Planetary Embryo Formation
Planetary Embryo Formation is a theoretical construct in planetary science that describes the stage in which kilometer-sized protoplanetary bodies coalesce through gravitational instability and collisional accretion within a protoplanetary disk, distinguishing it from earlier stages of dust coagulation and subsequent phases of planetary differentiation.
157
Publications
11.7K
Citations
258
Authors
160
Institutions
Publications per year
2017–2026
65
Parents
157
1–5 of 157
258
15
h-index
9
h-index
9
h-index
Consejo Nacional de Investigaciones Científicas y Técnicas, Argentina
8 publications · 227 citations
8
h-index
7
h-index
1–5 of 258
160

Centre National de la Recherche Scientifique
Paris, France
22 h-index
61 publications
5.6K citations
Observatoire de la Côte d’Azur
Nice, France
16 h-index
29 publications
4.1K citations
Max Planck Institute for Astronomy
Heidelberg, Germany
13 h-index
22 publications
1.2K citations

Consejo Nacional de Investigaciones Científicas y Técnicas
Buenos Aires, Argentina
13 h-index
32 publications
917 citations
University of Bern
Bern, Switzerland
12 h-index
24 publications
1.2K citations
Instituto de Astrofísica de La Plata
La Plata, Argentina
12 h-index
26 publications
824 citations
Planetary Science Institute
Tucson, United States
10 h-index
19 publications
800 citations
Université de Bordeaux
Bordeaux, France
10 h-index
26 publications
2.3K citations
1–8 of 160
32 publications · 2.3K citations
24
h-index
ApJ · 21 publications · 1.6K citations
19
h-index
25 publications · 1.1K citations
19
h-index
12 publications · 1.7K citations
12
h-index
Repository · 9 publications · 701 citations
9
h-index
1–5