Co-accretion Processes
Co-Accretion Processes is a theoretical framework in planetary science that explains the concurrent formation of a planetary satellite and its host planet from a shared circumplanetary disk, distinguishing it from alternative satellite origin models by emphasizing synchronized condensation and accumulation of mass within a gravitationally bound co-orbital environment.
16
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3.8K
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42
Authors
33
Institutions
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2017–2026
9
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16
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
The formation of Jupiter by hybrid pebble–planetesimal accretion
Nature Astronomy · 2018 · 114 citations · Full text
Natural Sciences, Astronomy, Physics +12
A. S. Wong · Icarus · 2002 · 74 citations
A co-accretional model of satellite formation
Alan W. Harris, W. M. Kaula · Icarus · 1975 · 66 citations
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33
University of California, Santa Cruz
Santa Cruz, United States
2 h-index
4 publications
6.3K citations
University of Bern
Bern, Switzerland
2 h-index
8 publications
718 citations

Southwest Research Institute
San Antonio, United States
2 h-index
4 publications
62 citations

University of Leicester
Leicester, United Kingdom
1 h-index
1 publications
16 citations
University of Zurich
Zurich, Switzerland
1 h-index
3 publications
342 citations
Stony Brook University
Stony Brook, United States
1 h-index
1 publications
3.1K citations
Max Planck Institute for Astronomy
Heidelberg, Germany
1 h-index
1 publications
38 citations

Trieste Astronomical Observatory
Trieste, Italy
1 h-index
1 publications
16 citations
1–8 of 33
3 publications · 71 citations
3
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3 publications · 3.3K citations
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ApJ · 2 publications · 31 citations
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2 publications · 143 citations
2
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1 publications · 193 citations
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