Forming Jupiter, Saturn, Uranus and Neptune in few million years by core accretion
Giant planet formation process is still not completely understood. The current most accepted paradigm, the core instability model, explains several observed properties of the Solar System’s giant planets but, to date, has faced difficulties to account for a formation time shorter than the observatio...
Guardado en:
| Autores principales: | Benvenuto, Omar Gustavo, Fortier, Andrea, Brunini, Adrián |
|---|---|
| Formato: | Articulo Preprint |
| Lenguaje: | Inglés |
| Publicado: |
2009
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/93653 https://www.sciencedirect.com/science/article/pii/S0019103509002875?via%3Dihub |
| Aporte de: |
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