Effect of the tiger stripes on the deformation of Saturn's moon Enceladus
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- Type
- article
- Published
- 2016-07-28
- Cited by
- 42
- References
- 26
- OpenAlex
- https://openalex.org/W2506014542
- Semantic Scholar
- https://api.semanticscholar.org/CorpusID:132555734
Keywords
Enceladus, Saturn, Icy moon, Tidal heating, Geology
References
- The fluffy core of Enceladus
- A salt-water reservoir as the source of a compositionally stratified plume on Enceladus
- Sodium salts in E-ring ice grains from an ocean below the surface of Enceladus
- High heat flow from Enceladus' south polar region measured using 10–600 cm−1 Cassini/CIRS data
- Cassini Encounters Enceladus: Background and the Discovery of a South Polar Hot Spot
- Shear heating as the origin of the plumes and heat flux on Enceladus
- Tidally-induced melting events as the origin of south-pole activity on Enceladus
- Association of the jets of Enceladus with the warmest regions on its south-polar fractures
- Ongoing hydrothermal activities within Enceladus
- Eruptions arising from tidally controlled periodic openings of rifts on Enceladus
- Keeping Enceladus warm
- Solid tidal friction above a liquid water reservoir as the origin of the south pole hotspot on Enceladus
- HOW THE GEYSERS, TIDAL STRESSES, AND THERMAL EMISSION ACROSS THE SOUTH POLAR TERRAIN OF ENCELADUS ARE RELATED
- An observed correlation between plume activity and tidal stresses on Enceladus
- Enceladus's measured physical libration requires a global subsurface ocean
- TIDALLY MODULATED ERUPTIONS ON ENCELADUS: CASSINI ISS OBSERVATIONS AND MODELS
- The role of episodic overturn in generating the surface geology and heat flow on Enceladus
- Structural mapping of Enceladus and implications for formation of tectonized regions
- Cassini Observes the Active South Pole of Enceladus
- Tidal dissipation by solid friction and the resulting orbital evolution
Cited by
- Thermally anomalous features in the subsurface of Enceladus’s south polar terrain
- Tidal effects in differentiated viscoelastic bodies: a numerical approach
- Plume Activity and Tidal Deformation on Enceladus Influenced by Faults and Variable Ice Shell Thickness
- Powering prolonged hydrothermal activity inside Enceladus
- Energy balance of glacial isostatic adjustment: importance of the rotational feedback
- Enceladus’s crust as a non-uniform thin shell: I tidal deformations
- Does Titan’s long-wavelength topography contain information about subsurface ocean dynamics?
- Maxwell-type viscoelasticity in small and large deformations of planetary mantles
- Long-term stability of Enceladus’ uneven ice shell
- Dust Emission by Active Moons
- Formation of the Cassini Division – II. Possible histories of Mimas and Enceladus
- Tidal dissipation in Enceladus' uneven, fractured ice shell
- Enceladus's crust as a non-uniform thin shell: II tidal dissipation
- Enceladus's ice shell structure as a window on internal heat production
- Tidal deformation of Enceladus' ice shell with variable thickness and Maxwell rheology
- Tides in subsurface oceans with meridional varying thickness
- Plume Sample Modification at Icy Moons: Implications for Biosignatures
- Ice-Ocean Exchange Processes in the Jovian and Saturnian Satellites
- Assessing the brittle crust thickness from strike-slip fault segments on Earth, Mars and Icy moons
- Enceladus' Tiger Stripes as Frictional Faults: Effect on Stress and Heat Production
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- Tidal Dissipation in Subsurface Oceans: Enceladus and Other Icy Moons
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