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Can I read Influence of an Inner Disc on the Orbital Evolution of Massive Planets Migrating in Resonance on EtoBox?
Influence of an Inner Disc on the Orbital Evolution of Massive Planets Migrating in Resonance by Crida, A.; Sándor, Z.; Kley, W. is a Physics and Astronomy article available to read on EtoBox.
What is Influence of an Inner Disc on the Orbital Evolution of Massive Planets Migrating in Resonance about?
Context. The formation of resonant planet pairs in exoplanetary systems involves planetary migration inside the protoplanetary disc. After a resonant capture, subsequent migration leads to a large increase in planetary eccentricities, if no damping mechanism is applied. This has led to the conclusion that the migration of resonant planetary systems cannot take place across large radial distances, but must be terminated rapidly by disc dissipation. Aims. We investigate if the presence of an inner disc could supply eccentricity damping to the inner planet, and if this effect could explain observed eccentricities in some planetary systems. Methods. We compute hydrodynamic simulations of giant planets, in orbits of a given eccentricity about an inner gas disc, and measure the effect of the gas disc on the planetary orbital parameters. We perform detailed long-term calculations of the GJ 876 system. We complete N-body simulations, which include artificial forces on the planets that recreate the effect of the inner and outer discs. Results. We find that we cannot neglect the influence of the inner disc, and that the disc could explain the observed eccentricities. In particular, we reprod
Who reads Influence of an Inner Disc on the Orbital Evolution of Massive Planets Migrating in Resonance?
It is typically read by researchers, students, and practitioners in Physics and Astronomy.
- Author
- Crida, A.; Sándor, Z.; Kley, W.
- Publisher
- EDP Sciences (ISSN 0004-6361)
- Published
- 2008
- Language
- EN
- Field
- Physics and Astronomy (Physical Sciences)