SYNTHESIS AND PHASE RELATIONS IN MONTMORILLONITE-STEVENSITE SERIES UNDER HYDROTHERMAL CONDITIONS
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- YAMADA HIROHISA
- Environmental Remediation Materials Unit, National Institute for Materials Science
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- YOKOYAMA SHINGO
- Central Research Institute of Electric Power Industry
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- TAMURA KENJI
- Environmental Remediation Materials Unit, National Institute for Materials Science
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- WATANABE YUJIRO
- College of Bioscience and Chemistry, Department of Applied Chemistry, Kanazawa Institute of Technology
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- MORIMOTO KAZUYA
- National Institute of Advanced Industrial Science and Technology
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- HATTA TAMAO
- Japan International Research Center for Agricultural Sciences
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- WATANABE TAKASHI
- Niigata College of Nursing
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Abstract
Smectites and related phases were synthesized systematically from quenched glasses with stoichiometric dehydrated Na-smectite compositions in a montmorillonite-stevensite pseudo-binary join under hydrothermal conditions. Experiments were conducted at temperatures from 250 to 500℃ and at 100 MPa, and durations ranged from 1 to 151 days. The existence of a chemical composition gap in the pseudo-binary join between dioctahedral and trioctahedral smectites at 350℃ or lower was confirmed from the time-temperature-transformation relationships obtained. The smectite with intermediate composition was recognized to be metastable; it changed to rectorite through coexisting dioctahedral and trioctahedral smectites. Regularly interstratified chlorite-smectite was then obtained above 500℃. In the montmorillonite composition system, a reaction sequence comparable to that of the natural system was obtained from montmorillonite to rectorite through beidellite plus saponite. Above 500℃, a mica and mica-like phase expanded by ethylene glycol appeared. In the region of trioctahedral composition, unusual high-crystallinity smectite appeared after the low-crystallinity smectite (which is comparable to natural smectite), and then mica was obtained. In the stevensite composition system, stevensite as an initial phase was transformed to a novel regularly interstratified talc-talc-stevensite (r.i.TTS) and then to mica. The structure of r.i.TTS was confirmed by a computer simulation of the XRD line profile.
Journal
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- Clay Science
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Clay Science 18 (1), 11-18, 2014
The Clay Science Society of Japan
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Details 詳細情報について
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- CRID
- 1390001204113199616
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- NII Article ID
- 110009818042
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- NII Book ID
- AA00607148
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- ISSN
- 21863555
- 00098574
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- NDL BIB ID
- 025522831
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- Text Lang
- en
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- Data Source
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- JaLC
- NDL
- CiNii Articles
- KAKEN
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- Abstract License Flag
- Disallowed