Extrasolar Planets and Mean-Motion Resonances
| dc.creator | Lee, Man Hoi | |
| dc.creator | Peale, S. J. | |
| dc.date | 2002-09-10 | |
| dc.date.accessioned | 2026-07-07T02:05:04Z | |
| dc.date.available | 2026-07-07T02:05:04Z | |
| dc.description | The 2:1 orbital resonances of the GJ 876 system can be easily established by the differential planet migration due to planet-nebula interaction. Significant eccentricity damping is required to produce the observed orbital eccentricities. The geometry of the GJ 876 resonance configuration differs from that of the Io-Europa pair, and this difference is due to the magnitudes of the eccentricities involved. We show that a large variation in the configuration of 2:1 and 3:1 resonances and, in particular, asymmetric librations can be expected among future discoveries. | |
| dc.description | 4 pages, including 4 figures; uses newpasp.sty; to appear in Scientific Frontiers in Research on Extrasolar Planets (ASP Conf. Series) | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0209176 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0209176 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/4991 | |
| dc.subject | Astrophysics | |
| dc.title | Extrasolar Planets and Mean-Motion Resonances | |
| dc.type | text |