Planetesimal fragmentation and giant planet formation: the role of planet migration

被引:0
|
作者
Guilera, O. M. [1 ,2 ]
Swoboda, D. [3 ,4 ]
Alibert, Y. [3 ,4 ,5 ]
de Elia, G. C. [1 ,2 ]
Santamaria, P. J. [1 ,2 ]
Brunini, A. [1 ,2 ]
机构
[1] UNLP, CONICET, Fac Ciencias Astron & Geofis, Grp Ciencias Planetarias, La Plata, Buenos Aires, Argentina
[2] UNLP, CONICET, Inst Astrofis La Plata, La Plata, Buenos Aires, Argentina
[3] Univ Bern, Phys Inst, Bern, Switzerland
[4] Univ Bern, Ctr Space & Habitabil, Bern, Switzerland
[5] Observ Besancon, Besancon, France
来源
COMPLEX PLANETARY SYSTEMS | 2014年 / 9卷 / 310期
关键词
planetary systems: formation; planetesimal fragmentation; planet migration; TORQUE FORMULA; DISC; ACCRETION; JUPITER; MODELS; MASS; IV;
D O I
10.1017/S1743921314008266
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In the standard model of core accretion, the cores of the giant planets form by the accretion of planetesimals. In this scenario, the evolution of the planetesimal population plays an important role in the formation of massive cores. Recently, we studied the role of planetesimal fragmentation in the in situ formation of a giant planet. However, the exchange of angular momentum between the planet and the gaseous disk causes the migration of the planet in the disk. In this new work, we incorporate the migration of the planet and study the role of planet migration in the formation of a massive core when the population of planetesimals evolves by planet accretion, migration, and fragmentation.
引用
收藏
页码:204 / 207
页数:4
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