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Enceladus’s measured physical libration requires a global subsurface ocean

Authors
  • P C, Thomas
  • R, Tajeddine
  • Matthew Tiscareno
  • J A, Burns
  • J, Joseph
  • T J, Loredo
  • P, Helfenstein
  • C, Porco
Type
Published Article
Journal
Icarus
Publisher
Elsevier
Publication Date
Jan 27, 2016
Volume
264
Pages
37–47
Identifiers
DOI: 10.1016/j.icarus.2015.08.037
Source
SETI Institute
License
Yellow

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 ...

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