Planetesimal Differentiation
Planetesimal Differentiation is a geological process within planetary science whereby planetesimals, the primordial building blocks of planets, undergo internal chemical and physical segregation due to heat-driven melting and gravitational separation, leading to the formation of compositionally distinct layers such as metallic cores and silicate mantles.
25
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2.1K
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99
Authors
72
Institutions
Publications per year
2017–2026
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A new family of planets? “Ocean-Planets”
A. Léger, Franck Selsis, C. Sotin et al. · Icarus · 2004 · 357 citations · Full text
A low-temperature origin for the planetesimals that formed Jupiter
Tobias Owen, P. R. Mahaffy, H. Niemann et al. · Nature · 1999 · 340 citations · Full text
Paleomagnetic Records of Meteorites and Early Planetesimal Differentiation
Benjamin P. Weiss, J. Gattacceca, S. Stanley et al. · Space Science Reviews · 2009 · 159 citations
Ice lines, planetesimal composition and solid surface density in the solar nebula
Sarah Dodson-Robinson, Karen Willacy, Peter Bodenheimer et al. · Icarus · 2008 · 144 citations · Full text
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Massachusetts Institute of Technology
Cambridge, United States
5 h-index
10 publications
1.2K citations

Centre National de la Recherche Scientifique
Paris, France
4 h-index
16 publications
3.3K citations
Planetary Science Institute
Tucson, United States
3 h-index
3 publications
212 citations
California Institute of Technology
Pasadena, United States
3 h-index
4 publications
398 citations
University of Michigan
Ann Arbor, United States
2 h-index
4 publications
828 citations

Institut de physique du globe de Paris
Paris, France
2 h-index
5 publications
172 citations
Jet Propulsion Laboratory
Pasadena, United States
2 h-index
4 publications
529 citations
University of Colorado Boulder
Boulder, United States
2 h-index
2 publications
118 citations
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7 publications · 676 citations
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3 publications · 372 citations
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2 publications · 172 citations
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2 publications · 80 citations
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1 publications · 28 citations
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