Petrographic comparison of refractory inclusions from different chemical groups of chondrites
Lin, Y; Kimura, M; Miao, B; Dai, D; Monoi, A
刊名METEORITICS & PLANETARY SCIENCE
2006
卷号41期号:1页码:67-81
ISSN号1086-9379
文献子类Article
英文摘要Twenty-four refractory inclusions (40-230 mu m, with average of 86 +/- 40 mu m) were found by X-ray mapping of 18 ordinary chondrites. All inclusions are heavily altered, consisting of fine-grained feldspathoids, spinel, and Ca-pyroxene with minor ilmenite. The presence of feldspathoids and lack of melilite are due to alteration that took place under oxidizing conditions as indicated by FeO-ZnO-rich spinel and ilmenite. The pre-altered mineral assemblages are dominated by two types: one rich in melilite, referred to as type A-like, and the other rich in spinel, referred to as spinel-pyroxene inclusions. This study and previous data show similar type and size distributions of refractory inclusions in ordinary and enstatite chondrites.
WOS关键词ALUMINUM-RICH INCLUSIONS ; UNEQUILIBRATED ORDINARY CHONDRITES ; MURCHISON CARBONACEOUS CHONDRITE ; OXYGEN-ISOTOPIC COMPOSITIONS ; ENSTATITE CHONDRITES ; CA-RICH ; ALLENDE METEORITE ; COSMIC GASES ; ORIGIN ; CHONDRULES
WOS研究方向Geochemistry & Geophysics
语种英语
出版者METEORITICAL SOC
WOS记录号WOS:000235919400006
内容类型期刊论文
源URL[http://ir.iggcas.ac.cn/handle/132A11/66426]  
专题中国科学院地质与地球物理研究所
通讯作者Lin, Y
作者单位1.Chinese Acad Sci, State Key Lab Lithospher Evolut, Inst Geol & Geophys, Beijing, Peoples R China
2.Chinese Acad Sci, Guangzhou Inst Geochem, Guangzhou, Peoples R China
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GB/T 7714
Lin, Y,Kimura, M,Miao, B,et al. Petrographic comparison of refractory inclusions from different chemical groups of chondrites[J]. METEORITICS & PLANETARY SCIENCE,2006,41(1):67-81.
APA Lin, Y,Kimura, M,Miao, B,Dai, D,&Monoi, A.(2006).Petrographic comparison of refractory inclusions from different chemical groups of chondrites.METEORITICS & PLANETARY SCIENCE,41(1),67-81.
MLA Lin, Y,et al."Petrographic comparison of refractory inclusions from different chemical groups of chondrites".METEORITICS & PLANETARY SCIENCE 41.1(2006):67-81.
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