摘要
Howardite-Eucrite-Diogenite(HED)族陨石是地球上发现数量最多的无球粒陨石类型,也是太阳系中除地球岩石之外数量最多的岩浆岩样品。本文对大量HED族陨石的岩石学和矿物化学特征进行了归纳总结,讨论了陨石的后期热变质作用和母体起源,对HED族陨石的中文定名提出了具体意见。
The Howardite-Eucrite-Diogenite（HED）meteorites are a group of achondrites discovered in largest quantity on the Earth.They are also the largest quantity magmatic rock samples in the Solar system with the exception of the magmatic rocks on the Earth.This paper has reviewed previous researches on the petrological and mineral chemical characteristics of the HED group of meteorites,discussed the late stage thermal metamorphism and the parent origin of the HED meteorites, and finally proposed some detailed suggestions on the Chinese naming of the HED meteorites.
作者
陈宏毅
缪秉魁
谢兰芳
黄丽霖
CHEN Hong-yi MIAO Bing-kui XIE Lan-fang HUANG Li-lin(Key Laboratory of Geological Fluid and Geological Process at Universities of Guangxi Province, Guangxi Scientific Experiment Center of Mining, Metallurgy and Environment, Guangxi Key Laboratory of Hidden Metallic Ore Deposits Exploration, Guilin University of Technology, Guilin Guangxi 541004,China)
出处
《矿物岩石地球化学通报》
CAS
CSCD
北大核心
2016年第5期1037-1052,共16页
Bulletin of Mineralogy, Petrology and Geochemistry
基金
广西高校科研项目(教育厅KY2015LX117)
国家自然科学基金项目(41173077)
国家自然资源平台建设项目(2005DKA21406-1)
关键词
HED族陨石
岩石学
矿物化学
热变质
灶神星
分异型小行星
HED meteorites
petrology
mineral chemistry
thermal metamorphism
Vesta
differentiated asteroids
