COMPUTER SIMULATIONS OF PLANETARY ACCRETION DYNAMICS - SENSITIVITY TO INITIAL CONDITIONS

被引：32

作者：

ISAACMAN, R

SAGAN, C

机构：

[1] CORNELL UNIV,CTR NATL ASTRON & IONOSPHERE,ITHACA,NY 14853

[2] CORNELL UNIV,PLANETARY STUDIES LAB,ITHACA,NY 14853

来源：

关键词：

D O I：

10.1016/0019-1035(77)90153-1

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：510 / 533

页数：24

共 26 条

[21] TEMPERATURE-GRADIENT IN SOLAR NEBULA [J].

LEWIS, JS .

[22] RESONANT STRUCTURE OF SOLAR SYSTEM - LAW OF PLANETARY DISTANCES [J].

MOLCHANO.AM .

[23] RESONANCES IN COMPLEX SYSTEMS - A REPLY TO CRITIQUES [J].

MOLCHANOV, AM .

[24]

MOLCHANOV AM, 1969, ICARUS, V11, P111

[25]

UREY HC, 1974, HIGHLIGHTS ASTRONOMY, V3, P475

[26] MODEL FOR ACCRETION OF TERRESTRIAL PLANETS [J].

WEIDENSCHILLING, SJ .