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Replenishment of Methane in Titan’s Atmosphere by Intrusion-driven Thermal Destabilization of Methane Clathrate Hydrates

  • Authors: Ashley Gerard Davies, Mathieu Choukroun, Christophe Sotin, Tuan H. Vu, Elodie Gloesener

Ashley Gerard Davies et al 2026 The Planetary Science Journal 7 .

  • Provider: AAS Journals

Caption: Figure 6.

Release of methane as a function of time (upper limit). Panels (a) and (b) are Cases 2 and 3. Panels (c) and (d) are cases 4 and 5. Profiles are shown for different depths of clathrate layer (5 km for Cases 2 and 3, and 10 km for Cases 4 and 5) and for the MCH brine pocket ammonia content limits, from a maximum of 32wt% down to the lowest ammonia content value where MCH is still destabilized. The horizontal dashed line denotes the required atmospheric replenishment rate of methane (290 kg s−1).

(The data used to create this figure are available in the online article.)

(The data used to create this figure are available.)

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