Cyclicity in the Main and Upper Zones of the Bushveld Complex, South Africa: Crystallization from a Zoned Magma Sheet   总被引：9，自引：0，他引：9  

TEGNER  CHRISTIAN; CAWTHORN  R. GRANT; KRUGER  F. JOHAN 《Journal of Petrology》2006,47(11):2257-2279

The major element composition of plagioclase, pyroxene, olivine,and magnetite, and whole-rock ⁸⁷Sr/⁸⁶Sr data are presented forthe uppermost 2·1 km of the layered mafic rocks (upperMain Zone and Upper Zone) at Bierkraal in the western BushveldComplex. Initial ⁸⁷Sr/⁸⁶Sr ratios are near-constant (0·7073± 0·0001) for 24 samples and imply crystallizationfrom a homogeneous magma sheet without major magma rechargeor assimilation. The 2125 m thick section investigated in drillcore comprises 26 magnetitite and six nelsonite (magnetite–ilmenite–apatite)layers and changes up-section from gabbronorite (An₇₂ plagioclase;Mg# 74 clinopyroxene) to magnetite–ilmenite–apatite–fayaliteferrodiorite (An₄₃; Mg# 5 clinopyroxene; Fo₁ olivine). The overallfractionation trend is, however, interrupted by reversals characterizedby higher An% of plagioclase, higher Mg# of pyroxene and olivine,and higher V₂O₅ of magnetite. In the upper half of the successionthere is also the intermittent presence of cumulus olivine andapatite. These reversals in normal fractionation trends definethe bases of at least nine major cycles. We have calculateda plausible composition for the magma from which this entiresuccession formed. Forward fractional crystallization modelingof this composition predicts an initial increase in total iron,near-constant SiO₂ and an increasing density of the residualmagma before magnetite crystallizes. After magnetite beginsto crystallize the residual magma shows a near-constant totaliron, an increase in SiO₂ and decrease in density. We explainthe observed cyclicity by bottom crystallization. Initiallymagma stratification developed during crystallization of thebasal gabbronorites. Once magnetite began to crystallize, periodicdensity inversion led to mixing with the overlying magma layer,producing mineralogical breaks between fractionation cycles.The magnetitite and nelsonite layers mainly occur within fractionationcycles, not at their bases. In at least two cases, crystallizationof thick magnetitite layers may have lowered the density ofthe basal layer of melt dramatically, and triggered the proposeddensity inversion, resulting in close, but not perfect, coincidenceof mineralogical breaks and packages of magnetitite layers. KEY WORDS: layered intrusion; mineral chemistry; isotopes; magma; convection; differentiation  相似文献   

Nd-Sr Isotopic Geochemistry of the Late Archean-Paleoproterozoic Granitoids in the Lüliang-Wutai Terrain, North China Craton,and Implications for Petrogenesis     

CHEN Bin  LIU Shuwen  WANG Rui  CHEN Zhichao  LIU Chaoqun 《《地质学报》英文版》2006,(6)

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陕西穆家庄铜矿床后生成矿作用的流体地球化学证据   总被引：2，自引：2，他引：2  

朱华平  李虹  张德全  刘平 《西北地质》2005,38(2):54-61

尽管秦岭泥盆系铅锌金多金属成矿带成矿作用均与热水喷流沉积作用有关，柞山地区却有别于风太地区，具有独特的铜矿成矿背景。流体包裹体研究揭示了后生成矿流体的两阶段流体演化过程：第一阶段的成矿流体为中温，中高盐度岩浆热液含CO2的NaCl—H2O流体。均一温度为190-265℃，盐度12．5～35．34(w1％NaCl)，压力12．8～21．3MPa，在同地寄主矿物中均一温度变化小，而盐度变化极大，是岩浆流体沸腾的产物；第二阶段成矿流体为中高温，中高盐度岩浆期后热液NaCl-H2O流体。均一温度为300～350℃，盐度7．4～41．59(w1％NaCl)，压力10．8～19．3MPa。反映了岩浆期后热液流体的二次沸腾。应用流体地球化学的综合方法(包裹体流体组成、演化)识别出后生交代流体性质。穆家庄铜矿的成矿流体第一阶段为岩浆水，第二阶段的成矿流体为岩浆水加部分地层水(建造水)。氢氧同位素分析也支持上述结论。  相似文献   

大别山双河超高压变质矿物O同位素平衡及其对Sm-Nd和Rb-Sr等时线年龄有效性的制约     

赵子福郑永飞  李曙光龚冰 《岩石学报》2005,21(4):1243-1254

对于变质岩 Sm-Nd 和 Rh-Sr 同位素年代学来说,其中一个重要问题是等时线矿物之间在一特定的变质事件过程中是否达到并在随后保持同位素平衡。矿物 O 同位素地质测温也是如此。由于许多情况下 Nd、Sr 和 O 在变质矿物中的扩散速率具有可比性,变质矿物之间 O 同位素平衡状况能够为矿物 Sm-Nd 和 Rb-Sr 内部等时线定年结果的有效性提供制约。为了验证其适用性,本文对大别造山带双河超高压榴辉岩和片麻岩 Sm-Nd 和 Rh-Sr 等时线矿物进行了 O 同位素地质测温。尽管Sm-Nd 等时线给出一致的三叠纪年龄(213～238Ma),同一样品 Rb-Sr 等时线却给出侏罗纪年龄(171～174Ma)。片麻岩、榴辉岩和榴闪岩矿物对 O 同位素测温得到600～720℃和420～550℃两组温度,分别对应于约225±5Ma 榴辉岩相变质和约 175±5Ma 角闪岩相退变质条件下停止同位素扩散交换的温度。同一样品三叠纪 Sm-Nd 等时线年龄的保存、侏罗纪 Rh-Sr 等时线年龄的出现以及有规律的 O 同位素温度,表明在角闪岩相退变质过程中,Sr 和 O 在含水矿物(如黑云母和角闪石)中的扩散速率在手标本尺度上比石榴石 Nd 和多硅白云母 Sr 的扩散速率快。在退变质作用过程中,等时线矿物之间的初始同位素比值均一化速率主要受扩散速率慢的矿物控制,而矿物等时线时钟的启动主要受具有高母/子体比值的矿物控制。只有当高母/子体比值矿物具有快的放射成因同位素扩散速率时,才能够应用合理的矿物等时线确定变质再造的时间。  相似文献   

新疆准噶尔地区富硫型与贫硫型浅成低温热液金矿床成矿流体与碳、硫、铅同位素   总被引：1，自引：2，他引：1  

王莉娟  王京彬  王玉往  朱和平曲丽丽 《岩石学报》2005,21(5):1382-1388

对新疆准噶尔地区浅成低温热液型金矿床中富硫型的阔尔真阔腊金矿、贫硫型的石英滩金矿进行了流依包裹体的均一温度、爆裂温度、包裹体气液相成分、H、O 同位素、矿体围岩及脉石英包裹体 C 同位素、矿体中黄铁矿等 S、Ph 同位素等系统地进行了研究,综合研究表明,本区该类型金矿成矿流体一般温度低、盐度低,来源主要为循环的大气水、矿石中黄铁矿的 S、Pb 同位素均为深源,暗示金的深部来源:矿体石英包裹体中 CO_2的δ~(13)C 为低于-10‰的有机碳,反映了本区年轻的富含有机质的沉积地层参与了金的成矿。此外,本文首次提出了富硫型阔尔真阔腊金矿床成矿流体中有侵入岩浆热液参与,深部有多金属成矿远景;贫硫型石英滩金矿没有侵入岩浆热液的参与,成矿仅与火山古热液活动有关,其成矿较单一。此外,阔尔真阔腊金矿中低温流体活动较强,金矿化也较强:石英滩金矿低温流体活动相对较弱,金矿化也较弱,也体现了该类型金矿床低温流体活动的越强烈,金矿化越强的规律。  相似文献   

成矿流体演化与成矿物理化学   总被引：7，自引：0，他引：7  

费红彩  肖荣阁 《矿物岩石地球化学通报》2002,21(2):139-144

成矿流体是富含挥发分 (CO2 、CH4等 )是具有较高含盐度的特殊地质流体。本文讨论了在流体演化过程中挥发分的来源 ,指出主要来自水岩作用、有机质分解及地幔去气和岩浆 ;碱金属及卤素同样具有多来源的性质 ,以海水、含盐系淋滤、建造水为主要来源 ,含盐系重熔可以形成富含碱金属的成矿流体。流体演化过程中氢氧同位素、硫同位素的分馏主要与温度、水岩比值或硫源丰度有关。一个重要的结论是 ,成矿流体的形成主要与地质作用有关 ,而流体来源是次要的。海底热水流体的地球化学特征以高δ3 4 S值、中稀土富集及正铕异常为特征。本文总结了热水流体成矿物理化学条件 ,指出水热流体物相点 :1) 10 80℃ ,7.5× 10 8Pa水溶液与硅酸岩熔浆分熔点 ;2 )水溶液的第二个临界点是气水溶液的超临界点 (374.15℃ ,2 .2 1× 10 7Pa) ;3)水溶液的沸点 (≥ 10 0℃ ,≥ 1× 10 5Pa) ;4)水溶液的冰点 (≤ 0℃ ,1× 10 5Pa) ;5 )H2 O CO2 体系的不混溶温度点 (2 6 6℃ ,2 .15×10 8Pa[1 3 ] 等是重要的成矿相变点。  相似文献   

Stable isotopic signature of a palaeoaquifer, Mississippian Alamogordo Member limestones, Sacramento Mountains, New Mexico, USA   总被引：1，自引：0，他引：1  

YongqiangWu  Henry S. Chafetz 《Sedimentology》2002,49(2):227-235

Nine stratigraphic sections, each ≈5 m thick, were sampled from the Alamogordo Member limestones of the Lake Valley Formation, Sacramento Mountains, New Mexico, USA. Four stratigraphic sections consist entirely of lime mudstone and wackestone, whereas the other five sections have a prominent layer of crinoidal packstone about 1 m thick at their base. Stable isotopic analyses reveal that the lime muds in the sections with basal packstone layers show a downward decrease in δ¹⁸O and constant δ¹³C values, whereas those in the sections solely composed of lime mudstone and wackestone have, in general, relatively uniform δ¹⁸O and δ¹³C values. The diagenesis of the Alamogordo Member limestones was previously believed to have been governed by the downward percolation of meteoric water from a regional pre-Pennsylvanian exposure surface ≈100 m above this unit. However, the uniform δ¹³C and downward decrease in δ¹⁸O values in the lime muds in the sections with basal packstones indicate that the meteoric water ascended within the Alamogordo Member, rather than descended from the overlying exposure surface. This indicates that the basal packstones were probably a conduit for meteoric water. This is further supported indirectly by the relatively uniform δ¹⁸O and δ¹³C values of the lime mud in the sections without basal packstones. The implications are that the oxygen isotopic gradients may be used to identify palaeoaquifers, flow directions within these aquifers and that meteoric diagenesis below an exposure surface could be governed by flow through a palaeoaquifer.  相似文献   

Isotopic constraints on growth conditions of multiphase calcite–pyrite–barite concretions in Carboniferous mudstones     

R. Raiswell  S. H. Bottrell  S. P. Dean  J. D. Marshall†  A. Carr‡  & D. Hatfield 《Sedimentology》2002,49(2):237-254

Carbonate concretions in the Lower Carboniferous Caton Shale Formation contain diagenetic pyrite, calcite and barite in the concretion matrix or in different generations of septarian fissures. Pyrite was formed by sulphate reduction throughout the sediment before concretionary growth, then continued to form mainly in the concretion centres. The septarian calcites show a continuous isotopic trend from δ¹³C=?28·7‰ PDB and δ¹⁸O=?1·6‰ PDB through to δ¹³C=?6·9‰ PDB and δ¹⁸O=?14·6‰ PDB. This trend arises from (1) a carbonate source initially from sulphate reduction, to which was added increasing contributions of methanogenic carbonate; and (2) burial/temperature effects or the addition of isotopically light oxygen from meteoric water. The concretionary matrix carbonates must have at least partially predated the earliest septarian cements, and thus used the same carbonate sources. Consequently, their isotopic composition (δ¹³C=?12·0 to ?10·1‰ PDB and δ¹⁸O=?5·7 to ?5·6‰ PDB) can only result from mixing a carbonate cement derived from sulphate reduction with cements containing increasing proportions of carbonate from methanogenesis and, directly or indirectly, also from skeletal carbonate. Concretionary growth was therefore pervasive, with cements being added progressively throughout the concretion body during growth. The concretions contain barite in the concretion matrix and in septarian fissures. Barite in the earlier matrix phase has an isotopic composition (δ³⁴S=+24·8‰ CDT and δ¹⁸O=+16·4‰ SMOW), indicating formation from near‐surface, sulphate‐depleted porewaters. Barites in the later septarian phase have unusual isotopic compositions (δ³⁴S=+6 to +11‰ CDT and δ¹⁸O=+8 to +11‰ SMOW), which require the late addition of isotopically light sulphate to the porewaters, either from anoxic sulphide oxidation (using ferric iron) or from sulphate dissolved in meteoric water. Carbon isotope and biomarker data indicate that oil trapped within septarian fissures was derived from the maturation of kerogen in the enclosing sediments.  相似文献   

Continental crust and lithospheric mantle interaction beneath North China: isotopic evidence from granulite xenoliths in Hannuoba, Sino-Korean craton   总被引：40，自引：0，他引：40  

Xinhua Zhou  Min Sun  Guohui Zhang  Shaohai Chen 《Lithos》2002,62(3-4):111-124

Mafic granulite and pyroxenite xenoliths from Cenozoic alkaline basalts at Hannuoba, Hebei Province, North China have been selected for a systematic geochemical and Sr–Nd–Pb isotopic study, which provides a unique opportunity to explore nature of the lower crust and the interaction between the continental crust and lithospheric mantle beneath an Archean craton. The major, compatible and incompatible elements and radiogenic isotopes of these xenoliths suggest great chemical heterogeneity of the lower crust beneath the Hannuoba region. Petrological and geochemical evidences indicate a clear cumulate origin, and most likely, they are related to basaltic underplating in different geological episodes. However, the Sr–Nd–Pb isotopic compositions of the xenoliths reveal a profound enriched source signature (EM I) with some influence of EM II, which implies that some portion of pre-existing, old metasomatized subcontinental lithospheric mantle could have played an important role in their genesis. It is suggested that the interaction between continental crust and subcontinental mantle as manifested by basaltic underplating would be closely related to regional tectonic episodes and geodynamic processes in the deep part of subcontinental lithospheric mantle.  相似文献   

Celestite formation, bacterial sulphate reduction and carbonate cementation of Eocene reefs and basinal sediments (Igualada, NE Spain)   总被引：5，自引：0，他引：5  

Conxita Taberner  James D. Marshall†  James P. Hendry‡  Catherine Pierre§  & M. F. Thirlwall¶ 《Sedimentology》2002,49(1):171-190

Petrographic and geochemical studies of an Upper Eocene reef and associated basinal sediments from the mixed carbonate–siliciclastic fill of the south‐eastern Pyrenean foreland basin near Igualada (NE Spain) provide new insights into the evolution of subsurface hydrology during the restriction of a marine basin. The reef deposits are located on delta‐lobe sandstones and prodelta marls, which are overlain by hypersaline carbonates and Upper Eocene evaporites. Authigenic celestite (SrSO₄) is an important component in the observed diagenetic sequences. Celestite is a significant palaeohydrological indicator because its low solubility constrains transportation of Sr²⁺ and SO₄^2? in the same diagenetic fluid. Stable isotopic analyses of carbonates in the reef indicate that meteoric recharge was responsible for aragonite stabilization and calcite cementation. Sulphur and oxygen isotope geochemistry of the celestite demonstrates that it formed from residual sulphate after bacterial sulphate reduction, but also requires that there was a prior episode of sulphate recycling. Meteoric water reaching the reef and basinal areas was most probably charged with SO₄^2? from the dissolution of younger Upper Eocene marine evaporites. This sulphate, combined with organic matter present in the sediments, fuelled bacterial sulphate reduction in the meteoric palaeoaquifer. Strontium for celestite precipitation was partly derived in situ from dissolution of aragonite corals in the reef and basinal counterparts. However, ⁸⁷Sr/⁸⁶Sr data also suggest that Sr²⁺ was partly derived from dissolution of overlying evaporites. Mixing of these two fluids promoted celestite formation. The carbonate stable isotopic data suggest that the local meteoric water was enriched in ¹⁸O compared with that responsible for stabilization of other reefs along the basin margin. Furthermore, meteoric recharge at Igualada post‐dated evaporite deposition in the basin, whereas other parts of the same reef complex were stabilized before evaporite formation. This discrepancy resulted from the spatial distribution of continental siliciclastic units that acted as groundwater conduits.  相似文献