Terrestrial Planet Migration
Terrestrial Planet Migration is a theoretical construct in planetary science that denotes the orbital displacement of rocky, Earth-like planets within protoplanetary disks due to gravitational interactions with disk material or other celestial bodies, distinguishing it from migration mechanisms affecting giant or gaseous planets.
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2.3K
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62
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51
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2017–2026
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The Non-carbonaceous–Carbonaceous Meteorite Dichotomy
T. Kleine, G. Budde, Christoph Burkhardt et al. · Space Science Reviews · 2020 · 184 citations · Full text
Volatile-rich Earth-Mass Planets in the Habitable Zone
The Astrophysical Journal · 2003 · 161 citations · Full text
Exchange of Meteorites (and Life?) Between Stellar Systems
H. J. Melosh · Astrobiology · 2003 · 107 citations
Natural Sciences, Astronomy, Physics +12
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Queen Mary University of London
London, United Kingdom
7 h-index
14 publications
788 citations
Observatoire de la Côte d’Azur
Nice, France
5 h-index
9 publications
722 citations

Centre National de la Recherche Scientifique
Paris, France
5 h-index
10 publications
652 citations
Ministry of Education
Brasília, Brazil
3 h-index
3 publications
197 citations

Southwest Research Institute
San Antonio, United States
3 h-index
4 publications
221 citations
Université de Bordeaux
Bordeaux, France
3 h-index
4 publications
329 citations
Laboratoire d'Astrophysique de Bordeaux
Bordeaux, France
3 h-index
4 publications
329 citations
University of California, Santa Cruz
Santa Cruz, United States
2 h-index
3 publications
504 citations
1–8 of 51
ApJ · 8 publications · 565 citations
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5 publications · 369 citations
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5 publications · 223 citations
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Repository · 3 publications · 134 citations
3
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2 publications · 267 citations
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