The Tides of Enceladus' Porous Core

The inferred density of Enceladus' core, together with evidence of hydrothermal activity within the moon, suggests that the core is porous. Tidal dissipation in an unconsolidated core has been proposed as the main source of Enceladus' geological activity. However, the tidal response of its...

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Detalles Bibliográficos
Autores principales: Rovira‐Navarro, Marc, Katz, Richard F., Liao, Yang, van der Wal, Wouter, Nimmo, Francis
Formato: Online Artículo Texto
Lenguaje:English
Publicado: John Wiley and Sons Inc. 2022
Materias:
Research Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9285949/
https://www.ncbi.nlm.nih.gov/pubmed/35865509
http://dx.doi.org/10.1029/2021JE007117

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9285949/
https://www.ncbi.nlm.nih.gov/pubmed/35865509
http://dx.doi.org/10.1029/2021JE007117

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