MODEL FOR ACCRETION OF TERRESTRIAL PLANETS

被引：50
作者：
WEIDENSCHILLING, SJ [1 ]
机构：
[1] MIT, DEPT EARTH & PLANETARY SCI, CAMBRIDGE, MA 02139 USA
来源：
ICARUS | 1974年 / 22卷 / 04期
关键词：
D O I：
10.1016/0019-1035(74)90075-X
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
引用
收藏
页码：426 / 435
页数：10
相关论文
共 31 条
[1]   ORIGIN AND EVOLUTION OF SOLAR SYSTEM, 2 [J].
ALFVEN, H ;
ARRHENIU.G .
ASTROPHYSICS AND SPACE SCIENCE, 1970, 9 (01) :3-&
[2]   FORMATION OF EARTHS CORE [J].
ANDERSON, DL ;
HANKS, TC .
NATURE, 1972, 237 (5355) :387-&
[3]  
BENFIELD AE, 1950, T AM GEOPHYS UNION, V31, P53
[4]  
BROUWER D, 1950, ASTRON PAPERS AM EPH, V13, P83
[5]   FORMATION OF OUTER PLANETS [J].
CAMERON, AGW .
SPACE SCIENCE REVIEWS, 1973, 14 (3-4) :383-391
[6]   ACCUMULATION PROCESSES IN PRIMITIVE SOLAR NEBULA [J].
CAMERON, AGW .
ICARUS, 1973, 18 (03) :407-450
[7]  
CHANDRASEKHAR S, 1960, PRINCIPLES STELLAR D, pCH1
[8]  
Cohen C. J., 1973, Celestial Mechanics, V7, P438, DOI 10.1007/BF01227509
[9]   FORMATION OF PLANETESIMALS [J].
GOLDREIC.P ;
WARD, WR .
ASTROPHYSICAL JOURNAL, 1973, 183 (03) :1051-1061
[10]   STOCHASTIC COALESCENCE MODEL FOR TERRESTRIAL PLANETARY ACCRETION [J].
HALLAM, M ;
MARCUS, AH .
ICARUS, 1974, 21 (01) :66-85
1234