检索规则说明:AND代表“并且”;OR代表“或者”;NOT代表“不包含”;(注意必须大写,运算符两边需空一格)
检 索 范 例 :范例一: (K=图书馆学 OR K=情报学) AND A=范并思 范例二:J=计算机应用与软件 AND (U=C++ OR U=Basic) NOT M=Visual
机构地区:[1]中国科学院广州地球化学研究所,同位素年代学和地球化学重点实验室 [2]中国科学院地质与地球物理研究所 [3]桂林工学院资源环境工程系,广西桂林541004
出 处:《极地研究》2005年第1期45-74,共30页Chinese Journal of Polar Research
基 金:国家自然科学基金项目(批准号: 40473037; 40232026)资助
摘 要:根据陨石的矿物岩石学特征、化学组成及结构可划分为球粒陨石及非球粒陨石质陨石两大类。球粒陨石进一步划分为碳质球粒陨石族(CI,CM,CO,CR,CB,CH,CV及CK球粒陨石)、普通球粒陨石族(H,L,LL球粒陨石)、顽辉石球粒陨石族(EH及EL球粒陨石)、R及K球粒陨石群,而非球粒陨石质陨石进一步划分为原始的无球粒陨石族(Acpulcoites,Lodranites,Wi nonaites,IAB硅酸盐包体及IIICD硅酸盐包体)和分异的陨石族。分异的陨石族包括:无球粒陨石(Angrites,Aubrites,Branchinites,橄辉无球粒陨石,HED灶神星陨石,SNCO火星陨石及月球陨石);石铁陨石(中铁陨石及橄榄陨铁);铁陨石(IAB,IC,IIAB,IIC,IID,IIE,IIIAB,IIICD,IIIE,II IF,IVA及IVB铁陨石化学群)。每一陨石族或陨石群,具有类似的成因或形成历史,并来自同一小行星体或行星体,藉此可建立不同陨石族或陨石群之间的成因联系,并可提供早期太阳星云的物理化学条件及其演化的信息。On the basis of minerologic-petrologic characteristics, chemical compositions,oxygen isotopes and textures meteorites are classified into two major categories : chondrites and nonchondritic meteorites.Chondrite can be further divided into carbonaceous chondrite clan (CI,CM,CO,CR,CB,CH,CV and CK chondrites),ordinary chondrite clan(H,L,LL chondrites), enstatite chondrite clan(EH and ELchondrites),R and K chondrite group, and that nonchondritic meteorites are further classified into primitive achondrites and the igneously differentiated meteorites.Primitive achondrites are including Acpulcoites,Lodranites,Winonaites,IAB silicate inclusions and IIICD silicate inclusions. The igneously differentiated meteorites are classified into achondrites (Angrites,Aubrites ,Branchinites,Ureilites,HEDVista meteorites,SNCO martian meteorites and lunar meteorites),stony irons(mesosiderirtes and pallasites) and iron meteorites(IAB,IC,IIAB,IIC,IID,IIE,IIIAB,IIICD,IIIE,IIIF,IVA and IVB iron meteorite groups).Every meteorite clan or meteorite group have similar origins or formation histories that could be derived same asteroidal or planetary parent body,thereby we can establish possible genetic relationships between various meteorire clans or meteorite groups .These different meteorite clans or meteorite groups may provide informations of physical-chemical conditions and their evolution history of early solar nebula.
正在载入数据...
正在载入数据...
正在载入数据...
正在载入数据...
正在载入数据...
正在载入数据...
正在载入数据...
正在链接到云南高校图书馆文献保障联盟下载...
云南高校图书馆联盟文献共享服务平台 版权所有©
您的IP:216.73.216.95