Experimental simulation of evaporation and condensation in the early solar system.
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- TACHIBANA Shogo
- Department of Geological Sciences, Arizona State University
Bibliographic Information
- Other Title
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- 実験室に原始太陽系をつくる 原始太陽系での蒸発・凝縮
- ジッケンシツ ニ ゲンシ タイヨウケイ オ ツクル ゲンシ タイヨウケイ デ ノ ジョウハツ ギョウシュク
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Abstract
Evaporation and condensation played a major role in producing chemical and/or isotopic variations in the early solar system, which have been recorded in primitive meteorites. Experimental studies on evaporation and condensation of various planetary materials have started in 1970's to reproduce chemical compositions and textures of constituents of primitive meteorites. In a recent decade, many evaporation experiments of minerals and melts have been carried out to obtain fundamental kinetic parameters and to comprehend the chemical (or isotopic) fractionations in the early solar system in terms of evolution. Experimental simulation of evaporation and condensation in the solar system should be combined with isotopic or chemical analyses of meteorites and observational and theoretical studies of the proto-planetary disk for complete understanding of the early solar system chemical evolution. The history of experimental studies of evaporation and condensation under the early solar system conditions and some recent progresses are reviewed in this paper.
Journal
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- Japanese Magazine of Mineralogical and Petrological Sciences
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Japanese Magazine of Mineralogical and Petrological Sciences 31 (4), 208-220, 2002
Japan Association of Mineralogical Sciences
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Keywords
Details 詳細情報について
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- CRID
- 1390001206526630656
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- NII Article ID
- 10009630539
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- NII Book ID
- AA1146088X
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- COI
- 1:CAS:528:DC%2BD38Xotlyqt78%3D
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- ISSN
- 13497979
- 1345630X
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- NDL BIB ID
- 6300223
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- Text Lang
- ja
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- Data Source
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- JaLC
- NDL
- Crossref
- CiNii Articles
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- Abstract License Flag
- Disallowed