The formation of lithium-rich pegmatites through multi-stage melting

IF 4.8 1区 地球科学 Q1 GEOLOGY Geology Pub Date : 2023-10-17 DOI:10.1130/g51633.1
Lot Koopmans, Tania Martins, Robert Linnen, Nicholas J. Gardiner, Catriona M. Breasley, Richard M. Palin, Lee A. Groat, David Silva, Laurence J. Robb
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Abstract

Lithium-cesium-tantalum−type pegmatites (the primary source of lithium) crystallize from highly evolved, volatile felsic melts that incorporated crustal material in their source. Pegmatites are classically thought to form either from extreme fractionation of a parental granite body or via low-degree partial melting of a metamorphic rock (anatectic origin). However, the processes that lead to the formation of economic lithium pegmatite deposits remain enigmatic, because precipitation of lithium ore minerals requires melt lithium concentrations in excess of 5000 ppm—∼500 times upper crustal abundances. We use petrological modeling to quantify lithium enrichment in an anatectic-origin scenario and show that it is primarily driven by the relative stability of residual biotite and muscovite at medium to high pressures (∼8 kbar), and biotite and cordierite at low pressures (∼3 kbar). We show anatexis of an average lithium-enriched metasedimentary source cannot sufficiently elevate the lithium content of the ensuing melt to form economic deposits; however, if this first-generation melt—now crystallized as granitic crust—is re-melted, the second-generation melt will be sufficiently concentrated in lithium to crystallize lithium ore minerals. We propose a petrogenetic model for anatectic-origin lithium pegmatites, in which a region experiences at least two stages of partial melting, ultimately generating lithium-rich melts without invoking extensive fractional crystallization. This mechanism can both account for the occurrence of unzoned lithium pegmatites and explain why economic pegmatites in many terranes are younger than their inferred source granites.
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富锂伟晶岩多阶段熔融形成
锂-铯-钽-型伟晶岩(锂的主要来源)是由高度演化、易挥发的长硅熔体结晶而成,熔体中含有地壳物质。伟晶岩通常被认为是由母花岗岩体的极端分馏形成的,或者是由变质岩的低程度部分熔融形成的。然而,导致经济锂伟晶岩矿床形成的过程仍然是个谜,因为锂矿石矿物的沉淀需要熔融锂浓度超过5000 ppm -上地壳丰度的500倍。研究人员利用岩石学模型量化了碳酸盐岩起源情景下的锂富集,并表明其主要是由残余黑云母和白云母在中高压(~ 8 kbar)和残余黑云母和堇青石在低压(~ 3 kbar)下的相对稳定性驱动的。研究表明,一般富锂变质沉积岩源的深熔不能充分提高随后熔体的锂含量以形成经济矿床;然而,如果第一代熔体(现在结晶为花岗岩外壳)再次熔化,第二代熔体将充分集中在锂中,使锂矿石矿物结晶。我们提出了一种成岩模型,在这种模型中,一个区域至少经历了两个阶段的部分熔融,最终产生了富锂熔体,而不需要广泛的分离结晶。这一机制既可以解释无分带锂伟晶岩的出现,也可以解释为什么许多地体中的经济伟晶岩比推断的来源花岗岩更年轻。
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来源期刊
Geology
Geology 地学-地质学
CiteScore
10.00
自引率
3.40%
发文量
228
审稿时长
6.2 months
期刊介绍: Published since 1973, Geology features rapid publication of about 23 refereed short (four-page) papers each month. Articles cover all earth-science disciplines and include new investigations and provocative topics. Professional geologists and university-level students in the earth sciences use this widely read journal to keep up with scientific research trends. The online forum section facilitates author-reader dialog. Includes color and occasional large-format illustrations on oversized loose inserts.
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