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

Publications

7.3K

Citations

182

Authors

123

Institutions

Publications per year

2017–2026

16

Variants

Runaway Accretion

Authors

182

  1. SI
    Shigeru Ida

    Tokyo Institute of Technology, Japan

    4 publications · 837 citations

    4

    h-index

  2. EC
    Eugene Chiang

    University of California, Berkeley, United States

    3 publications · 97 citations

    3

    h-index

  3. CW
    Chris W. Ormel

    University of Amsterdam, Netherlands

    3 publications · 219 citations

    3

    h-index

  4. MH
    Man Hoi Lee

    University of Hong Kong, Hong Kong SAR China

    2 publications · 162 citations

    2

    h-index

  5. MS
    M. Spaans

    University of Groningen, Netherlands

    2 publications · 151 citations

    2

    h-index

1–5 of 182

Venues

  1. The Astrophysical Journal

    ApJ · 16 publications · 1.6K citations

    16

    h-index

  2. 10

    h-index

  3. Icarus

    9 publications · 1.1K citations

    9

    h-index

  4. The Astronomical Journal

    AJ · 4 publications · 451 citations

    4

    h-index

  5. Astronomy and Astrophysics

    4 publications · 141 citations

    4

    h-index

1–5