On the accretion of Uranus and Neptune

被引:4
作者
Brunini, A [1 ]
Melita, MD [1 ]
机构
[1] Univ Nacl La Plata, Astron Observ, La Plata, Buenos Aires, Argentina
关键词
accretion; accretion discs; planets and satellites : formation; planets and satellites : individual : Uranus; planets and satellites : individual : Neptune; Solar system : formation;
D O I
10.1046/j.1365-8711.2002.05104.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In this paper, we discuss some problems concerning the formation of Uranus and Neptune. We find that the adoption of reduced Hill spheres as the region of close interaction between planetesimals introduces an enhancement of the gravitational cross-sections in previous numerical simulations. We also discuss a way to make possible the formation of Uranus and Neptune on time-scales shorter than the age of the Solar system.
引用
收藏
页码:184 / 186
页数:3
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