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Diffusive fractionation of noble gases and helium isotopes during mantle melting

机译:地幔融化过程中稀有气体和氦同位素的扩散分级

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The large differences in He and Ar diffusivities in silicate minerals could result in fractionation of the He/Ar ratio during melting of the mantle, producing He/Ar ratios in the primary mantle melts that are higher than those of the bulk mantle. Modeling noble gas diffusion out of the bulk mantle into fast diffusion pathways (such as fractures or melt channels) suggests that significant (order of magnitude) He/Ar fractionation will occur if the fast diffusion channels are spaced several meters apart and the noble gas residence in these diffusion channels is of the order days to weeks. In addition, the 15% difference in ~3He and ~4He diffusivities could also produce isotopic fractionation between the melt and its solid source. Modeling the behavior of He and Ar during melting shows that small increases (few %) in ~3He/~4He should be correlated with larger variations (factor of 5) in ~4He/~(40)Ar. However, in order to test this hypothesis the effects of subsequent He–Ar fractionation that occur during degassing have to be corrected. I describe a scheme that can separate He/Ar variations in the primary melt from overprinted fractionation during magmatic degassing. Using the degassing-corrected data, there is a correlation between the primary melt's ~4He/~(40)Ar and ~3He/~4He in mid-ocean ridge basalts (MORBs). The slope of the correlation is consistent with the models of preferential diffusion of ~3He relative to ~4He and of ~4He relative to ~(40)Ar from the solid mantle into the melt. Diffusive fractionation of noble gases during melting of the mantle can also account for low ~4He/(40)Ar ratios commonly found in residual mantle xenoliths: preferential diffusion of He relative to Ar will produce some regions of the mantle with low ~4He/~(40)Ar, the complement of the high 4He/40Ar ratios in basalts. Diffusive fractionation cannot, however, account for differences between the He and Ne isotopic compositions of MORBs compared with ocean island basalts (OIBs); not only are the extremely high ~3He/~4He ratios of OIBs (up to 50 Ra) difficult to produce at reasonable mantle time and lengthscales, but also the Ne isotopic compositions of MORBs and OIBs do not lie on a single mass fractionation line, therefore cannot result from diffusive fractionation of a single mantle Ne source. If preferential diffusion of He from the solid mantle into primary melts is a significant process during generation of MORBs, then it is difficult to constrain the He concentration of the mantle: He concentrations in basalts and the He flux to the ocean essentially result from extraction of He from a larger (and unknown) volume of mantle than that that produced the basalts themselves. The He concentration of the mantle cannot be constrained until more accurate estimates of the diffusion contribution are available.
机译:硅酸盐矿物中He和Ar扩散率的巨大差异可能会导致地幔融化过程中He / Ar比的分馏,从而使主要地幔熔体中的He / Ar比值高于散装地幔。对稀有气体从散装地幔中扩散到快速扩散通道(例如裂缝或熔体通道)中的模型表明,如果快速扩散通道间隔数米并且稀有气体滞留,则会发生显着(数量级)的He / Ar分馏在这些扩散通道中,数天至数周。此外,〜3He和〜4He扩散率的15%差异也可能在熔体及其固体源之间产生同位素分馏。对He和Ar在熔化过程中的行为进行建模表明,〜3He /〜4He中的少量增加(几%)应与〜4He /〜(40)Ar中的较大变化(5的因数)相关。但是,为了检验该假设,必须纠正脱气过程中随后发生的He-Ar分级分离的影响。我描述了一种方案,该方案可以在岩浆脱气过程中将主熔体中的He / Ar变化与叠印分馏分开。使用经脱气校正的数据,洋中脊玄武岩(MORBs)的初熔体〜4He /〜(40)Ar和〜3He /〜4He之间存在相关性。相关的斜率与〜3He相对于〜4He优先扩散和〜4He相对于〜(40)Ar从固态地幔到熔体的优先扩散模型一致。地幔融化过程中稀有气体的扩散分馏也可以解释残留地幔异种岩中常见的〜4He /(40)Ar比低:He相对于Ar的优先扩散将产生约〜4He /〜低的地幔区域(40)Ar,是玄武岩中高4He / 40Ar比的补充。然而,与海洋岛屿玄武岩(OIBs)相比,扩散分级不能解释MORBs的He和Ne同位素组成之间的差异。不仅难以在合理的地幔时间和长度尺度上产生极高的OIBs〜3He /〜4He比(高达50 Ra),而且MORBs和OIBs的Ne同位素组成也不位于单一的质量分馏线上,因此不能由单个幔源Ne的扩散分级产生。如果在MORB生成过程中将He从固态地幔优先扩散到初级熔体中是一个重要的过程,那么很难限制He地幔中的He浓度:玄武岩中He的浓度以及进入海洋的He流量主要是由于提取了他来自地幔的体积更大(且未知)比产生玄武岩本身的体积大。在获得更准确的扩散贡献估计之前,不能限制地幔中的He浓度。

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