Runaway Growth
Runaway Growth is a theoretical model in planetary formation that describes the rapid, self-amplifying accretion of solid material by a protoplanetary embryo due to its gravitational focusing advantage over smaller neighbors, leading to the preferential growth of a few dominant bodies within a swarm of planetesimals.
95
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7.3K
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182
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123
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2017–2026
16
Variants
Runaway Accretion
Parents
95
Richard B. Larson · Reports on Progress in Physics · 2003 · 366 citations · Full text
Natural Sciences, Astronomy, Physics +17
On Runaway Growth of Planetesimals
Eiichiro Kokubo, Shigeru Ida · Icarus · 1996 · 346 citations
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Tokyo Institute of Technology
Tokyo, Japan
11 h-index
15 publications
1.6K citations
Planetary Science Institute
Tucson, United States
6 h-index
7 publications
263 citations
The University of Tokyo
Tokyo, Japan
6 h-index
11 publications
1.7K citations
University of California, Berkeley
Berkeley, United States
5 h-index
8 publications
600 citations
University of Maryland, College Park
College Park, United States
3 h-index
4 publications
284 citations
National Astronomical Observatory of Japan
Mitaka-shi, Japan
3 h-index
3 publications
166 citations
University of California, Santa Barbara
Santa Barbara, United States
3 h-index
4 publications
981 citations
Max Planck Society
Munich, Germany
3 h-index
6 publications
389 citations
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ApJ · 16 publications · 1.6K citations
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10 publications · 459 citations
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9 publications · 1.1K citations
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AJ · 4 publications · 451 citations
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4 publications · 141 citations
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