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Enceladus’s Tidal Heating: A Simple Approach

  • Authors: Yoram Lithwick

Yoram Lithwick 2025 The Planetary Science Journal 6 .

  • Provider: AAS Journals

Caption: Figure 1.

Orientation of the tidal bulge. Panel (a) displays the bulge of the ice shell under the action of the static tide, and the other panels display the bulge under the action of the total tide, depending on whether the shell is hard (panel (b)) or soft (panel (c)). For given values of γS and γice (angles of Saturn in its epicycle and of the shell, respectively), the resulting orientation of the bulge (γbul) depends on the shell’s hardness. When it is hard, the shell hardly changes its shape relative to γice. When it is soft, the bulge nearly points at Saturn, whatever the value of γice. The hardness parameter ﹩{ \mathcal R }﹩ is defined in Equation (27).

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