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논문 기본정보
#23455; #39443;室に原始太陽系をつくる minus;原始太陽系での蒸 #30330; #12539;凝縮 minus;
논문 개요
| 기관명 | NDSL |
|---|---|
| 저널명 | 岩石鑛物科學 = Japanese magazine of mineralogical and petrological sciences |
| ISSN | 1345-630x, |
| ISBN |
논문저자 및 소속기관 정보
| 저자(한글) | |
|---|---|
| 저자(영문) | |
| 소속기관 | |
| 소속기관(영문) | |
| 출판인 | |
| 간행물 번호 | |
| 발행연도 | 2002-01-01 |
| 초록 | 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 apos;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. |
| 원문URL | http://click.ndsl.kr/servlet/OpenAPIDetailView?keyValue=03553784&target=NART&cn=NART57594001 |
| 첨부파일 |
추가정보
| 과학기술표준분류 | |
|---|---|
| ICT 기술분류 | |
| DDC 분류 | |
| 주제어 (키워드) | Evaporation,Condensation,Kinetics,Elemental fractionation,Isotopic fractionation,Chondrite,Early solar system |