Precambrian sedimentary carbonates: carbon and oxygen isotope geochemistry and implications for the terrestrial oxygen budget

Carbon isotope values of 260 Precambrian limestones and dolomites (most of them being substantially unaltered) have yielded an overall mean of $\text{δ}{}^{13}\text{C}\text{= +0.4 ± 2.7‰}$ vs. PDB; the corresponding oxygen values average at $\text{δ}{}^{13}\text{O = +20.0 ± 4.2‰}$ vs. SMOW. Like the overall mean, the δ ¹³C values furnished by individual carbonate occurrences are, as a rule, fairly “modern” and almost constant as from the very beginning of the sedimentary record. A remarkable exception are the “heavy” dolomites of the Middle Precambrian Lomagundi Group, Rhodesia, with $\text{δ}{}^{13}\text{C}\text{= +9.4 ± 2.0‰}$ vs. PDB. As a result of our measurements, the sporadic occurrence in the geological past of anomalously heavy carbonates seems to be established.The approximate constancy around zero per mill of the δ ¹³C values of marine carbonates through geologic time would imply a corresponding constancy of the relative proportion of organic carbon in the total sedimentary carbon reservoir since about 3.3 · 10⁹ y ago (with C_org/C_total ? 0.2). Utilizing this ratio and current models for the accumulation of the sedimentary mass as a function of time, we get a reasonable approximation for the absolute quantity of organic carbon buried in sediments and, accordingly, of photosynthetic oxygen released. Within the constraints of our model (based on a terrestrial degassing constant λ = 1.16 · 10^?9 y^?1) close to 80% of the amount of oxygen contained in the present oxygen budget should have been released prior to 3 · 10⁹ y ago. Since geological evidence indicates an O₂-deficient environment during the Early and most parts of the Middle Precambrian, there is reason to believe that the distribution of this oxygen between the “bound” and the “molecular” reservoir was different from that of today (with effective O₂-consuming reactions bringing about an instantaneous transfer to the crust of any molecular oxygen released). Accordingly, the amount of C_org in the ancient sedimentary reservoir as derived from our isotope data is just a measure of the gross amount of photosynthetic oxygen produced, withholding any information as to how this oxygen was partitioned between the principal geochemical reservoirs. As a whole, the carbon isotope data accrued provide evidence of an extremely early origin of life on Earth since the impact of organic carbon on the geochemical carbon cycle can be traced back to almost 3.5 · 10⁹y.     

Geochronology of Precambrian rocks in the Laramie Range and implications for the tectonic framework of Precambrian southern Wyoming

From Casper Mountain; at its northern end, to the northwestern margin of the Laramie anorthosite—syenite complex, in its central parts, the Laramie Range is underlain by granite and granitic gneiss that has a minimum age of 2.54 ± 0.04 Ga (Rb/Sr whole-rock isochron) and by metasedimentary rocks, including marble and quartzite, that appear to overlie the granitic gneiss nonconformably (minimum age: 1.7 Ga based on several horn-blende K/Ar dates). Southward from the anorthosite—syenite complex into Colorado, the Range is underlain chiefly by the Sherman Granite (1.41 Ga; Peterman and Hedge, 1968) and scattered patches of gneiss that are not dated, but are tentatively correlated wit similar gneiss in the southern Medicine Bow Mountains and in the Colorado Front Range, where they are dated as ? 1.7 Ga (Peterman and Hedge, 1968).The Laramie anorthosite—syenite complex (minimum age: ? 1.42 Ga or ? 1.51 Ga if a hornblende K/Ar date is accepted) apparently intruded the suture separating the old (? 2.5 Ga) continental edge from younger (? 1.7 Ga) geosynclinal rocks. The suture, which manifests itself as the Mullen Creek—Nash Fork shear zone in the Medicine Bow Mountains, also is the boundary between ensialic and ensimatic geosynclinal deposition that occurred during the interval 1.7–2.5 Ga ago.K/Ar dates on biotite and muscovite from rocks north of the anorthosite—syenite complex grade from 2.5 Ga on Casper Mountain down to 1.38 Ga near the complex. Near its northern tip, the Laramie Range is crossed by a geochronologic front, separating 2.5 Ga old gneiss whose K/Ar dates were not lowered by subsequent metamorphism from 2.5 Ga old gneiss whose mica dates were reset between 1.4 and 1.6 Ga ago.     

Xenocrystic/inherited Precambrian zircons entrained within igneous rocks from eastern South China: Tracking unexposed ancient crust and implications for late Paleoproterozoic orogenesis

South China is characterized by widespread igneous rocks with varied ages and nature in its eastern part, which contain abundant Precambrian xenocrystic/inherited zircons that bear important information of the composition and evolution of the underlying ancient crust. This paper for the first time presents a compiled U-Pb age database of 1416 Precambrian xenocrystic/inherited zircons from igneous rocks in eastern South China, and attempts to provide a constraint on the Precambrian crustal evolution of the constituent Yangtze and Cathaysia blocks. These xenocrystic/inherited zircons, as a conceivable proxy of the unexposed continental crust, document three major tectonothermal events related to continental accretion and subsequent modification that possibly built the continental crust of the eastern Yangtze Block (EYB) at 2.70–2.40 Ga, 2.10–1.55 Ga, and 0.95–0.70 Ga, and the Cathaysia Block (CAB) at 2.70–2.40 Ga, 2.05–1.75 Ga, and 1.10–0.70 Ga, pointing to a complex Precambrian evolutionary history for South China. The EYB zircons are unexpectedly dominated by a 2.10–1.55 Ga age population that shows a multimodal distribution with peaks at 2.05 Ga, 2.0 Ga, 1.90 Ga, 1.85 Ga, and 1.58 Ga, and the CAB zircons are characterized by a unimodal 2.0–1.75 Ga age population that conspicuously peaked at 1.85 Ga, both of which overlap with the tenure of the Nuna supercontinent. These xenocrystic/inherited zircons from both blocks generally have negative ε_Hf(t) values, which in combination with coeval regional magmatic and metamorphic records can assist to trace a possible prolonged (2.05–1.75 Ga) orogenic process in the EYB and a short-lived (1.9–1.8 Ga) orogeny in the CAB. Such orogeneses are proposed to be correlated with the assembly of the Nuna supercontinent.     

Nitrogen recycling in subducted mantle rocks and implications for the global nitrogen cycle

The nitrogen concentrations [N] and isotopic compositions of ultramafic mantle rocks that represent various dehydration stages and metamorphic conditions during the subduction cycle were investigated to assess the role of such rocks in deep-Earth N cycling. The samples analyzed record low-grade serpentinization on the seafloor and/or in the forearc wedge (low-grade serpentinites from Monte Nero/Italy and Erro Tobbio/Italy) and two successive stages of metamorphic dehydration at increasing pressures and temperatures (high-pressure (HP) serpentinites from Erro Tobbio/Italy and chlorite harzburgites from Cerro del Almirez/Spain) to allow for the determination of dehydration effects in ultramafic rocks on the N budget. In low-grade serpentinites, δ¹⁵N_air values (?3.8 to +3.5 ‰) and [N] (1.3–4.5 μg/g) are elevated compared to the pristine depleted MORB mantle (δ¹⁵N_air ~ ?5 ‰, [N] = 0.27 ± 0.16 μg/g), indicating input from sedimentary organic sources, at the outer rise during slab bending and/or in the forearc mantle wedge during hydration by slab-derived fluids. Both HP serpentinites and chlorite harzburgites have δ¹⁵N_air values and [N] overlapping with low-grade serpentinites, indicating no significant loss of N during metamorphic dehydration and retention of N to depths of 60–70 km. The best estimate for the δ¹⁵N_air of ultramafic rocks recycled into the mantle is +3 ± 2 ‰. The global N subduction input flux in serpentinized oceanic mantle rocks was calculated as 2.3 × 10⁸ mol N₂/year, assuming a thickness of serpentinized slab mantle of 500 m. This is at least one order of magnitude smaller than the N fluxes calculated for sediments and altered oceanic crust. Calculated global input fluxes for a range of representative subducting sections of unmetamorphosed and HP-metamorphosed slabs, all incorporating serpentinized slab mantle, range from 1.1 × 10¹⁰ to 3.9 × 10¹⁰ mol N₂/year. The best estimate for the δ¹⁵N_air of the subducting slab is +4 ± 1 ‰, supporting models that invoke recycling of subducted N in mantle plumes and consistent with general models for the volatile evolution on Earth. Estimates of the efficiency of arc return of subducted N are complicated further by the possibility that mantle wedge hydrated in forearcs, then dragged to beneath volcanic fronts, is capable of conveying significant amounts of N to subarc depths.     

Lead isotopic compositions in fault gouges and their parent rocks: implications for ancient fault activities

This is the first study on Pb stable isotopes in fault gouges and their parent rocks. We analyzed the composition of Pb isotopes and contents of U and Pb in 10 pairs of fault gouges and their parent rocks collected along several active faults in central Japan. Thorium-232-²⁰⁸Pb ages of two fault systems were determined as pre-Tertiary, which are consistent with the data from KAr ages and geological considerations.Naturally, the²³⁵U²⁰⁷Pb system is of little use for dating because the magnitude of difference in²⁰⁷Pb/²⁰⁴Pb between gouges and parent rocks is too small. It is found that the²⁰⁶Pb/²⁰⁴Pb can indicate the contribution of²⁰⁶Pb resulting from excess supplies of²²⁶Ra and²²²Rn along the fault. The excess²⁰⁶Pb accumulation rate corresponds to the average²²²Rn concentration in soil gas or groundwater through geological time since the gouge formation. A comparison of Quaternary fault activity and estimated Tertiary activity reveals the characteristics of each fault system.     

柴北缘前寒武纪岩体（地层）变质年龄 及其对早古生代造山作用的指示

柴北缘前寒武纪岩体（地层）分布广泛。为确定柴北缘地区前寒武纪岩体（地层）受早古生代碰撞造山作用的影响,采用LA-ICP-MS技术,对大柴旦地区前寒武纪黑云斜长片麻岩、斜长角闪岩及石榴子石斜长角闪岩中的锆石进行了U-Pb同位素定年。黑云斜长片麻岩获得479~472Ma的变质年龄,斜长角闪岩获得440Ma和470Ma 2个变质年龄,石榴子石斜长角闪岩获得418.8Ma±3.0Ma的变质年龄。初步确定,柴北缘早古生代造山作用对前寒武纪岩体构成了3次强度不等的变质作用叠加,分别为大洋俯冲末期阶段(495~467Ma)岛弧花岗岩弱热烘烤变质作用、大陆碰撞造山阶段(467~423Ma)区域变质作用、S型花岗岩热动力变质作用和大陆后碰撞造山阶段(423~371Ma) I型花岗岩强烈接触热变质作用。     

Precambrian banded iron formations in the North China Craton: Silicon and oxygen isotopes and genetic implications

Banded iron formations (BIFs) are Precambrian chemical marine sedimentary formations that record major transitions of chemical composition, and oxidation–reduction state of oceans at the time of their deposition. In this paper, we report silicon and oxygen isotope compositions of a variety of BIFs from the North China Craton (NCC) in order to deduce the mechanism of their formation. Quartz in the various types of BIFs from the NCC are generally depleted in ³⁰Si, where δ³⁰Si_NBS-28 values range from − 2.0‰ to − 0.3‰ (average, − 0.8‰), similar to δ³⁰Si_NBS-28 values measured from modern submarine black chimneys and sinters. The δ¹⁸O_V-SMOW values of quartz in the BIFs are relatively high (8.1‰–21.5‰; average, 13.1‰), similar to those of siliceous rock formed by hydrothermal activities. The δ³⁰Si_NBS-28 values of quartz in magnetite bands are commonly lower than those of quartz in adjacent siliceous bands within the same sample, whereas δ¹⁸O_V-SMOW values are higher in the magnetite bands. A negative correlation is observed between δ³⁰Si_NBS-28 and δ¹⁸O_V-SMOW values of quartz from siliceous and magnetite bands in BIF from Fuping, Hebei Province. The isotopic compositions of silicon and oxygen of quartz in BIFs provide insights for the formation mechanisms of silicon–iron cyclothems in BIFs. After the silicon- and iron-rich hydrothermal solution was injected onto the seabed, the abrupt temperature drop caused oversaturation of silicic acid, resulting in rapid precipitation of SiO₂ and deposition of siliceous layers. Ferric hydroxide was precipitated later than SiO₂ because of low free-oxygen concentration in the ocean bottom. Progressive mixing of hydrothermal solution with seawater caused a continuous drop in temperature and an increase in Eh values, resulting in gradual oxidation of hydrothermal Fe^2 + and deposition of iron-rich layers. In summary, each silicon–iron cyclothem marks a large-scale submarine hydrothermal exhalation. The periodic nature of these exhalations resulted in the formation of regular silicon–iron cyclothems. The widespread distribution of BIFs indicates that volcanism and submarine hydrothermal exhalation were extensive; the low δ³⁰Si_NBS-28 and high δ¹⁸O _V-SMOW values of the BIFs indicate that the temperature of seawater was relatively high at the time of BIF formation, and that concentrations of Fe^2 + and H₄SiO₄ in seawater were saturated.     

柴北缘前寒武纪岩体（地层）变质年龄及其对早古生代造山作用的指示

柴北缘前寒武纪岩体（地层）分布广泛。为确定柴北缘地区前寒武纪岩体（地层）受早古生代碰撞造山作用的影响,采用LA—ICP—MS技术．对大柴旦地区前寒武纪黑云斜长片麻岩、斜长角闪岩及石榴子石斜长角闪岩中的锆石进行了u—Pb同位素定年。黑云斜长片麻岩获得479-472Ma的变质年龄,斜长角闪岩获得440Ma和470Ma2个变质年龄,石榴子石斜长角闪岩获得418．8Ma±3．0Ma的变质年龄。初步确定,柴北缘早古生代造山作用对前寒武纪岩体构成了3次强度不等的变质作用叠加,分别为大洋俯7中末期阶段（495-467Ma）岛弧花岗岩弱热烘烤变质作用、大陆碰撞造山阶段（467-423Ma）区域变质作用、S型花岗岩热动力变质作用和大陆后碰撞造山阶段（423-371Ma）I型花岗岩强烈接触热变质作用。     

前寒武纪条带状硅铁建造的形成机制与地球早期的大气和海洋

前寒武纪条带状硅铁建造(BIFs)是地球早期特有的化学沉积建造类型,记录了当时大气和海洋的化学成分、氧化还原状态及演化。本文系统测定了华北地台条带状硅铁建造的硫硅氧同位素组成。不同时代和不同类型条带状硅铁建造中石英的硅同位素组成非常相似,强烈亏损30Si,δ30SiNBS-28大部分位于-2.0‰～-0.3‰之间,平均-0.8‰;硅铁建造中石英的δ18OV-SMOW相对较高,8.1‰～21.5‰,平均13.9‰;二者均与现代海底黑烟囱、泉华及热水沉积硅质岩的硅氧同位素组成相似。在同一样品中,磁铁矿条带中石英的δ30SiNBS-28普遍低于相邻硅质条带中石英的值,而δ18OV-SMOW刚好相反,反映了硅铁建造沉积时的初始特征。BIFs中硫化物的δ34SV-CDT变化范围很大,-22.0‰～+11.8‰,但大部分集中分布在0值附近。Δ33S=-0.89‰～+1.2‰,显示出了明显的硫同位素非质量分馏特征,说明当时大气氧浓度很低。与火山活动关系密切的Algoma型硅铁建造的Δ33S多为负值,而远离火山活动中心的Superior型硅铁建造的Δ33S多为正值。提出无论是Algoma型,还是Superior型BIFs都是由海底热液喷气作用形成的。富含溶解硅和铁的热水溶液喷发到在海底以后,由于温度突然下降,硅酸H4SiO4在海水中达到过饱和状态,导致SiO2首先沉淀,形成硅质层;随着热水溶液与海水的不断混合,温度不断降低,Eh值不断升高,Fe2+逐渐被氧化生成Fe3+随后沉淀,形成富铁层。一套硅铁韵律层代表了一次大的海底喷气活动;海底热液喷气的周期性活动形成了规律性的硅铁韵律层。BIFs的广泛分布和硫同位素非质量分馏效应的普遍存在,表明当时大气氧水平很低,可能不足现在氧水平的1‰;火山和海底喷气活动非常强烈,海水温度较高,呈酸性,pH值在3.0～5.5之间;海洋中可溶解硅H4SiO4和Fe2+的浓度很高;而可溶硫酸盐的浓度极低,1mM。早元古代(1.8Ga)以后海洋硫酸盐浓度升高,由富铁海洋转化为富硫酸盐的海洋,是造成BIFs消失的根本原因。大规模火山喷发和海底喷气活动对海洋的成分和氧化还原状态影响很大,使海洋的氧化时间较大气至少推迟了6亿年。     

Molybdenum distribution in Precambrian rocks of the Colorado Mineral Belt

The average Mo content of more than one hundred rock samples from the Precambrian basement of the Colorado Mineral Belt corresponds well to the global molybdenum content of crustal rocks of 1.0 ppm. There are no indications of a regional geochemical molybdenum anomaly in that part of the crust or upper mantle.     

Problems of Iron and Phosphorus Geochemistry in the Precambrian

The localization of economic sedimentary iron ore and phosphorite resources is discussed in comparative aspects. It is shown that the major economic resources of iron ore are hosted in Precambrian rocks, whereas the phosphorites are related to Upper Phanerozoic. High-temperature hydrothermal solutions served as an important source of iron for jaspilite ores. The low P₂O₅content therein indicates that the phosphorus deposition was only weakly related to the hydrothermal activity. Thus, the hydrothermal origin of phosphorite is denied from the geochemical standpoint.     

Improved methods for isolating and validating indigenous biomarkers in Precambrian rocks

Hydrocarbon biomarkers in highly mature Precambrian rocks have the potential to provide important information about the diversity ecology, and evolution of early life, but studying them presents special analytical challenges. Extractable hydrocarbons are present in Archean and most Paleoproterozoic sedimentary rocks in such trace concentration that even slight contamination from petroleum-derived materials in situ or during drilling, storage, sampling, handling and laboratory analysis would compromise the results and, thereby, any consequent inferences. Here we report protocols that we have developed for the analysis of cores from several recently completed deep-time scientific drilling initiatives. By paying special attention to cutting, cleaning, crushing and extraction, it is possible to significantly reduce laboratory blanks to acceptable levels. When these methods are utilized, meaningful variations in the patterns of biomarkers over stratigraphic and lithologic boundaries provide compelling evidence for syngeneity.     

Precambrian tidal and glacial clastic deposits: implications for Precambrian Earth–Moon dynamics and palaeoclimate

Over the past decade the study of Precambrian clastic tidal rhythmites — stacked laminae of sandstone, siltstone and mudstone that display periodic variations in thickness reflecting a strong tidal influence on sedimentation — has provided accurate palaeotidal and palaeorotational data. Palaeotidal records obtained from tidal rhythmites may be systematically abbreviated, however, and derived periods and frequencies can be misleading. The validity of such values, including past length of day, can be assessed by testing for internal self-consistency through application of the laws of celestial mechanics. Such a test supports the estimated length of day of h derived from the late Neoproterozoic (620 Ma) Elatina–Reynella rhythmites in South Australia, and the indicated mean rate of lunar retreat of cm/year since 620 Ma. The validity of estimated lengths of day obtained from other Precambrian tidal rhythmites remain unverified because the data sets contain only one primary value directly determined from the rhythmites. The Elatina–Reynella data militate against significant Earth expansion at least since 620 Ma, and suggest that the free nutation or ‘tipping' of the Earth's fluid core has undergone a resonance with the Earth's annual forced nutation since the Neoproterozoic. Glaciogenic deposits are readily distinguishable from ejecta resulting from impacts with Earth-crossing bodies. Palaeomagnetic data, based on the geocentric axial dipole model for the geomagnetic field, indicate that Neoproterozoic and Palaeoproterozoic glaciation and cold climate near sea level occurred in low palaeolatitudes. This enigmatic finding may imply global glaciation or an increased obliquity of the ecliptic, and is relevant to modelling the effect of ice sheet formation on the Earth's obliquity history by obliquity–oblateness feedback mechanisms. Through multidisciplinary studies, clastic sedimentology and geophysics together can make substantial contributions to understanding Precambrian Earth–Moon dynamics and global palaeoenvironments.     

A problem of total glaciations on the Earth in the Late Precambrian

Ideas of global glaciations on the Earth repeatedly emerged in geology since the middle of the 19th century, but they all did not withstand the test of time. The hypothesis of snowball Earth that suggests long-lasted continuous glaciations over the entire land and oceans in the Late Riphean and Vendian became a popular topic of discussions worldwide. These glaciations must last continuously 15 million years or more owing to enormous stability of climate on the “White Earth,” and one can expect their cessation only when CO₂ concentration in the atmosphere is getting by several orders of magnitude higher in the course of volcanic eruptions. However, many sections of the Late Precambrian glacial deposits evidence repeated alternations of glacial and interglacial events of variable rank and oscillations of glaciers. Consequently, liquid water existed on the Earth, hydrological cycle had not been interrupted, and development of phototrophic phytoplankton, the eukaryotic organisms inclusive, was always in progress. These facts and results of the climate mathematical simulation are inconsistent with the concept of long continuous glaciations over the globe and their consequences. Paleomagnetic data represent main starting point of the snowball Earth hypothesis, although they are to a great extent still of insufficient validity for the Precambrian. Equitable criticism of the hypothesis weak sides turns sometimes into denying all the glacial periods of the Late Proterozoic, when tillites are regarded in majority as deposits of subaqueous slumps and debris flows accumulated on walls of oceanic rifts prograding along splitting lines into the Rodinia continent. Doubtless marks of glaciations in the sedimentary succession are regarded therewith as heterochronous indications of local mountain glaciers on risen shoulders of prograding rifts. Widespread occurrence of the Late Precambrian discrete glacial horizons on the platforms means, however, that glaciations of that time have been associated not always with the rifts and consisted of separate glacial events. Glaciogenic horizons comparable in thickness and structure with those of the Phanerozoic Eonothem are also indicative of discrete glacial periods in the Precambrian. Being confined predominantly to the Late Precambrian succession of rifts, these horizons characterize a high burial potential of these structures, whereas outside them glacial horizons of lesser thickness could be easily subjected to erosion. The hypothesis of snowball Earth is inadequately consistent with well-known facts and needs in additional substantiation. There are also grounds to think that oceans have not been completely covered with ice at the time of Precambrian glaciations.     

Present status of the geochronology of the Precambrian rocks of Rajasthan

Age determinations, mostly by Rb---Sr analyses, of the Precambrian rocks of Rajasthan by us and by others are summarized and discussed. Broad periods of acid magmatism at (1) 3000−2900 m.y., (2) 2600−2500 m.y., (3) 2000−1900 m.y., (4) 1700−1500 m.y. and (5) 850−750 m.y. were identified. The oldest rocks in the area are the yet undated banded gneisses (BGC) east of Udaipur, intruded by the Untala granite dated at 2950 m.y. and hence of mid-Archean age. The basal status hitherto attributed to the Berach granite dated at 2600 m.y. is no longer tenable. The radiometric control on the beginning and duration of the overlying Aravalli Supergroup is not yet satisfactory, though a lower limit at 2000 m.y. is indicated. Heron's original Delhi rocks have recorded two magmatic events widely separate in space and time. While the earliest granitic activity at 1600 m.y. is recorded only in the Alwar basin in the northeast, the younger activity between 850-750 m.y. is widespread, as shown by the nearly concordant ages of “Erinpura-type” granites along the Aravalli mountain Range and the Malani rhyolites in the western plains of the Aravalli Range.     

桂北前寒武纪花岗岩类岩石的地球化学与成因

桂北广泛发育前寒武纪花岗岩类岩石，按岩石组合特征可区分为二类，一类为花岗闪长质岩石，另一类为黑云母花岗质岩石。二类岩石的A／NKC值均在1．10以上，属铝过饱和岩石，但花岗闪长质岩石相对贫硅、钾，富铁，镁，贫铷，富锶、钡，并具有较高的稀土元素总量和轻重稀土元素比值；黑云母花岗质岩石则具更显著的铕负异常，二类岩石εNd(T)值的变化范围与四堡群基底相近，但花岗闪长岩石更接近四堡群基底中的变质镁铁质－超镁铁质杂岩，黑云母花岗质岩石则更靠近四堡群基底中的浅变质沉积岩，对岩石产出动力地质背景的全面分析表明，区内二类花岗质岩石是华夏地块与扬子地块碰撞俯冲作用的不同阶段由成熟度不同的四堡群变质基底在不同深度经部分熔融作用的产物。     

A model to estimate the depositional brine depths of ancient halite rocks: Implications for ancient subaqueous evaporite depositional environments

A model is derived which allows a more general approach to the interpretation of bromine profiles in halite rocks than is possible with the models of Kuhn or Holser. Allowing for an open system, with influx and reflux, reduces the depth of brine necessary to generate a given salt deposit. Even very small and regular bromine gradients, which historically have been interpreted as the result of deposition from deep brine bodies, can be generated in an open system from brine no more than a few tens of metres deep. The bromine gradient produced from a given depth of brine is strongly dependent on the composition and amount of influx, but less so on the composition of brine already in the basin. A Zechstein profile is analysed which in a closed basin would require brine 2665 m deep. It can equally be modelled by influx of normal seawater which fully replenishes a basin no more than 140 m deep. A somewhat irregular profile from the Paradox Basin, instead of requiring a basin 100–400 m deep, can be modelled as being produced by deposition from brines only 10 m deep. Reflux in both cases can only be a few per cent of influx at a maximum.     

韩国Hadong-Sanchung地区斜长岩Sr-Nd同位素初步研究——成因和前寒武纪构造意义

斜长岩呈长条带出露于朝鲜半岛南部,侵入到年代约为2.0Ga的Yeongnam前寒武纪基底岩石中,虽然岩石类型简单(斜长岩和辉长岩质斜长岩),但可以同世界已知块状类型斜长岩相对比。这些斜长岩具有几个重要的差别,例如呈层状构造,镁铁相成分是角闪石而不是辉石,并且不具斜方辉石巨晶。应用Rb-Sr和Sm-Nd同位素系统研究这些岩石的年龄和成因,测定出一种页理化辉长岩质斜长岩矿物的Sm-Nd等时线年龄为1678±90Ma,推断其为侵位年龄,因为中生代绿岩相变质期间这些岩石的Sm-Nd同位素体系呈封闭状态。这一年龄和过去曾报道的元古宙块状斜长岩的年龄范围(1.1~1.7Ga)相吻合。认为斜长岩成因可以用所谓元古宙斜长岩事件来解释。斜长岩的岩浆活动对朝鲜半岛南部前寒武纪基底岩石的构造历史有重要意义。全岩εNd(t)值范围-1.6~-5.2,而87Sr/86Sr初始值变化于0.704~0.706之间,据此可解释地幔成因的斜长岩岩浆是在其结晶作用期间吸收了地壳物质的结果。然而不能排除是下地壳源的可能性。     

Prehnite-pumpellyite facies metamorphism in Precambrian basement rocks of S Sweden

Very small amounts of prehnite and pumpellyite have been found, often as lenses in biotite crystals, in otherwise quite ordinary quartzo-feldspathic gneisses and granitoid rocks forming common components of the Precambrian basement of S Sweden. It is concluded that both minerals belong to the same metamorphic paragenesis, which also includes quartz, K-feldspar, albite, epidote, colourless mica and chlorite. The presence of this paragenesis, in however slight amounts, signifies that the rocks bear the imprint of a phase of metamorphism belonging to the prehnite-pumpellyite facies.