Nd and Sr isotopes in ultrapotassic volcanic rocks from the Leucite Hills,Wyoming

Nd and Sr isotopic compositions and Rb, Sr, Sm and Nd concentrations are reported for madupites, wyomingites and orendites from the Pleistocene volcanic field of the Leucite Hills, Wyoming. All Leucite Hills rocks have negative εNd signatures, indicating derivation or contribution from an old light rare earth element (LREE) enriched source. In this respect they are similar to all occurrences of high potassium magmas so far investigated. But Sr isotopic variations are comparatively small and ⁸⁷Sr/ ⁸⁶Sr ratios are unusually low for high-K magmas (0.7053–0.7061, one sample excluded). These values suggest that the light REE enrichment of the source was not accompanied by a strong increase in Rb/Sr. Wyomingites and orendites are isotopically indistinguishable which is consistent with chemical and petrographic evidence for their derivation from a common magma series depending on emplacement conditions. Basic to ultrabasic madupites and more silicic wyomingites/orendites are distinct in their Nd isotopic variations (madupites: εNd= ?10.5 to ?12.3; wyomingites/orendites: εNd= ?13.7 to ?17.0) despite similar Sm/Nd ratios and complete overlap in ⁸⁷Sr/⁸⁶Sr. Selective or bulk assimilation of crustal material is unlikely to have significantly affected the Nd and Sr isotopic compositions of the magmas. The measured isotopic ratios are considered to reflect source values. The distinct isotopic characteristics of madupite and wyomingite/orendite magmas preclude their derivation by fractional crystallization, from a common primary magma, by liquid immiscibility or by partial melting of a homogeneous source. Two isotopically distinct, LREE enriched and slightly heterogeneous sources are required. Heterogeneities were most pronounced between magma sources from each volcanic centre (butte or mesa). The relationship between the madupite and wyomingite/orendite sources and their evolution is discussed on the basis of two simple alternative sets of models:

1. a two-stage evolution model with an old enrichment event (a metasomatic event?) perhaps taking place during the stabilization of the Wyoming Craton 3.2 to 2.5 Gyr ago but not later than 1.2 Gyr ago or
2. a mixing model involving mixing between one endmember with εNd near zero and another end-member with a strong negative εNd signature.

     

The mineralogy and petrology of the volcanic rocks from the Leucite Hills,Wyoming

Examples of the three volcanic rock types, wyomingite, orendite and madupite from the Leucite Hills have been examined with the electron microprobe. The results show that leucite is non-stoichiometric as predicted byCross (1897), having an excess of potassium and silicon, and that the only feldspar found, a sanidine, contains up to 18 percent of the iron-feldspar molecule. The co-existing phlogopite, diopside and olivine together with the groundmass amphibole are all highly magnesian. Of the varied accessory minerals, priderite (K₂Ti₈O₁₆) and wadeite (K₄Zr₂Si₆O₁₈) have been identified and analyzed together with ubiquitous apatite and perovskite, both of which contain rare earths in abundance. Comparative mineralogical data has been obtained on a few representative specimens from West Australia and on the jumillite from Spain.The new rock analyses together with the existing data from the Leucite Hills show the rare but characteristic molecular excess of potassium over aluminium; this excess is considered to account for the ahsence of the iron-titanium oxides in the orendites and wyomingites, and of course for the unusual composition and species of the minerals. Exploratory melting experiments show that these potassic lavas have a comparable melting range to magnesian basalts, and a crustal origin is thereby considered precluded. There is no evidence that sialic contamination contributed notably to the composition of the oversaturated orendites and wyomingites, and their relationship by any process of crystal fractionation to the undersaturated madupite is obscure. The generation of madupite could be achieved by crystal fractionation at high pressure of a liquid derived by partial fusion of mantle material.     

Origin and Source Evolution of the Leucite Hills Lamproites: Evidence from Sr-Nd-Pb-O Isotopic Compositions

Whole-rock major and trace element and O, Sr, Nd and Pb isotopicdata are reported for 3·0–0·89 Ma lamproitesfrom the Leucite Hills, Wyoming, USA. The two main groups oflamproites, madupitic lamproites and phlogopite lamproites,are geochemically distinct and cannot be related to one anotherby either fractional crystallization or crustal contamination.It seems likely that the geochemical differences between thesetwo rock types are related to variations in source mineralogyand depth of partial melting. The high Mg-number and large ionlithophile element abundances and negative Nd values of thelamproites indicate a mantle source that has experienced stagesof both depletion and enrichment. The negative Nb, Ta and Tianomalies in mantle-normalized trace element diagrams and lowtime-integrated U/Pb, Rb/Sr and Sm/Nd ratios of both lamproitegroups and other Cenozoic igneous rocks from the Wyoming ArcheanProvince indicate an ancient metasomatic enrichment (>1·0Ga) of the mantle source associated with the subduction of carbonate-bearingsediments. Other chemical characteristics of the Leucite Hillslamproites, especially their high K₂O and volatile contents,are attributed to more recent metasomatism (<100 Ma) involvinginflux from upwelling mantle during back-arc extension or plumeactivity. KEY WORDS: isotopes; lamproites; metasomatism; Leucite Hills; Wyoming     

The melting relationships of a madupite from the Leucite Hills,Wyoming, to 30 Kb

The water-undersaturated melting relationships of a mafic, peralkaline, potassic madupite (with about 3% H₂O as shown by chemical analysis) from the Leucite Hills, Wyoming, have been studied at pressures up to 30 kb. At low pressures (<5 kb) leucite is the dominant liquidus phase, but it is replaced at higher pressures by clinopyroxene plus olivine (<5–7 kb), clinopyroxene (7–12.5 kb), clinopyroxene plus minor spinel (12.5–17.5 kb), and clinopyroxene alone (17.5–> 30 kb). At all pressures there is a reaction relationship with falling temperature between melt, olivine and probably clinopyroxene to yield phlogopite. Apatite is stable within the melting interval to pressures above 25 kb. Electron microprobe analyses demonstrate that the clinopyroxene is diopsidic, with low aluminium and titanium contents. Pressure has relatively little effect on the composition of the pyroxene. Phlogopite is also aluminium-poor and has only a moderate titanium content. The experimental results indicate that madupite is not the partial melting product of hydrous lherzolite or garnet lherzolite in the upper mantle and it seems improbable that it is derived by melting of mantle peridotite with a mixed H₂O-CO₂ volatile component. Madupite could, however, be the partial melting product of mica-pyroxenite or mica-olivine-pyroxenite in the upper mantle. It is pointed out that the chemistry of some potassium-rich volcanics may have been affected by volatile transfer and other such processes during eruption and that experimental studies of material affected in this way have little bearing upon the genesis of potassic magmas. Finally, the experimental results enable constraints to be placed upon the P-T conditions of the formation of richterite-bearing mica nodules found in kimberlites and associated rocks. Maximum conditions are 25 kb and 1,100 ° C.     

Water-saturated melting relations to 5 kilobars of three Leucite Hills lavas

The water-saturated phase relations of three Leucite Hills lavas have been determined at pressures up to 5 kb. Phlogopite is the major primary liquidus phase in orendite and wyomingite at pressures, > 1 kb, but clinopyroxene and olivine are the major primary liquidus phases in madupite at pressures up to 5 kb. Leucite is a liquidus phase in all three magmas at pressures <0.5kb. The experimental results are in reasonable agreement with the inferred crystallization sequences for the Leucite Hills lavas and have applications to the crystallization and differentiation of potassium-rich magmas within the crust.     

Green clinopyroxenes and associated phases in a potassium-rich lava from the Leucite Hills,Wyoming

Green, salitic pyroxenes occur as megacrysts and as cores in diopsidic pyroxene phenocrysts and microphenocrysts in a wyomingite lava from Hatcher Mesa, Leucite Hills, Wyoming. Al-rich phlogopite (16–21% Al₂O₃), apatite, Fe-Ti-oxide, Mg-rich olivine (Fo₉₃) and orthopyroxene (En₆₁) also occur as megacrysts or as inclusions in diopside phenocrysts. All of these phases are found in ultramafic xenoliths in the host lava, and petrographic and chemical evidence is presented that the megacrysts originate by the disaggregation of the xenoliths. It is concluded that the latter are accidental fragments of the wall rocks traversed by the wyomingite magma and it is suggested that the clinopyroxene-rich xenoliths, from which the green pyroxenes are derived, formed in the upper mantle as a result of local metasomatism or by crystallization from magmas of unknown composition during an earlier igneous event. The precise role of the clinopyroxene-rich xenoliths (which also contain apatite, Fe-Ti-oxide and amphibole) in the genesis of the Leucite Hills magmas cannot be elucidated on the basis of the available data, but it is unlikely that they represent the source material from which these magmas are derived.     

The Kinetics of Degassing-Induced Crystallization at Soufriere Hills Volcano, Montserrat

A series of decompression experiments at 875°C, with a 16h anneal period at 160 MPa, and depressurizations to a finalwater pressure (P_f) of 125–30 MPa, were run for between1 and 504 h. Using an experimentally derived plagioclase liquidus,the depressurizations are estimated to impose an undercooling(     

Crystallization sequences of Ca-Al-rich inclusions from Allende: The effects of cooling rate and maximum temperature

We have studied the crystallization sequences, mineral chemistries, and textures that develop when an average Type B Ca-Al-rich inclusion composition is cooled in air from 1275–1580° C to below 1000°C at rates between 0.5 and 1000°C/hr. Crystallization sequences, the textures of all the major phases, pyroxene chemistry, and melilite zoning patterns are functions of both the cooling rate and the temperature from which cooling begins. Determination of the order of pyroxene and plagioclase crystallization has been identified as an important goal for petrographic studies of CAIs because it can be used to set constraints on the cooling rate experienced by an individual inclusion. Overall textures plus melilite zoning patterns and pyroxene chemistry can give important clues as to whether pyroxene or plagioclase began to crystallize first. Melilite texture and chemistry appear to yield the most valuable information on the maximum temperature to which an inclusion was raised prior to cooling.Comparison of our experimental results with petrographic observations of Type B CAIs suggests that most inclusions were partially melted and then cooled at rates on the order of a few tenths to tens of degrees per hour. Maximum temperatures of about 1400°C appear most likely for intermediate Type B Allende inclusions. Our results do not support the suggestion that the textures observed in these inclusions formed by crystallization of supercooled, metastable melt droplets condensed from nebular gas. The slow cooling rates we infer for CAIs are difficult to reconcile with models for their origin that imply simple radiative cooling of individual molten or partially molten droplets in a cold, low density environment. On the other hand, cooling rates of the nebular cloud are believed to have been much slower than those we have inferred for Type B CAIs. Scenarios that could be reconciled with the thermal history that we have inferred include drag heating of particles falling through nebular gas, heating by intense radiation (e.g., via flares) from the early sun, heating in nebular shock fronts, or other thermal heterogeneities in the early nebula allowing time scales for cooling (and heating) of CAIs much shorter than those for the nebular cloud as a whole. Successful models for the origin of Type B CAIs must account for the fact that most Type B CAIs cooled relatively slowly from a partially molten state.     

Harkerite from the Alban Hills,Italy

Harkerite, found in metamorphic ejecta of the Alban Hills associated with cuspidine, grossular, phlogopite, vesuvian, biotite, and minor amounts of diopside, aegirinaugite, leucite, magnetite and calcito, shows cubic Laue symmetry m3m, possible space groups Fm3m, F432, F43m, a₀ = 14.82 Å.On the basis of isomorphous replacements suggested by the crystal structure analysis, chemical data may be represented by the formula: Ca₄₈Mg₁₆(AlSi₄O₁₆)₄(BO₃)₁₂(CO₃)₂₀ · 4H₂O. Refractive index n_D = 1.6490.The relations between harkerite from Albano, harkerite from Skye and other known harkerites and sakhaites are discussed.     

Reconnaissance of quaternary sediments from Khasi Hills,Meghalaya

Khasi Hills area of Meghalaya, one of the highest rainfall zones of the world has been explored to understand the spatial and temporal extent of Quaternary sediments. In general such deposits are restricted to shallow depths in most of the sites except in one site where it is 600 cm thick. AMS C-14 dates of these deposits suggest that sediments deposited are mostly of Holocene or in rare cases belong to later part of Pleistocene. Early Quaternary deposit is either missing or yet to be explored from this region. Natural hazards combined with human activity effecting degradation of vegetation and sediment cover are probably the main cause for poor Quaternary exposure at the region.     

Crystallization conditions and evolution of magmatic fluids in the Harney Peak Granite and associated pegmatites, Black Hills, South Dakota—Evidence from fluid inclusions

A microthermometric study of inclusions in granites and pegmatites in the Proterozoic Harney Peak Granite system identified four types of inclusions. Type 1 inclusions are mixtures of CO₂ and H₂O and have low salinities, on average 3.5 wt.% NaCl_eq; type 2 inclusions are aqueous solutions of variable salinities, from 0 to 40% wt.% NaCl_eq; type 3 inclusions are carbonic, dominated by CO₂, with no detectable water; and type 4 inclusions consist of 20 to 100% solids, with the remaining volume occupied by a CO₂-H₂O fluid. Many inclusions have a secondary character; however, a primary character can be unambiguously established in several occurrences of the type 1 inclusions. These inclusions were trapped above the solidus and represent the exsolved magmatic fluid. The secondary populations of types 1, 2, and 3 probably formed as a result of reequilibration and unmixing of the type 1 fluid that progressively changed composition and density with decreasing temperature and pressure and was finally trapped along healed microfractures under subsolidus conditions. Type 4 inclusions are primary and are interpreted to be trapped, fluid-bearing, complex silicate melts that subsequently solidified or underwent other posttrapping changes.It is demonstrated that primary type 1 fluid inclusions that coexist with crystallized melt inclusions in the complex, Li-bearing Tin Mountain pegmatite were trapped along the two-fluid phase boundary in the system CO₂-H₂O-NaCl_eq. Consequently, the temperature and pressure conditions of trapping are identical to the bulk homogenization conditions—on average 340°C and 2.7 kbar. These conditions indicate that this Li-, Cs-, Rb-, P-, and B-rich pegmatite crystallized at some of the lowest known temperatures for a silicate melt in the crust. An internally consistent, empirical solvus surface in P-T-X_CO2 coordinates was generated for the pseudobinary CO₂-(H₂O-4.3 wt.% NaCl_eq) pegmatite fluid system. Distribution coefficients for the major species CO₂, H₂O, NaCl, and CH₄ between the immiscible CO₂-rich and H₂O-rich fluid phases as a function of pressure and temperature were extracted from data for the two cogenetic fluid inclusions types.     

Basalts of unusual composition from the Chyulu Hills,Kenya

Five Ne-normative basalts are unusually rich in Cr, to a lesser degree in Co, and have very high La/Lu ratios and high contents of several excluded trace elements resembling kimberlites in these and other aspects. They seem to represent mantle-derived magmas, only slightly modified by shallow level crystal/liquid fractionation. Cr was apparently excluded from the crystalline phases in equilibrium with these magmas in the upper mantle.The Chyulu rocks differ in several respects from other Gregory Rift basalts, but closely resemble those from Jan Mayen Island near the Mid-Atlantic ridge. The generation of these unusual basalts is therefore not related simply to mantle composition or tectonic setting, but may reflect unusually high-T (1450°C), low-P (15–29 kbars) environments in the zones of last effective equilibration of these magmas with mantle rocks.     

Metamorphic evolution of aluminous granulites from Labwor Hills,Uganda

Sapphirine-cordierite-quartz and spinel-cordierite-quartz form relic assemblages of probable Archaean age in Fe-rich aluminous metapelites from Labwor Hills, Uganda, and reflect an unusually high temperature metamorphism (1,000° C) at pressures in the vicinity of 7–9 kbars and a(O₂) near the magnetite-hematite buffer. Subsequent reaction textures include the replacement of spinel and cordierite by sillimanite and hypersthene and formation of sapphirine-hypersthene-K-feldspar-quartz symplectites which are interpreted as pseudomorphs after osumilite. A petrogenetic grid appropriate to these assemblages suggests these reaction textures may be due to cooling at constant or increasing pressure and constant a(O₂), or decreasing a(O₂) at constant temperature and pressure. The former interpretation is supported by the coexistence of ilmenohematite and magnetite during the development of the reaction textures, and by the comparatively low Al₂O₃-contents of secondary hypersthene. This pressure-temperature path implies that: (1) metamorphism occurred at deep levels within normal thickness crust, probably less than 40–45 km thick, due to an extreme thermal perturbation induced either by emplacement of mantle-derived magmas or by thinning of the subcontinental lithosphere in an extensional tectonic regime, (2) the excavation and surface exposure of the granulites is due to a subsequent, postgranulite facies metamorphism, crustal thickening most probably involving their incorporation into an allochthonous upper crustal thrust sheet during the formation of the Mozambique foldbelt.     

Crystallization of chromite from nickel-iron sulphide melts

An experiment, in which an iron-nickel-copper sulphide melt was heated with synthetic chromite and then cooled, showed that substantial quantities of chromite had dissolved in the melt and had then recrystallized as euhedral crystals rimmed with magnetite. This experiment suggests that the unusual chromite (low in Mg and Al) which is associated with the sulphide phase in Western Australian nickel ores may have formed in a similar way.J.M.R. carried out the experimental part of this investigation as a post-graduate student at Flinders University, South Australia, working under a CSIRO extramural grant.     

A Cromerian Complex stalagmite from the Mendip Hills,England

In order to provide a better chronological constraint on a British Middle Pleistocene interglacial, a large stalagmite boss from the Mendip Hills was selected for palaeoclimate data using pollen analysis. Dating analyses by thermal ionisation mass spectrometry (TIMS) of uranium–thorium ratios and by magnetostratigraphy constrain the age of the sample to 450–780 ka. The isotopic consistency of the TIMS analyses, plus the presence of luminescence laminations, suggest that the sample has been preserved under closed-system conditions. Pollen assemblages have been recovered from the speleothems, despite the fact that the pH of calcite deposition is usually greater than 7. Furthermore the evidence presented here indicates that the pollen was probably transported by the speleothem feedwater, rather than entering the cave aerially. The pollen record contained within the stalagmite is interpreted as early–mid-interglacial but does not have clear Cromerian affinity. © 1997 John Wiley & Sons, Ltd.     

东南极拉斯曼丘陵泥质麻粒岩变质作用演化

普里兹湾拉斯曼丘陵代表了东南极一条重要的早古生代的～530Ma泛非期(Pan-African)高级构造活动带。然而,该区早期的晚元古代的～1000Ma格林维尔期(Grenvellian)高级变质作用的演化历史至今仍有争论。该区呈透镜状产出的泥质麻粒岩峰期矿物组合(M1)为石榴石+堇青石+斜方辉石+钾长石+石英,峰期石榴石变斑晶发育堇青石或堇青石+斜方辉石反应边(M2)。利用Thermocalc程序在KFMASH模式体系对该泥质麻粒岩进行的定量模拟表明,其峰期矿物组合是由反应石榴石+黑云母+石英=堇青石+斜方辉石+钾长石+熔体形成的。利用Themocalc平均P-T计算方法获得峰期M1变质P-T条件为～0.9GPa和～900℃,而叠加的M2组合反映了一个减压冷却的过程,其变质P-T条件为～0.7GPa和800～850℃。结合已有的年代学数据,认为该区泥质麻粒岩的峰期M1矿物组合反映晚元古代(～1000Ma)格林维尔期挤压D1构造事件,而叠加的M2矿物组合与M3蠕虫状结构则形成于早古生代泛非期(～530Ma)D2～D3高级扭压剪切构造期间。该扭压事件导致了面状高低应变带的发育以及进步花岗岩和伟晶岩的侵入。     

Clinopyroxene chemistry of the high-Potassium suite from the Alban Hills,Italy

Summary Chemical data on clinopyroxene phenocrysts in twenty-four lava samples from the Alban Hills (Roman comagmatic region) show coexistence, within the same rock, of two core-rim evolution trends: diopside-salite and salite-diopside, respectively. The Alban volcanics can be divided in two groups depending on which type of core predominates.Geochemical mixing tests, conducted with elements showing a different degree of incompatibility, such as Ce, Sr, Th, La, Ta, and Hf, show no evidence of a mixing process which might be responsible for coexistence of both diopside and salite clinopyroxenes within the same lava.Taking into account the results of known experiments on the influence of water on clinopyroxene composition in potassium rich lavas, the reverse zoning trend observed and the consequent predominance of salite cores in some lavas are ascribed to the effect of volatiles, and particularly to water. Changes of water pressure may also be responsible for phenocryst corrosion and salitic clinopyroxene replacement by olivine, phlogopite and titaniferous magnetite.The prominent role of water in the Alban Hills magma evolution is also supported by the high fluorine content found in the Alban products, which enhances water solubility in the magmas, by the frequent occurrence of mica in the rock groundmass and, finally, by the explosive character of Alban volcanism.

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Zusammenfassung Die Ergebnisse chemischer Analysen von Klinopyroxen in vierundzwanzig Lavaproben aus den Albaner Bergen (Römische Komagmatische Region) zeigen die Koexistenz von zwei Kern-Rand-Entwicklungstendenzen: Diopsid-Salit und Salit-Diopsid. Die Vulkanite können auf Grund der Zusammensetzung der Kerne in zwei Gruppen unterteilt werden.Mit Elementen verschiedener Inkompatibilität, wie Ce, Sr, Th, La, Ta und Hf, ausgeführte Mischversuche geben keinen Hinweis dafür, daß ein Mischungsprozeß für die Koexistenz von Diopsid und Salit in derselben Lava verantwortlich sei.In Anbetracht der Ergebnisse von Experimenten über den Einfluß von H₂O auf die Klinopyroxen-Zusammensetzung in K-reichen Laven, werden die beobachtete Zonierung und die daraus folgende Dominanz von Salit-Kernen in bestimmten Lavatypen der Wirkung von volatilen Bestandteilen, besonders Wasser, zugeschrieben. änderungen des H₂O-Drucks können für Phenokristall-Korrosion und Verdrängung der salitischen Klinopyroxene durch Olivin, Phlogopit und Titanomagnetit verantwortlich sein.Die entscheidende Rolle des Wassers in der Entwicklung des Magmas stimmt mit dem hohen Fluor-Gehalt der Produkte, der die H₂O-Löslichkeit in Magmen erhöht, mit der Häufigkeit des Glimmers in der Grundmasse der Gesteine und mit der explosiven Natur des Vulkanismus im Untersuchungsgebiet überein.

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Zur Chemie der Klinopyroxene in den Kali-reichen Gesteinen der Albaner Berge

     

Late Eocene brachiopods from the Euganean Hills (NE Italy)

Five species belonging to five genera and an unidentified rhynchonellid have been recognised in a Late Eocene (Priabonian) brachiopod assemblage from Castelnuovo in the Euganean Hills, north-eastern Italy. One genus and two species are new, i. e. Venetocrania euganea gen. et sp. nov. and “Terebratula” italica sp. nov. Orthothyris pectinoides (von Koenen 1894) is recorded for the first time from Italy. The other species are Terebratulina sp. cf. T. tenuistriata (Leymerie 1846) and Lacazella mediterranea (Risso 1826), both already known from the Italian Eocene.     

东南极拉斯曼丘陵镁铁质麻粒岩的变质作用演化

拉斯曼丘陵（Larsemann Hills）位于东南极普里兹构造带的中部,研究该区麻粒岩的变质作用演化对于理解普里兹带的构造属性至关重要。通过对该区含石榴石镁铁质麻粒岩转石详细的岩相学观察表明,峰期前进变质阶段矿物组合（M1）由角闪石+斜方辉石+单斜辉石+斜长石+黑云母+钛铁矿±石英±磁铁矿组成,其峰期矿物组合（M2）为石榴石+斜方辉石+单斜辉石+角闪石+钛铁矿±磁铁矿±石英,而代表后期与降压有关的叠加变质组合（M3）为斜方辉石+斜长石+单斜辉石+黑云母+钛铁矿±磁铁矿。矿物化学分析,结果显示其中石榴子石和斜方辉石具有弱的成分环带特征。利用THERMOCALC软件在NCFMASHTO体系下对该麻粒岩进行了详细的热力学模拟,结合传统温压计和平均温压计算结果,得出不同阶段温压条件分别为650~750℃/5.5~6.5kb （M1）,850~950℃/8~8.5kb （M2）,800~900℃/5.5~7.5kb （M3）。其变质作用演化为典型的峰期后近等温减压的（ITD）顺时针P-T轨迹。通过区域上镁铁质麻粒岩的对比分析,我们认为该镁铁质麻粒岩可能来源拉斯曼丘陵基岩露头。结合已有的年代学资料,表明该镁铁质麻粒岩的峰期变质事件可能对应于晚元古代格林威尔期构造事件,而后期退变质作用与早古生代的泛非期构造事件有关,意味着泛非期普里兹带可能是陆内造山带。     

东南极拉斯曼丘陵富硼岩系中硅硼镁铝矿-柱晶石-电气石矿物的硼同位素组成及其意义

东南极拉斯曼丘陵地区麻粒岩相岩石中出露一套罕见的含硅硼镁铝矿-柱晶石-电气石矿物组合的富硼岩系.由于高级变质作用已使原岩的性质难以确定,变质原岩及其形成环境的恢复变得十分困难,而硼同位素组成则可以作为判定硼来源的有效示踪剂和指相标志.报道了东南极拉斯曼丘陵硅硼镁铝矿-柱晶石-电气石富硼岩系的硼同位素组成资料,其δ11B值变化范围为-12.0‰～-34.6‰,硼同位素的低比值和其他地质证据表明,其原岩为非海相蒸发硼酸盐岩.