Early Planetary Differentiation
Early Planetary Differentiation is a geological process paradigm in planetary science denoting the initial large-scale separation of a planet's constituent materials into chemically distinct layers—such as core, mantle, and crust—driven primarily by density contrasts and convective instabilities during the early stages of planetary formation.
79
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10K
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247
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143
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Publications per year
2017–2026
16
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79
Calibration of the Lutetium-Hafnium Clock
Erik E. Scherer, Carsten Münker, Klaus Mezger · Science · 2001 · 2.5K citations
The generation and evolution of the continental crust
Chris J. Hawkesworth, Bruno Dhuime, Anna Pietranik et al. · Journal of the Geological Society · 2010 · 788 citations
What we have learned about Mars from SNC meteorites
H. Y. McSween · Meteoritics · 1994 · 618 citations
Planetary crusts: their composition, origin and evolution
Choice Reviews Online · 2009 · 428 citations
Natural Sciences, Astronomy, Geology +17
The persistent myth of crustal growth
R. L. Armstrong · Australian Journal of Earth Sciences · 1991 · 344 citations
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143
Massachusetts Institute of Technology
Cambridge, United States
9 h-index
16 publications
1.2K citations
Planetary Science Institute
Tucson, United States
8 h-index
15 publications
1.4K citations

Centre National de la Recherche Scientifique
Paris, France
7 h-index
19 publications
840 citations
University of Münster
Münster, Germany
7 h-index
20 publications
8.6K citations
University of New Mexico
Albuquerque, United States
6 h-index
8 publications
1.1K citations
University of Bern
Bern, Switzerland
4 h-index
7 publications
315 citations
Max Planck Society
Munich, Germany
4 h-index
7 publications
338 citations
University of Maryland, College Park
College Park, United States
4 h-index
9 publications
612 citations
1–8 of 143
13 publications · 988 citations
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11 publications · 892 citations
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10 publications · 666 citations
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5 publications · 3.2K citations
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PNAS · 5 publications · 261 citations
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