Implications from Ithaca Chasma for the thermal and orbital history of Tethys

• Published in: Geophysical research letters Vol. 35; no. 19; pp. L19203 - n/a
• Main Authors: Chen, E. M. A., Nimmo, F.
• Format: Journal Article
• Language: English
• Published: Washington, DC American Geophysical Union 01.10.2008; Blackwell Publishing Ltd
• Subjects: Earth sciences; Earth, ocean, space; Exact sciences and technology; Hydrology and fluvial processes; Ices; Planetary Sciences; satellites; Saturn; Saturnian satellites; Solar System Objects; Solid Surface Planets; Tethys; Greece; Southern Europe; Greek Ionian Islands; Europe; Ithaca; USA, New York, Ithaca; satellites; Saturn; Tethys; thickness; eccentricity; damping; resonance; Modeling; Dione; heat sources; Enceladus; Internal structure; warming; equilibrium; heat flux; heat transfer
• ISSN: 0094-8276; 1944-8007
• DOI: 10.1029/2008GL035402

Flexural modeling of Ithaca Chasma on Tethys suggests that the elastic thickness and the surface heat flux were 5–7 km and 18–30 mW/m2 respectively, when the feature formed (∼4 Gyr B.P.). Tidal heating is a plausible heat source, suggesting that Tethys' eccentricity was higher in the past. Depending on Tethys' internal structure, eccentricities in the range 0.001 to 0.02 are sufficient to have generated the inferred heat flux. Because the eccentricity damping timescale is short, <20 Myr, it is unlikely that this eccentricity was primordial. More likely, Tethys' eccentricity increased during passage through a 3:2 resonance with Dione. In equilibrium, this resonance produces ∼2.5 mW/m2 suggesting that non‐equilibrium or periodic heating was important, similar to the case for Enceladus at present.