Accretion Of Solids
Accretion of Solids is a theoretical construct in planetary formation that describes the process by which microscopic dust particles in a protoplanetary disk coalesce under mutual gravitational and collisional interactions to form progressively larger solid bodies, ultimately leading to planetesimals.
264
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27.3K
Citations
523
Authors
292
Institutions
Publications per year
2017–2026
88
Parents
264
Formation of the Giant Planets by Concurrent Accretion of Solids and Gas
James B. Pollack, O. Hubickyj, Peter Bodenheimer et al. · Icarus · 1996 · 3.1K citations
Natural Sciences, Astronomy, Physics +14
Toward an Astrophysical Theory of Chondrites
Frank H. Shu, Hsien Shang, Typhoon Lee · Science · 1996 · 515 citations
Natural Sciences, Astronomy, Physics +13
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292

Centre National de la Recherche Scientifique
Paris, France
23 h-index
62 publications
5.5K citations
University of Bern
Bern, Switzerland
17 h-index
37 publications
2.6K citations
Max Planck Institute for Astronomy
Heidelberg, Germany
16 h-index
29 publications
1.9K citations
Planetary Science Institute
Tucson, United States
14 h-index
24 publications
2.9K citations
University of California, Santa Cruz
Santa Cruz, United States
14 h-index
20 publications
9K citations
University of Münster
Münster, Germany
11 h-index
18 publications
5K citations

Ames Research Center
Mountain View, United States
10 h-index
15 publications
4.3K citations

Southwest Research Institute
San Antonio, United States
10 h-index
61 publications
5.4K citations
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ApJ · 38 publications · 3.4K citations
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36 publications · 3.7K citations
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23 publications · 1.1K citations
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22 publications · 4.6K citations
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17 publications · 1.7K citations
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