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Enceladus’s measured physical libration requires a global subsurface ocean

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Thomas, P.C., Tajeddine, R., Tiscareno, M.S., Burns, J.A., Joseph, J., Loredo, T.J., Helfenstein, P., Porco, C.·2016·Icarus

Abstract

Abstract Several planetary satellites apparently have subsurface seas that are of great interest for, among other reasons, their possible habitability. The geologically diverse saturnian satellite Enceladus vigorously vents liquid water and vapor from fractures within a south polar depression and thus must have a liquid reservoir or active melting. However, the extent and location of any subsurface liquid region is not directly observable. We use measurements of control points across the surface of Enceladus accumulated over seven years of spacecraft observations to determine the satellite’s precise rotation state, finding a forced physical libration of 0.120 ± 0.014° (2σ). This value is too large to be consistent with Enceladus’s core being rigidly connected to its surface, and thus implies the presence of a global ocean rather than a localized polar sea. The maintenance of a global ocean within Enceladus is problematic according to many thermal models and so may constrain satellite properties or require a surprisingly dissipative Saturn.

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Metadata

Authors
Thomas, P. C., Tajeddine, R., Tiscareno, M. S., Burns, J. A., Joseph, J., Loredo, T. J., Helfenstein, P., & Porco, C.
Venue
Icarus
Publisher
Elsevier BV
Published
2016-01
Volume
264
Pages
37-47
ISSN
0019-1035 (ISSN-L)
OpenAlex
W2097197675
Cited by
414
References
37
FWCI
21.22
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: Enceladus’s measured physical libration requires a global subsurface ocean. https://app.cochat.ai/papers/10.1016/j.icarus.2015.08.037
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Thomas, P. C., Tajeddine, R., Tiscareno, M. S., Burns, J. A., Joseph, J., Loredo, T. J., Helfenstein, P., & Porco, C. (2016). Enceladus’s measured physical libration requires a global subsurface ocean. Icarus. https://doi.org/10.1016/j.icarus.2015.08.037

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