盖耶尔西南锡矽卡岩矿床的矿物化学:了解可变的流体/岩石比率和金属通量

IF 4.4 2区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS
Nicolas Meyer, Mathias Burisch, Jens Gutzmer, Joachim Krause, Henning Scheibert, Gregor Markl
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引用次数: 0

摘要

德国厄尔士山脉的盖耶锡矽卡岩由早期矽卡岩阶段(第一阶段,约 320 Ma)和较年轻的变质阶段(第二阶段,约 305 Ma)组成,但矽卡岩蚀变的锡来源和分布以及物理化学条件尚未得到确定。我们的研究结果表明,第一阶段的接触变质矽卡岩只含有少量的锡。REE 模式和高浓度的 HFSE 表明,第一阶段的石榴石、榍石和蛭石是在岩石缓冲条件下(低流体/岩石比)形成的。与此相反,第二阶段的原生集合体包含两代石榴石、榍石-马拉雅岩和蛭石。在岩石缓冲和流体缓冲条件之间摆动的特点是元石榴石中 HFSE、W、In 和 Sn 的浓度不同。在高流体/岩石比条件下形成的矿物的痕量和稀土元素特征似乎与岩浆-热液特征相似,而岩浆-热液特征则导致了变质矽卡岩蚀变。随着流体-岩石比的降低,锡从富含锡的硅酸盐中被重新移动,并重新沉淀为孔雀石。第二阶段末期,陨石水的进入和温度的降低导致锡石、低锡闪石、绿泥石和硫化物矿物的形成。锡石的微量和痕量元素组成变化不大,即使主岩和煤矸石矿物变化很大,这表明岩浆-热液流体占主导地位,流体/岩石比率较高。因此,主要矽卡岩形成矿物的矿物化学成分记录了流体/岩石比率的变化,以及多相锡矽卡岩系统中岩浆流体对锡的到达、分布和再移动。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Mineral chemistry of the Geyer SW tin skarn deposit: understanding variable fluid/rock ratios and metal fluxes

Mineral chemistry of the Geyer SW tin skarn deposit: understanding variable fluid/rock ratios and metal fluxes

The Geyer tin skarn in the Erzgebirge, Germany, comprises an early skarnoid stage (stage I, ~ 320 Ma) and a younger metasomatic stage (stage II, ~ 305 Ma), but yet, the source and distribution of Sn and the physicochemical conditions of skarn alteration were not constrained. Our results illustrate that contact metamorphic skarnoids of stage I contain only little Sn. REE patterns and elevated concentrations of HFSE indicate that garnet, titanite and vesuvianite of stage I formed under rock-buffered conditions (low fluid/rock ratios). Prograde assemblages of stage II, in contrast, contain two generations of stanniferous garnet, titanite-malayaite and vesuvianite. Oscillation between rock-buffered and fluid-buffered conditions are marked by variable concentrations of HFSE, W, In, and Sn in metasomatic garnet. Trace and REE element signatures of minerals formed under high fluid/rock ratios appear to mimic the signature of the magmatic-hydrothermal fluid which gave rise to metasomatic skarn alteration. Concomitantly with lower fluid-rock ratio, tin was remobilized from Sn-rich silicates and re-precipitated as malayaite. Ingress of meteoric water and decreasing temperatures towards the end of stage II led to the formation of cassiterite, low-Sn amphibole, chlorite, and sulfide minerals. Minor and trace element compositions of cassiterite do not show much variation, even if host rock and gangue minerals vary significantly, suggesting a predominance of a magmatic-hydrothermal fluid and high fluid/rock ratios. The mineral chemistry of major skarn-forming minerals, hence, records the change in the fluid/rock ratio, and the arrival, distribution, and remobilization of tin by magmatic fluids in polyphase tin skarn systems.

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来源期刊
Mineralium Deposita
Mineralium Deposita 地学-地球化学与地球物理
CiteScore
11.00
自引率
6.20%
发文量
61
审稿时长
6 months
期刊介绍: The journal Mineralium Deposita introduces new observations, principles, and interpretations from the field of economic geology, including nonmetallic mineral deposits, experimental and applied geochemistry, with emphasis on mineral deposits. It offers short and comprehensive articles, review papers, brief original papers, scientific discussions and news, as well as reports on meetings of importance to mineral research. The emphasis is on high-quality content and form for all articles and on international coverage of subject matter.
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