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H2O content of deep-seated orogenic continental crust: the Ulten Zone, Italian Alps

机译:深层造山带地壳中H 2 O含量:意大利阿尔卑斯山的Ulten带

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To estimate the amount of H2O stored at lower crustal levels after burial, we considered the pile of migmatitic paragneisses in the Variscan Ulten Zone as a case study area. We constructed a pseudosection in the system K2O-Na2O-CaO-FeO-MnO-MgO-Al2O3-SiO2-TiO2-H2O for an average paragneiss, a relevant prograde PT path (8.5 kbar, 600°C; 11.5 kbar, 750°C; 14.0 kbar, 1000°C) and H2O contents between 0 and 10 wt.%. Based on an assemblage of garnet + biotite + white mica + kyanite + 20-30 vol.% former melt (now represented mainly by leucosomes composed of plagioclase + quartz), a bulk H2O content of 3.2 ± 1.1 wt.% was estimated for a peak temperature ranging between 770 and 800°C. Before melting, somewhat less than 1.8 wt.% H2O was stored in minerals. Thus, a considerable amount of H2O must have either resided in pore spaces along grain boundaries or, much less likely, infiltrated the paragneisses from below. Evidently, significant quantities of H2O as a free phase may be stored in buried sialic crust, resulting in considerable melting of deep-seated rocks during continent-continent collision.View full textDownload full textKeywordsmigmatites, continent - continent collision, high pressure, phase equilibria, water, lower crust, Ulten ZoneRelated var addthis_config = { ui_cobrand: "Taylor & Francis Online", services_compact: "citeulike,netvibes,twitter,technorati,delicious,linkedin,facebook,stumbleupon,digg,google,more", pubid: "ra-4dff56cd6bb1830b" }; Add to shortlist Link Permalink http://dx.doi.org/10.1080/00206814.2010.548155
机译:为了估计埋藏后处于较低地壳水平的H 2 O的量,我们将瓦里斯坎Ulten带中的大量玛格达尼干酪作为​​案例研究区域。我们在系统K 2 O-Na 2 O-CaO-FeO-MnO-MgO-Al 2 O 中构造了一个伪截面3 -SiO 2 -TiO 2 -H 2 O表示平均帕拉尼萨斯,相关的PT路径(8.5 kbar, 600°C; 11.5 kbar,750°C; 14.0 kbar,1000°C)和H 2 O含量在0至10 wt。%之间。基于石榴石+黑云母+白云母+蓝晶石+ 20-30 vol。%的前熔体组成的组合物(现在主要由隐含的脂质体组成斜长石(+斜纹石英),3.2±1.1 wt。%的散装H <2> O含量估计为770至800°C的峰值温度。在熔化之前,矿物质中储存了略少于1.8 wt。%的H 2 O。因此,必须有大量的H 2 O沿晶界存在于孔隙中,或者不太可能从下方渗透到核仁石中。显然,大量的H 2 O作为自由相可能被储存在地下唾液中,导致大陆与大陆碰撞时深层岩石大量熔化。查看全文下载全文关键字大陆大陆相撞,高压,相平衡,水,下地壳,乌尔滕带google,more“,发布号:” ra-4dff56cd6bb1830b“};添加到候选列表链接永久链接http://dx.doi.org/10.1080/00206814.2010.548155

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