Impact-driven Core Formation
Impact-Driven Core Formation is a theoretical framework within planetary science that explains the differentiation of metallic cores in terrestrial planets through high-energy impact events as the primary mechanism driving mass segregation and core accretion.
203
Publications
15.4K
Citations
582
Authors
263
Institutions
Publications per year
2017–2026
47
Parents
203
Forming a Moon with an Earth-like Composition via a Giant Impact
R. M. Canup · Science · 2012 · 642 citations
Evolution of Planetary Cores and the Earth-Moon System from Nb/Ta Systematics
Carsten Münker, Jörg A. Pfänder, Stefan Weyer et al. · Science · 2003 · 451 citations
Young chondrules in CB chondrites from a giant impact in the early Solar System
Alexander N. Krot, Yuri Amelin, P. Cassen et al. · Nature · 2005 · 330 citations
1–5 of 203
582
6
h-index
6
h-index
6
h-index
6
h-index
Johns Hopkins University Applied Physics Laboratory, United States
5 publications · 397 citations
5
h-index
1–5 of 582
263
Planetary Science Institute
Tucson, United States
23 h-index
63 publications
7.4K citations

Southwest Research Institute
San Antonio, United States
18 h-index
39 publications
5.1K citations

Centre National de la Recherche Scientifique
Paris, France
16 h-index
42 publications
1.6K citations
California Institute of Technology
Pasadena, United States
12 h-index
19 publications
1.7K citations
University of California, Santa Cruz
Santa Cruz, United States
11 h-index
18 publications
1.8K citations

Johns Hopkins University Applied Physics Laboratory
North Laurel, United States
10 h-index
17 publications
1.8K citations
University of Arizona
Tucson, United States
10 h-index
19 publications
1.7K citations
Arizona State University
Tempe, United States
9 h-index
15 publications
985 citations
1–8 of 263
36 publications · 2.9K citations
27
h-index
13 publications · 2.3K citations
13
h-index
ApJ · 12 publications · 666 citations
12
h-index
12 publications · 469 citations
12
h-index
JGR · 11 publications · 1K citations
11
h-index
1–5