Interior Composition Models is a scientific framework that specifies the distribution and abundance of chemical elements and minerals within a planet's layers, distinguishing it from other structural models by focusing on material properties and thermodynamic constraints to infer planetary formation and evolution histories.
52
Publications
5.8K
Citations
119
Authors
99
Institutions
Publications per year
2017–2026
23
Parents
Publications
52
Mass‐Radius Relationships for Solid Exoplanets
Sara Seager, Marc J. Kuchner, C. A. Hier‐Majumder et al. · The Astrophysical Journal · 2007 · 821 citations · Full text
Natural Sciences, Astronomy, Physics +17
MASS–RADIUS RELATION FOR ROCKY PLANETS BASED ON PREM
Li Zeng, Dimitar Sasselov, S. B. Jacobsen · The Astrophysical Journal · 2016 · 433 citations · Full text
1–5 of 52
Authors
119
- RH
8
h-index
- TG
5
h-index
- DV
4
h-index
- JI
4
h-index
- MP
4
h-index
1–5 of 119
Institutions
99
University of Zurich
Zurich, Switzerland
11 h-index
18 publications
794 citations
Centre National de la Recherche Scientifique
Paris, France
11 h-index
20 publications
2.1K citations
Planetary Science Institute
Tucson, United States
7 h-index
10 publications
2.4K citations
ETH Zurich
Zurich, Switzerland
6 h-index
10 publications
494 citations
Tel Aviv University
Tel Aviv, Israel
5 h-index
10 publications
873 citations
Observatoire de la Côte d’Azur
Nice, France
5 h-index
9 publications
931 citations
Leiden University
Leiden, The Netherlands
4 h-index
4 publications
150 citations
University of Arizona
Tucson, United States
4 h-index
5 publications
805 citations
1–8 of 99
Venues
- The Astrophysical Journal
ApJ · 14 publications · 3K citations
14
h-index
- Astronomy and Astrophysics
10 publications · 946 citations
10
h-index
- Monthly Notices of the Royal Astronomical Society
6 publications · 282 citations
6
h-index
- The Astrophysical Journal Letters
5 publications · 290 citations
4
h-index
- Icarus
3 publications · 178 citations
3
h-index
1–5