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地质科学  2013, Vol. 48 Issue (3): 762-772    DOI: 10.3969/j.issn.0563-5020.2013.03.014
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富橄榄石的富Ca,Al组分集合体的矿物岩石学特征及对比研究
戴德求1,2, 陈新跃1, 杨荣丰1,3
1. 湖南科技大学地质研究所 湖南 湘潭 411201;
2. 中国科学院地球化学研究所 贵阳 550002;
3. 页岩气开发与利用湖南省重点实验室 湖南 湘潭 411201
Comparation of petrography and mineral chemistry characteristics among olivine and Ca,Al-rich assemblages
Dai Deqiu1,2, Chen Xinyue1, Yang Rongfeng1,3
1. Institute of Geology, Hunan University of Science and Technology, Xiangtan, Hunan 411201;
2. Institute of Geochemistry, Chinese Academy of Sciences, Guiyang 550002;
3. Hunan Provincial Key Laboratory of Shale Gas Resource Utilization, Xiangtan, Hunan 411201
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摘要 富Ca,Al包体、球粒和蠕虫状橄榄石集合体都是早期星云事件的产物。本文探讨了4个富橄榄石的富Ca,Al组分集合体的矿物岩石学特征,并对它们进行了对比。矿物岩石学特征表明含橄榄石边的富尖晶石—辉石型包体和富Ca,Al组分蠕虫状橄榄石集合体都属于星云直接凝聚的产物,而富钙长石—橄榄石型包体(POI)和富Ca,Al组分球粒经历过熔融结晶过程。矿物模式组成表明POI包体和富Ca,Al组分球粒可能是认识典型富Ca,Al包体与球粒之间相互关系的钥匙。蠕虫状橄榄石集合体GRV022459-2C1中尖晶石普遍具有高的FeO含量,表明其蚀变发生于高氧逸度的星云环境。球粒与粗粒富Ca,Al包体可能属于同一热事件的产物,粗粒富Ca,Al包体形成于富Ca,Al矿物富集的区域,Mg,Fe质硅酸盐球粒形成于富Ca,Al矿物缺失的区域,POI包体和富Ca,Al组分球粒可能形成于上述两个区域之间的过渡区域。
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关键词富Ca   Al包体   球粒   蠕虫状橄榄石集合体   富钙长石&mdash   橄榄石型包体   星云     
Abstract: Ca-, Al-rich inclusions, chondrules and amoeboid olivine aggregates are the early assemblages of the solar nebula.4 olivine and Ca, Al-rich assemblages were studied to compare with their petrography and mineral chemistry. The petrography and mineral chemistry characteristics argues that spinel-pyroxene-rich inclusion embedded in olivine and Ca, Al-rich amoeboid olivine aggregates are likely assemblages of solar nebular condensates.The plagioclase-olivine inclusions(POIs)and Ca-, Al-rich chondrules were crystallized from melts. The characteristics of mineral modal compositions of POIs and Ca-, Al-rich chondrules argues they probably represent intermediate assemblages between typical refractory inclusions and chondrules.Spinel in amoeboid olivine aggregates(GRV022459-2C1)is the most remarkably FeO-rich in all assemblages, and it indicates alteration of the aggregate happened under high oxygen fugacity.Chondrules and coarse-grained Ca-, Al-rich inclusions are probably crystallized from melt in the same affair.The coarse-grained Ca-, Al-rich inclusions form probably the reservoir of Ca-, Al-rich prior matters, and Mg, Fe silicate chondrules form in the reservoir of Ca-, Al-poor prior matters.POIs and Ca-, Al-rich chondrules form the district between coarse-grained inclusions and Mg, Fe silicate chondrules.
Key wordsCa-,Al-rich inclusions   Chondrules   Amoeboid olivine aggregates   Plagioclase-olivine inclusions(POIs)   Nebula   
收稿日期: 2012-12-30;
基金资助:

国家自然科学基金项目(编号: 41103032);环境地球化学国家重点实验室开放基金项目(编号:SKLE1106)和湖南省教育厅项目(编号: 10C0670, 12B039)资助

作者简介: 戴德求, 男, 1976年11月生, 博士, 副教授, 陨石学和天体化学专业。E-mail: ddqygf@163.com
引用本文:   
. 2013, 富橄榄石的富Ca,Al组分集合体的矿物岩石学特征及对比研究. 地质科学, 48(3): 762-772.
. Comparation of petrography and mineral chemistry characteristics among olivine and Ca,Al-rich assemblages[J]. Chinese Journal of Geology, 2013, 48(3): 762-772.
 
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[3] 刘钦甫, 张鹏飞, 杨晓杰. 淮南下石盒子组球粒状高岭岩结构及成因探讨[J]. 地质科学, 1995, (4): 393-400.
 
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