The 8/5 resonance between TRAPPIST-1 innermost planets
Interactions between the planets with the protoplanetary gas disk produce migration, whose rates depend on the features of the gas-disk and the mass of the migrating planets. Due to the uncertainties in the estimations of masses of the TRAPPIST-1 planets, their migration rates are not well determine...
Guardado en:
| Autores principales: | Charalambous, C., Beaugé, C. |
|---|---|
| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2021
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/165454 |
| Aporte de: |
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