On the tidal interaction between protoplanets and the protoplanetary disk. III - Orbital migration of protoplanets
Abstract
The tidal interaction between a protoplanet and a gaseous protoplanetary disk is investigated, and the dynamical evolution of the disk and the orbital migration of the protoplanet in a self-consistent manner is considered. It is shown that the orbital migration of a protoplanet does not suppress the tendency for tidal truncation in the vicinity of its orbit. If the necessary condition for tidal truncation is satisfied, the protoplanet induces a tidal feedback mechanism that regulates the rate of angular momentum transfer between the protoplanet and the disk. Significant orbital migration can only occur on the viscous evolution time scale of the disk.
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- Authors
- Lin, D. N. C., & Papaloizou, J.
- ORCID
- Lin, D. N. C.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 1986-10
- Volume
- 309
- Pages
- 846
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W2004511524
- Cited by
- 1,054
- References
- 0
- Citations by year
- 2026: 35 · 2025: 48 · 2024: 55 · 2023: 40 · 2022: 47 · 2021: 53 · 2020: 75 · 2019: 44 · 2018: 62 · 2017: 39 · 2016: 51 · 2015: 39 · 2014: 39 · 2013: 49 · 2012: 44
- FWCI
- 1.82
- Type
- journal article
- Language
- en
- Open access
- closed
- Locations
- The Astrophysical Journal (publishedVersion)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astrophysics and Star Formation Studies
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astro and Planetary Science
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
- Keywords
- protoplanets, protoplanetary disks, tidal interactions, planet migration, tidal truncation, angular momentum transport, planet formation
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