The DOI matches its Crossref record; 72 of the 72 references it cites were found in a registry or an index.
Toward a Deterministic Model of Planetary Formation. III. Mass Distribution of Short‐Period Planets around Stars of Various Masses
Open accessAbstract
The origin of a recently discovered close-in Neptune-mass planet around GJ 436 poses a challenge to the current theories of planet formation. On the basis of the sequential accretion hypothesis and the standard theory of gap formation and orbital migration, we show that around M dwarf stars, close-in Neptune-mass ice giant planets may be relatively common, while close-in Jupiter-mass gas giant planets are relatively rare. The mass distribution of close-in planets generally has two peaks at about Neptune mass and Jupiter mass. The lower mass peak takes the maximum frequency for M dwarfs. Around more massive solar-type stars (G dwarfs), the higher mass peak is much more pronounced. Planets around G dwarfs undergo orbital migration after fully accreting gas, while those around M dwarfs tend to migrate before starting rapid gas accretion. Close-in Neptune-mass planets may also exist around G dwarfs, although they tend to be mostly composed of silicates and iron cores and their frequency is expected to be much smaller than that of Neptune-mass planets around M dwarfs and that of gas giants around G dwarfs. We also show that the conditions for planets' migration due to their tidal interaction with the disk and the stellar mass dependence in the disk mass distribution can be calibrated by the mass distribution of short-period planets around host stars with various masses.
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Cites
Mannings, V (2000) · Icarus · doi:10.1006/icar.1999.6299 · Cited by 4,151
A Jupiter-mass companion to a solar-type star
Mayor, M., & Queloz, D. (1995) · Nature · doi:10.1038/378355a0 · Cited by 4,111
On the Gravitational Stability of a Disk of Stars
Toomre, A. (1964) · The Astrophysical Journal · doi:10.1086/147861 · Cited by 3,349 · cited 1×
“The condition of the gravitational instability is 1 > Q = csΩK/πGΣg ∝ M 1/2 ∗ M 1/2 ∗ /Σg = M 1−β ∗ , and its radial wavelength λ = 2π2GΣg/Ω 2 K ∝ M β−1 ∗ (Toomre 1964) where Σg ∝ M β ∗ .”
Formation of the Giant Planets by Concurrent Accretion of Solids and Gas
Pollack, J. B., Hubickyj, O., Bodenheimer, P., Lissauer, J. J., Podolak, M., & Greenzweig, Y. (1996) · Icarus · doi:10.1006/icar.1996.0190 · Cited by 3,127
(1993) · Choice Reviews Online · doi:10.5860/choice.31-2093 · Cited by 1,929
Hayashi, C. (1981) · Progress of Theoretical Physics Supplement · doi:10.1143/ptps.70.35 · Cited by 1,843
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
The Planet‐Metallicity Correlation
Fischer, D. A., & Valenti, J. (2005) · The Astrophysical Journal · doi:10.1086/428383 · Cited by 1,654
Goldreich, P., & Tremaine, S. (1980) · The Astrophysical Journal · doi:10.1086/158356 · Cited by 1,645
Evolution of the protoplanetary cloud and formation of the earth and the planets
Safronov, V. S. (1972) · Medical Entomology and Zoology · Cited by 1,341
Cited by
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
THE OCCURRENCE RATE OF SMALL PLANETS AROUND SMALL STARS
Dressing, C. D., & Charbonneau, D. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/767/1/95 · Cited by 749
The HARPS search for southern extra-solar planets: XXXI. The M-dwarf sample
Bonfils, X., Delfosse, X., Udry, S., Forveille, T., Mayor, M., Perrier, C., Bouchy, F., Gillon, M., Lovis, C., Pepe, F., et al. (2013) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201014704 · Cited by 653
The Occurrence and Mass Distribution of Close-in Super-Earths, Neptunes, and Jupiters
Howard, A. W., Marcy, G. W., Johnson, J. A., Fischer, D. A., Wright, J. T., Isaacson, H., Valenti, J. A., Anderson, J., Lin, D. N. C., & Ida, S. (2010) · Science · doi:10.1126/science.1194854 · Cited by 635
Self-citationCameron, A. C., Guenther, E., Smalley, B., McDonald, I., Hebb, L., Andersen, J., Augusteijn, T., Barros, S. C. C., Brown, D. J. A., Cochran, W. D., et al. (2010) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2010.16922.x · Cited by 324
Metadata
- Authors
- Ida, S., & Lin, D. N. C.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 2005-06-20
- Volume
- 626
- Issue
- 2
- Pages
- 1045-1060
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W2083351405
- Cited by
- 490
- References
- 72
- FWCI
- 18.94
- Type
- journal article
- Language
- en
- Open access
- bronze
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- Ida, S., & Lin, D. N. C. (2005). Toward a Deterministic Model of Planetary Formation. III. Mass Distribution of Short‐Period Planets around Stars of Various Masses. The Astrophysical Journal. https://doi.org/10.1086/429953
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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
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