The genesis of agates and amethyst geodes

IF 1.1 4区 地球科学 Q3 MINERALOGY Canadian Mineralogist Pub Date : 2019-11-30 DOI:10.3749/canmin.1900028
I. N. Kigai
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引用次数: 6

Abstract

Practically all aspects of agate genesis generate debate. The time is ripe to clarify the most important enigmas concerning the environments of formation of agates and the related famous amethyst geodes of Brazil and Uruguay. Agates form over a wide range of temperatures, from those of basaltic and andesitic melts (about 1100 °C) down to about 50 °C, and at rather low pressures. Their formation in liquid mafic magmas is indicated by a correlation between (1) the orientation of amygdules and the inclination of onyx banding in them and (2) the attitude of amygdules in the lava flow layers. The correlation arises because lava moves at a different rate close to and far from the upper and lower rims of a flow. The alkaline supercritical fluid fills gas vesicles in lavas and dissolves silica, mainly, from ambient lava or rock to produce a silica sol. If the pressure on the fluid causes percolation of water from amygdules, the sol coagulates on the walls of the vesicle to form a concentric lining. If the pressure in amygdules falls below the maximum osmotic pressure of a sol (about 0.1 MPa for a silica sol), percolation of fluid stops, and coagulation leads to the formation of horizontal onyx banding. Multiple repetitions of precipitation of various gel layers can be caused by overlapping fresh flows upon the cooling older agate-bearing lava flow. In a submarine setting, phase separation of the fluid and the formation of a film of gel between vapor (or diluted solution) and brine stimulate the osmotic processes, which result in growth of hollow membrane tubes and branching moss-like arrays at the bottom of amygdules. Some agates exhibit numerous channels as a result of repeated extrusion of fluid or gel from inner zones to the periphery of amygdules that were compressed under the burden of new flows. Previously, such channels were interpreted to be feeding channels for silica supply in amygdules. Periodic compression of amygdules after percolation of fluid from them requires no additional supply of silica because the volume of the amygdules is reduced in proportion to the loss of fluid. The concentric and horizontal banding and mossy textures of agates from the lithophysae of felsic volcanic rocks were created during active volcanism as well. The agates from dissolution-induced cavities in carbonate rocks and the famous amethyst druses of Brazil and Uruguay formed at the moderate temperatures associated with low-grade burial metamorphism, as indicated by the lack of moss textures and onyx banding.
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玛瑙和紫水晶晶洞的起源
实际上,玛瑙起源的各个方面都引发了争论。澄清关于玛瑙形成环境以及巴西和乌拉圭相关著名紫水晶地球仪的最重要谜团的时机已经成熟。玛瑙形成的温度范围很广,从玄武岩和安山岩熔体的温度(约1100°C)到约50°C,压力也很低。它们在液态镁铁质岩浆中的形成由(1)颗粒的取向和其中的玛瑙带的倾斜与(2)熔岩流层中颗粒的姿态之间的相关性来指示。这种相关性的产生是因为熔岩在靠近和远离流动的上下边缘时以不同的速度移动。碱性超临界流体填充熔岩中的气泡,主要溶解周围熔岩或岩石中的二氧化硅,从而产生硅溶胶。如果流体上的压力导致淀粉粒中的水渗透,则溶胶在囊泡壁上凝结,形成同心内衬。如果淀粉粒中的压力低于溶胶的最大渗透压(硅溶胶约为0.1MPa),则流体的渗透停止,凝结导致水平玛瑙带的形成。不同凝胶层的多次重复沉淀可能是由冷却的老玛瑙熔岩流上重叠的新鲜流引起的。在潜艇环境中,流体的相分离以及蒸汽(或稀释溶液)和盐水之间凝胶膜的形成刺激了渗透过程,从而导致中空膜管的生长和淀粉底部的苔藓状分支阵列。由于流体或凝胶从内部区域反复挤压到在新流的负载下被压缩的淀粉粒的外围,一些玛瑙表现出许多通道。以前,这种通道被解释为淀粉粒中二氧化硅供应的供给通道。在流体从颗粒中渗透出来之后,颗粒的周期性压缩不需要额外的二氧化硅供应,因为颗粒的体积与流体的损失成比例地减少。长英质火山岩岩相中玛瑙的同心、水平条纹和苔藓结构也是在活跃的火山活动中形成的。碳酸盐岩中溶解引起的洞穴中的玛瑙,以及巴西和乌拉圭著名的紫水晶核果,是在与低级埋藏变质作用相关的中等温度下形成的,这表明缺乏苔藓纹理和玛瑙带。
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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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