the pegmatite or from the host granite.
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来源期刊
Canadian Mineralogist
Canadian Mineralogist 地学-矿物学
CiteScore
2.20
自引率
22.20%
发文量
45
审稿时长
4-8 weeks
期刊介绍: Since 1962, The Canadian Mineralogist has published papers dealing with all aspects of mineralogy, crystallography, petrology, economic geology, geochemistry, and applied mineralogy.
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