Petrogenesis of lunar meteorite EET 96008     

Mahesh Anand  Lawrence A. Taylor  Gregory A. Snyder  Yuji Sano 《Geochimica et cosmochimica acta》2003,67(18):3499-3518

Lunar meteorite EET 96008 is a fragmental breccia that predominantly consists of basaltic mineral clasts (0.5-2 mm), along with minor lithic fragments and breccia clasts. The matrix consists mainly of smaller mineral fragments (<0.5 mm), bound by glassy cement, the majority of which are pyroxene and plagioclase. The pyroxene possesses extensive exsolution lamellae. These lamellae, up to 1 μm in width, are atypical for mare-basalts. One of the distinguishing textures of EET 96008 is the presence of small pockets (∼400 × 500 μm) of mesostasis areas consisting of coarse (∼20 μm) intergrowths of ferroaugite, fayalite and Si-rich glass. Laths of ilmenite, armalcolite, apatite and whitlockite are also distributed in these areas. Ilmenite grains are abundant and dispersed throughout the thin sections. Chromite and ulvöspinel are present but in minor abundance. Troilite, generally rare in this rock, occurs as several grains in one pyroxene crystal. FeNi metal is conspicuously absent from this meteorite.The molar Fe/Mn ratio in olivines and pyroxenes and the age of the meteorite are evidence for a lunar origin. The mineralogy of EET 96008 shows close affinity to a mare-basalt source, albeit with possible minor highland/non-mare components. The bulk-rock, major-, trace- and rare-earth-element (REE) contents are similar to that of very low-titanium (VLT) basalts, which have experienced extreme fractional crystallization to the point of silicate liquid immiscibility. Mineralogical and textural features of this sample suggest that at least some of the breccia components were derived from a slow-cooled magma. The mineralogy and petrology of EET 96008 is strikingly similar to the lunar meteorite EET 87521, and we support the conclusion that EET 96008 and EET 87521 should be paired.Isochron ages of 3530 ± 270 Ma for apatite and 3519 ± 100 Ma for whitlockite of this rock are consistent with derivation from a mare-basalt precursor. These ages are within error of the low-Ti basalts, dated from the Apollo 12 and 15 sites. The whole-rock, platinum-group-element (PGE) contents of EET 96008 overlap with pristine low-Ti mare basalts, suggesting the presence of only a minimal extraterrestrial component.  相似文献   

Re-os isotope systematics of the Taklimakan Desert sands, moraines and river sediments around the taklimakan desert, and of Tibetan soils     

Yuji Hattori  Masatoshi Honda 《Geochimica et cosmochimica acta》2003,67(6):1203-1213

Reported here are the first ¹⁸⁷Os/¹⁸⁸Os ratios and abundances of Os and Re for Taklimakan Desert sands and glacial moraines from the Kunlun Mountains. Osmium isotopic data are also reported for river sediments around the Taklimakan Desert, river sediments from the Kunlun and Tianshan Mountains, Tibetan soils and loesses from the Loess Plateau, as well as Sr and Nd isotopic data for these samples. The Taklimakan Desert sands from various regions show surprisingly homogeneous Os isotopic ratios (¹⁸⁷Os/¹⁸⁸Os = 1.29 ± 0.08) and abundances (Os = 11 ppt), with some variations in Re abundances (Re = 130 to 260 ppt) and ¹⁸⁷Re/¹⁸⁸Os ratios (60 to 140). The ¹⁸⁷Os/¹⁸⁸Os ratios for the Taklimakan Desert sands are close to the average for Kunlun moraines, river sediments around the Taklimakan Desert sands, and the Tibetan soils, supporting the idea that the Taklimakan Desert sands are derived from moraines and river sediments around the desert or from Tibetan soils and are homogenized by aeolian activity in the desert. Furthermore, the Os isotopic data for the sediments studied here are compared with those (¹⁸⁷Os/¹⁸⁸Os = 1.04, Os = 32 ppt, Re = 206 ppt, ¹⁸⁷Re/¹⁸⁸Os = 35) of loesses from the Loess Plateau reported elsewhere, and it is concluded that the Re-Os data for the loess can be used as proxy for the upper continental crust.  相似文献   

Adjustment of regularization in ill-posed linear inverse problems by the empirical Bayes approach   总被引：1，自引：0，他引：1  

Yuji Mitsuhata 《Geophysical Prospecting》2004,52(3):213-239

Regularization is the most popular technique to overcome the null space of model parameters in geophysical inverse problems, and is implemented by including a constraint term as well as the data‐misfit term in the objective function being minimized. The weighting of the constraint term relative to the data‐fitting term is controlled by a regularization parameter, and its adjustment to obtain the best model has received much attention. The empirical Bayes approach discussed in this paper determines the optimum value of the regularization parameter from a given data set. The regularization term can be regarded as representing a priori information about the model parameters. The empirical Bayes approach and its more practical variant, Akaike's Bayesian Information Criterion, adjust the regularization parameter automatically in response to the level of data noise and to the suitability of the assumed a priori model information for the given data. When the noise level is high, the regularization parameter is made large, which means that the a priori information is emphasized. If the assumed a priori information is not suitable for the given data, the regularization parameter is made small. Both these behaviours are desirable characteristics for the regularized solutions of practical inverse problems. Four simple examples are presented to illustrate these characteristics for an underdetermined problem, a problem adopting an improper prior constraint and a problem having an unknown data variance, all frequently encountered geophysical inverse problems. Numerical experiments using Akaike's Bayesian Information Criterion for synthetic data provide results consistent with these characteristics. In addition, concerning the selection of an appropriate type of a priori model information, a comparison between four types of difference‐operator model – the zeroth‐, first‐, second‐ and third‐order difference‐operator models – suggests that the automatic determination of the optimum regularization parameter becomes more difficult with increasing order of the difference operators. Accordingly, taking the effect of data noise into account, it is better to employ the lower‐order difference‐operator models for inversions of noisy data.  相似文献   

Petrochemical evidence for off-ridge magmatism in a back-arc setting from the Yakuno ophiolite, Japan   总被引：2，自引：0，他引：2  

Yuji Ichiyama  Akira Ishiwatari 《Island Arc》2004,13(1):157-177

Abstract The Permian ophiolite emplaced in the Yakuno area, Kyoto Prefecture, consists of metavolcanic sequences, metagabbro and a troctolitic intrusion. The metavolcanics are associated with thick mudstone through a contact that shows the flowage of lava over unconsolidated mud layers on the sea floor. The metavolcanics and metagabbro have rare earth element (REE) patterns that are similar to enriched (E)‐ and transitional (T)‐types ([La/Yb]_N = 0.77–11.2) of mid‐oceanic ridge basalts (MORB), whereas their Nb/La ratios (0.40–1.20) are as low as those of back‐arc basin basalts (BABB). Cr‐spinels in the metavolcanic rocks have Cr? of 40–73 and an Fe³⁺? of 9–24, numbers which are comparable to the values of BABB. These lines of evidence suggest that the Yakuno ophiolite originated more likely from an early stage back‐arc basin rather than from an oceanic plateau, as has been suggested by some researchers. The troctolitic body that intrudes as a 0.5‐km long lens in the metagabbro is composed of troctolite, olivine gabbro and microgabbro. The troctolite is marked by an olivine–plagioclase crystallization sequence, different from the commonly observed olivine–clinopyroxene sequence in other mafic/ultramafic cumulates of the Yakuno ophiolite. The microgabbro, with a composition close to that of the parental magma of the troctolite, is depleted in light REE ([La/Yb]_N = 0.18–0.55) so that it has an REE pattern that mimics normal (N)‐type MORB. The interstitial clinopyroxene of the troctolite has highly variable TiO₂ contents (0.2–1.4 wt%), which is interpreted to result from postcumulus crystallization of heterogeneous intercumulus melts. The troctolitic intrusion may represent a late stage intrusion that formed in an off‐ridge environment during sea floor spreading of the back‐arc basin. The geochemical variation observed in the Yakuno ophiolite, ranging from N‐ to E‐MORB affinities, reflects the changes in both mantle source compositions and processes involved in magma generation during the evolution of the back‐arc basin.  相似文献   

Japanese anchovy egg accumulation at the sea surface or pycnocline—Observations and model     

Yuji Tanaka 《Journal of Oceanography》1992,48(4):461-472

Near surface vertical distributions of Japanese anchovy eggs (isolated and pelagic) were studied at western Wakasa Bay, Japan. Samples were collected in horizontal tows with four plankton nets simultaneously operated at different four depths of 0, 0.5, 1.0, and 2.0 m. The egg concentration was found to decrease exponentially with depth. The egg concentration profile can be explained by considering the balance of the eggs' ascent and vertical diffusion. Taking further into account vertical difference in rising/sinking rates of the eggs, a clear accumulation of the eggs on a pycnocline, observed elsewhere, also can be explained. Vertical eddy diffusivity in the surface layer in a calm sea was 1–10 cm² s^–1, as estimated from the egg concentration profile and the velocities of the eggs in the vertical direction.  相似文献   

Preface     

Yoshihisa Shirayama  Kazuhiro Kogure  Peter G. Brewer  Takashi Ohsumi  Joji Ishizaka  Jun Kita  Yuji Watanabe 《Journal of Oceanography》2004,60(4):691-691

  相似文献   

<Emphasis Type="Italic">In situ</Emphasis> Enclosure Experiment Using a Benthic Chamber System to Assess the Effect of High Concentration of CO<Subscript>2</Subscript> on Deep-Sea Benthic Communities     

Hiroshi?IshidaEmail author  Yuji?Watanabe  Tatsuo?Fukuhara  Sho?Kaneko  Kazushi?Furusawa  Yoshihisa?Shirayama 《Journal of Oceanography》2005,61(5):835-843

In order to evaluate the environmental impact associated with sequestration of carbon dioxide in the deep sea, a free fall type field experimental device, the benthic chamber, was developed. In situ experiments to expose deep-sea communities to elevated concentrations of carbon dioxide (average of 20,000 ppm, 5,000 ppm and control) were carried out using this device 3 times, viz., in the winter of 2002 and in the spring and the summer of 2003, in the Kumano Trough at a depth of 2,000 m. In the long-term experiments (about two weeks in winter of 2002 and summer of 2003), the abundance of meiobenthos declined whereas that of bacteria increased under the condition of 20,000 ppm carbon dioxide compared with the control. Among meiofauna, the abundance of foraminifers at the same concentration of carbon dioxide became less than the control even in the short-term (3 days in spring of 2003) experiment, suggesting that organisms with a calcium carbonate exoskeleton are more sensitive to the raised concentration of carbon dioxide. The respiration rate of the benthic community exposed to 20,000 ppm was lower in the early stage of the experiment than in the latter half, whereas it was opposite under the condition of 5,000 ppm. The increase of biological activity in the 20,000 ppm exposure group is probably due to an increase of bacteria adapted to high carbon dioxide concentrations. The present results suggest that the influence of carbon dioxide on the deep-sea benthic ecosystem does not follow a simple, linear relationship with concentration.  相似文献   

Measurement of Noble Gas Solubility in Seawater Using a Quadrupole Mass Spectrometer     

Yuji?SanoEmail author  Naoto?Takahata 《Journal of Oceanography》2005,61(3):465-473

A quadrupole-based mass spectrometric system for determining noble gas (He, Ne, Ar, Kr and Xe) abundances in a liquid sample has been developed and applied to seawater equilibrated with the atmosphere at several temperatures. After known amounts of isotopic spikes (²²Ne, ³⁶Ar, ⁸⁶Kr and ¹²⁴Xe) were introduced into the preparation vacuum line, dissolved gases were extracted from seawater and well mixed with the spikes by ultrasonic vibration. Noble gases were purified using three-stage hot Ti getters and separated by two activated charcoal traps held at low temperature (liquid nitrogen and dry ice—ethanol). Noble gas abundances were measured by a relatively inexpensive quadrupole mass spectrometer based on the isotope dilution technique. Precisions obtained by repeated measurements for He, Ne, Ar, Kr and Xe are 1.5%, 0.4%, 0.4%, 0.4% and 0.6%, respectively. Noble gas abundances in air-saturated seawater at eight temperature steps (1.0°C, 5.5°C, 10.0°C, 14.4°C, 17.0°C, 21.3°C, 24.6°C, and 29.6°C) were measured using the analytical system. The overall variation of the abundances with temperature agrees well with those of NaCl brines reported in the literature. We propose here new constants to fit observed data to empirical equation of noble gas solubility in seawater with its temperature variation.  相似文献   

江西弋阳晚白垩世塘边组风成砂岩碎屑锆石U-Pb定年及其物源意义     

王宇佳  陈留勤  李文灏  李鹏程 《地质通报》2019,38(4):667-679

赣东北信江盆地晚白垩世圭峰群塘边组以发育大型高角度交错层理的风成砂岩为特征,总体为干旱气候条件下沙漠沉积环境的产物。该地区所采砂岩样品为紫红色中-细粒长石石英砂岩,碎屑颗粒主要包括石英、长石、云母和岩屑,多呈次圆状,分选性较好。利用碎屑锆石LA-ICP-MS测年法,对塘边组风成砂岩进行U-Pb同位素定年,分析物源。碎屑锆石颗粒大多数大于100μm,Th/U值为0.1～2.1,且大部分锆石内部具有清晰的振荡环带结构,表明多数为岩浆锆石。~(206)Pb/~(238)U年龄加权平均值为141.4±1.2Ma。锆石U-Pb年龄主要集中于5个年龄段,分别是137～170Ma、431～506Ma、798～1172Ma、1268～2493Ma、2501～3488Ma。这些主要年龄区间与中国东南地区已知的岩浆事件对应,分别为燕山运动、加里东运动、晋宁运动、吕梁运动。其中,燕山期酸性火山-侵入杂岩提供了主要物源。结合风成砂岩交错层理反映的古风向数据,认为弋阳塘边组碎屑物质主要来自盆地北西部的九岭地区及北东部地区。  相似文献   

Magnetotelluric survey for exploration of a volcanic-rock reservoir in the Yurihara oil and gas field,Japan*     

Yuji Mitsuhata  Koichi Matsuo  Masato Minegishi 《Geophysical Prospecting》1999,47(2):195-218

The Yurihara oil and gas field is located on the southern edge of Akita Prefecture, northeastern Japan. In this area, drilling, surface geological surveys and many seismic surveys have been used to investigate the geological structure. Wells drilled into the Nishikurosawa Basalt Group (NBG) of Miocene age found oil and gas reservoirs at depths of 1.5–2 km. Oil and gas are now being produced commercially and further exploration is required in the surrounding areas. However, since the neighbouring areas are covered with young volcanic products from the Chokai volcano, and have a rough topography, the subsurface distribution of the NBG must be investigated using other methods in addition to seismic reflection. According to the well data, the resistivity of the NBG is comparatively higher than that of the overlying sedimentary formations, and therefore the magnetotelluric (MT) method is expected to be useful for the estimation of the distribution of the NBG. An MT survey was conducted along three survey lines in this area. Each line trended east–west, perpendicular to the regional geological strike, and was composed of about 25 measurement sites. Induction vectors evaluated from the magnetic field show that this area has a two-dimensional structure. The evaluated resistivity sections are in agreement with the log data. In conclusion, we were able to detect resistive layers (the NBG) below conductive layers. The results indicate that the NBG becomes gradually less resistive from north to south. In the centre of the northern line, an uplifted resistive area is interpreted as corresponding to the reservoir. By comparison with a seismic section, we prove the effectiveness of the integration of seismic and MT surveys for the investigation of the morphology and internal structure of the NBG. On other survey lines, the resistive uplifted zones are interpreted as possible prospective areas.  相似文献