Plume-ridge interaction along the Galapagos Spreading Center: discerning between gas loss and source effects using neon isotopic compositions and He-Ar-CO₂ relative abundances     

A. Colin  P.G. Burnard  Y. Marrocchi 《Geochimica et cosmochimica acta》2011,75(4):1145-1160

To document the plume-ridge interaction at the Galapagos Spreading Center (GSC), we present neon 3-isotope analyses performed on vesicles-trapped volatiles of MORB glasses dredged along the ridge axis between 86°W and 98°W. ⁴He-⁴⁰Ar^∗-CO₂ relative abundances were also measured in order to study gas loss in this context and discern between source and degassing effects. Neon isotopic compositions are in the MORB range with ²¹Ne/²²Ne ratios extrapolated to the ²⁰Ne/²²Ne mantle ratio of 12.5 varying between 0.053 and 0.072. Unradiogenic plume-like compositions were not measured. The ⁴He-⁴⁰Ar^∗-CO₂ relative abundances are highly variable along the ridge, for example ⁴He/⁴⁰Ar^∗ ratio varies between 3 and 433, but these variations can be fully explained by a simple model of Rayleigh distillation, with a single volatile source composition for the entire GSC. Magma fractional crystallisation, which increases in the plume influenced zone, seems to be the main motor for degassing. As other geochemical and geophysical studies indicate a significant plume influence on the GSC, these results suggest the plume component feeding the ridge is either degassed or else different from the plume core.  相似文献   

Noble gas evidence for two fluids in the Baca (Valles Caldera) geothermal reservoir     

S.P. Smith  B.M. Kennedy 《Geochimica et cosmochimica acta》1985,49(4):893-902

Noble gas elemental and isotopic abundances were measured in steam from four wells in the Baca geothermal reservoir located in the Valles Caldera, New Mexico. The ${}^{40}\text{Ar}{}^{36}\text{Ar}$ ratio and noble gas elemental abundances relative to ³⁶Ar are all strongly correlated with 1/³⁶Ar, the inverse of the argon content. Ratios of (α,n)-produced ²¹Ne1 and radiogenic ⁴⁰Ar1 to total ⁴He (dominantly radiogenic) are nearly constant at 2.1 × 10?8 and 0.20, respectively. The ${}^3\text{He}{}^4\text{He}$ ratio covers a restricted range of 3.9 to 4.8 times atmospheric. The high ³He content of the gas indicates the presence of a helium component ultimately derived from the mantle. Kr and Xe isotopic compositions are close to atmospheric; excess ¹²⁹Xe1 is <0.25% of the total ¹²⁹Xe.The high degree of linear correlation among the various noble gas results strongly suggests that the Baca reservoir contains two distinct fluids that are produced in varying proportions from individual wells. The noble gases in fluid A (~2900 mg/1 C1) are air-like, but with lighter gases and isotopes preferentially enriched. The fluid A ³⁶Ar content is low, only 13% that of 10°C air-saturated water (ASW). The second fluid, B (~ 1700 mg/1 C1), is the dominant carrier of the radiogenic and mantle-derived gases. The heavier non-radiogenic gases are preferentially enriched in fluid B, and its ³⁶Ar content is very low, only 5–7% ASW. The source of the noble gases in fluid A is tentatively ascribed to leaching of the relatively young (<1.4 m.y.) volcanic Bandelier Tuff. The radiogenic gases and mantle-derived helium in fluid B suggest a deeper source, possibly including gases escaping from a magma.  相似文献   

Improving noble gas based paleoclimate reconstruction and groundwater dating using Ne/Ne ratios     

Frank Peeters  Urs Beyerle  Johannes Holocher  Rolf Kipfer 《Geochimica et cosmochimica acta》2003,67(4):587-600

The interpretation of noble gas concentrations in groundwater with respect to recharge temperature and fractionated excess gas leads to different results on paleo-climatic conditions and on residence times depending on the choice of the gas partitioning model. Two fractionation models for the gas excess are in use, one assuming partial re-equilibration of groundwater supersaturated by excess air (PR-model, Stute et al., 1995), the other assuming closed-system equilibration of groundwater with entrapped air (CE-model, Aeschbach-Hertig et al., 2000). In the example of the Continental Terminal aquifers in Niger, PR- and CE- model are both consistent with the data on elemental noble gas concentrations (Ne, Ar, Kr, and Xe). Only by including the isotope ratio ²⁰Ne/²²Ne it can be demonstrated that the PR-model has to be rejected and the CE-model should be applied to the data. In dating applications ³He of atmospheric origin (³He_atm) required to calculate ³H-³He water ages is commonly estimated from the Ne excess presuming that gas excess is unfractionated air (UA-model). Including in addition to the Ne concentration the ²⁰Ne/²²Ne ratio and the concentration of Ar enables a rigorous distinction between PR-, CE- and UA-model and a reliable determination of ³He_atm and of ³H-³He water ages.  相似文献   

Noble gas study of HIMU and EM ocean island basalts in the Polynesian region     

《Geochimica et cosmochimica acta》1999,63(7-8):1181-1201

Noble gas isotopes of HIMU and EM ocean island basalts from the Cook-Austral and Society Islands were investigated to constrain their origins. Separated olivine and clinopyroxene (cpx) phenocrysts were used for noble gas analyses. Since samples are relatively old, obtained from the oceanic area and showing chemical zoning in cpx phenocrysts, several tests on sample preparation and gas extraction methods were performed. First, by comparing heating and crushing methods, it has been confirmed that the crushing method is suitable to obtain inherent magmatic noble gases without radiogenic and cosmogenic components which were yielded after eruption, especially for He and Ne analyses. Second, noble gas compositions in the core and the rim of cpx phenocrysts were measured to evaluate the zoning effect on noble gases. The result has been that noble gas concentrations and He and Ne isotope ratios are different between them. The enrichment of noble gases in the rim compared to the core is probably due to fractional crystallization. Difference of He and Ne isotope ratios is explained by cosmogenic effect, and isotope ratios of the trapped component seem to be similar between the rim and the core. Third, leaching test reveals no systematic differences in noble gas compositions between leached and unleached samples.³He/⁴He ratios of HIMU samples in the Cook-Austral Islands are uniform irrespective of phenocryst type (olivine and cpx) and age of samples (10–18 Ma), and lower (average 6.8 R_A) than those of the Pacific MORB. On the other hand, ³He/⁴He of EM samples in the Cook-Austral Islands are similar to MORB values. EM samples in the Society Islands show rather higher ³He/⁴He than MORB. Ne, Kr and Xe isotope ratios are almost atmospheric within analytical uncertainties. ⁴⁰Ar/³⁶Ar are not so high as those of MORB. Anomalous noble gas abundance pattern such as He and Ne depletion and Kr and Xe enrichment relative to atmospheric abundances was observed. Furthermore, Ne/Ar and Kr/Ar show correlation with some trace elemental ratios like La/Yb.Lower ³He/⁴He of HIMU than MORB values requires relatively high time-integrated (U + Th)/³He for the HIMU source, which suggests that the HIMU source was produced from recycled materials which had been once located near the Earth’s surface. Moreover, extreme noble gas abundance pattern and strong correlation of Ne/Ar and Kr/Ar with La/Yb indicate that the HIMU endmember is highly depleted in light noble gases and enriched in heavy noble gases. Such feature is not common to mantle materials and is rather similar to the noble gas abundance patterns of the old oceanic crust and sediment, which supports the model that the HIMU source originates from subducted oceanic crust and/or sediment.If the HIMU source corresponds to the oceanic crust which subducted at 1–2 Ga as suggested by Pb isotope studies, however, the characteristic ³He/⁴He of HIMU (6.8 R_A) would be too high because radiogenic ⁴He produced by U and Th decay should dramatically decrease ³He/⁴He. To overcome this problem, the He open system model is introduced which includes the effects of ⁴He production and diffusion between the HIMU source material and the surrounding mantle. This model favors that the HIMU source resides in the upper mantle, rather than in the lower mantle. Furthermore, this model predicts the thickness of the HIMU source to be in the order of 1 km.In contrast to low and uniform ³He/⁴He character of HIMU, ³He/⁴He of EM are rather variable. Entrainment of upper mantle material and/or a less-degassed component are required to explain the observed ³He/⁴He of EM in the Polynesian area. Participation of the less-degassed component would be related to the “superplume” below the Polynesian region.  相似文献   

稀有气体在深部地质研究中的意义   总被引：4，自引：0，他引：4  

汤华云  郑建平 《世界地质》2004,23(1):20-27

幔源物质中的稀有气体蕴藏着丰富的地球深部过程信息。它们可对地幔结构、地幔脱气历史、大陆地幔不均一性、幔源岩浆演化和CO2天然气成因等研究提供独特的示踪作用。结合中国东部地幔捕虏体的资料,综述了稀有气体在这些方面的研究进展。研究表明,MORB源和OIB源玄武岩稀有气体组成差异强烈支持地幔双层结构的存在,地幔脱气过程主要受溶解度控制脱气模式(SCD)控制;同时,中国东部地幔存在不均一性可以在稀有气体方面得到印证;郯庐断裂可能为东部幔源无机CO2的脱出提供了良好的通道。  相似文献   

Regional groundwater focusing of nitrogen and noble gases into the Hugoton-Panhandle giant gas field, USA     

Chris J. Ballentine  Barbara Sherwood Lollar 《Geochimica et cosmochimica acta》2002,66(14):2483-2497

The Hugoton-Panhandle giant gas field, located across SW Kansas and the Texas and Oklahoma panhandles in the USA, is the case type example of high nitrogen concentrations in a natural gas being linked with high helium concentrations. We collected 31 samples from producing wells in a north-south traverse of the 350-km-long field. The samples reflect the previously observed north-south change in ⁴He/N₂, with values changing from 0.020 to 0.049 respectively. ³He/⁴He, ²¹Ne/²²Ne, and ⁴⁰Ar/³⁶Ar vary between 0.14-0.25 Ra, 0.0373-0.0508, and 818-1156 respectively, and are caused by quantifiable contributions from mantle, crustal, and atmosphere-derived sources. The atmosphere-derived ²⁰Ne/³⁶Ar ratios are indistinguishable from groundwater values. The crustal ⁴He/²¹Ne* and ⁴He/⁴⁰Ar* ratios show a 60% excess of ⁴He compared to predicted production ratios in the crust and are typical of noble gases released from the shallow crust. The mantle ³He/N₂ and groundwater-recharge ³⁶Ar/N₂ ratios enable us to rule out significant magmatic or atmosphere contributions to the gas field N₂, which is dominantly crustal in origin.Correlated ²⁰Ne/N₂ and ⁴He/N₂ shows mixing between two distinct crustal N₂ components. One N₂ component (N₂*) is associated with the crustal ⁴He and groundwater-derived ²⁰Ne, and the other with no resolvable noble gas contribution. Measured δ¹⁵N_N2 values vary from +2.7‰ to +9.4‰. The N₂* and non-He-associated N₂ endmembers are inferred to have δ¹⁵N_N2 = −3‰ and +13‰ and contribute from between 25-60% and 75-40% of the nitrogen respectively. The non-He-associated nitrogen is probably derived from relatively mature organic matter in the sedimentary column. The δ¹⁵N_N2* value is not compatible with a crystalline or high-grade metamorphic source and, similar to the ⁴He, is inferred to be from a shallow or low metamorphic-grade source rock. ⁴He mass balance requires a regional crustal source, its association with significant magmatic ³He pointing to a tectonically active source to the west of the Hugoton system. The volume of groundwater required to source the ²⁰Ne in the gas field demonstrates the viability of the groundwater system in providing the collection, transport, and focusing mechanism for the ⁴He and N₂*. The N₂*/²⁰Ne ratio shows that the N₂* transport must be in the aqueous phase, and that the degassing mechanism is probably contact between the regional groundwater system and the preexisting reservoir hydrocarbon gas phase.  相似文献   

稀有气体同位素地球化学在矿床学研究中的应用进展     

武丽艳 《岩石学报》2019,35(1):215-232

稀有气体因其化学惰性以及在不同来源地质体中的同位素组成差异很大,在研究成矿流体来源、演化和壳-幔相互作用过程中具有非常重要的意义。另外,由于~4He、⁴⁰Ar是放射成因子体同位素,具有年代积累效应,因此,它们常被用于同位素测年。本文简要回顾了流体包裹体中稀有气体同位素的后生影响和样品、分析方法选择注意事项,以及近年来稀有气体同位素在成矿流体示踪,⁴⁰K-⁴⁰Ar、⁴⁰Ar-39Ar定年及(U-Th)/He定年方面的研究进展。已有研究证实流体包裹体中的稀有气体可能受后期扩散丢失、后生叠加和同位素分馏的影响,要根据目的选择不同的分析方法;稀有气体同位素可以示踪不同类型矿床的流体来源、演化及壳-幔相互作用、稀有气体同位素与卤素联合运用可以用来指示流体和盐度来源、演化过程以及矿物沉淀机制等,~3He/热的研究可以追溯流体的热源及其运移方式;流体包裹体⁴⁰Ar-³⁹Ar可以用于矿床直接定年,表生含钾矿物的⁴⁰K-⁴⁰Ar、⁴⁰Ar-³⁹Ar定年以及锆石、磷灰石和铁氧化物(U-Th)/He定年可为矿床及氧化带的形成时间、矿床形成后的抬升、剥露历史、古气候演化等重大地质问题讨论提供大量有意义的信息。  相似文献   

Noble gas and carbon isotopes in Mariana Trough basalt glasses     

《Applied Geochemistry》1998,13(4):441-449

Noble gas elemental and isotopic compositions have been measured as well as the abundance of C and its isotopic ratios in 11 glasses from submarine pillow basalts collected from the Mariana Trough. The ³He/⁴He ratios of 8.22 and 8.51 R_atm of samples dredged from the central Mariana Trough (∼18°N) agree well with that of the Mid-Ocean Ridge Basalt (MORB) glasses (8.4±0.3 R_atm), whereas a mean ratio of 8.06±0.35 R_atm in samples from the northern Mariana Trough (∼20°N) is slightly lower than those of MORB. One sample shows apparent excess of ²⁰Ne and ²¹Ne relative to atmospheric Ne, suggesting incorporation of solar-type Ne in the magma source. There is a positive correlation between ³He/⁴He and ⁴⁰Ar/³⁶Ar ratios, which may be explained by mixing between MORB-type and atmospheric noble gases. Excess ¹²⁹Xe is observed in the sample which also shows ²⁰Ne and ²¹Ne excesses. Observed δ¹³C values of ∼20°N samples vary from −3.76‰ to −2.80‰, and appear higher than those of MORB, and the corresponding CO₂/³He ratios are higher than those of MARA samples at ∼18°N, suggesting C contribution from the subducted slab.  相似文献   

Apparent decoupling of the He and Ne isotope systematics of the Icelandic mantle: The role of He depletion, melt mixing, degassing fractionation and air interaction     

Evelyn Füri  D.R. Hilton  T.P. Fischer 《Geochimica et cosmochimica acta》2010,74(11):3307-3332

We present new He-Ne data for geothermal fluids and He-Ne-Ar data for basalts from throughout the Icelandic neovolcanic zones and older parts of the Icelandic crust. Geothermal fluids, subglacial glasses, and mafic phenocrysts are characterized by a wide range in helium isotope ratios (³He/⁴He) encompassing typical MORB-like ratios through values as high as 36.8 R_A (where R_A = air ³He/⁴He). Although neon in geothermal fluids is dominated by an atmospheric component, samples from the northwest peninsula show a small excess of nucleogenic ²¹Ne, likely produced in-situ and released to circulating fluids. In contrast, geothermal fluids from the neovolcanic zones show evidence of a contribution of mantle-derived neon, as indicated by ²⁰Ne enrichments up to 3% compared to air. The neon isotope composition of subglacial glasses reveals that mantle neon is derived from both depleted MORB-mantle and a primordial, ‘solar’ mantle component. However, binary mixing between these two endmembers can account for the He-Ne isotope characteristics of the basalts only if the ³He/²²Ne ratio of the primordial mantle endmember is lower than in the MORB component. Indeed, the helium to neon elemental ratios (⁴He/²¹Ne∗ and ³He/²²Ne_s where ²¹Ne∗ = nucleogenic ²¹Ne and ²²Ne_s = ‘solar’-derived ²²Ne) of the majority of Icelandic subglacial glasses are lower than theoretical values for Earth’s mantle, as observed previously for other OIB samples. Helium may be depleted relative to neon in high-³He/⁴He ratio parental melts due to either more compatible behavior during low-degree partial melting or more extensive diffusive loss relative to the heavier noble gases. However, Icelandic glasses show higher ⁴He/⁴⁰Ar∗ (⁴⁰Ar∗ = radiogenic Ar) values for a given ⁴He/²¹Ne∗ value compared to the majority of other OIB samples: this observation is consistent with extensive open-system equilibrium degassing, likely promoted by lower confining pressures during subglacial eruptions of Icelandic lavas. Taken together, the He-Ne-Ar systematics of Icelandic subglacial glasses are imprinted with the overlapping effects of helium depletion in the high-³He/⁴He ratio parental melt, binary mixing of two distinct mantle components, degassing fractionation and interaction with atmospheric noble gases. However, it is still possible to discern differences in the noble gas characteristics of the Icelandic mantle source beneath the neovolcanic zones, with MORB-like He-Ne isotope features prevalent in the Northern Rift Zone and a sharp transition to more primitive ‘solar-like’ characteristics in central and southern Iceland.  相似文献   

Noble gas tracing of groundwater/coalbed methane interaction in the San Juan Basin, USA   总被引：1，自引：0，他引：1  

Zheng Zhou  Chris J. Ballentine  Martin Schoell 《Geochimica et cosmochimica acta》2005,69(23):5413-5428

The San Juan Basin natural gas field, located in northwestern New Mexico and southwestern Colorado in the USA, is a case-type coalbed methane system. Groundwater is thought to play a key role in both biogenic methane generation and the CO₂ sequestration potential of coalbed systems. We show here how noble gases can be used to construct a physical model that describes the interaction between the groundwater system and the produced gas. We collected 28 gas samples from producing wells in the artesian overpressured high production region of the basin together with 8 gas samples from the underpressured low production zone as a control. Stable isotope and major species determination clearly characterize the gas in the high production region as dominantly biogenic in origin, and the underpressured low producing region as having a significant admix of thermogenic coal gas. ³He/⁴He ratios increase from 0.0836R_a at the basin margin to 0.318R_a towards the center, indicating a clear but small mantle He signature in all gases. Coherent fractionation of water-derived ²⁰Ne/³⁶Ar and crustal ⁴He/⁴⁰Ar* are explained by a simple Rayleigh fractionation model of open system groundwater degassing. Low ²⁰Ne concentrations compared to the model predicted values are accounted for by dilution of the groundwater-associated gas by desorbed coalbed methane. This Rayleigh fractionation and dilution model together with the gas production history allows us to quantify the amount of water involved in gas production at each well. The quantified water volumes in both underpressured and overpressured zones range from 1.7 × 10³ m³ to 4.2 × 10⁵ m³, with no clear distinction between over- and underpressured production zones. These results conclusively show that the volume of groundwater seen by coal does not play a role in determining the volume of methane produced by secondary biodegradation of these coalbeds. There is no requirement of continuous groundwater flow for renewing the microbes or nutrient components. We furthermore observe strong mass related isotopic fractionation of ²⁰Ne/²²Ne and ³⁸Ar/³⁶Ar isotopic ratios. This can be explained by a noble gas concentration gradient in the groundwater during gas production, which causes diffusive partial re-equilibration of the noble gas isotopes. It is important for the study of other systems in which extensive groundwater degassing may have occurred to recognize that severe isotopic fractionation of air-derived noble gases can occur when such concentration gradients are established during gas production. Excess air-derived Xe and Kr in our samples are shown to be related to the diluting coalbed methane and can only be accounted for if Xe and Kr are preferentially and volumetrically trapped within the coal matrix and released during biodegradation to form CH₄.  相似文献   

The origin of rare gases on Earth: The noble gas ‘subduction barrier’ revisited     

《Comptes Rendus Geoscience》2007,339(14-15):937-945

The origin of the Earth's atmosphere can be constrained by the study of noble gases in oceanic basalts. If it is clear that the mantle is degassed and formed part of the present atmosphere, it has been proposed that an important subduction of atmospheric noble gases in the mantle occurred during Earth's history, altering the primordial signature of the solid Earth. This subduction process has been suggested on the basis of the measurements of light xenon isotopes in CO₂ well gases. Moreover, the fact that the ³⁸Ar/³⁶Ar ratio is atmospheric in all oceanic basalts, even for uncontaminated samples (e.g. with high ²⁰Ne/²²Ne), may also suggest that a massive subduction of atmospheric argon occurred, if the primitive Earth had a solar-like ³⁸Ar/³⁶Ar. This also implies that the atmosphere suffered a massive gas loss accompanied by mass fractionation (e.g. hydrodynamic escape) after mantle degassing or that a late veneer with an atmospheric composition occurred. Such a hypothesis is explored for rare gases, by developing a model in which degassing and subduction of atmospheric noble gases started ∼4.4 Ga ago. In the model, both radiogenic and non-radiogenic isotopic ratios are used (e.g. ³⁸Ar/³⁶Ar and ⁴⁰Ar/³⁶Ar; ¹²⁴Xe/¹³⁰Xe and ¹²⁹Xe/¹³⁰Xe) to constrain the subduction flux and the degassing parameters. It is shown that subduction and massive contamination of the entire mantle is possible, but implies that the ⁴⁰Ar/³⁶Ar and the ¹²⁹Xe/¹³⁰Xe ratios were higher in the past than today, which is not observed in Archean samples. It also implies that the sediments and the altered oceanic crust did not loose their noble gases during subduction or that the contaminated mantle wedge is mixed by the convective mantle. Moreover, such a model has to apply to the oceanic island source, since this later shows the same signature of argon and xenon non-radiogenic isotopic ratios. A scenario where the isotopic compositions of the argon and xenon were settled before or during accretion is therefore preferred to the subduction.  相似文献   

Primary and secondary processes constraining the noble gas isotopic signatures of carbonatites and silicate rocks from Brava Island: evidence for a lower mantle origin of the Cape Verde plume     

Cyntia Mourão  Manuel Moreira  João Mata  Aude Raquin  José Madeira 《Contributions to Mineralogy and Petrology》2012,163(6):995-1009

We present and discuss noble gas compositions of minerals from silicate rocks (olivines) and carbonatites (apatites and calcites) from Brava Island. The presence of an almost ubiquitous atmosphere-derived fingerprint is explained as reflecting contamination by seawater. Because of the high U and Th content in apatites, which are responsible for ⁴He production by α-decay, the high measured ⁴He/³He ratios do not represent magmatic signatures. In contrast, low values of ⁴He/³He in calcites (≥61,223; R/R _a ≤ 11.80) and olivines (≥56,240; R/R _a ≤ 12.85) are considered to be representative of signatures trapped at the time of crystallization, given that there are no evidences for significant cosmogenic additions. These relatively low ⁴He/³He ratios depicted by silicate and carbonatite rocks imply the contribution of a reservoir that evolved under low (U + Th)/³He; this is considered a strong evidence for the genesis of Brava by a mantle plume deeply anchored in the lower mantle. The inferred low ⁴He/⁴⁰Ar* ratio (≈0.3), before degassing, is thought to reflect the contribution to the carbonatites source of a mantle domain evolving under high K/U, which cannot be explained by recycling of crustal components. The possible link between the low ⁴He/⁴⁰Ar* source and the “missing Ar reservoir” is discussed. The usually referred geochemical dichotomy between Northern and Southern Cape Verde islands, which is markedly evident from Sr, Nd, and Pb isotope signatures, is not apparent from Brava Island (Southern Cape Verde), where some samples present relatively unradiogenic ⁴He/³He signatures, similar to those reported for the Northern islands of the archipelago.  相似文献   

Vesiculation and vesicle loss in mid-ocean ridge basalt glasses: He, Ne, Ar elemental fractionation and pressure influence     

Philippe Sarda  Manuel Moreira 《Geochimica et cosmochimica acta》2002,66(8):1449-1458

Sarda and Graham (1990) proposed that in mid-ocean ridge basalts (MORBs), degassing occurs through equilibrium vesiculation followed by various extents of vesicle loss. This model predicts that in a bulk sample of MORB glass with vesicles, the rare gases represent a binary mixture between a vesicle component and a component dissolved in the melt. As vesiculation is expected to produce very different rare gas concentrations and elemental ratios in gas and melt, binary mixing systematics should be recorded in the MORB rare gas abundance data. Indeed, a large range of ⁴He/⁴⁰Ar∗ ratios was known to exist, but these binary mixing systematics remained elusive because helium was used as a proxy for rare gas abundance because helium is not affected by air addition. Here we show that using Ar instead of He, the ⁴He/⁴⁰Ar∗ ratio is higher where the Ar concentration is lower, as expected from simple binary mixing systematics.Taking advantage of the growing Ne database, we further show that the predicted binary mixing is recorded by the He-Ar and He-Ne couples, provided He concentration is not used to trace vesicle abundance. This is because a significant part of helium remains in the melt due to its higher solubility. In contrast, Ar or Ne concentrations, which can both be corrected for air addition, clearly trace vesicles and yield binary mixing patterns that hold for ridges worldwide. The model of vesiculation and vesicle loss thereby finds geochemical support in the rare gas abundance data.The He-Ne-Ar concentration data is best explained by assuming the ratio of helium to neon or argon solubility is about 5 to 15 times higher than values measured in 1 bar laboratory experiments, due to higher He and lower Ne and Ar solubilities. We propose that this is a pressure effect, and vesiculation mainly occurs during magma ascent in the mantle after melting.  相似文献   

Intensive sampling of noble gases in fluids at Yellowstone: I. Early overview of the data; regional patterns     

B.M. Kennedy  M.A. Lynch  J.H. Reynolds  S.P. Smith 《Geochimica et cosmochimica acta》1985,49(5):1251-1261

The Roving Automated Rare Gas Analysis (RARGA) lab of Berkeley's Physics Department was deployed in Yellowstone National Park for a 19 week period commencing in June, 1983. During this time 66 gas and water samples representing 19 different regions of hydrothermal activity within and around the Yellowstone caldera were analyzed on site. Routinely, the abundances of five stable noble gases and the isotopic compositions of He, Ne, and Ar were determined for each sample. In a few cases the isotopes of Kr and Xe were also determined and found to be of normal atmospheric constitution.Correlated variations in the isotopic compositions of He and Ar can be explained within the precision of the measurements by mixing of only three distinct components. The first component is of magmatic origin and is enriched in the primordial isotope ³He with ${}^3\text{He}{}^4\text{He}\text{≥ 16}$ times the air value. This component also contains radiogenic ⁴⁰Ar and possible ³⁶Ar with ${}^{40}\text{Ar}{}^{36}\text{Ar}\text{≥ 500}$, resulting in a ${}^3\text{He}{}^{36}\text{Ar}$ ratio ≥ 41,000 times the air value. The second component is assumed to be purely radiogenic ⁴He and ⁴⁰Ar (${}^{41}\text{He}{}^{401}\text{Ar}\text{= 4.08 ± .33}$). This component is the probable carrier of observed excesses of ²¹¹Ne, attributed to the α,n reaction on ¹⁸O. Its radiogenic character implies a crustal origin in U. Th, and Krich aquifer rocks. The third component, except for possible mass fractionation, is isotopically indistinguishable from the noble gases in the atmosphere. This component originates largely from infiltrating run-off water saturated with atmospheric gases.In addition to exhibiting nucleogenic ²¹¹Ne, Ne data show anomalies in the ratio ${}^{20}\text{Ne}{}^{20}\text{Ne}$, which correlate roughly with the ${}^{21}\text{Ne}{}^{22}\text{Ne}$ anomalies for the most part, but not as would occur from simple mass fractionation. Some exaggerated instances of the ${}^{20}\text{Ne}{}^{22}\text{Ne}$ anomaly occur which could be explained by combined mass fractionation of Ne and Ar isotopes to a severe degree coupled with remixing with normally isotopic gases. Otherwise exotic processes have to be invoked to explain the ²⁰Ne data.Relative abundances of the non-radiogenic and non-nucleogenic noble gases (²²Ne, ³⁶Ar, ⁸⁴Kr, and ¹³²Xe) are highly variable but strongly correlated. High Xe/Ar ratios are always accompanied by low Ne/ Ar ratios and vice versa. Except for water from the few cold (T < 20°C) springs analyzed, none of the samples have relative abundances consistent with air saturated water and the observed variations are not readily explained by the distillation of air saturated water.In characterizing each area of hydrothermal activity by the highest ${}^3\text{He}{}^4\text{He}$ ratio found for that area, we find that within the caldera this parameter is somewhat uniform at ~7 ± 1 times the air value. There are exceptions, most notably at Mud Volcano, an area located along a crest of recent and rapid uplift. Here the maximum ${}^3\text{He}{}^4\text{He}$ ratio is ~ 16 times the air value. Also noteworthy is Gibbon Basin which is in the vicinity of the most recent rhyolitic volcanism and exhibits a ${}^3\text{He}{}^4\text{He}$ ratio ~ 13 times the air value. Immediately outside the caldera the maximum $\text{sol}{}^3\text{He}{}^4\text{He}$ ratio decreases rapidly to values < ~3 times the air value.  相似文献   

Fluid inclusion noble gas and halogen evidence on the origin of Cu-Porphyry mineralising fluids     

《Geochimica et cosmochimica acta》2001,65(16):2651-2668

The naturally occurring noble gas isotopes (⁴⁰Ar, ³⁶Ar, ⁸⁴Kr and ¹²⁹Xe) and halogens (Cl, Br, I) have been determined simultaneously in irradiated quartz vein samples by noble gas mass spectrometry. Quartz vein samples were collected from the potassic and propylitic alteration zones of six porphyry copper deposits (PCD): Bingham Canyon, Utah; and Silverbell, Ray, Mission, Pinto Valley and Globe-Miami in Arizona. In addition, analyses of ³He/⁴He have been obtained from sulphide minerals hosted by the quartz veins at Silverbell, Ray, Pinto Valley and Globe-Miami.The majority of PCD fluids studied have Br/Cl and I/Cl ratios that overlap those of fluids included in mantle diamond, suggesting that the salinity had a juvenile origin. The high I/Cl (121 × 10⁻⁶ mole, M) in samples from the propylitic zone of Silverbell is attributed to the presence of sedimentary formation water.³He/⁴He ratios have R/Ra values in the range 0.3 to 1.72, and provide evidence for the involvement of a crustal component in addition to mantle volatiles. ⁴⁰Ar/³⁶Ar ratios vary from meteoric values of ∼317 in the propylitic zone of Bingham Canyon, and 323 in the skarn alteration of Mission up to 3225 in the potassic zone of Pinto Valley. Fluids in both the potassic and propylitic alteration zones of every deposit are a mixture of a low salinity end-member comprising meteoric water and air, and a high salinity end-member consisting of a mixed mantle and crustal fluid.The ⁴⁰Ar/Cl ratio of fluid inclusions at Pinto Valley (∼10⁻⁴ M) is similar to values obtained previously for mantle fluids. The ⁴⁰Ar/Cl value is two orders of magnitude lower at Bingham Canyon, where a depleted ³⁶Ar concentration (0.2 × 10⁻⁶ cm³/g) below that of air saturated water (ASW), and a range of highly fractionated noble gas compositions (F⁸⁴Kr = 13 and F¹²⁹Xe = 160) indicate that boiling and pulsed fluid flow have occurred.  相似文献   

地幔脱气作用和大气圈惰性气体形成与演化   总被引：5，自引：0，他引：5  

朱岳年  许多  张友学 《地学前缘》1998,(Z1)

惰性气体同位素地球化学是研究地幔脱气作用和地球大气形成与演化的有效工具。根据惰性气体提供的信息,地球大气圈中惰性气体主要由地幔脱气形成。地球有三个截然不同的惰性气体储集库：ＭＯＲＢ（洋中脊玄武岩）型地幔（大量脱了气的地幔）,Ｌｏｉｈｉ（夏威夷洛尹黑海山）型地幔（少量脱了气的地幔）,和大气圈＋海洋＋大陆地壳。为了探索这三个气体储集库之间的联系,国外学者已建立了三种地幔脱气模式：①整体脱气（ＢＤ）模式,②溶解度控制脱气（ＳＣＤ）模式,和③稳定态脱气（ＳＳＤ）模式。其中ＳＣＤ模式能较好地解释各储集库中惰性气体同位素体系特征。ＳＣＤ模式认为地幔中各种气体的脱出程度和脱出历史不完全相同,主要受气体在硅酸盐熔体中的溶解度所控制,因而认为地球大气中的各种气体的演化史也不完全相同。从地球形成时算起,大气中惰性气体主要形成和演化的平均时间分别为：１３０Ｘｅ为（２１±７）Ｍａ,３６Ａｒ为（５６±１９）Ｍａ,３Ｈｅ为（３１０±１２０）Ｍａ,４０Ａｒ为１５００Ｍａ,４Ｈｅ为８００Ｍａ。  相似文献   

Rare gas isotopic composition of natural gases     

Yongchang Xu  Xianbin Wang  Renming Wu  Ping Shen  Youxiao Wang  Yongping He 《中国地球化学学报》1982,1(2):218-232

One hundred natural gas samples of different geological periods collected from various localities were determined for their nitrogen, helium and argon contents as well as the isotopic composition of argon. The ratio Ar⁴⁰/Ar³⁶ was found to be from 305 to 9,255. A current heliumargon chronological formula for calculating natural gas ages was corrected. Instead, based upon the chronological accumulating effect of radiogenic Ar⁴⁰, an Ar⁴⁰-Ar³⁹ empirical formula for calculating natural gas ages has been proposed. It can be seen from the ratio of nitrogen to atmospheric argon that most of the nitrogen in these natural gases could not be derived from atmospheric nitrogen. The range of radiogenic He/Ar⁴⁰ is from 5.19 to 23. 18, and that for most samples from 7 to 14. The He/Ar⁴⁰ ratios of Sinian samples are from 5.39 to 6.14, indicating their derivation from the deep interior of the earth. It should be noted that the Ar⁴⁰/Ar³⁶ ratio shows a general trend of approaching the atmospheric value from the Sinian to the Tertiary period, or from old to young in geological age, mirroring, to a great extent, the evolutionary tendency of the rare gas isotopic composition of natural gases with continuous degassing of the earth.  相似文献   

Refertilization of lithospheric mantle beneath the Yangtze craton in south-east China: Evidence from noble gases geochemistry     

《Gondwana Research》2016

The Yangtze craton (YC), in eastern China, is one of the oldest cratons in the world and is characterized by a complex tectonic and geodynamic evolution. This evolution regards most of the eastern China craton, which since Mesozoic time has undergone significant thinning (> 200 km) of Archean lithosphere. This thinning favored the refertilization of the old refractory subcontinental lithospheric mantle (SCLM) by the upwelling of younger fertile asthenosphere. Whether this feature is localized only beneath certain areas of eastern China or is a more widespread characteristic of the mantle, including the YC, is a matter of debate.In order to constrain the history of the YC SCLM, we have measured the He- and Ar-isotopic compositions of fluid inclusions hosted in mantle xenoliths in the Lianshan area, which is part of the poorly investigated YC in south-east China. We also report new mineral chemistry and trace element compositions of clinopyroxenes from the same suite of samples, for comparison with noble gases. Two distinct types of xenoliths can be identified: Type 1, characterized by mantle-like He-isotopic (³He/⁴He) ratios (up to 9.1 Ra), represents fragments of a fertile lithospheric mantle; Type 2, showing ³He/⁴He values in the SCLM range (³He/⁴He < 7 Ra), represents shallow relicts of a refractory mantle. The patterns of rare-earth elements as well as the Y and Yb concentrations in the clinopyroxenes normalized to primitive mantle (Y_N and Yb_N, respectively) indicate that fractional partial melting might have affected the local mantle by < 3% in Type 1 and up to 20% in Type 2 xenoliths from Lianshan, respectively. The range of ⁴He/⁴⁰Ar* (⁴⁰Ar* is corrected for atmospheric contamination) ranges from 4.9 × 10^− 4 to 3.6 × 10^− 1, which is below the typical production ratio of the mantle (⁴He/⁴⁰Ar* = 1–5); this range is however compatible with this fractional partial melting. The variable ³He/⁴He and ⁴He/⁴⁰Ar* values in Lianshan xenoliths suggest that the local mantle source was also influenced by kinetic fractionation, possibly triggered by metasomatic melts. Metasomatism associated with carbonatitic melts, together with fluxing by CO₂-rich fluids, have permeated the mantle beneath Lianshan, generating the observed decoupling between noble gases and trace elements. The interpretative framework is also applicable for other mantle xenoliths from eastern China, indicating that the refertilization of the SCLM by ascending mantle-like melts is common also to YC, which can be identified using noble gases.  相似文献   

Low solubility of He and Ar in carbonatitic liquids: Implications for decoupling noble gas and lithophile isotope systems     

Pete Burnard  Michael J. Toplis 《Geochimica et cosmochimica acta》2010,74(5):1672-236

In order to asses the importance of carbonatitic liquids in transporting noble gases in the mantle, the solubilities of He and Ar in carbonatitic liquids were estimated from analyses of calcium-potassium carbonate glasses that had been synthesized at 1 bar and temperatures between 850 and 950 °C under He or Ar enriched atmospheres. Despite poor reproducibility related to difficulties synthesizing carbonatite glass, we have been able to estimate He and Ar solubilities in carbonatite liquids to be 1 × 10⁻⁸ and 2 × 10⁻⁹ mol g⁻¹ at 1 bar respectively (with ?50% uncertainty). Despite the significant uncertainties on these estimates, it is clear that the noble gases are not massively soluble in carbonatite liquids (within error, these solubilities are identical to their equivalent solubilities in tholeiitic melts). Assuming the results of these low pressure experiments can be applied to mantle conditions, it seems unlikely that carbonatite metasomatism per se transports noble gases within the mantle. It is nevertheless possible that partitioning of lithophile trace elements (including the important radioelements, U, K and Th) and noble gases between a carbonatitic melt and a silicate melt could effectively decouple lithophile and noble gas isotope systematics because the carbonatitic melt expressedly does not transport noble gases, yet is known to efficiently transport incompatible trace elements.  相似文献   

Inert gas patterns in the regolith at the Apollo 15 landing site     

J.L. Jordan  D. Heymann  S. Lakatos 《Geochimica et cosmochimica acta》1974,38(1):65-78

He, Ne, Ar, Kr and Xe were measured mass spectrometrically in eight bulk fines and one sample of 2–4 mm fines (15603) from stations LM-ALSEP, 2, 6, 6¹, 7^a, and 9. We have also measured these gases in size fractions of samples 15091 and 15601. These samples come from three morphologically distinct selenographic settings: the Appenine Front, the Mare and Hadley Rille. Measured gas contents in these samples are comparable to those from previous Apollo missions. He⁴ and the other trapped gases are inversely proportional to grain diameter in the size fractions of 15091 and 15601. More than 90 per cent of the trapped gas in 15601 is surface correlated; hence is probably directly implanted solar wind. Size fractions of 15091 contain large volume correlated amounts of He⁴, Ne²⁰ and Ar³⁶. He⁴/Ne²⁰ ranges from about 20 to 60; Ne²⁰/Ar³⁶ from 5 to 8: Ar³⁶/Kr⁸⁴ from 2400 to 3200; and Kr⁸⁴/Xe¹³² from 3·2 to 7·3. The lowest He⁴/Ne²⁰ ratios occur in samples rich in green glass spherules which have He⁴/Ne²⁰ ≤ 10 (Lakatos, Heymann, and Yaniv, unpublished). He⁴/He³ ranges from about 210 to 2700; Ne²⁰/Ne²² from 12·7 to 13·2; Ne²¹/Ne²² from 0·035 to 0·041; and Ar³⁶/Ar³⁸ from 5·26 to 5·45. The measured Ar⁴⁰/Ar³⁶ ratios range from 0·757 to 3·56; when corrected for radiogenic Ar⁴⁰, the range becomes 0·6 to 3·4. The largest corrected Ar⁴⁰/Ar³⁶ ratios occur in samples from the Apennine Front, the smallest occur in the Mare. This could be due to slope effects between the front as opposed to the mare terrain. An alternative possibility is that the Front fines acquired their atmospheric Ar⁴⁰ at a time when the concentration of neutral Ar⁴⁰ in the lunar atmosphere was relatively large.Ne²¹ radiation ages were calculated for all samples. There is evidence in the landing area for debris from craters with ages less than 100 × 10⁶ yr, but these craters cannot be firmly identified from the data.  相似文献