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清镇顽辉石球粒陨石(EH3)不透明相的岩石,矿物学研究
引用本文:林杨挺 Gore.,AE.清镇顽辉石球粒陨石(EH3)不透明相的岩石,矿物学研究[J].地球化学,1995,24(1):76-88,T001.
作者姓名:林杨挺 Gore.  AE
作者单位:中国科学院广州地球化学研究所,中国科学院贵阳地球化学研究所
摘    要:通过对最新鲜、最原始的EH3型损石-清镇员石不透明矿物的岩石学、矿物学研究,揭示了不透明矿物化学组成与产状的成因关系,提出了星云冷凝,金属与星去气相组分的硫化反应,矿物出熔及矿物分解等四种形成机制。对不透明物的各种环带结构及闪锌矿、矿镁矿等矿物温度计的研究,揭示了该陨石在星云阶段和母体中的热历史,与Yamato-691(EH3)的对比表明,清镇陨石不透明矿物形成于更加还原的星云条件。

关 键 词:清镇陨石  顽辉石球粒陨石  不透明矿物  陨石

^^PETROGRAPHICAL AND MINERALOGICAL STUDY OF OPAQUE MINERALS IN THE QINGZHEN ENSTATITE CHONDRITE (EH3)
Lin Yangting,Goresy A. El,Ouyang Ziyuan,Wang Daode.^^PETROGRAPHICAL AND MINERALOGICAL STUDY OF OPAQUE MINERALS IN THE QINGZHEN ENSTATITE CHONDRITE (EH3)[J].Geochimica,1995,24(1):76-88,T001.
Authors:Lin Yangting  Goresy A El  Ouyang Ziyuan  Wang Daode
Abstract:The petrographical and mineralogical studies on the opaque minerals of the Qingzhen meteorite, a highly unequilibrated and very fresh EH3 chondrite, reveal the relationship between their chemical composition and occurrence. Four types of formation mechanism for the opaque minerals were suggested. They are: (1)condensation, (2)sulfurization of metal, (3)exsolution, and(4) decomposition. Thermal history of the Qingzhen meteorite in solar nebula and in its parent body was also discussed based on various zonings of opaque minerals and the cosmothermometer of sphalerite and niningerite. The comparative study between the Qingzhen meteorite and the Yamato-691(EH3) meteorite indicates that the opaque minerals in the former was formed under more reducing condition in the nebula than the later.
Keywords:Qingzhen meteorite  enstatite chondrite  opaque mineral
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