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INFRARED MICROTHERMOMETRY AND CHEMISTRY OF WOLFRAMITE FROM THE BAIA SPRIE EPITHERMAL DEPOSIT ROMANIA

机译:拜亚斑皮表皮沉积物罗马尼亚的白云母的红外热力学和化学性质

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The chemical and microthermometric characteristics of wolframite crystals from the Baia Sprie Au-Ag-Pb-Zn-Cu-W ore deposit (Baia Mare district, Romania) have been investigated using electron probe microanalysis (EPMA), X-ray elemental mapping, and infrared microscopy. The chemical composition of wolframite changes from a nearly pure huebnerite (MnWO_4) core to nearly pure ferberite (FeWO_4) rims. This zonation correlates with a decrease in infrared transmittance from core to rims of wolframite crystals as demonstrated by Fourier transform infrared spectra. The Fe content of wolframite may control its infrared transparency, just as the Fe~(2+) reversible Mn~(2+) substitution controls its transparency in visible light. Microthermometric measurements, performed with an infrared microscope, indicate salinities ranging from 4.6 to 6.4 wt percent NaCl equiv and homogenization temperatures of 154 deg to 240 deg C for primary fluid inclusions, all trapped in the Mn-rich zones of the studied crystals. Secondary fluid inclusions showed similar microthermometric characteristics (4.6-6.4 wt percent NaCl equiv; temperature of homogenization, 171 deg-232 deg C). These microthermometric data agree well with data from previous studies on transparent minerals (quartz, sphalerite) from the Baia Sprie ore deposit. However, it is notable that wolframite appears to have precipitated after scheelite and at lower temperatures. A possible magmatic contribution to ore has been invoked for epithermal gold deposits that contain wolframite, including Baia Sprie. The unexpected low temperatures and low salinities of ore-forming fluids responsible for forming wolframite at Baia Sprie may indicate a mixing of magmatic fluids with a dominant meteoric water component.
机译:使用电子探针显微分析(EPMA),X射线元素标测和X射线衍射研究了Baia Sprie Au-Ag-Pb-Zn-Cu-W矿床(罗马尼亚Baia Mare区)中黑钨矿晶体的化学和微观热学特征。红外显微镜。钨铁矿的化学成分从近乎纯的辉锰矿(MnWO_4)芯变为近乎纯的铁锰矿(FeWO_4)轮辋。如傅立叶变换红外光谱所证实的,该分区与从黑钨矿晶体的核心到边缘的红外透射率的降低相关。钨铁矿中的Fe含量可以控制其红外透明度,就像Fe〜(2+)可逆Mn〜(2+)取代控制可见光下的透明度一样。用红外显微镜进行的显微热测量表明盐度范围为4.6至6.4 wt%NaCl当量,初级流体夹杂物的均质温度为154℃至240℃,所有这些均被困在研究晶体的富锰区中。次生流体包裹体显示出相似的微热学特征(4.6-6.4 wt%NaCl当量;均质温度,171℃至232℃)。这些微量热测量数据与先前对Baia Sprie矿床中的透明矿物(石英,闪锌矿)的研究数据吻合。然而,值得注意的是,白钨矿之后和较低的温度下黑钨矿似乎已经沉淀。对于包含黑钨矿的超热金矿床,包括拜亚斯普里(Baia Sprie),都提出了可能的岩浆作用。导致在Baia Sprie形成黑钨矿的成矿流体出乎意料的低温和低盐度可能表明岩浆流体与主要的陨石水成分混合。

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