Compositions and possible sources of lunar meteorite NWA 4884  

作　　者：CHEN Jian LING Zongcheng LI Bo SUN Lingzhi ZHANG Jiang HUANG Yihang WU Zhongchen NI Yuheng LIU Jianzhong 

机构地区：[1]Institute of Space Sciences,Shandong Provincial Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment,Shandong University [2]Key Laboratory of Lunar and Deep Space Exploration,Chinese Academy of Sciences [3]Institute of Geochemistry,Chinese Academy of Sciences

出　　处：《Acta Geologica Sinica(English Edition)》2017年第S1期269-270,共2页地质学报（英文版）

基　　金：supported by the National Natural Science Foundation of China (41473065, 41373068);Natural Science Foundation of Shandong Province (JQ201511);Qilu Young Scholar (TANG SCHOLAR) Program of Shandong University,Weihai (2015WHWLJH14)

摘　　要：1 Introduction Lunar mare basalts represent the products of partial remelting of deep mantle sources and provide windows into the compositions of lunar interior.Nine Apollo andLuna missions returned large amounts of mare basaltic samples,while remote sensing suggests that sampled basalts may cover only a small number of the lunar basalt

关 键 词：TH CA Compositions and possible sources of lunar meteorite NWA 4884 GRS 

分 类 号：P184[天文地球—天文学]