Last giant impact on Uranus: constraints on oligarchic masses in the trans-Saturnian region
Context. Modern models of the formation of ice giants attempt to account for the formation of Uranus and Neptune within the protoplanetary disk lifetime. These models assume a higher initial surface density well above that of the minimum mass solar nebula model and/or the formation of all giant plan...
Guardado en:
| Autor principal: | Parisi, Mirta Gabriela |
|---|---|
| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2011
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/123995 |
| Aporte de: |
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