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Study of Europa’s crust via a Stefan model with convection

Author

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  • Cerimele, Maria M.
  • Mansutti, Daniela
  • Pistella, Francesca

Abstract

We present results of a numerical simulation of the thermal convection in the subsurface mushy ice layer of Europa, one of the Jupiter’s moons. Beside fluid dynamics and heat transfer within such a layer, heat conduction in the solid crustal surface and heat exchange between the two phases – mushy ice and solid crust – are included in our model in order to follow also the evolution of the phase front.

Suggested Citation

  • Cerimele, Maria M. & Mansutti, Daniela & Pistella, Francesca, 2008. "Study of Europa’s crust via a Stefan model with convection," Mathematics and Computers in Simulation (MATCOM), Elsevier, vol. 79(3), pages 258-268.
    • Handle: RePEc:eee:matcom:v:79:y:2008:i:3:p:258-268
    DOI: 10.1016/j.matcom.2007.11.011
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    References listed on IDEAS

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    1. Michael H. Carr & Michael J. S. Belton & Clark R. Chapman & Merton E. Davies & Paul Geissler & Richard Greenberg & Alfred S. McEwen & Bruce R. Tufts & Ronald Greeley & Robert Sullivan & James W. Head , 1998. "Evidence for a subsurface ocean on Europa," Nature, Nature, vol. 391(6665), pages 363-365, January.
    2. K. K. Khurana & M. G. Kivelson & D. J. Stevenson & G. Schubert & C. T. Russell & R. J. Walker & C. Polanskey, 1998. "Induced magnetic fields as evidence for subsurface oceans in Europa and Callisto," Nature, Nature, vol. 395(6704), pages 777-780, October.
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