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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
An Equation of State for Low-Mass Stars and Giant Planets
Saumon, D., Chabrier, G., & van Horn, H. V. (1995) · The Astrophysical Journal Supplement Series · doi:10.1086/192204 · Cited by 959
Ida, S., & Lin, D. N. C. (2004) · The Astrophysical Journal · doi:10.1086/381724 · Cited by 948
Using FU Orionis outbursts to constrain self-regulated protostellar disk models
Bell, K. R., & Lin, D. N. C. (1994) · The Astrophysical Journal · doi:10.1086/174206 · Cited by 881
ACCRETION AND THE EVOLUTION OF T TAURI DISKS
Paola, H. (1998) · Cited by 814
Lissauer, J. J. (1993) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.aa.31.090193.001021 · Cited by 733
Accumulation of a swarm of small planetesimals
Wetherill, G. W., & Stewart, G. R. (1989) · Icarus · doi:10.1016/0019-1035(89)90093-6 · Cited by 565
Drag Coefficients of Spheres in Continuum and Rarefied Flows
Henderson, C. B. (1976) · AIAA Journal · doi:10.2514/3.61409 · Cited by 531
Calculations of the accretion and evolution of giant planets: The effects of solid cores
Bodenheimer, P. H., & Pollack, J. B. (1986) · Icarus · doi:10.1016/0019-1035(86)90122-3 · Cited by 506
Bronshtén, V. A. (1983) · Springer eBooks · doi:10.1007/978-94-009-7222-3 · Cited by 482
The fragmentation of small asteroids in the atmosphere
Hills, J. G., & Goda, M. P. (1993) · The Astronomical Journal · doi:10.1086/116499 · Cited by 325
Circumstellar disks and the search for neighbouring planetary systems
Beckwith, S. V. W., & Sargent, A. I. (1996) · Nature · doi:10.1038/383139a0 · Cited by 282
Three-dimensional calculations of high- and low-mass planets embedded in protoplanetary discs
Bate, M. R., Lubow, S. H., Ogilvie, G. I., & Miller, K. A. (2003) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.2003.06406.x · Cited by 282
Oligarchic growth of giant planets
Thommes, E. W., Duncan, M. J., & Levison, H. F. (2003) · Icarus · doi:10.1016/s0019-1035(02)00043-x · Cited by 281
Nelson, R. P., & Papaloizou, J. C. B. (2004) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2004.07406.x · Cited by 266
Hydrodynamic instability of the solar nebula in the presence of a planetary core
Perri, F., & Cameron, A. G. W. (1974) · Icarus · doi:10.1016/0019-1035(74)90074-8 · Cited by 247
Physics of meteor flight in the atmosphere
ÖPIK, E. J. (1958) · Medical Entomology and Zoology · Cited by 240
Papaloizou, J. C. B., & Terquem, C. (1999) · The Astrophysical Journal · doi:10.1086/307581 · Cited by 230
Ward, W. R. (1997) · The Astrophysical Journal · doi:10.1086/310701 · Cited by 221
Migration and giant planet formation
Alibert, Y., Mordasini, C., & Benz, W. (2004) · Astronomy and Astrophysics · doi:10.1051/0004-6361:20040053 · Cited by 215
Self-citationDisintegration of Large Meteoroids in Earth's Atmosphere: Theoretical Models
Svetsov, V. V. (1995) · Icarus · doi:10.1006/icar.1995.1116 · Cited by 196
Interactions of planetesimals with protoplanetary atmospheres
Podolak, M., Pollack, J. B., & REYNOLDS, R. T. (1988) · Icarus · doi:10.1016/0019-1035(88)90090-5 · Cited by 186
Growth of a Migrating Protoplanet
Tanaka, H., & Ida, S. (1999) · Icarus · doi:10.1006/icar.1999.6107 · Cited by 182
Oligarchic growth of giant planetsPreprint
Thommes, E. W., Duncan, M. J., & Levison, H. F. (2003) · Cited by 171
Outward migration of extrasolar planets to large orbital radii
Veras, D., & Armitage, P. J. (2003) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2004.07239.x · Cited by 160
Low‐Mass Protoplanet Migration in T Tauri α‐Disks
Kristen Menou, A., & Goodman, J. (2004) · The Astrophysical Journal · doi:10.1086/382947 · Cited by 151
The Collision of Jupiter and Comet Shoemaker-Levy 9
Zahnle, K., & Low, M. M. (1994) · Icarus · doi:10.1006/icar.1994.1038 · Cited by 149
Accretion rates of protoplanets
Greenzweig, Y., & Lissauer, J. J. (1992) · Icarus · doi:10.1016/0019-1035(92)90110-s · Cited by 147
On the structure of circumbinary accretion disks and the tidal evolution of commensurable satellites
Lin, D. N. C., & Papaloizou, J. C. B. (1979) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/188.2.191 · Cited by 145
Accretion rates of protoplanets
Greenzweig, Y., & Lissauer, J. J. (1991) · A Bibliography of Planetary Geology and Geophysics Principal Investigators and their Associates, 1990 - 1991 · Cited by 109
Airburst origin of dark shadows on Venus
Zahnle, K. J. (1992) · Journal of Geophysical Research Atmospheres · doi:10.1029/92je00787 · Cited by 108
A quasi-simple ablation model for large meteorite entry: theory vs observations
ReVelle, D. O. (1979) · Journal of Atmospheric and Terrestrial Physics · doi:10.1016/0021-9169(79)90071-0 · Cited by 103
Explosion of comet Shoemaker-Levy 9 on entry into the Jovian atmosphere
Low, M. M., & Zahnle, K. J. (1994) · The Astrophysical Journal · doi:10.1086/187565 · Cited by 95
Formation of Giant Planets in Dense Nebulae: Critical Core Mass Revisited
Ikoma, M., Emori, H., & Nakazawa, K. (2001) · The Astrophysical Journal · doi:10.1086/320954 · Cited by 83
The Collision of Comet Shoemaker-Levy 9 and Jupiter
Noll, K., Weaver, H. A., & Feldman, P. D. (1996) · Cited by 72
Distribution of Planetesimals around a Protoplanet in the Nebula Gas
Tanaka, H., & Ida, S. (1997) · Icarus · doi:10.1006/icar.1996.9998 · Cited by 67
Comet Shoemaker-Levy 9: Impact on Jupiter and Plume Evolution
Takata, T., O’Keefe, J. D., Ahrens, T. J., & Orton, G. S. (1994) · Icarus · doi:10.1006/icar.1994.1074 · Cited by 61
Disintegration Phenomena Expected During Collision of Comet Shoemaker-Levy 9 with Jupiter
Sekanina, Z. (1993) · Science · doi:10.1126/science.262.5132.382 · Cited by 56
Explosions of infalling comets in Jupiter's atmosphere
Chevalier, R. A., & Sarazin, C. L. (1994) · The Astrophysical Journal · doi:10.1086/174371 · Cited by 46
Biberman, L. M., Bronin, S. Y., & Brykin, M. V. (1980) · Acta Astronautica · doi:10.1016/0094-5765(80)90116-2 · Cited by 43
The behavior of fragments of comet Shoemaker-Levy 9 in the atmosphere of Jupiter
Field, G. B., & Ferrara, A. (1995) · The Astrophysical Journal · doi:10.1086/175137 · Cited by 41
High-Resolution Calculations of Asteroid Impacts into the Venusian Atmosphere
Korycansky, D. G. (2000) · Icarus · doi:10.1006/icar.2000.6426 · Cited by 36
Impact Mechanics and Frequency of SL9-Type Events on Jupiter☆
Roulston, M. S., & Ahrens, T. J. (1997) · Icarus · doi:10.1006/icar.1996.5636 · Cited by 18
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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Self-citationPLANET OCCURRENCE WITHIN 0.25 AU OF SOLAR-TYPE STARS FROM KEPLER
Howard, A. W., Marcy, G. W., Bryson, S. T., Jenkins, J. M., Rowe, J. F., Batalha, N. M., Borucki, W. J., Koch, D. G., Dunham, E. W., Gautier, T. N., et al. (2012) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/201/2/15 · Cited by 1,151
Andrews, S. M., Huang, J., Pérez, L. M., Isella, A., Dullemond, C. P., Kurtovic, N. T., Guzmán, V. V., Carpenter, J. M., Wilner, D. J., Zhang, S., et al. (2018) · The Astrophysical Journal Letters · doi:10.3847/2041-8213/aaf741 · Cited by 1,134
The Growth Mechanisms of Macroscopic Bodies in Protoplanetary Disks
Blum, J., & Wurm, G. (2008) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.46.060407.145152 · Cited by 897
Cumming, A., Butler, R. P., Marcy, G. W., Vogt, S. S., Wright, J. T., & Fischer, D. A. (2008) · Publications of the Astronomical Society of the Pacific · doi:10.1086/588487 · Cited by 892
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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