Planetary Migration
Planetary Migration is a dynamical process in planetary systems whereby a planet’s orbit—especially its semi-major axis—undergoes systematic change over time due to gravitational and tidal interactions with a protoplanetary disk, planetesimals, other planets, or the central star.
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Citations
1.3K
Authors
532
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Publications per year
2017–2026
317
1K
A low mass for Mars from Jupiter’s early gas-driven migration
K. J. Walsh, Alessandro Morbidelli, Sean N. Raymond et al. · Nature · 2011 · 1.2K citations · Full text
Natural Sciences, Astronomy, Physics +16
Protoplanet Migration by Nebula Tides
William R. Ward · Icarus · 1997 · 1.1K citations
Natural Sciences, Astronomy, Physics +11
Planet-Disk Interaction and Orbital Evolution
W. Kley, Richard P. Nelson · Annual Review of Astronomy and Astrophysics · 2012 · 730 citations · Full text
Natural Sciences, Astronomy, Physics +17
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532

Centre National de la Recherche Scientifique
Paris, France
57 h-index
315 publications
29.1K citations
Observatoire de la Côte d’Azur
Nice, France
45 h-index
122 publications
12.9K citations

Southwest Research Institute
San Antonio, United States
44 h-index
78 publications
10.6K citations
Queen Mary University of London
London, United Kingdom
41 h-index
105 publications
10.2K citations
University of California, Santa Cruz
Santa Cruz, United States
38 h-index
72 publications
8.7K citations
University of Cambridge
Cambridge, United Kingdom
35 h-index
97 publications
5.9K citations
Max Planck Institute for Astronomy
Heidelberg, Germany
35 h-index
100 publications
6.6K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
33 h-index
95 publications
7.8K citations
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ApJ · 223 publications · 23.9K citations
91
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158 publications · 12K citations
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224 publications · 12.9K citations
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AJ · 67 publications · 5K citations
38
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46 publications · 3.3K citations
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