PLANET FORMATION - COMPOSITIONAL MIXING AND LUNAR COMPOSITIONAL ANOMALIES

被引：14
作者：
HARTMANN, WK
机构：
[1] INST PLANETARY SCI,TUCSON,AZ 85719
[2] UNIV HAWAII,INST ASTRON,HONOLULU,HI 96822
[3] UNIV HAWAII,DEPT PHYS & ASTRON,HONOLULU,HI 96822
来源：
ICARUS | 1976年 / 27卷 / 04期
关键词：
D O I：
10.1016/0019-1035(76)90171-8
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
引用
收藏
页码：553 / 559
页数：7
相关论文
共 12 条
[1]   MOON MAY BE A FORMER PLANET [J].
BAILEY, JM .
NATURE, 1969, 223 (5203) :251-&
[2]  
BANDERMANN LW, 1971, MODERN GEOLOGY, V3, P53
[3]  
Cameron A. G. W., 1973, Moon, V7, P377, DOI 10.1007/BF00564641
[4]  
GANAPATHY R, 1974, GEOCHIM COSMOCHIM AC, V2, P1181
[5]   SATELLITE-SIZED PLANETESIMALS AND LUNAR ORIGIN [J].
HARTMANN, WK ;
DAVIS, DR .
ICARUS, 1975, 24 (04) :504-515
[6]   METAL-SILICATE FRACTIONATION IN SOLAR SYSTEM [J].
LEWIS, JS .
EARTH AND PLANETARY SCIENCE LETTERS, 1972, 15 (03) :286-&
[7]  
MORGAN J, 1974, 5TH P LUN SCI C, V2, P1703
[8]  
SAFRONOV VS, 1972, F677 TT NASA
[9]   WHERE WAS MOON FORMED [J].
SINGER, SF ;
BANDERMANN, LW .
SCIENCE, 1970, 170 (3956) :438-+
[10]   ACCRETION OF TERRESTRIAL PLANETS .2. [J].
WEIDENSCHILLING, SJ .
ICARUS, 1976, 27 (01) :161-170
12