Journal article icon

Journal article

The tides of Enceladus' porous core

Abstract:
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 core has generally been modeled assuming it behaves viscoelastically rather than poroviscoelastically. In this work, we analyze the poroviscoelastic response to better constrain the distribution of tidal dissipation within Enceladus. A poroviscoelastic body has a different tidal response than a viscoelastic one; pressure within the pores alters the stress field and induces a Darcian porous flow. This flow represents an additional pathway for energy dissipation. Using Biot's theory of poroviscoelasticity, we develop a new framework to obtain the tidal response of a spherically symmetric, self-gravitating moon with porous layers and apply it to Enceladus. We show that the boundary conditions at the interface of the core and overlying ocean play a key role in the tidal response. The ocean hinders the development of a large-amplitude Darcian flow, making negligible the Darcian contribution to the dissipation budget. We therefore infer that Enceladus' core can be the source of its geological activity only if it has a low rigidity and a very low viscosity. A future mission to Enceladus could test this hypothesis by measuring the phase lags of tidally induced changes of gravitational potential and surface displacements.
Publication status:
Published
Peer review status:
Peer reviewed

Actions


Access Document


Publisher copy:
10.1029/2021je007117

Authors


More by this author
Role:
Author
ORCID:
0000-0002-9980-5065
More by this author
Institution:
University of Oxford
Division:
MPLS
Department:
Earth Sciences
Oxford college:
St Anne's College
Role:
Author
ORCID:
0000-0001-8746-5430
More by this author
Role:
Author
ORCID:
0000-0002-8201-4152
More by this author
Role:
Author
ORCID:
0000-0001-8030-9080
More by this author
Role:
Author
ORCID:
0000-0003-3573-5915


Publisher:
American Geophysical Union
Journal:
Journal of Geophysical Research: Planets More from this journal
Volume:
127
Issue:
5
Article number:
e2021JE007117
Publication date:
2022-05-24
Acceptance date:
2022-04-27
DOI:
EISSN:
2169-9100
ISSN:
2169-9097


Language:
English
Keywords:
Pubs id:
1257188
Local pid:
pubs:1257188
Deposit date:
2022-06-01

Terms of use



Views and Downloads






If you are the owner of this record, you can report an update to it here: Report update to this record

TO TOP