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Models of giant planet formation with migration and disc evolution
Open accessAbstract
We present a new model of giant planet formation that extends the core-accretion model of Pollack et al. (1996, Icarus, 124, 62) to include migration, disc evolution and gap formation. We show that taking these effects into account can lead to much more rapid formation of giant planets, making it compatible with the typical disc lifetimes inferred from observations of young circumstellar discs. This speed up is due to the fact that migration prevents the severe depletion of the feeding zone as observed in in situ calculations. Hence, the growing planet is never isolated and it can reach cross-over mass on a much shorter timescale. To illustrate the range of planets that can form in our model, we describe a set of simulations in which we have varied some of the initial parameters and compare the final masses and semi-major axes with those inferred from observed extra-solar planets.
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“A hot Jupiter that underwent disk migration may have an intermediate composition if it accreted gas along the way (e.g., Alibert et al. 2005).”
From Origins of Hot Jupiters (2018) · cites this paper as Alibert et al. 2005
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Cites
A Jupiter-mass companion to a solar-type star
Mayor, M., & Queloz, D. (1995) · Nature · doi:10.1038/378355a0 · Cited by 4,111
Formation of the Giant Planets by Concurrent Accretion of Solids and Gas
Pollack, J. B., Hubickyj, O., Bodenheimer, P. H., Lissauer, J. J., Podolak, M., & Greenzweig, Y. (1996) · Icarus · doi:10.1006/icar.1996.0190 · Cited by 3,152
The Evolution of Viscous Discs and the Origin of the Nebular Variables
Donald Lynden-bell, A., & Pringle, J. E. (1974) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/168.3.603 · Cited by 2,603
Disk frequencies and lifetimes in Young clusters
Haisch, Jr., Lada, E. A., & Lada, C. J. (2001) · The Astrophysical Journal · doi:10.1086/320685 · Cited by 1,723
Accretion and the Evolution of T Tauri Disks
Hartmann, L. W., Calvet, N., Gullbring, E., & D’Alessio, P. (1998) · The Astrophysical Journal · doi:10.1086/305277 · Cited by 1,560
Orbital migration of the planetary companion of 51 Pegasi to its present location
Lin, D. N. C., Bodenheimer, P., & Richardson, D. C. (1996) · Nature · doi:10.1038/380606a0 · Cited by 1,235
Low-temperature Rosseland opacities
Alexander, D. R., & Ferguson, J. W. (1994) · The Astrophysical Journal · doi:10.1086/175039 · Cited by 1,161
Disk Frequencies and Lifetimes in Young Clusters
Haisch, K. E., & Lada, C. J. (2001) · CERN Document Server (European Organization for Nuclear Research) · Cited by 1,074
Lin, D. N. C., & Papaloizou, J. (1986) · The Astrophysical Journal · doi:10.1086/164653 · Cited by 1,054
Tanaka, H., Takeuchi, T., & Ward, W. R. (2002) · The Astrophysical Journal · doi:10.1086/324713 · Cited by 1,041
Research works printed but not linked: 7
- Boss, 2002, ApJ, 566, 472
- Guillot, T., Stevenson, D. J., Hubbard, W. B., & Saumon, D. 2004, in Jupiter, ed. F. Bagenal, T. E. Dowling, W. B. McKinnon, in press
- Landau, L. D., & Lifshitz, E. M. 1959, Course of theoretical physics, Fluid Mechanics, third edition (London: Pergamon Press)
- Press, W. H., Flannery, B. P., Teukolsky, S. A., & Vetterling, W. T. 1992, Numerical Recipes: The Art of Scientific Computing, third edition (Cambridge: Cambridge Univ. Press)
- Shakura, 1973, A&A, 24, 337
- Sharp, 1984, Physica, 12D, 3
- Sibulkin, 1952, J. Aeronaut. Sci., 19, 570
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Astrometric Methods and Instrumentation to Identify and Characterize Extrasolar Planets: A ReviewPreprint
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Giant Planet Accretion and Migration: Surviving the Type I Regime
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Capture of solids by growing proto-gas giants: effects of gap formation and supply limited growth
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Framework for the architecture of exoplanetary systems
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Self-citationPlanetary Migration: What Does It Mean for Planet Formation?
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Substellar Companions to Evolved Intermediate-Mass Stars: HD 145457 and HD 180314
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On the formation and chemical composition of super Earths
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Runaway gas accretion and gap opening versus type I migration
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PROTOPLANETARY DISKS IN THE ORION OMC1 REGION IMAGED WITH ALMA
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Metadata
- Authors
- Alibert, Y., Mordasini, C., Benz, W., & Winisdoerffer, C.
- Affiliations
- University of Bern (CH)
- University of Leicester (GB)
- Venue
- Astronomy & Astrophysics
- Publisher
- EDP Sciences
- Published
- 2005-04
- Volume
- 434
- Issue
- 1
- Pages
- 343-353
- ISSN
- 0004-6361 (ISSN-L)
- 1432-0746
- OpenAlex
- W2134475956
- Cited by
- 685
- References
- 52
- Citations by year
- 2026: 20 · 2025: 19 · 2024: 23 · 2023: 20 · 2022: 27 · 2021: 32 · 2020: 37 · 2019: 38 · 2018: 36 · 2017: 34 · 2016: 34 · 2015: 30 · 2014: 37 · 2013: 26 · 2012: 39
- FWCI
- 23.64
- Type
- journal article
- Language
- en
- Open access
- bronze
- doi.org
- Locations
- Astronomy and Astrophysics (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- Springer Link (Chiba Institute of Technology) (submittedVersion)
- Bern Open Repository and Information System (University of Bern) (submittedVersion)
- CERN Document Server (European Organization for Nuclear Research) (submittedVersion)
- arXiv (Cornell University)
- Funders
- National Science Foundation
- Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung
- Topics
- Physical Sciences › Earth and Planetary Sciences › Space and Planetary Science › Astro and Planetary Science
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astrophysics and Star Formation Studies
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
- Keywords
- giant planet formation, core accretion, planet migration, protoplanetary disc evolution, gap formation, disc lifetime, semi-major axis, exoplanets, planetary mass
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