Powering prolonged hydrothermal activity inside Enceladus
Tidal forcing within a very porous (unconsolidated) core can generate enough energy to drive all the observed global features of Enceladus. This activity can be sustained up to several billion years.</p>
Gespeichert in:
| Hauptverfasser: | , , , |
|---|---|
| Dokumenttyp: | Article (Journal) Editorial |
| Sprache: | Englisch |
| Veröffentlicht: |
06 November 2017
|
| In: |
Nature astronomy
Year: 2017, Pages: 841-847 |
| ISSN: | 2397-3366 |
| DOI: | 10.1038/s41550-017-0289-8 |
| Online-Zugang: | Verlag, Volltext: http://dx.doi.org/10.1038/s41550-017-0289-8 Verlag, Volltext: https://www.nature.com/articles/s41550-017-0289-8 
|
| Verfasserangaben: | Christophe Sotin, Frank Postberg, Gaël Choblet, Gabriel Tobie, Marie Běhounková, Ondřej Čadek, Ondřej Souček |
| Zusammenfassung: | Tidal forcing within a very porous (unconsolidated) core can generate enough energy to drive all the observed global features of Enceladus. This activity can be sustained up to several billion years.</p> |
|---|---|
| Beschreibung: | Gesehen am 05.08.2022 |
| Beschreibung: | Online Resource |
| ISSN: | 2397-3366 |
| DOI: | 10.1038/s41550-017-0289-8 |