© 2016 Elsevier Inc. We determine constraints on the ice shell and ocean of Enceladus from the observed libration at orbital period by assessing the effects of uncertainties in the size, density, rigidity, and viscosity of the internal layers and of the non-hydrostatic structure on the libration. The observed libration amplitude implies that the average thickness of the ice shell is between 14 km and 26 km and that the ocean is 21 km to 67 km thick.status: publishe
The year 2017 saw Cassini plunge to its demise into Saturn's atmosphere, putting an end to a twenty-...
International audiencePhysical librations could significantly contribute to Enceladus' geophysics th...
Comsol Multiphysics models solving the stress field in Enceladus' ice shell when a regional sea of g...
We determine constraints on the ice shell and ocean of Enceladus from the observed libration at orbi...
©2016. American Geophysical Union. All Rights Reserved. The intense plume activity at the South Pole...
The latest measurements of the librations of Enceladus suggest that it could have a global subsurfac...
The Saturnian moon Enceladus is one of the most geologically active bodies in the solar system. Ridg...
Europa, the smallest of the Galilean satellites, has a young icy surface and most likely contains an...
The process by which the subsurface ocean on Enceladus is heated remains a puzzle. Tidal interaction...
Recent geodetic measurements for Enceladus suggest a global subsurface ocean that is thicker beneath...
The extraordinary activity at Enceladus’ warm south pole indicates the presence of an internal globa...
[1] Enceladus’s south polar thermal anomaly and water‐ rich plumes suggest the existence of a subsur...
The four Galilean satellites are thought to harbor one or even two global internal liquid layers ben...
The past close encounters of the CASSINI spacecraft in the Saturnian system have provided unpreceden...
Given the non-spherical shape of Enceladus, the satellite may experience gravitational torques that ...
The year 2017 saw Cassini plunge to its demise into Saturn's atmosphere, putting an end to a twenty-...
International audiencePhysical librations could significantly contribute to Enceladus' geophysics th...
Comsol Multiphysics models solving the stress field in Enceladus' ice shell when a regional sea of g...
We determine constraints on the ice shell and ocean of Enceladus from the observed libration at orbi...
©2016. American Geophysical Union. All Rights Reserved. The intense plume activity at the South Pole...
The latest measurements of the librations of Enceladus suggest that it could have a global subsurfac...
The Saturnian moon Enceladus is one of the most geologically active bodies in the solar system. Ridg...
Europa, the smallest of the Galilean satellites, has a young icy surface and most likely contains an...
The process by which the subsurface ocean on Enceladus is heated remains a puzzle. Tidal interaction...
Recent geodetic measurements for Enceladus suggest a global subsurface ocean that is thicker beneath...
The extraordinary activity at Enceladus’ warm south pole indicates the presence of an internal globa...
[1] Enceladus’s south polar thermal anomaly and water‐ rich plumes suggest the existence of a subsur...
The four Galilean satellites are thought to harbor one or even two global internal liquid layers ben...
The past close encounters of the CASSINI spacecraft in the Saturnian system have provided unpreceden...
Given the non-spherical shape of Enceladus, the satellite may experience gravitational torques that ...
The year 2017 saw Cassini plunge to its demise into Saturn's atmosphere, putting an end to a twenty-...
International audiencePhysical librations could significantly contribute to Enceladus' geophysics th...
Comsol Multiphysics models solving the stress field in Enceladus' ice shell when a regional sea of g...