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给出红外点源IRAS 20231 3440附近恒星形成区近红外．JHK’和H2成像观测结果，以及与该IRAS点源成协的近红外点源IRS1的K波段分光观测结果．．JHK’观测显示该区域存在嵌埋的年轻星天体，H2窄波段观测揭示了若干个氢分子发射结点，其中有几个结点排列成线形，暗示分子氢喷流的存在．喷流的北部与已知观测的分子外流成协，表明二者之间存在联系．喷流的走向提示IRS1可能是其激发源，对IRS1的K波段分光观测给出了进一步的证据．从近红外、MSX及IRAS资料估计出IRS1的能谱分布，表明它是一个处于ClassI状态的中等质量的年轻星天体． 相似文献
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Penelope J. WOZNIAKIEWICZ Hope A. ISHII Anton T. KEARSLEY Mark J. BURCHELL John P. BRADLEY Mark C. PRICE Nick TESLICH Martin R. LEE Mike J. COLE 《Meteoritics & planetary science》2012,47(4):708-728
Abstract– The grains returned by NASA’s Stardust mission from comet 81P/Wild 2 represent a valuable sample set that is significantly advancing our understanding of small solar system bodies. However, the grains were captured via impact at ～6.1 km s?1 and have experienced pressures and temperatures that caused alteration. To ensure correct interpretations of comet 81P/Wild 2 mineralogy, and therefore preaccretional or parent body processes, an understanding of the effects of capture is required. Using a two‐stage light‐gas gun, we recreated Stardust encounter conditions and generated a series of impact analogs for a range of minerals of cometary relevance into flight spare Al foils. Through analyses of both preimpact projectiles and postimpact analogs by transmission electron microscopy, we explore the impact processes occurring during capture and distinguish between those materials inherent to the impactor and those that are the product of capture. We review existing and present additional data on olivine, diopside, pyrrhotite, and pentlandite. We find that surviving crystalline material is observed in most single grain impactor residues. However, none is found in that of a relatively monodisperse aggregate. A variety of impact‐generated components are observed in all samples. Al incorporation into melt‐derived phases allows differentiation between melt and shock‐induced phases. In single grain impactor residues, impact‐generated phases largely retain original (nonvolatile) major element ratios. We conclude that both surviving and impact‐generated phases in residues of single grain impactors provide valuable information regarding the mineralogy of the impacting grain whilst further studies are required to fully understand aggregate impacts and the role of subgrain interactions during impact. 相似文献
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The temperatures at which pigeonite began to crystallize intholeiitic basalts and andesite of Hakone volcano range from1123 to 1019 ?C based on the three-pyroxene geothermometer ofIshii (1975). These values are lower than the temperatures ofother tholeiitic magmas of similar solidification index, suchas the magmas of Funagata-yama, O-shima, and Akita-komagatakevolcanoes and the Skaergaard intrusion. The cores of Ca-poorpyroxene phenocrysts formed in the Hakone subvolcanic magmareservoir are invariably orthopyroxene; the groundmass and microphenocrystpyroxenes crystallized in the lava during ascent and extrusionof magma are generally pigeonite, but orthopyroxene is alsopresent occasionally. The subvolcanic temperature-compositionpath [T-XFe path; XFe = Fe/(Mg + Fe), atomic ratio] of the Ca-poorpyroxenes does not intersect the pigeonite eutectoid reactionline (PER-line) of Ishii & Takeda (1974), whereas the lava-flowpaths characteristically intersect it at XFe values between0. 31 and 0–52. These two different kinds of T XFe pathsmay be interpreted as reflecting different solidus temperatures,and the content of volatiles, particularly water, appears tobe the controlling factor. It is suggested that the water contentof the magma increased because of fractional crystallizationof anhydrous minerals from a relatively hydrous magma in thesubvolcanic reservoir; then each erupted batch of the fractionatedmagma had its water content lowered by degassing as it ascendedto the volcano. Pigeonite is common in the groundmass of basalticrocks throughout the world, both extrusive and intrusive, butit is rare as phenocrysts in the former, a feature that mayalso be explained by the different solidus temperatures. Calc-alkalirocks in Hakone volcano appear to be derived by fractionationof hydrous tholeiitic magma. 相似文献
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J. M. PAQUE J. R. BECKETT H. A. ISHII A. ALÉON‐TOPPANI D. S. BURNETT N. TESLICH Z. R. DAI J. P. BRADLEY 《Meteoritics & planetary science》2009,44(5):665-687
Abstract— We used focused ion beam thin section preparation and scanning transmission electron microscopy (FIB/STEM) to examine the interfacial region between spinel and host melilite for spinel grains in type B1 inclusions from the Allende and Leoville carbonaceous chondrites. Boundary clinopyroxenes decorating spinel surfaces have compositions similar to those of coarser clinopyroxenes from the same region of the inclusion, suggesting little movement after formation. Host melilite displays no anomalous compositions near the interface and late‐stage minerals are not observed, suggesting that boundary pyroxenes did not form by crystallization of residual liquid. Allende spinels display either direct spinel‐melilite contact or an intervening boundary clinopyroxene between the two phases. Spinel‐melilite interfacial regions in a Leoville B1 are more complex, with boundary clinopyroxene, as observed in Allende, but also variable amounts of glass, secondary calcite, perovskite, and an Mg‐, Al‐, OH‐rich and Ca‐, Si‐poor crystalline phase that may be a layered double hydrate. One possible scenario of formation for the glass veins is that open system alteration of melilite produced a porous, hydrated aggregate of Mg‐carpholite or sudoite + aluminous diopside that was shock melted and quenched to a glass. The hydrated crystalline phase we observed may have been a shocked remnant of the precursor phase assemblage, but is more likely to have formed later by alteration of the glass. In the mantle, boundary clinopyroxenes may have been crystallized from Ti‐rich liquids formed by the direct dissolution of perovskite and an associated Sc‐Zr‐rich phase or as a reaction product between dissolving perovskite and liquid. In the core, any perovskite and associated Ti‐enriched liquids that may have originally been present disappeared before the growth of boundary clinopyroxene, and the observed boundary clinopyroxene may have nucleated and grown from the liquid, along with the larger core clinopyroxene. 相似文献
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随着地球系统科学研究的深入开展以及解决人类所面临的环境、资源、防灾等科学问题的需要，20世纪90年代以来，世界大陆、大洋科学钻探工程研究以及在钻孔深井内进行的地震、地球物理长期观测得到飞速发展，并取得了初步的观测研究成果。本文介绍了日本、德国、美国在深井长期观测方面的最新进展和科研成果，结合中国现实情况，展示了中国大陆科学钻探工程江苏东海现场开展深井地球物理综合观测的初步方案及其观测研究前景。该深井观测站将成为中国第一个无地面干扰的综合性深井地球物理和流体长期实验观测站，预期可以获取客观真实的深井综合地球物理资料，开创中国零干扰条件下地球科学观测研究的崭新局面。 相似文献
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Petrogenesis of Mafic Inclusions in Rhyolitic Lavas from Narugo Volcano, Northeastern Japan 总被引：1，自引：0，他引：1
Mafic inclusions present in the rhyolitic lavas of Narugo volcano,Japan, are vesiculated andesites with diktytaxitic texturesmainly composed of quenched acicular plagioclase, pyroxenes,and interstitial glass. When the mafic magma was incorporatedinto the silica-rich host magma, the cores of pyroxenes andplagioclase began to crystallize (>1000°C) in a boundarylayer between the mafic and felsic magmas. Phenocryst rim compositionsand interstitial glass compositions (average 78 wt % SiO2) inthe mafic inclusions are the same as those of the phenocrystsand groundmass glass in the host rhyolite. This suggests thatthe host felsic melt infiltrated into the incompletely solidifiedmafic inclusion, and that the interstitial melt compositionin the inclusions became close to that of the host melt (c.850°C). Infiltration was enhanced by the vesiculation ofthe mafic magma. Finally, hybridized and density-reduced portionsof the mafic magma floated up from the boundary layer into thehost rhyolite. We conclude that the ascent of mafic magma triggeredthe eruption of the host rhyolitic magma. KEY WORDS: mafic inclusion; stratified magma chamber; magma mixing; mingling; Narugo volcano; Japan 相似文献
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Volcanoes of the southwestern extension of the active Mariana island arc: New swath-mapping and geochemical studies 总被引：1，自引：0，他引：1
P. FRYER H. SUJIMOTO M. SEKINE L. E. JOHNSON J. KASAHARA H. MASUDA T. GAMO T. ISHII M. ARIYOSHI & K. FUJIOKA 《Island Arc》1998,7(3):596-607
Until recently it was thought that the volcanoes of the Mariana island arc of the western Pacific terminated at Tracey Seamount at ∼ 14°N immediately west of Guam. Sea floor mapping in 1995 shows a series of large volcanic seamounts stretching westward for nearly 300 km beyond that point. The morphology, spacing, and composition of those sampled are consistent with their having formed as a consequence of eruption of suprasubduction zone arc magmas. The relationships of the volcanoes to the tectonic processes of subduction of the Pacific plate beneath the southern portion of the Mariana convergent plate margin are becoming increasingly clear as new bathymetry and geochemical data are amassed. The volcanoes along this trend that lie closest to Guam are forming where the center of active extension in the back-arc basin intersects the line of arc volcanoes. They develop well-defined rifts that are parallel to rift structures along the extension center, whereas volcanoes of the spreading axis to the north are smaller than the frontal arc volcanoes and tend to form along lineaments. Compositions of lavas from these intersection volcanoes bear some similarities to back-arc basin basalt, but are on the whole well within the range of compositions for Mariana island arc lavas. The Pacific plate subducts nearly orthogonal to the strike of the trench along the southern part of the Mariana system and the distance to the arc line from the trench axis is only ∼ 150 km. Several deep fault-controlled canyons on the inner slope of the southern Mariana trench indicate an enhanced tectonic extension of this plate margin. The presence of these active arc volcanoes and the existence of the orthogonal normal faulting along the southern Mariana forearc supports a model of radial extension for formation of the Mariana Trough, a model previously dismissed because of the lack of evidence of these two major geological features. 相似文献
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HIDEKAZU MATSUEDA HISAYUKI YOSHIKAWA INOUE MASAO ISHII 《Tellus. Series B, Chemical and physical meteorology》2002,54(1):1-21
Abstract The spatial and temporal variations of atmospheric CO2 at 8–13 km from April 1993 to April 1999 were observed by measuring CO2 mixing ratios in samples collected biweekly from a commercial airliner between Australia and Japan. The CO2 growth rate showed a considerable interannual variation, with a maximum of about 3 ppm yr−1 during late 1997. This variation is related to the El Niño/Southern Oscillation (ENSO) events. A year-to-year change related to the ENSO events was also found in the latitudinal distribution pattern of the CO2 annual mean between 30°N and 30°S. The averaged CO2 seasonal cycle in the Northern Hemisphere gradually decayed toward the equator, and a relatively complicated variation with a double seasonal maximum appeared in the Southern Hemisphere. A significant yearly change of the seasonal cycle pattern was observed in the Southern Hemisphere. The impact of a tropical biomass-burning injection on the upper tropospheric CO2 was estimated on the basis of the CO data from the same airliner observation. 相似文献