Publishing type：Research paper (scientific journal)   Publisher：Mary Ann Liebert Inc  

DOI： 10.1089/ast.2021.0158

researchmap

Other Link： https://www.liebertpub.com/doi/pdf/10.1089/ast.2021.0158

Publishing type：Research paper (scientific journal)   Publisher：Japan Academy  

DOI： 10.2183/pjab.98.015

researchmap

Publishing type：Research paper (scientific journal)   Publisher：Geological Society of America  

Abstract

Lithium is of great interest as a tracer of metamorphic reactions and related fluid-mineral interactions because of its potential to isotopically fractionate during inter- and intracrystalline diffusional processes. Study of its transfer through subduction zones, based on study of arc volcanic and metamorphic rocks, can yield insight regarding ocean-to-mantle chemical cycling.

We investigated major- and trace-element concentrations and δ7Li in garnet in ultrahigh-pressure (UHP) Lago di Cignana metasedimentary rocks, relating these observations to reconstructed prograde devolatilization history. In all garnet crystals we studied, heavy rare earth elements (HREEs), Y, and Li showed strong zoning, with elevated concentrations in cores (15–50 ppm Li) and marked high-concentration anomalies (up to 117 ppm Li, 5500 ppm Y; little or no major-element shift) as growth annuli, in which some crystals showed subtle elevation in δ7Li greater than analytical error of ~3% (2σ). Rutile inclusions appeared abruptly at annuli and outward toward rims, accompanied by inclusions of a highly zoned, Ca- and rare earth element–rich phase and decreased Nb concentrations in garnet. These relationships are interpreted to reflect prograde garnet-forming reaction(s), in part involving titanite breakdown to stabilize rutile, which resulted in delivery of more abundant Y and HREEs at surfaces of growing garnet crystals to produce annuli. Co-enrichments in Li and Y + REEs are attributed to mutual incorporation via charge-coupled substitutions; thus, increased Li uptake was a passive consequence of elevated concentrations of Y + REEs. The small-scale fluctuations in δ7Li (overall range of ~9%) observed in some crystals may correlate with abrupt shifts in major- and trace-element concentrations, suggesting that changes in reactant phases exerted some control on the evolution of δ7Li. For one garnet crystal, late-stage growth following partial resorption produced deviation in major- and trace-element compositions, including Li concentration, accompanied by a 10%–15% negative shift in δ7Li, perhaps reflecting a change in the mechanism of incorporation or source of Li.

These results highlight the value of measuring the major- and trace-element and isotope compositions of garnets in high-pressure and UHP metamorphic rocks in which matrix mineral assemblages are extensively overprinted by recrystallization during exhumation histories. Lithium concentrations and isotope compositions of the garnets can add valuable information regarding prograde (and retrograde) reaction history, kinetics of porphyroblast growth, intracrystalline diffusion, and fluid-rock interactions. This work, integrated with previous study of devolatilization in the Schistes Lustrés/Cignana metasedimentary suite, indicates retention of a large fraction of the initially subducted sedimentary Li budget to depths approaching those beneath volcanic fronts, despite the redistribution of this Li among mineral phases during complex mineral reaction histories.

DOI： 10.1130/ges02473.1

researchmap

Language：English   Publishing type：Research paper (scientific journal)   Publisher：Elsevier {BV}  

DOI： 10.1016/j.lithos.2022.106609

researchmap

Language：English   Publishing type：Research paper (scientific journal)   Publisher：Wiley  

Sample return missions represent great opportunities to study terrestrially uncontaminated solar system materials. However, the size of returned samples will be limited, and thus, it is necessary to understand the most appropriate techniques to apply. Accordingly, the sensitivity of laser ablation inductively coupled plasma mass spectrometry (LA-ICPMS) and secondary ion mass spectrometry (SIMS) was compared through the analyses of trace elements in reference materials and the Allende CV3 chondrite. While the SIMS method was found to be more sensitive than the laser method toward all elements of interest, the LA-ICPMS appears to be more suitable in terms of precision for certain elements. Using both analytical techniques, we measured chemical composition of an Allende chondrule and its igneous rim. These data were used to understand the nature of the reservoir that interacted with the host chondrule during formation of its igneous rim. We find that the igneous rim is enriched in silica, alkalis, and rare earth elements compared to the host chondrule. We suggest that the igneous rim could be explained by melting of a mixture of the chondrule-like and REE-enriched CAI-like precursors that accreted on the surface of the host chondrule followed by gas-melt interaction with a silica- and alkali-rich gas. Alternatively, these observations could be interpreted as a result of interaction between the chondrule and the melt resulting from partial melting of a pre-existing planetesimal in the early stages of its differentiation.

DOI： 10.1111/maps.13665

Web of Science

researchmap

Language：English   Publishing type：Research paper (scientific journal)   Publisher：American Geophysical Union ({AGU})  

DOI： 10.1029/2021je007052

researchmap

Other Link： https://onlinelibrary.wiley.com/doi/full-xml/10.1029/2021JE007052

Language：English   Publishing type：Research paper (scientific journal)   Publisher：Mary Ann Liebert Inc  

DOI： 10.1089/ast.2019.2107

researchmap

Language：English   Publishing type：Research paper (scientific journal)   Publisher：Elsevier {BV}  

DOI： 10.1016/j.micromeso.2019.03.050

researchmap

Publishing type：Research paper (scientific journal)  

Carbonaceous chondrites contain many abiotic organic compounds, some of which are found in life on Earth. Both the mineral and organic matter phases, of these meteorites, have been affected by aqueous alteration processes. Whilst organic matter is known to be associated with phyllosilicate phases, no such relationship has yet been identified for specific organic compound classes. Furthermore, ongoing sample return missions, Hyabusa 2 and OSIRIS-Rex, are set to return potentially organic rich C-type asteroid samples to the Earth. Consequently, strategies to investigate organic-mineral relationships are required. Here we report spatial data for free/soluble organic matter (FOM/SOM) components (akylimidazole and alkylpyridine homologues) and mineral phases. Low and intermediate molecular weight alkylimidazole homologues are more widely distributed than higher molecular weight members, likely due to their affinity for the aqueous phase. On aqueous alteration of anhydrous mineral phases, transported FOM is adsorbed onto the surface or into the interlayers of the resulting phyllosilicates and thus concentrated and protected from oxidising fluids. Therefore, aiding the delivery of biologically relevant molecules to earth, shortly preceding the origin of life.

DOI： 10.7185/geochemlet.2010

Scopus

researchmap

Language：English   Publishing type：Research paper (scientific journal)   Publisher：Mary Ann Liebert Inc  

Boron is associated with several Archean stromatolite deposits, including the tourmaline-rich Barberton stromatolites in South Africa and tourmaline-bearing pyritic laminae associated with stromatolites of the 3.48 Ga Dresser Formation in the Pilbara Craton, Australia. Boron is also a critical element in prebiotic organic chemistry, including in the formation of ribose, a crucial component in RNA. As geological evidence and advances in prebiotic chemistry are now suggesting that hot spring activity may be associated with the origins of life, an understanding of boron and its mobility and isotopic fractionation in geothermal settings may provide important insights into the setting for the origin of life. Here, we report on the boron isotopic compositions and elemental concentrations in a range of fluid, sediment, and mineral samples from the active, boron-rich Puga geothermal system in the Himalayas, India. This includes one of the lowest boron isotope values ever recorded in modern settings: diatom-rich sediments (delta B-11 = -41.0 parts per thousand) in a multiphase fractionation system where evaporation is not the dominant form of isotope fractionation. Instead, the extreme boron isotopic fractionation is ascribed to the incorporation of tetrahedral B-10 borate anions in precipitating amorphous silica. These findings expand the known limits and drivers of boron isotope fractionation, as well as provide insight into the concentration and fractionation of boron in Archean hot spring environments.

DOI： 10.1089/ast.2018.1966

Web of Science

researchmap

Language：English   Publishing type：Research paper (scientific journal)  

DOI： 10.1016/j.precamres.2019.105475

researchmap

Language：English   Publishing type：Research paper (scientific journal)   Publisher：PERGAMON-ELSEVIER SCIENCE LTD  

We report in situ ion-microprobe analyses of Li- and O-isotope compositions for olivine, low-Ca pyroxene, high-Ca pyroxene, and chondrule mesostasis/plagioclase in nine chondrules from the Allende CV3 chondrite. Based on their mineralogy and O-isotope compositions, we infer that the chondrule mesostasis/plagioclase and ferroan olivine rims were extensively modified or formed during metasomatic alteration and metamorphism on the Allende parent asteroid. We excluded these minerals in order to determine the correlations between Li and both O and the chemical compositions of olivines and low-Ca pyroxenes in the chondrules and their igneous rims. Based on the O-isotope composition of the olivines, nine chondrules were divided into three groups. Average Delta O-17 of olivines (Fo(>65)) in group 1 and 2 chondrules are -5.3 +/- 0.4 and -6.2 +/- 0.4 parts per thousand, respectively. Group 3 chondrules are characterized by the presence of O-16-rich relict grains and the Delta O-17 of their olivines range from -23.7 to -6.2 parts per thousand. In group 1 olivines, as Fa content increases, variation of delta Li-7 becomes smaller and delta Li-7 approaches the whole-rock value (2.4 parts per thousand; Seitz et al., 2012), suggesting nearly complete Li-isotope equilibration. In group 2 and 3 olivines, variation of delta Li-7 is limited even with a significant range of Fa content. We conclude that Li-isotope compositions of olivine in group 1 chondrules were modified not by an asteroidal process but by an igneous-rim formation process, thus chondrule olivines retained Li-isotope compositions acquired in the protosolar nebula. In olivines of the group 3 chondrule PO-8, we observed a correlation between O and Li isotopes: In relict O-16-rich olivine grains with Delta O-17 of similar to-25 to -20 parts per thousand, delta Li-7 ranges from -23 to -3 parts per thousand; in olivine grains with Delta O-17 > -20 parts per thousand, delta Li-7 is nearly constant (-8 +/- 4 parts per thousand). Based on the Li-isotope composition of low-Ca pyroxenes, which formed from melt during the crystallization of host chondrules and igneous rims, the existence of a gaseous reservoir with a delta Li-7 similar to -11 parts per thousand is inferred. (C) 2019 Elsevier Ltd. All rights reserved.

DOI： 10.1016/J.GCA.2019.02.038

Web of Science

researchmap

Language：English   Publishing type：Research paper (scientific journal)   Publisher：JAPAN ACAD  

A comprehensive geochemical study of the Chelyabinsk meteorite reveals further details regarding its history of impact-related fragmentation and melting, and later aqueous alteration, during its transit toward Earth. We support an similar to 30 Ma age obtained by Ar-Ar method (Beard et al., 2014) for the impact-related melting, based on Rb-Sr isotope analyses of a melt domain. An irregularly shaped olivine with a distinct 0 isotope composition in a melt domain appears to be a fragment of a silicate-rich impactor. Hydrogen and Li concentrations and isotopic compositions, textures of Fe oxyhydroxides, and the presence of organic materials located in fractures, are together consistent with aqueous alteration, and this alteration could have pre-dated interaction with the Earth's atmosphere. As one model, we suggest that hypervelocity capture of the impact-related debris by a comet nucleus could have led to shock-wave-induced supercritical aqueous fluids dissolving the silicate, metallic, and organic matter, with later ice sublimation yielding a rocky rubble pile sampled by the meteorite.

DOI： 10.2183/pjab.95.013

Web of Science

PubMed

researchmap

Language：English   Publishing type：Research paper (scientific journal)   Publisher：Springer Nature  

DOI： 10.1038/s41598-018-28219-x

researchmap

Other Link： http://www.nature.com/articles/s41598-018-28219-x

Language：English   Publishing type：Research paper (scientific journal)   Publisher：Japan Association of Mineralogical Sciences  

<p>Omphacite replacing after relic edenitic pargasite has been found in an omphacite–bearing jadeitite block of the Itoigawa–Omi area in the Hida–Gaien belt. Omphacite occurs sporadically as fine–grained aggregate reaching a few cm in length in a jadeite–albite matrix, and sometimes contains edenitic pargasite as a core. The edenitic pargasite is chemically and optically homogeneous and does not show direct contact with jadeite and albite. An irregular shaped omphacite–diopside mixed area occurs near edenitic pargasite in a coarse omphacite aggregate. The texture suggests that the breakdown of edenitic pargasite was triggered by the addition of a hydrothermal fluid, from which jadeite and albite were precipitated later, passing through diopside and omphacite by the reaction:</p><p>&nbsp;</p><p><img align="middle" src="./Graphics/abst-170402a.jpg"/> </p><p>&nbsp;</p><p>At the periphery of pseudomorphic omphacite, a hydrothermal fluid removed the breakdown components of the reaction other than omphacite.</p><p>&emsp;New in–situ LA–ICP–MS U–Pb dating revealed that zircons in edenitic pargasite yield apparent age up to ~ 590 Ma, with mean ages of 560 ± 16 Ma, interpreted as the minimum age of a precursor rock. A zircon age of 519 ± 21 Ma from jadeitite without omphacite corresponds to a timing of crystallization of omphacite, jadeite, and albite. The studied jadeitite is a typical R–type jadeitite, and the nearly total replacement from a precursor rock to the omphacite–bearing jadeitite has been attributed to hydrothermal activity at Middle Cambrian times.</p>

DOI： 10.2465/JMPS.170402A

Web of Science

CiNii Article

researchmap

Publishing type：Research paper (scientific journal)  

DOI： 10.2138/am-2016-5359

Scopus

researchmap

Publishing type：Research paper (scientific journal)  

We report ion microprobe U-Th-Pb geochronology of in situ zircon from the Himalayan high- and ultrahigh-pressure eclogites, Kaghan Valley of Pakistan. Combined with the textural features, mineral inclusions, cathodoluminescence image information and the U-Th-Pb isotope geochronology, two types of zircons were recognized in Group I and II eclogites. Zircons in Group I eclogites are of considerably large size (&gt;100. μm up to 500. μm). A few grains are euhederal and prismatic, show oscillatory zoning with distinct core-rim luminescence pattern. Several other grains show irregular morphology, mitamictization, embayment and boundary truncations. They contain micro-inclusions such as muscovite, biotite, quartz and albite. Core or middle portions of zircons from Group I eclogites yielded concordant U-Th-Pb age of 267.6±2.4. Ma (MSWD=8.5), have higher U and Th contents with a Th/U ratio. &gt;1, indicating typical magmatic core domains. Middle and rim or outer portions of these zircons contain inclusions of garnet, omphacite, phengite and these portions show no clear zonation. They yielded discordant values ranging between 210 and 71. Ma, indicating several thermal or Pb-loss events during their growth and recrystalization prior to or during the Himalayan eclogite-facies metamorphism. Zircons in Group II eclogites are smaller in size, prismatic to oval, display patchy or sector zoning and contain abundant inclusions of garnet, omphacite, phengite, quartz, rutile and carbonates. They yielded concordant U-Th-Pb age of 44.9±1.2. Ma (MSWD=4.9). The lower U and Th contents and a lower Th/U ratio (&lt;0.05) in these zircons suggest their formation from the recrystallization of the older zircons during the Himalayan high and ultrahigh-pressure eclogite-facies metamorphism. © 2012 Elsevier Ltd.

DOI： 10.1016/j.jseaes.2012.04.025

Web of Science

Scopus

researchmap

Language：English   Publishing type：Research paper (other academic)  

DOI： 10.5772/32859

researchmap

Publishing type：Research paper (scientific journal)  

DOI： 10.1016/j.chemgeo.2010.11.001

Scopus

researchmap

Publishing type：Research paper (scientific journal)  

DOI： 10.5026/JGEOGRAPHY.120.52

Web of Science

CiNii Article

researchmap

Publishing type：Research paper (scientific journal)  

DOI： 10.1016/j.gr.2010.02.009

Scopus

researchmap

Publishing type：Research paper (scientific journal)  

Web of Science

researchmap

Language：English   Publishing type：Research paper (scientific journal)   Publisher：Elsevier B.V.  

DOI： 10.1016/j.lithos.2009.05.018

Scopus

CiNii Article

CiNii Books

researchmap

Publishing type：Research paper (scientific journal)  

DOI： 10.1016/j.lithos.2009.05.020

Scopus

researchmap

Publishing type：Research paper (scientific journal)  

DOI： 10.1016/j.rgg.2007.09.011

Scopus

researchmap

Publishing type：Research paper (scientific journal)  

DOI： 10.1016/j.gr.2007.11.003

Scopus

CiNii Article

researchmap

Publisher：GEOCHEMICAL SOCIETY OF JAPAN  

DOI： 10.14862/geochemproc.55.0.67.0

CiNii Article

researchmap

Publishing type：Research paper (scientific journal)  

DOI： 10.1016/j.gr.2006.04.007

Scopus

CiNii Article

researchmap

Publishing type：Research paper (scientific journal)  

DOI： 10.1016/j.gr.2006.04.013

Scopus

researchmap

Publishing type：Research paper (scientific journal)  

DOI： 10.1016/j.sedgeo.2007.07.005

Scopus

CiNii Article

researchmap

Publishing type：Research paper (scientific journal)   Publisher：Superplumes: Beyond Plate Tectonics  

DOI： 10.1007/978-1-4020-5750-2_13

Scopus

researchmap

Publishing type：Research paper (scientific journal)  

DOI： 10.1016/j.jseaes.2007.03.001

Scopus

researchmap

Publishing type：Research paper (scientific journal)  

DOI： 10.1016/j.lithos.2007.04.003

Scopus

researchmap

Language：Japanese   Publisher：The Geological Society of Japan  

DOI： 10.14863/geosocabst.2007.0.475.0

CiNii Article

researchmap

Publishing type：Research paper (scientific journal)  

DOI： 10.2747/0020-6814.47.10.1058

Web of Science

Scopus

researchmap

Publishing type：Research paper (scientific journal)  

DOI： 10.1016/j.lithos.2004.01.001

Scopus

researchmap

Publishing type：Research paper (scientific journal)  

DOI： 10.1016/j.precamres.2004.03.009

Scopus

researchmap

Language：English   Publishing type：Research paper (scientific journal)   Publisher：The Japan Academy  

The Baratal limestone in the Gorny Altai Mountains, southern Siberia, occurs as large allochthonous blocks within a Cambrian accretionary complex that developed around the Siberia craton. Before the final accretion to Siberia in the Cambrian, the terrigenous clastic-free Baratal limestone was deposited directly upon a basaltic basement with a geochemical signature identical to that of modern oceanic plateau. The Baratal limestone with 598&plusmn;25 Ma (Early Vendian) Pb-Pb isochron age consists of three distinct facies; 1) massive lime mudstone with ooids and stromatolites, 2) bedded lime mudstone, and 3) limestone conglomerate/breccia dominated by ooid-bearing lime mudstone clasts. The first represents a shallow marine environment on top of an ancient oceanic plateau, while the latter two represent the deeper slope to bottom-of-slope facies of a plateau. The Vendian Baratal limestone provides the oldest example of a reconstructed shallow marine carbonate buildup complex developed on a plateau/seamount in a mid-ocean.<br> <br> <br> (Communicated by Tatsuro MATSUMOTO, M.J.A.)<br>

DOI： 10.2183/pjab.80.422

Scopus

CiNii Article

CiNii Books

researchmap

Publishing type：Research paper (scientific journal)  

Web of Science

researchmap

Publisher：Tokyo Geographical Society  

DOI： 10.5026/jgeography.112.4_Plate9

CiNii Article

researchmap

Language：Japanese   Publisher：The Geological Society of Japan  

DOI： 10.14863/geosocabst.2002.0_239_2

CiNii Article

CiNii Books

researchmap

Publishing type：Research paper (scientific journal)  

DOI： 10.2747/0020-6814.44.9.819

Web of Science

Scopus

researchmap

Publishing type：Research paper (scientific journal)  

DOI： 10.2747/0020-6814.44.9.837

Web of Science

Scopus

researchmap

Publishing type：Research paper (scientific journal)  

Web of Science

Scopus

researchmap

Publishing type：Research paper (scientific journal)  

Web of Science

Scopus

researchmap

Publishing type：Research paper (scientific journal)  

Scopus

researchmap

Publishing type：Research paper (scientific journal)  

Scopus

researchmap

Publishing type：Research paper (scientific journal)  

DOI： 10.1046/j.1440-1738.2000.00278.x

Scopus

researchmap

Publishing type：Research paper (scientific journal)  

DOI： 10.1046/j.1440-1738.2000.00282.x

Scopus

CiNii Article

researchmap

Language：Japanese   Publisher：The Geological Society of Japan  

DOI： 10.14863/geosocabst.1999.0_305_2

CiNii Article

CiNii Books

researchmap

Language：Japanese   Publisher：The Geological Society of Japan  

DOI： 10.14863/geosocabst.1998.0_444

CiNii Article

researchmap

Language：Japanese   Publisher：The Geological Society of Japan  

DOI： 10.14863/geosocabst.1998.0_513

CiNii Article

researchmap

Language：Japanese   Publisher：The Geological Society of Japan  

DOI： 10.14863/geosocabst.1998.0_431

CiNii Article

researchmap

Language：Japanese   Publisher：The Geological Society of Japan  

DOI： 10.14863/geosocabst.1998.0_432

CiNii Article

researchmap

Publishing type：Research paper (scientific journal)  

researchmap

Language：Japanese   Publisher：The Geological Society of Japan  

DOI： 10.14863/geosocabst.1997.0_193_1

CiNii Article

CiNii Books

researchmap

Language：Japanese   Publisher：The Geological Society of Japan  

DOI： 10.14863/geosocabst.1997.0_200_2

CiNii Article

researchmap

Language：Japanese   Publisher：The Geological Society of Japan  

DOI： 10.14863/geosocabst.1997.0_201_1

CiNii Article

researchmap

Publishing type：Research paper (scientific journal)  

Scopus

researchmap

Publishing type：Research paper (scientific journal)  

Scopus

researchmap

Language：English   Publisher：MINERALOGICAL SOC AMER  

Partially crystalline hornblende gabbro inclusions from the Little Glass Mountain Rhyolite contain euhedral plagioclase, orthopyroxene, hornblende, and apatite crystals in contact with interstitial rhyolitic (71-76% SiO(2)) glass. Textural and mineral compositional data indicate that the gabbros crystallized sufficiently slowly that surface equilibrium was closely approached at the interface between crystals and the liquid. This rare occurrence represents a natural dynamic crystallization experiment with a "run time" that is not realistically achievable in the laboratory. SIMS analysis of mineral rim-glass pairs have permitted the determination of high-quality, equilibrium trace-element partition coefficients for all four minerals. These data augment the limited partition coefficient database for minerals in high-SiO(2) rhyolitic systems. For all minerals, the D values are consistent with those anticipated from crystal-chemical considerations. These data further support a liquid SiO(2) control on the REEs (and presumably other elements) partitioning wherein D values systematically increase with increasing liquid SiO(2) content.

DOI： 10.2138/am.2011.3857

Web of Science

researchmap

Language：English   Publisher：ELSEVIER SCIENCE BV  

In this paper, Late Miocene blueschist and eclogite belts, including the world's youngest blueschist belt in Timor-Tanimbar Island chain, eastern Indonesia, and the world's youngest coesite-bearing eclogite, Papua New Guinea, together with selected Cenozoic high-pressure and ultrahigh-pressure metamorphic rocks are reviewed. From a synthesis of the geology, metamorphism and chronology of these rocks, the formation and exhumation process are evaluated and the significance on tectonics at convergent plate boundaries is discussed. (c) 2010 International Association for Gondwana Research. Published by Elsevier B.V. All rights reserved.

DOI： 10.1016/j.gr.2010.02.013

Web of Science

Scopus

researchmap

Language：English   Publisher：ELSEVIER SCIENCE BV  

In this paper, Late Miocene blueschist and eclogite belts, including the world's youngest blueschist belt in Timor-Tanimbar Island chain, eastern Indonesia, and the world's youngest coesite-bearing eclogite, Papua New Guinea, together with selected Cenozoic high-pressure and ultrahigh-pressure metamorphic rocks are reviewed. From a synthesis of the geology, metamorphism and chronology of these rocks, the formation and exhumation process are evaluated and the significance on tectonics at convergent plate boundaries is discussed. (c) 2010 International Association for Gondwana Research. Published by Elsevier B.V. All rights reserved.

DOI： 10.1016/j.gr.2010.02.013

Web of Science

researchmap

DOI： 10.1016/j.lithos.2009.01.013

Scopus

researchmap

Language：English   Publisher：PERGAMON-ELSEVIER SCIENCE LTD  

Subduction of lithosphere, involving surficial materials, into the deep mantle is fundamental to the chemical evolution of the Earth. However, the chemical evolution of the lithosphere during subduction to depth remains equivocal. In order to identify materials subjected to geological processes near the surface and at depths in subduction zones, we examined B and Li isotopes behavior in a unique diamondiferous, K-rich tourmaline (K-tourmaline) from the Kokchetav ultrahigh-pressure metamorphic belt. The K-tourmaline, which includes microdiamonds in its core, is enriched in B-11 relative to B-10 (delta B-11 = -1.2 to +7.7) and Li-7 relative to Li-6 (delta Li-7 = -1.1 to +3.1). It is suggested that the K-tourmaline crystallized at high-pressure in the diamond stability field from a silicate melt generated at high-pressure and temperature conditions of the Kokchetav peak metamorphism. The heavy isotope signature of this K-tourmaline differs from that of ordinary Na-tourmalines in crustal rocks, enriched in the light B isotope (delta B-11 = -16.6 to -2.3), which experienced isotope fractionation through metamorphic dehydration reactions. A possible source of the heavy B-isotope signature is serpentine in the subducted lithospheric mantle. Serpentinization of the lithospheric mantle, with enrichment of heavy B-isotope, can be produced by normal faulting at trench-outer rise or trench slope regions, followed by penetration of seawater into the lithospheric mantle. Serpentine breakdown in the lithospheric mantle subducted in subarc regions likely provided fluids with the heavy B-isotope signature, which was acquired during the serpentinization prior to subduction. The fluids could ascend and cause partial melting of the overlying crustal layer, and the resultant silicate melt could inherit the heavy B-isotope signature. The subducting lithospheric mantle is a key repository for modeling the flux of fluids and associated elements acquired at a near the surface into the deep mantle. (c) 2008 Elsevier Ltd. All rights reserved.

DOI： 10.1016/j.gca.2008.05.002

Web of Science

Scopus

researchmap

Language：English   Publisher：PERGAMON-ELSEVIER SCIENCE LTD  

Subduction of lithosphere, involving surficial materials, into the deep mantle is fundamental to the chemical evolution of the Earth. However, the chemical evolution of the lithosphere during subduction to depth remains equivocal. In order to identify materials subjected to geological processes near the surface and at depths in subduction zones, we examined B and Li isotopes behavior in a unique diamondiferous, K-rich tourmaline (K-tourmaline) from the Kokchetav ultrahigh-pressure metamorphic belt. The K-tourmaline, which includes microdiamonds in its core, is enriched in B-11 relative to B-10 (delta B-11 = -1.2 to +7.7) and Li-7 relative to Li-6 (delta Li-7 = -1.1 to +3.1). It is suggested that the K-tourmaline crystallized at high-pressure in the diamond stability field from a silicate melt generated at high-pressure and temperature conditions of the Kokchetav peak metamorphism. The heavy isotope signature of this K-tourmaline differs from that of ordinary Na-tourmalines in crustal rocks, enriched in the light B isotope (delta B-11 = -16.6 to -2.3), which experienced isotope fractionation through metamorphic dehydration reactions. A possible source of the heavy B-isotope signature is serpentine in the subducted lithospheric mantle. Serpentinization of the lithospheric mantle, with enrichment of heavy B-isotope, can be produced by normal faulting at trench-outer rise or trench slope regions, followed by penetration of seawater into the lithospheric mantle. Serpentine breakdown in the lithospheric mantle subducted in subarc regions likely provided fluids with the heavy B-isotope signature, which was acquired during the serpentinization prior to subduction. The fluids could ascend and cause partial melting of the overlying crustal layer, and the resultant silicate melt could inherit the heavy B-isotope signature. The subducting lithospheric mantle is a key repository for modeling the flux of fluids and associated elements acquired at a near the surface into the deep mantle. (c) 2008 Elsevier Ltd. All rights reserved.

DOI： 10.1016/j.gca.2008.05.002

Web of Science

researchmap

Language：English   Publisher：SPRINGER  

Pressure-temperature conditions of tourmaline breakdown in a metapelite were determined by high-pressure experiments at 700-900 degrees C and 4-6 GPa. These experiments produced an eclogite-facies assemblage of garnet, clinopyroxene, phengite, coesite, kyanite and rare rutile. The modal proportions of tourmaline clearly decreased between 4.5 and 5 GPa at 700 degrees C, between 4 and 4.5 GPa at 800 degrees C, and between 800 and 850 degrees C at 4 GPa, with tourmaline that survived the higher temperature conditions appearing corroded and thus metastable. Decreases in the modal abundance of tourmaline are accompanied by decreasing modal abundance of coesite, and increasing that of clinopyroxene, garnet and kyanite; the boron content of phengite increases significantly. These changes suggest that, with increasing pressure and temperature, tourmaline reacts with coesite to produce clinopyroxene, garnet, kyanite, and boron-bearing phengite and fluid. Our results suggest that: (1) tourmaline breakdown occurs at lower pressures and temperatures in SiO(2)-saturated systems than in SiO(2)-undersaturated systems. (2) In even cold subduction zones, subducting sediments should release boron-rich fluids by tourmaline breakdown before reaching depths of 150 km, and (3) even after tourmaline breakdown, a significant amount of boron partitioned into phengite could be stored in deeply subducted sediments.

DOI： 10.1007/s00410-007-0228-2

Web of Science

Scopus

researchmap

Language：English   Publisher：SPRINGER  

Pressure-temperature conditions of tourmaline breakdown in a metapelite were determined by high-pressure experiments at 700-900 degrees C and 4-6 GPa. These experiments produced an eclogite-facies assemblage of garnet, clinopyroxene, phengite, coesite, kyanite and rare rutile. The modal proportions of tourmaline clearly decreased between 4.5 and 5 GPa at 700 degrees C, between 4 and 4.5 GPa at 800 degrees C, and between 800 and 850 degrees C at 4 GPa, with tourmaline that survived the higher temperature conditions appearing corroded and thus metastable. Decreases in the modal abundance of tourmaline are accompanied by decreasing modal abundance of coesite, and increasing that of clinopyroxene, garnet and kyanite; the boron content of phengite increases significantly. These changes suggest that, with increasing pressure and temperature, tourmaline reacts with coesite to produce clinopyroxene, garnet, kyanite, and boron-bearing phengite and fluid. Our results suggest that: (1) tourmaline breakdown occurs at lower pressures and temperatures in SiO(2)-saturated systems than in SiO(2)-undersaturated systems. (2) In even cold subduction zones, subducting sediments should release boron-rich fluids by tourmaline breakdown before reaching depths of 150 km, and (3) even after tourmaline breakdown, a significant amount of boron partitioned into phengite could be stored in deeply subducted sediments.

DOI： 10.1007/s00410-007-0228-2

Web of Science

researchmap

Publisher：GEOCHEMICAL SOCIETY OF JAPAN  

DOI： 10.14862/geochemproc.55.0.301.0

CiNii Article

researchmap

Language：Japanese   Publisher：The Geological Society of Japan  

DOI： 10.14863/geosocabst.2007.0.256.0

CiNii Article

CiNii Books

researchmap

Language：Japanese   Publisher：The Geological Society of Japan  

CiNii Article

CiNii Books

researchmap

Publisher：The Geological Society of Japan  

DOI： 10.5575/geosoc.113.S103

CiNii Article

researchmap

Language：Japanese   Publisher：公益社団法人 東京地学協会  

Vendian-Cambrian Baratal limestone occurs as large allochthonous blocks in the Cambrian accretionary complex of the Gorny Altai Mountains, southern Russia. We analyzed the primary stratigraphy and depositional environments of Baratal limestone in the Kurai and Akkaya areas in the eastern part of the Gorny Altai Mountains.&lt;BR&gt;In the Kurai and the Akkaya areas, Baratal limestone conformably overlies basaltic greenstone. Geochemistry of this greenstone is similar to that found in modern oceanic plateau basalt or oceanic island basalt. The limestone lacks terrigeneous elastic influx. These suggest that the Baratal limestone was originally deposited on and around a plateau or seamount far from the continents in a mid-oceanic environment.&lt;BR&gt;Baratal limestone in the study area is lithologically divided into four types; 1) massive lime mudstone, 2) massive limestone conglomerate 3) bedded lime mudstone with slump structures, and 4) laminated lime mudstone. Massive lime mudstone contains stromatolites and ooids. This evidence suggests that the massive lime mudstone was formed in a shallowmarine environment. The massive limestone conglomerate contains angular clasts of lime mudstone, greenstone and chert. Its poorly graded and poorly sorted characteristics suggest that the limestone conglomerate was formed as debris flow deposits. Some parts of bedded lime mudstone have slump structures, and are interpreted as sliding deposits. In addition, laminated lime mudstone that shares an affinity with limestone turbidite, is associated with the massive limestone conglomerate.&lt;BR&gt;Sedimentary environments of these four types of limestone are inferred, respectively as follows ; massive lime mudstone may have been diposited on the top of a paleo-plateau/ -seamount, while massive limestone conglomerate, bedded lime mudstone with slump structures, and laminated lime mudstone on the slope of a paleo-plateau/-seamount.

DOI： 10.5026/jgeography.112.4_563

CiNii Article

CiNii Books

researchmap

Language：Japanese   Publisher：The Geological Society of Japan  

DOI： 10.14863/geosocabst.2002.0_7_2

CiNii Article

CiNii Books

researchmap

Language：Japanese   Publisher：The Geological Society of Japan  

DOI： 10.14863/geosocabst.2001.0_231_2

CiNii Article

CiNii Books

researchmap

Language：Japanese   Publisher：The Geological Society of Japan  

DOI： 10.14863/geosocabst.2000.0_74_1

CiNii Article

CiNii Books

researchmap

CiNii Article

researchmap

Language：Japanese   Publisher：The Geological Society of Japan  

DOI： 10.14863/geosocabst.1994.0_252_1

CiNii Article

CiNii Books

researchmap

CiNii Article

CiNii Books

researchmap

CiNii Article

researchmap

Language：Japanese   Publisher：Volcanological Society of Japan  

DOI： 10.18940/vsj.1991.2.0_109

CiNii Article

researchmap

Language：Japanese   Publisher：The Geological Society of Japan  

DOI： 10.14863/geosocabst.1991.0_435

CiNii Article

CiNii Books

researchmap