Models of heat convection suggested that any liquid on Callisto, one of Jupiter's moons, must be frozen. But those models did not take into account the different properties a surface layer of ice might have.
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References
Ruiz, J. Nature 412, 409–411 (2001).
Cassen, P. M., Peale, S. J. & Reynolds, R. T. Satellites of Jupiter (Univ. Arizona Press, Tucson, 1982).
Zimmer, C., Khurana, K. K. & Kivelson, M. G. Icarus 147, 329–347 (2000).
Lewis, J. S. Science 280, 1573–1576 (1998).
Consolmagno, G. J. & Lewis, J. S. Icarus 34, 280–293 (1978).
Solomatov, V. S. Phys. Fluids 7, 266–274 (1995).
Durham, W. B., Kirby, S. H. & Stern, L. A. J. Geophys. Res. 102, 16293–16302 (1997).
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Bennett, K. Uncool Callisto. Nature 412, 395–396 (2001). https://doi.org/10.1038/35086688
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DOI: https://doi.org/10.1038/35086688