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1.
东天山造山带的图拉尔根镁铁-超镁铁杂岩体为一个早古生代长期活动的幔源岩浆通道，大型铜镍钴硫化物矿体赋存于Ⅰ号超镁铁质岩体的顶部，不同类型岩石中辉石矿物的流体挥发份化学组成以H2O为主（平均91%，5400.4mm3/g），其次为H2（2.0%）、H2S（2.3%）和CO2（2.1%）；赋矿角闪橄榄岩中CO2和H2S含量最高，辉长岩中流体挥发份含量低于辉石橄榄岩和橄榄辉石岩等岩浆早期结晶的岩石。CO2和CH4的δ13C值位于地壳与甲烷氧化的范围内，甲烷同系物的碳同位素组成具有正序分布模式，部分样品（TLG512）释出的CH4和C2H6具有较重的δ13C值和反序分布特征。表明I号岩体不同类型岩石可能是不同期次岩浆活动的产物，成矿岩浆具有富H2O和H2S的特征，可能起源于被流体交代的亏损地幔源区，混染壳源组分可能为俯冲板片来源蚀变沉积有机质组分。 相似文献
2.
《Chemie der Erde / Geochemistry》2021,81(1):125686
Aubrites are achondritic meteorites (enstatite pyroxenites) that were formed in highly reduced magmatic environments on a differentiated parent body sharing a common oxygen isotope reservoir with enstatite chondrites (EC), Earth and Moon, and could be considered as a geochemical model of the early proto-Earth. Some pyroxenes of the Pesyanoe aubrite have high abundance of gaseous inclusions, captured during the crystallization of the rocks. Investigation of the inclusions by IR spectroscopy reveals presence of OH− groups and C–H bonds. The former are assigned to protonated point defects in enstatite lattice and the latter to compounds occupying void walls. Molecular water and CO2 were not observed. Volatile components released from the samples of the Pesyanoe enstatite by stepwise crushing and heating are composed of CO2, H2O and a non-condensable phase. Hydrogen isotopic composition of volatiles extracted in form of molecular water in Px-separates varies in the range δD = −61 – −84‰ with mean value of δD = −73 ± 16‰ VSMOW and is within the ranges of ECs and Earth’s mantle. The total abundance of H2 in the pyroxene of Pesyanoe were estimated as at least 0.047 ppm that is too low in comparison with that of enstatite chondrites (≥30 ppm H2) and could indicate nearly complete degassing of the Pesyanoe primitive precursor material during the Pesyanoe parent body accretion or a mantle degassing in igneous differentiation process. In a last case a primitive precursor could have D/H ratio different from that of enstatite chondrites. 相似文献
3.
During the 1944 eruption of Vesuvius a sudden change occurred in the dynamics of the eruptive events, linked to variations
in magma composition. K-phonotephritic magmas were erupted during the effusive phase and the first lava fountain, whereas
the emission of strongly porphyritic K-tephrites took place during the more intense fountain. Melt inclusion compositions
(major and volatile elements) highlight that the magmas feeding the eruption underwent differentiation at different pressures.
The K-tephritic volatile-rich melts (up to 3 wt.% H2O, 3000 ppm CO2, and 0.55 wt.% Cl) evolved to reach K-phonotephritic compositions by crystallization of diopside and forsteritic olivine
at total fluid pressure higher than 300 MPa. These magmas fed a very shallow reservoir. The low-pressure differentiation of
the volatile-poor K-phonotephritic magmas (H2O<1 wt.%) involved mixing, open-system degassing, and crystallization of leucite, salite, and plagioclase. The eruption was
triggered by intrusion of a volatile-rich magma batch that rose from a depth of 11–22 km into the shallow magma chamber. The
first phase of the eruption represents the partial emptying of the shallow reservoir, the top of which is within the volcanic
edifice. The newly arrived magma mixed with that resident in the shallow reservoir and forced the transition from the effusive
to the lava fountain phase of the eruption.
Received: 14 September 1998 / Accepted: 10 January 1999 相似文献
4.
《Comptes Rendus Geoscience》2014,346(7-8):190-199
Melt inclusions (MIs) in quartz from granitoids in the northern Qinling belt were studied using microthermometry and laser Raman spectroscopy. The total homogenization of melt inclusions occurs in a mean range between 1050 and 1100 °C. Laser Raman experiments reveal H2O, C2H6, C4H6 and CH4 as the dominant volatile compounds. Our results provide insights into the temperatures of magma crystallization and the dominantly reducing environment during the early magmatic stage. Based on ore mineralogy, and on the volatile species content in the MIs, we evidence firstly that the Qiushuwan porphyry Cu–Mo deposit in the Qinling–Dabie–Sulu orogenic belt was derived from a reduced magmatic system, emplaced at relatively deep domains more than 10 km deep, and secondly, that the magmas that are responsible for the generation of Qiushuwan were either derived from an inherently reduced source, or reduced during ascent and emplacement. The mechanism might have involved the assimilation of sedimentary material with minimal crustal interaction. The parental magmas likely underwent reduction essentially by loss of all of their SO2 by degassing, as evidenced by the low S content in melt inclusions. These reduced materials provided adequate sulfur source for the formation of the porphyry Cu–Mo deposits with obvious zonation, which plays a key role in the mineralization; finally, we conclude that the reduced environment and the relatively deep domain of magma emplacement probably limited the extent of mineralization, generating only a relatively small Cu–Mo deposit in Qiushuwan, located within the northern Qinling accretionary belt. 相似文献
5.
Fluid sources for the La Guitarra epithermal deposit (Temascaltepec district, Mexico): Volatile and helium isotope analyses in fluid inclusions 总被引：1，自引：0，他引：1
Antoni Camprubí Beverly A. Chomiak Ruth E. Villanueva-Estrada David I. Norman Martin Stute 《Chemical Geology》2006,231(3):252-284
The La Guitarra deposit (Temascaltepec district, South-Central Mexico), belongs to the low/intermediate sulfidation epithermal type, has a polymetallic character although it is currently being mined for Ag and Au. The mineralization shows a polyphasic character and formed through several stages and sub-stages (named I, IIA, IIB, IIC, IID, and III). The previous structural, mineralogical, fluid inclusion and stable isotope studies were used to constrain the selection of samples for volatile and helium isotope analyses portrayed in this study. The N2/Ar overall range obtained from analytical runs on fluid inclusion volatiles, by means of Quadrupole Mass Spectrometry (QMS), is 0 to 2526, and it ranges 0 to 2526 for stage I, 0 to 1264 for stage IIA, 0 to 1369 for stage IIB, 11 to 2401 for stage IIC, 19 to 324 for stage IID, and 0 to 2526 for stage III. These values, combined with the CO2/CH4 ratios, and N2-He-Ar and N2-CH4-Ar relationships, suggest the occurrence of fluids from magmatic, crustal, and shallow meteoric sources in the forming epithermal vein deposit. The helium isotope analyses, obtained by means of Noble Gas Mass Spectrometry, display R/Ra average values between 0.5 and 2, pointing to the occurrence of mantle-derived helium that was relatively diluted or “contaminated” by crustal helium. These volatile analyses, when correlated with the stable isotope data from previous works and He isotope data, show the same distribution of data concerning sources for mineralizing fluids, especially those corresponding to magmatic and crustal sources. Thus, the overall geochemical data from mineralizing fluids are revealed as intrinsically consistent when compared to each other.The three main sources for mineralizing fluids (magmatic, and both deep and shallow meteoric fluids) are accountable at any scale, from stages of mineralization down to specific mineral associations. The volatile and helium isotope data obtained in this paper suggest that the precious metal-bearing mineral associations formed after hydrothermal pulses of predominantly oxidized magmatic fluids, and thus it is likely that precious metals were carried by fluids with such origin. Minerals from base-metal sulfide associations record both crustal and magmatic sources for mineralizing fluids, thus suggesting that base metals could be derived from deep leaching of crustal rocks. At the La Guitarra epithermal deposit there is no evidence for an evolution of mineralizing fluids towards any dominant source. Rather than that, volatile analyses in fluid inclusions suggest that this deposit formed as a pulsing hydrothermal system where each pulse or set of pulses accounts for different compositions of mineralizing fluids.The positive correlation between the relative content of magmatic fluids (high N2/Ar ratios) and H2S suggests that the necessary sulfur to carry mostly gold as bisulfide complexes came essentially from magmatic sources. Chlorine necessary to carry silver and base metals was found to be abundant in inclusion fluids and although there is no evidence about its source, it is plausible that it may come from magmatic sources as well. 相似文献
6.
Degassing and microlite crystallization during pre-climactic events of the 1991 eruption of Mt. Pinatubo, Philippines 总被引：2，自引：2，他引：0
Dacite tephras produced by the 1991 pre-climactic eruptive sequence at Mt. Pinatubo display extreme heterogeneity in vesicularity,
ranging in clast density from 700 to 2580 kg m–3. Observations of the 13 surge-producing blasts that preceded the climactic plinian event include radar-defined estimates
of column heights and seismically defined eruptive and intra-eruptive durations. A comparison of the characteristics of erupted
material, including microlite textures, chemical compositions, and H2O contents, with eruptive parameters suggests that devolatilization-induced crystallization of the magma occurred to a varying
extent prior to at least nine of the explosive events. Although volatile loss progressed to the same approximate level in
all of the clasts analyzed (weight percent H2O=1.26-1.73), microlite crystallization was extremely variable (0–22%). We infer that syn-eruptive volatile exsolution from
magma in the conduit and intra-eruptive separation of the gas phase was facilitated by the development of permeability within
magma residing in the conduit. Correlation of maximum microlite crystallinity with repose interval duration (28–262 min) suggests
that crystallization occurred primarily intra-eruptively, in response to the reduction in dissolved H2O content that occurred during the preceding event. Detailed textural characterization, including determination of three-dimensional
shapes and crystal size distributions (CSD), was conducted on a subset of clasts in order to determine rates of crystal nucleation
and growth using repose interval as the time available for crystallization. Shape and size analysis suggests that crystallization
proceeded in response to lessening degrees of feldspar supersaturation as repose interval durations increased. We thus propose
that during repose intervals, a plug of highly viscous magma formed due to the collapse of vesicular magma that had exsolved
volatiles during the previous explosive event. If plug thickness grew proportionally to the square root of time, and if magma
pressurization increased during the eruptive sequence, the frequency of eruptive pulses may have been modulated by degassing
of magma within the conduit. Dense clasts in surge deposits probably represent plug material entrained by each subsequent
explosive event.
Received: 4 December 1997 / Accepted: 13 September 1998 相似文献
7.
Apatite phenocrysts from the 1963 and 1723 eruptions of Irazú volcano (Costa Rica) record a volatile evolution history that
confirms previous melt inclusion studies, and provides additional information concerning the relative and absolute timing
of subvolcanic magmatic events. Measurements of H, Cl, and F by secondary ion mass spectrometry reveal multiple populations
of apatite in both 1723 and 1963 magmas. Assuming nominal apatite/melt partition coefficients allows us to compare the pattern
of melt inclusions and apatites in ternary space, demonstrating the fidelity of the record preserved in apatite, and revealing
a complex history of magma mixing with at least two components. The preservation of heterogeneous populations of apatite and
of internally heterogeneous crystals requires short timescales (days to years) for these magmatic processes to occur. 相似文献
8.
东昆仑夏日哈木镍铜硫化物矿床成矿岩浆条件:流体挥发份化学组成与碳同位素组成制约 总被引：4，自引：3，他引：1
夏日哈木镍铜硫化物矿床是我国东昆仑造山带新发现的全球岛弧环境最大的岩浆镍铜硫化物矿床。早泥盆世镁铁-超镁铁质成矿岩体中不同类型岩石的辉石中流体挥发份化学组成和碳同位素组成表明,流体挥发份总量较低,平均含量为888mm~3.STP/g(STP:标准温度和大气压)。流体挥发份组成以H_2O为主(48mol%),其次为H_2(26%)、CO_2(15%)和CO(5%)。H_2S含量从二辉橄榄岩(10mm~3/g)、橄榄辉石岩(18mm~3/g)到二辉辉石岩(28mm~3/g)逐渐增加,表明岩浆就位结晶演化过程中含硫组分的加入。CO_2的δ~(13)C值(-23.5‰~-5.0‰)位于地壳和地幔值范围之间。CH_4同系物碳同位素组成随碳数具有总体正序、局部反序的分布特征,显示大洋沉积有机质热裂解成因特征。夏日哈木成矿镁铁-超镁铁质岩体流体组分中较低的H2_O含量和较高的H_2含量表明,岩浆演化处于还原性挥发份条件,地幔岩浆源区存在俯冲洋壳沉积有机质,岩浆房围岩的混染和富S流体的加入可能是夏日哈木岩浆镍铜硫化物矿床硫饱和的主要机制。 相似文献
9.
Joseph A. Nuth III 《Earth, Moon, and Planets》2008,102(1-4):435-445
Is there an asteroid type or meteorite class that best exemplifies the materials that went into the Earth? Carbonaceous chondrites were once the objects of choice, and in the minds of many this choice is still valid. However, the origin of primitive chondritic meteorites is unclear. At the extremes they could either be fragments of very small parent bodies that never became hot enough to undergo geochemical modification other than mild lithification, or remnants of the uppermost layers of a body that had undergone a significant degree of internal differentiation, while the top layers remained cool due to radiative heat loss or loss of volatiles to space. This latter case is problematic if one considers these objects as precursors to the Earth since the timescale for the evolution of such a small body could be longer than the timescale for the accretion of the Earth. Large-scale circulation of materials in the primitive solar nebula could greatly increase the diversity of materials near 1 AU while also making the entire inner solar system both more homogeneous and much wetter than previously expected. The total mass of the nebula is an important, but poorly constrained factor controlling the growth of planetesimals. There is also a selection effect that dominates our sampling of the planetesimals that may have existed 4.5 billion years ago; namely, small fragile bodies are more likely to be lost from the system or ground down by collisions between small bodies, yet these are precisely those that may have dominated the population from which the Earth accreted. The composition of these aggregates could have played a very important role in the early chemical evolution of the Earth. In particular, the Earth may have been much wetter and richer in hydrocarbons and other reducing materials than previously suspected. 相似文献
10.
F. Zaccarini S. Morales-Ruano M. Scacchetti K. Heide 《Chemie der Erde / Geochemistry》2008,68(3):265-277
Datolite, ideally CaB[(OH/SiO4)], from hydrothermal veins crosscutting pillow basalt in 10 different localities of the Northern Apennine ophiolites was investigated with regard to mineral chemistry and fluid inclusion microthermometry. Bulk analyses of datolite crystals show REE contents below chondritic, except for La and Ce. With respect to host rock, datolite is occasionally enriched in La, Rb, Cs, Be, and shows relatively high contents of chalcophile elements (Cu, Zn, Pb, Ni) when occurring in contact with sulfide-mineralized basalt. Volatiles escaped during the decomposition in the temperature range 600 and 700 °C. The main component is water. The temperature maximum of water release is different and frequently with a shoulder or a second maximum. Together with water, sulfur species as H2S and SO2 and traces of boron species escaped. The CO2 release by the decomposition especially of datolite from Castellaro and Cinghi has a maximum in the range of 500-580 °C and is different from the decomposition of calcite. Together with CO2 a boron species escaped. Chlorine does not detect. Two-phase (L+V) fluid inclusions texturally identifiable as primary and secondary were observed, yielding average homogenization-temperatures of 236 and 173 °C, respectively. Fluid inclusion cooling data yield calculated salinity in the range of 10-16 wt% NaCl equivalents, thus relatively higher compared with seawater. The results are compatible with those reported for fluids formed under diagenetic conditions, but differ from those observed in seafloor hydrothermal systems and/or emanating from magmas. Distribution of trace elements between datolite and host basalt indicates enrichment with respect to the host rock limited to a few elements such as La, Rb, Cs, Be, Ni, Cu, Zn and Pb. The lithophile elements can be hosted in the datolite lattice, whereas the chalcophile metals and Ni are probably carried in sub-microscopic inclusions. 相似文献