Guilera, O. M.; Swoboda, D.; Alibert, Y.; De Elía, G. C.; Santamaría, P. J.; Brunini, A. (2014). Planetesimal fragmentation and giant planet formation: the role of planet migration. Proceedings of the International Astronomical Union, 9(S310), pp. 204-207. Cambridge University Press 10.1017/S1743921314008266
|
Text
S1743921314008266.pdf - Published Version Available under License Publisher holds Copyright. Download (165kB) | Preview |
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.
Item Type: |
Journal Article (Further Contribution) |
|---|---|
Division/Institute: |
08 Faculty of Science > Physics Institute > Space Research and Planetary Sciences 08 Faculty of Science > Physics Institute 10 Strategic Research Centers > Center for Space and Habitability (CSH) |
UniBE Contributor: |
Swoboda, David, Alibert, Yann Daniel Pierre |
Subjects: |
500 Science > 530 Physics 500 Science > 520 Astronomy 600 Technology > 620 Engineering |
ISSN: |
1743-9213 |
Publisher: |
Cambridge University Press |
Language: |
English |
Submitter: |
Marceline Brodmann |
Date Deposited: |
17 Jul 2020 10:13 |
Last Modified: |
05 Dec 2022 15:13 |
Publisher DOI: |
10.1017/S1743921314008266 |
BORIS DOI: |
10.7892/boris.115449 |
URI: |
https://boris.unibe.ch/id/eprint/115449 |
Actions (login required)
 |
Edit item |