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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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Self-citationVigan, A., Bonavita, M., Biller, B. A., Forgan, D. H., Rice, K., Chauvin, G., Desidera, S., Meunier, J.-C., Delorme, P., Schlieder, J. E., et al. (2017) · arXiv (Cornell University) · doi:10.48550/arxiv.1703.05322 · Cited by 3
Self-citationPlanet Formation Imager (PFI): science vision and key requirements
Kraus, S., Monnier, J., Ireland, M., Duchêne, G., Espaillat, C., Hönig, S., Juhász, A., Mordasini, C., Olofsson, J., Paladini, C., et al. (2016) · Astronomical Telescopes + Instrumentation · doi:10.1117/12.2231067 · Cited by 16
Self-citationKimura, T., Kokubo, E., Matsumoto, Y., Mordasini, C., & Ikoma, M. (2025) · The Astrophysical Journal · doi:10.3847/1538-4357/adef15 · Cited by 2
Self-citationZhang, E. Y., Carmichael, T. W., Huber, D., Stassun, K. G., Fukui, A., Narita, N., Murgas, F., Palle, E., Latham, D. W., Calkins, M., et al. (2026) · The Astronomical Journal · doi:10.3847/1538-3881/ae23c7 · Cited by 3
Towards a global model for planet formation in layered MHD wind-driven discs
Weder, J., & Mordasini, C. (2026) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202557262 · Cited by 2
Self-citation
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
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
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