Kiglapait Mineralogy III: Olivine Compositions and Rayleigh Fractionation Models

Olivines, present throughout the layered cumulates of the KiglapaitIntrusion, record extreme iron enrichment during fractionalcrystallization. Mn is less compatible than Fe; the exchangecoefficient K_D for Mn/Fe (OL-LIQ) has values near 0.95 but theydrop to 0.7 near the Lower Zone-Upper Zone boundary. Ca is depletedby more than a factor of 30 relative to experimental valuesat 5 kbar pressure. Attempts to find a sink for Ca in the LowerZone without invoking liquid as a reactant are unconvincing,and questions of metastability arise. Cumulus olivines varysystematically to lower Fo contents with stratigraphic height.Using equilibrium values for the exchange coefficient K_D (Fe/Mg,OL-LIQ), and the observed mode of olivine and residual porosity,a Rayleigh fractionation calculation reproduces the observedLower Zone trend without recourse to multiple injections ofmagma. An anomalously Fe-rich region above the Main Ore Bandin the Upper Zone is ascribed to ponding of Fe-rich magma atthe floor of the intrusion until later, buoyant residual magmaentrained the Fe-rich residua. Such Fe-rich ponds probably accountfor the abnormal Feenrichment shown by some other Fenner-trendlayered intrusions. Summation over the observed crystal compositionsyields values of X_Mg that do not represent the equilibrium liquid,but that reduce to it by a simple multiplier p = 0.78. Thisresult means that if K_D is known, the high-temperature, liquidusolivine compositions can be retrieved, or vice versa. Becausethe observed olivine compositions are supported by realisticforward models, there is no need to invoke evolved boundary-layerliquids to explain the in situ crystallization of Kiglapaitcumulates. Classical cumulate theory suffices. KEY WORDS: olivine; Rayleigh fractionation; Kiglapait Intrusion; cumulative theory     

Kiglapait Geochemistry I: Systematics, Sampling, and Density

The Kiglapait intrusion affords many opportunities for evaluatingplutonic fractionation processes. Estimates of boundary conditionsinclude emplacement of anhydrous high alumina basaltic magmaat 4 kbar and about 1250 °C, initial crystallization nearthe WM buffer, and fractionation to Mg-free ferrosyenite whichcrystallized at 960°C, somewhat above the WM buffer. Thelast ferrosyenites represent fractionation to 0.01 per centof the initial volume. Plagioclase varies from An₆₇ to An₁₀, olivine from Fo₆₉ to Fo₀,and augite from En₇₃ to En₀. The specific gravity of the intrusionis 2.93, varying between 2.87 and 3.18 on smoothed models. Crystals accumulated chiefly at the floor. As they did so, themagma depth decreased as the square root of the volume fractionof liquid. The volume fraction solidified was roughly proportionalto time. Cooling was slower than the t relation because of hotsurroundings on one side. The crystallization time was about10⁶ yr, and the average accumulation rate was about 1 cm/yr.Average crystal concentrations of 3–300 ppm are impliedfor the nucleation zone. The cooling rate corresponds to crystallizationof 2 x 10⁷ kg/yr per km² roof area, about 550 times slower thana lava lake. Calculated liquid densities range from 2.67 to 2.88 g/cm³ athigh temperatures. Feldspar almost surely did not sink in themagma, but nevertheless it accumulated mainly on the floor.Cooperative sinking with mafics as proposed by Coats, combinedwith oscillatory nucleation as proposed by Wager, may accountfor this paradox. Oscillatory nucleation leading to feldspar-supersaturatedliquids is supported by laboratory evidence on the feldspar-likestructure of liquids and the concave-úp plagioclase liquidusin systems involving olivine. Both lines of evidence imply highpolymerization of feldspar-rich liquids, particularly in slowprocesses. Such polymerization can help to explain the genesisof primary Eu anomalies and anorthositic magmas in additionto the floor accumulation of feldspar and rhythmic layering.     

Kiglapait Mineralogy II: Fe-Ti Oxide Minerals and the Activities of Oxygen and Silica

Cumulus titanomagnetite and subordinate ilmenite first appearin the Upper Zone of the Kiglapait intrusion. They arrive graduallyand then reach abnormal abundances before falling to a sustainedcotectic mode near seven volume per-cent. The most Ti-rich titanomagnetites(to Usp ₆₆) are preserved in ore bands (layers) which solidifiedby adcumulus growth leading to the complete expulsion of interstitialsilicate liquid. Analyses from three of these ore bands, appliedto the solution model of Lindsley (1977), form a single lineararray in f_o2 versus 1/T ?K, with log f_o2 = (–28,283 ?89)/T + 11.03 ? 0.25. This array implies log f_o2 = –9.65at 1094 ?C, the model temperature of the Main Ore Band, consistentwith primary mineral compositions Ilm₈₉, Usp₇₉ and a weightmode of 18 per cent ilmenite. Silicate rocks yield another linear array, i.e. log f_o2 = (–37,910? 102)/T + 22.57 ? 0.61. This array is ascribed to closure ofsubsolidus reactions from initial compositions near Usp_79–80Ilm₉₀. The center of gravity of the data falling on this arraysuggests a primary mode of about 50 per cent ilmenite for thesilicate rocks, implying somewhat more reducing conditions ofcrystallization than for the ore bands. The modal overproductionrepresented by the ore bands is attributed to super-saturationin oxygen, which is demonstrated by the Al-depleted compositionsof titanomagnetite in ore bands, by direct evidence for elevatedf_o2 at the top of the Main Ore Band, and by abnormally magnesiansilicate mineral compositions in and near the ore bands. The primary titanomagnetite composition for average rocks isestimated at Usp₈₀ for the base, and Usp₇₃ for the top of theUpper Zone, from rock and mineral chemistry and observed textures.The idealized magma path for the Upper Zone runs from (T andlog f_o2) 1154 ?C, –9.0 to 960 ?C, –12.2. The orebands lie above this path and are interpreted as lying on themetastable extension of the Lower Zone path, which originatesat 1250 ?C, –8.1, on the WM buffer at 4 kbar total pressure. Silica activity is estimated from mineral compositions nearthe ore bands as applied to the FMQ equilibrium, and mappedfor the Lower Zone by an adjustment downward from the En-Fo-Silequilibrium, with resultant values near 0.55 relative to quartz= 1.0. The logarithmic oxygen/silica activity ratio (OSAR) coincideswith that of the Skaergaard intrusion in the Lower Zones. TheSkaergaard OSAR is offset downward from the Kiglapait trendduring MZ time, and remains below it at the end of crystallization.The more highly silicated Skaergaard magma was initially moreoxidized than the Kiglapait magma, but this relation was reversedafter the loss of olivine in the Skaergaard intrusion, as couldhave been predicted from theory and the mineralogy of the twointrusions.     

郭家岭花岗闪长岩中黑云母的成因矿物学研究

通过对郭家岭花岗闪长岩中黑云母的形态、成分及穆斯堡尔谱等分析，表明其具深棕褐色到淡黄色多色性、云母律双晶、波状消光、集合体呈六方锥状，在不稳定、氧化条件下形成，并且富Ｆｅ、Ｆｅ＾３＋、Ｆ＾－，贫ＯＨ＾－。其蚀变产物常为绿泥石和黄铁矿。以上特征表明其对形成金矿有利。     

冀南綦村岩体斑状黑云母角闪闪长岩的成因矿物学研究

綦村岩体是冀南邯邢地区典型的中生代高镁闪长岩杂岩体,主要由斑状黑云母角闪闪长岩、角闪闪长岩、闪长岩、二长岩和少量辉长岩组成。对綦村斑状黑云母角闪闪长岩进行了较为详细的成因矿物学研究,探讨了其成因及其地质意义。研究发现,綦村斑状黑云母角闪闪长岩中的角闪石多为镁铝钙闪石和镁角闪石;黑云母主要为富镁黑云母;斜长石发育环带结构,核部以中长石和拉长石为主,边部多为更长石。角闪石矿物温压计估算结果显示,角闪石斑晶的形成温度为930~970 ℃,压力介于300~340 MPa之间,深度10~15 km,氧逸度为ΔNNO+0.1~+2.3,平衡熔融体中的水含量4.8%~5.5%;与黑云母平衡的角闪石形成温度为684~760 ℃,压力降低至42~61 MPa,熔体中水含量降至3.1%~4.3%,氧逸度为ΔNNO+0.7~+2.4。黑云母温度计和氧逸度计获得的结果与角闪石温压计估算结果一致。该结果表明,研究区高氧逸度的铁镁质岩浆在中地壳曾经驻留,并发生了以角闪石为主的结晶分异,富含挥发分的分异岩浆在后期快速侵位形成高镁闪长岩和矽卡岩型铁矿。     

Kiglapait Geochemistry II: Petrography

The mode of the Kiglapait intrusion carries 73 per cent feldspar,but average rocks near the base of the Upper Zone contain aslittle as 48 per cent feldspar. Olivine remained stable throughoutthe crystallization, but was locally suppressed by abundantcrystallization of augite and titano-magnetite. Red biotiteoccurs as rims on Fe–Ti oxide minerals and is probablyfluorine oxybiotite; its frequently similar occurrence in troctoliticrocks may, perversely, indicate dry magmas rather than dampones. Excluded modal components follow Rayleigh fractionation behaviour;their presence in trace amount permits estimation of residualporosity in the Lower Zone. This porosity diminishes directlywith accumulation rate from 0.14 to 0.03 over the first 80 percent of crystallization history. The saturation ratio of excludedmodal components is a well-behaved function of fraction solidified,and implies that the decrease in porosity continues above the80 per cent solidified level. The saturation ratio links withbulk composition, porosity, and F_L, allowing one of these parametersto be estimated from the others. The cumulus arrival of apatite is abrupt, but the earlier arrivalsof augite, oxide minerals, and sulfide each occur over an interval,followed by an interval of overproduction. This behaviour isattributed to feedback on concentration gradients generatedby a long history of plagioclase + olivine extraction, in theabsence of perfect stirring. Diffusion plays a role in the differentiationof large, slowly cooled magma systems because radial mixingby convection is inefficient. Inherited potential supersaturationis the inevitable result. This leads to modal irregularities,and to crystallization effectively on metastable extensionsof field boundaries. The track of the liquid in the Lower Zone is closely parallelto that in the system Fo–Di–An, but offset fromit by the combined effects of Ab and P (toward plagioclase)and Fa (away from plagioclase). The latter effect is important,with the result that the shedding of plagioclase by an ascendingmagma will be much less marked than predicted from iron-freeexperimental systems.     

Kiglapait geochemistry V: Strontium

The Kiglapait intrusion contains 330 ppm Sr and has $\text{Sr}\text{Ca}\text{= 5 × 10}{}^{\mathrm{?3}}$ and $\text{Rb}\text{Sr}\text{= 3 × 10}{}^{\mathrm{?3}}$, as determined by summation over the Layered Group of the intrusion. Wholerocks in the Lower Zone contain 403 F_L^0.141 ppm Sr, where F_L is the fraction of liquid remaining; Sr drops to 180 ppm at the peak of augite production (F_L = 0.11) and rises to a maximum of 430 ppm in the Upper Zone before decreasing to 172 ppm at the end of crystallization. Feldspars in the Lower Zone contain 532 F_L^0.090 ppm Sr, increasing to 680 ppm in the Upper Zone before decreasing to 310 ppm at the end. Clinopyroxenes contain 15 to 30 ppm Sr and have a mineral-melt distribution coefficient D = 0.06 except near the top of the intrusion where D = 0.10.The calculated feldspar-liquid distribution coefficient has an average value near 1.75 but shows four distinct trends when plotted against X_An of feldspar. The first two of these are strongly correlated with the modal augite content of the liquid, on average by the relation D = 1.4 + 0.02 Aug^L. The third (decreasing) trend is due to co-crystallization of apatite, and the fourth (increasing) trend can best be attributed to a triclinic-monoclinic symmetry change in the feldspar at An₂₆, 1030°C. The compound feldspar-liquid distribution coefficient K_D for $\text{Sr}\text{Ca}$ bears out these deductions in detail and yields ΔG_r for the Sr-Ca exchange ranging from nearly zero at the base of the Lower Zone to ?26 kJ/gramatom at the end of crystallization. The compound feldspar-liquid distribution coefficient K_D for $\text{Rb}\text{Sr}$ varies from 0.3 in the Lower Zone to 1.1 at the end of crystallization.The ratio $\text{Ca}{}^{\mathrm{F}}\text{Ca}{}^{\mathrm{L}}$ is about 1.45 for troctolitic liquids containing 5% augite, for which K_D (Sr-Ca) = 1.0 and D_Ca = D_Sr. For common basaltic liquids containing 20% augite, the Kiglapait data predict $\text{solSr}{}^{\mathrm{F}}\text{Sr}{}^{\mathrm{L}}\text{= 1.8}$, as commonly found elsewhere. The strong dependence of D_sr on augite content of the liquid illuminates the role of liquid composition and structure in determining the feldspar-liquid distribution coefficient. Conversely, a discontinuous change in the trend of D_Sr when apatite arrives shows that the effect is due to apatite crystallization itself, not to the continuous variation of the liquid as it becomes enriched in apatite component.     

Kiglapait Geochemistry III: Potassium and Rubidium

The regular geometry and completeness of the Kiglapait intrusion permit its bulk composition to be obtained by summation, and the composition of successive liquids to be obtained by subtraction. The summations for K and Rb give 1806 and 1.08 ppm, yielding Rfrsol|K/Rb= 1670 for the intrusion, taken as equal to the parent magma. R increases slightly from this initial value to 2000 at the end of crystallization where MgO approaches zero in the rocks. K and Rb are therefore closely coherent and their distribution coefficients can differ only by a small amount in the Kiglapait system.Apparent feldspar/liquid distribution coefficients (D^F/L) can be estimated from detailed plots of feldspar and liquid compositions against F_L. The Kiglapait data imply that these coefficients are linear 1:1 functions of plagioclase composition within experimental error, having values given by D_KF/L = 1.42? X_AnD_RbF/L = 1.13? X_An with minimum values of 0.75 and 0.49, respectively. The ratio $\text{R}{}^{\mathrm{F}}\text{R}{}^{\mathrm{L}}$ lies in the range of 1.53± 0.03 for the plagioclase composition range X_An= 0.34 to 0.67 showing that high-R rocks such as anorthosite crystallized from high-R liquids.The apparent feldspar distribution coefficients are much closer to 1.0 than common literature values. They can be reduced by assuming that the cumulate pile was continuously recharged by the circulating magma until an advanced stage of differentiation was reached, and assuming that alkalies were exchanged to the feldspars from the magma. When such an ‘aquifer recharge’ model is calibrated using olivine-liquid equilibria as a time marker for the liquid, the inferred minimum equilibrium values of the distribution coefficients are $\text{D}{}_{\mathrm{K}}\text{F}\text{L}$= 0.42, $\text{D}{}_{\mathrm{Rb}}\text{F}\text{L}$ = 0.25 at the base of the intrusion. Their variation is given by $\text{D}{}_{\mathrm{K}}\text{F}\text{L}\text{= 1.66?1.88X}{}_{\mathrm{An}}$, $\text{D}{}_{\mathrm{Rb}}\text{F}\text{L}\text{= 1.17?1.41X}{}_{\mathrm{An}}$, The equilibrium values are considered to be appropriate for deducing liquid compositions in plutonic bodies where alkali exchange can be shown or inferred to have been inhibited, such as in small intrusions. The apparent values are considered to be appropriate, even though they may be artificial, for large intrusions similar to the Kiglapait.The bulk K and Rb concentrations in the Kiglapait intrusion are consistent with a plagioclase-rich abyssal tholeiite magma. Clinopyroxene and olivine fractionation in the mantle may contribute to the production of such high-Rmagmas.     

Isotopic Studies of Processes in Mafic Magma Chambers: I. The Kiglapait Intrusion, Labrador

The initial Nd and Sr isotopic ratios of cumulate rocks andminerals of the Kiglapait intrusion are pertinent as indicatorsof the processes that affected the Kiglapair magma while itwas resident in the crust. A Sm–Nd mineral isochron indicatesthat the crystallization age of the intrusion is 1305?22 millionyears. The initial _Nd values range from—1?6 in the LowerZone to 6 in the Upper Zone and correlate with the anorthitecontent of plagioclase. The initial ₈₇Sr/⁸⁶Sr ratios are 0.70407to 0.70433 in the Lower Zone, and increase monotonically up-section(decreasing plagioclase anorthite content) to 0.7068 in theUpper Zone. These variations are attributed to assimilationof roof rock concurrently with crystallization. It is evidentthat replenishment of the chamber with uncontaminated magmawas important during the accumulation of the lower zone rocks,but did not occurduring crystallization of the Upper Zone. Amathematical model relating isotope ratio shifts to the relativerates of crystallization, assimilation, and replenishment ispresented. It is estimated that the rate of assimilation wasbetween 0.01 and 0.04 of the crystallization rate, and thatduring the accumulation of the Lower Zone, the rate of replenishmentwas about half of the crystallization rate. A formulation for‘assimilation efficiency’is presented that relatedthe actual amount of assimilation (determined from the isotopedata) to the thermodynamic maximum allowable amount. The assimilationefficiency of the Kiglapait intrusion is not tightly constrained,but appears to be of the order of 0.01 near the end of crystallizationand perhaps as high as 0.07 near the beginning. Further quantitativeestimates of assimilation efficiency in different intrusionsemplaced under different conditions may aid in understandingassimilation mechanisms and in assessing the role of assimilationin magmatic evolution in general. Many layered intrusions studiedto date have initial Nd isotope ratios close to the chondriticvalue (_Nd= 0), suggestive of mantle magma sources that are chemicallyundepleted, and thus different from the sources of mid-oceanridge basalt and island-arec basalt.     

Kiglapait geochemistry VI: Oxygen isotopes

The Kiglapait layered intrusion is the first major intrusion found to have all whole rock and calculated liquid δ¹⁸O values close to a normal uncontaminated gabbroic value of 6.0. The intrusion experienced no detectable oxygen isotope exchange with its surrounding rocks and cooling of the magma was conductive. The δ¹⁸O values of average whole rocks vary smoothly from 6.0 at the base of the Lower Zone to 6.3 at the top of the Upper Zone. The calculated liquid δ¹⁸O values lie practically superimposed on the whole rock trend. The whole-rock data and the modelled δ¹⁸O of the magma and cumulates rigorously demonstrate that the effect of incoming cumulus phases such as magnetite and augite on the δ¹⁸O of the liquid and rocks during fractional crystallization is negligible. The cancelling effects of complementary modal variations among the mafic mineral phases and feldspar, keep the δ¹⁸O of the whole rocks constant to within ±0.1 %.. The minor change in δ¹⁸O that does occur with fractionation is consistent with the enrichment of residual liquids in feldspar component and the increasing fractionation factor δ Liquid-Fsp with falling temperature.The δ¹⁸O values of the country rocks bracket the estimated δ¹⁸O of the Kiglapait magma. Modelling with oxygen isotopes indicates that contamination of the intrusion, indicated by published radiogenic Sr and Nd isotopic data, was minor. The most probable contaminant had δ¹⁸O?7.7 and the contamination most likely occurred at >99% solidified. Subsolidus oxygen isotope exchange with an external source appears to have been very minor.     

Kiglapait geochemistry VII: Yttrium and the rare earth elements

Based on 51 wholerock analyses by XRF and summation over the layered group, the Kiglapait Intrusion contains 4.7_?1.6^+1.2 ppm Y, which resides principally in augite and apatite. Using liquid compositions calculated by summation, the partition coefficient D^AUG/L_Y is 0.95 ± 0.12 from 84 to 97 PCS (percent solidified) and 1.5 ± 0.4 above 97 PCS. For feldspar, the most likely value for D is 0.028 ± 0.02 (N = 6).REE analyses for 13 whole rocks were interpreted with the aid of yttrium models to yield trends for wholerocks and liquids vs PCS. Summations over the rocks of the layered group gave La = 2.5, Ce = 5.8, Nd = 3.9, Sm = 1.0, Eu = 0.8, Tb = 0.17, Yb = 0.37, and Lu = 0.06 ppm, with 2 s.d. errors near ± 30%. All these elements are highly incompatible until the arrival of augite, which affects chiefly the HREE, and apatite, which affects all (but more strongly, the LREE). The net result is that after apatite arrival at 94 PCS, the liquid compositions are nearly constant, hence D^WR/L_REE ≈ 1.0. These results are compatible with the mineralogy of the intrusion and the estimated partition coefficients for feldspar, olivine, augite, apatite, and Fe-Ti oxide minerals. For pre-apatite liquids, D^FSP/L_REE vary regularly with the normative di content of the liquid and change by an order of magnitude, hence the bulk liquid composition must be considered in any attempt to invert the compositions of feldspars to parent liquids.The Eu anomaly at first decreases in Kiglapait liquids due to plagioclase fractionation, but then increases due to removal of augite and apatite with negative Eu anomalies. The features dominantly responsible for Eu partitioning are liquid structure and, for monoclinic ternary feldspars, crystal structure. The former is best monitored by the augite or diopside content of the liquid and the latter, by the K content of the feldspar.The chondrite-normalized REE pattern for the intrusion has La_N = 7.4, Lu_N = 1.6, (Ce/Yb)_N = 3.6, and Eu/Eu* = 2.4, indicating its feldspar-rich nature. The chilled margin of the nearby Hettasch Intrusion has a similar but more evolved pattern, corresponding roughly to the Kiglapait liquid at 70 PCS. As with other data, those for the REE suggest source differences for the two intrusions rather than a relationship due to fractionation.     

云南因民铁铜矿区次火山杂岩中黑云母和绿泥石矿物化学特征与成矿指示

云南因民铁铜矿区次火山杂岩主要由铁质熔岩、辉绿岩、辉长辉绿岩、火山集块岩、火山角砾岩、热液角砾岩等组成,岩相分带明显,热液蚀变与矿化关系密切。通过对次火山杂岩中不同岩相的黑云母和绿泥石电子探针结果分析得出,黑云母为镁质黑云母,大多数为再平衡黑云母,形成温度为505~590℃,lgf(O2)为-12.4~-5.25,压力为116~226 MPa,推测成岩深度为4.27~8.37 km,属于高温强氧化环境;绿泥石为密绿泥石、蠕绿泥石、透绿泥石、叶绿泥石,形成温度为170~235℃,lgf(O2)为-51.93~-43.70,lgf(S2)为-13.34~-2.50,属于中低温强还原环境。矿物产状、矿物组合与矿物中主要阳离子关系显示,两种矿物均具有多期多源性的特征。黑云母化蚀变代表铁矿的主成矿期,绿泥石化蚀变代表铜矿的主成矿期;多期次构造-岩浆-热事件形成了高-中低温的碱性强还原流体,叠加改造富集铁铜矿床,揭示了本区次火山杂岩是铁铜矿床稳定持续性成矿元素的供给系统。     

Kiglapait Geochemistry IV: The Major Elements

The summed bulk composition of the Kiglapait intrusion is SiO₂ 47.46 (31). TiO₂ 0.81 (20), Al₂O₃ 19.46 (48), Fe₂O₃ 1.91 (46), FeO 9.36 (36), MnO 0.15 (01). MgO 8.04 (21), CaO 9.27 (46). Na₂O 3.13 (05), K₂O 0.22 (01), P₂O₅, 0.09 (01), and BaO 0.02 (01). total 99.98 wt% (estimated standard deviations of the last two decimals in parentheses). The CIPW norm isap 0.34, mt 2.78, il 1.52, or 1.11, ab 26.27, an 38.64, (fsp 66.47), di 5.38, hy 2.45, ol 21.58. Molar X_An is 0.58; molar x_fo is 0.65.The variation curves for oxides in calculated liquids are explained in detail by the petrographic variations shown in earlier papers of this series. The Kiglapait FeO + MnO:MgO:Alkalies (FMA) trend reaches higher iron concentrations than the Skaergaard liquid and constitutes a new limiting case of the Fenner trend of fractional crystallization, implying low oxygen fugacity and silica activity. The end-stage Kiglapait ferrosyenite lies on the FeO + MnO-Alkalies sideline, being essentially devoid of MgO.Except in$\text{K and K}\text{Rb.}$the Kiglapait composition is the same within experimental error as the chilled margin of the nearby Hettasch intrusion (BERG, 1980.), but slight systematic differences show that the Hettasch composition is slightly more fractionated or represents a smaller fraction of melting at the source. Both are low-augite troctolite compositions, and they require troctolitic parent liquids. Such liquids are related to common augite-rich basalts by addition of spinel, and they imply exhaustion of clinopyroxene in the source. Except for their low augite and high Al₂O₃, the Kiglapait and Hettasch compositions resemble modern MORB and suggest a depleted source.     

Komatiite Flows from the Reliance Formation, Belingwe Belt, Zimbabwe: I. Petrography and Mineralogy

The 2.7-Ga Reliance Formation of the Ngezi Group, Belingwe GreenstoneBelt, Zimbabwe, contains extremely fresh komatiite lavas. Detailedfield mapping and a 200-m deep drill-hole, with excellent corerecovery, demonstrated the existence of a suite of lava flows.Each major flow is 10 m thick and characteristically exhibitschilled top and bottom margins, a spinifex zone dominated byrandom spinifex, a B1 zone, and a thick cumulate zone that typicallycomposes two-thirds of the flow thickness. Preservation of olivineand pyroxene mineralogy is superb by Archaean standards, tothe extent that even the tips of skeletal crystals survive.The matrix, although devitrified, is well preserved. Detailedstudy of two flows shows that skeletal grains from the spinifexzone have maximum Fo contents of 91.4. The Fo contents of microphenocrystsfrom the cumulate zone range from Fo_91.2 to Fo_91.6, but rarelarge phenocrysts ( 5 vol.%) have maximum Fo contents of 93.6.The Fo contents of the cumulate olivines do not vary with stratigraphicheight, implying that the cumulate zone formed rapidly, by accumulationof transported crystals. The cumulate zones contain 42–57%modal olivine and display reverse size grading of the olivinemicrophenocrysts. This grain-size variation is believed to resultfrom adcumulus growth within a cumulate pile formed by the formedby the gravitational settling of clusters of olivine crystals.Textural relationships indicate that the final part of the flowto start to crystallize was the lowermost part of the spinifexzone. Reprint requests.     

Apatite Mineralogy and Chemistry of the Taocun Magnetite-Apatite Deposit in Ningwu Volcanic Basin: Implications for Ore Genesis of IOA Deposits

Please refer to the attachment(s) for more details.     

Stability Relations of the Ferruginous Biotite, Annite

Annite, KFe₃AISi₃O₁₀(OH)₂ a member of the iron biotites andthe ferrous analogue of phlogopite, has been synthesized andits phase relations have been determined as functions of temperature,fugacity of oxygen (fo₂), and total pressure (P_totalPH₂O+PH₂).A method for controlling fo₂at high total pressures is described,and data for the ‘oxygen buffers’ used are given.Buffers range from quartz+iron+fayalite assemblages (low fo₂)to magnetite-hematite assemblages (high fo₂). Optical propertiesand unit-cell dimensions of synthetic annites depend on theconditions of synthesis. By recalculating published analyses of natural iron-rich biotitesit can be shown that one cannot assume a constant hydrogen contentfor such biotites. Oxidation may have occurred by drying at115?C. Octahedral occupancy therefore cannot be calculated fromsuch data. Phase relations of annite are presented in 2,070 and 1,035 barsections. Depending on fo₂-T values annite was found to decomposeto one of the following assemblages: hematite+ sanidine, magnetite+sanidine,fayalite+leucite+kalsilite, iron+sanidine. All decompositionsare dehydration and redox reactions and are sensitive to changesin fH₂0 and fo₂ (or fH₂0 and fH₂). At 2, 070 bars total pressureannite+magnetite+sanidine can coexist between 425?C and 825?C, depending upon the magnitude of fo₂. In the presence of quartz the stability field of annite is morerestricted. Phase equilibria in the system KAlSiO₄–SiO₂–Fe–O₂–H₂have been summarized schematically. Wherever possible, thermodynamic extrapolations are made totest the internal consistency of the data. Enthalpies of formationare calculated for both annite and phlogopite. Ranges of fo₂values in nature as well as mechanisms for changes in fo₂ areinvestigated. It is useful to distinguish between assemblageswhich are internally buffered with respect to fo₂changes andthose which are not buffered. The applications of individualreactions involving annite to specific geologic problems arediscussed with respect to igneous, metamorphic, and sedimentaryrocks.     

环境矿物学：矿物学在环境科学研究中的应用

矿物学在环境科学中的应用将是21世纪矿物学研究的一个主要方面。 作者所在实验室曾做过的一些环境矿物学研究的实例有：核废料的处置,矿物表面性质的研究,对有毒金属的还原和固定作用的微生物效应,大气烟尘微粒的研究,矿物表面阳离子的本征吸附常数之理论计算,等等。矿物-水-微生物体系在分子级别上之相互作用的定量研究,对于理解低温地球化学和生物地球化学过程将是重要的。     

The volcanoes and caldera of Talasea,New Britain: Mineralogy

The Talasea Peninsula is composed of a chain of Quaternary volcanoes whose lavas range from basalt to rhyolite. The peninsula is situated in an orogenic environment and the lavas, while essentially calc-alkaline, show some differences from other orogenic suites on the Pacific rim. The most distinctive feature of the Talasea series is absolute iron enrichment in some lavas. Mineralogically, the andesites are characterized by phenocrysts of plagioclase, orthopyroxene, clinopyroxene and titanomagnetite, while the basalts lack titanomagnetite phenocrysts but contain olivine. The acid rocks have a mineralogy similar to that of the andesites, but also contain quartz, amphibole, biotite and ilmenite. The compositions of coexisting titanomagnetite and ilmenite in the acid lavas indicate equilibration temperatures in the range 920° to 860° C and oxygen fugacities ( ) above those of the fayalitemagnetite-quartz buffer assemblage. The mineralogical evidence supports the hypothesis of a crystal fractionation origin for this series and there is a possibility that the was more or less constant during the early stages of its evolution. The iron enriched lavas may be an offshoot from the main line of descent, resulting from near-surface fractionation, with the dominance of plagioclase in the crystal residuum producing an iron-rich liquid.     

Neogene basanites in western Kamchatka: Mineralogy,geochemistry, and geodynamic setting

Neogene (N ₁ ² -N ₂ ¹ ?) K-Na alkaline rocks were found in western Kamchatka as a subvolcanic basanite body at Mount Khukhch. The basanites have a microphyric texture with olivine phenocrysts in a fine-grained doleritic groundmass. The olivine contains inclusions of Al-Cr spinel. The microlites consist of clinopyroxene, plagioclase, magnetite, and apatite, and the interstitial phases are leucite, nepheline, and analcime. The Mount Khukhch basanites are characterized by elevated concentrations of MgO, TiO₂, Na₂O, and K₂O, high concentrations of Co, Ni, Cr, Nb, Ta, Th, U, LREE (La_N/Yb_N = 10.8?12.6, Dy_N/Yb_N = 1.4?1.6) at moderate concentrations of Zr, Hf, Rb, Ba, Sr, Pb, and Cu. The values of indicator trace-element ratios suggest that basanites in western Kamchatka affiliate with the group of basaltoids of the within-plate geochemical type: Ba/Nb = 10?12, Sr/Nb = 17?18, Ta/Yb = 1.3?1.6. The basanites of western Kamchatka show many compositional similarities with the Miocene basanites of eastern Kamchatka, basanites of some continental rifts, and basalts of oceanic islands (OIB). The geochemistry of these rocks suggests that the basanite magma was derived via the ～6% partial melting of garnet-bearing peridotite source material. The crystallization temperatures of the first liquidus phases (olivine and spinel) in the parental basanite melt (1372–1369°C) and pressures determined for the conditions of the “mantle” equilibrium of the melt (25–26 kbar) are consistent with the model for the derivation of basanite magma at the garnet depth facies in the mantle. The geodynamic environment in which Neogene alkaline basaltic magmas occur in western Kamchatka was controlled by the termination of the Oligocene—Early Miocene subduction of the Kula oceanic plate beneath the continental margin of Kamchatka and the development of rifting processes in its rear zone. The deep faulting of the lithosphere and decompression-induced magma generation simultaneous with mantle heating at that time could be favorable for the derivation of mantle basite magmas.