Planet migration
| dc.creator | Thommes, Edward W. | |
| dc.creator | Lissauer, Jack J. | |
| dc.date | 2002-09-19 | |
| dc.date.accessioned | 2026-07-07T02:05:19Z | |
| dc.date.available | 2026-07-07T02:05:19Z | |
| dc.description | A planetary system may undergo significant radial rearrangement during the early part of its lifetime. Planet migration can come about through interaction with the surrounding planetesimal disk and the gas disk--while the latter is still present--as well as through planet-planet interactions. We review the major proposed migration mechanisms in the context of the planet formation process, in our Solar System as well as in others. | |
| dc.description | 14 pages, 1 figure. To appear in proceedings of STSci Astrophysics of Life symposium (May 6-9, 2002) | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0209416 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0209416 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/5067 | |
| dc.subject | Astrophysics | |
| dc.title | Planet migration | |
| dc.type | text |