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2015
DOI: 10.1016/j.icarus.2014.11.007
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Elastic thickness and heat flux estimates for the uranian satellite Ariel

Abstract: 10The surface of Ariel, an icy satellite orbiting Uranus, shows extensional tectonic features 11suggesting an episode of endogenic heating in the satellite's past. Using topography derived from 12 stereo-photoclinometry, we identified flexural uplift at a rift zone suggesting elastic thickness 13 values in the range 3.8-4.4 km. We estimate the temperature at the base of the lithosphere to be 14 in the range 99 to 146 K, depending on the strain rate assumed, with corresponding heat fluxes 15

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Cited by 27 publications
(54 citation statements)
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“…This value is similar to that inferred at Arden Corona, Miranda ( Pappalardo et al, 1997 ). It is less than the T e values of 5–7 km for Ithaca Chasma on Tethys ( Giese et al, 2007 ) and 3.8–4.4 km from a rift zone on Ariel ( Peterson et al, 2015 ) (although some of our fits are in that range). The Charon value and those of the others are all larger than the 0.9 km for a rift flank on Ganymede ( Nimmo et al, 2002 ).…”
Section: Resultsmentioning
confidence: 54%
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“…This value is similar to that inferred at Arden Corona, Miranda ( Pappalardo et al, 1997 ). It is less than the T e values of 5–7 km for Ithaca Chasma on Tethys ( Giese et al, 2007 ) and 3.8–4.4 km from a rift zone on Ariel ( Peterson et al, 2015 ) (although some of our fits are in that range). The Charon value and those of the others are all larger than the 0.9 km for a rift flank on Ganymede ( Nimmo et al, 2002 ).…”
Section: Resultsmentioning
confidence: 54%
“…To investigate this issue further, we carried out flexural fits to a sub-set of rift-flank profiles ( Fig. 18 ) using the same approach that Peterson et al (2015) used for Ariel, and the same parameter values except for the gravity, 0.29 m s −2 . The mean elastic thickness T e we infer for Charon is 2.5 km.…”
Section: Resultsmentioning
confidence: 99%
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“…The leading explanation for this event is that the satellite was tidally heated when it was trapped in a "Laplace-like" resonance, prior to attaining its present-day orbital configuration (Showman & Malhotra1997). Similarly, the high ancient heat flux inferred at Tethys may have been due to passage through a 3:2 resonance with Dione (Chen & Nimmo 2008), and something similar may also have happened at Ariel (Peterson et al 2015). The Uranian satellites almost certainly experienced paleo-resonances, but there are no resonances at the present day.…”
Section: Tidal Heating and Orbital Evolutionmentioning
confidence: 92%