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Evidence for Possible N2 Basal Flow beneath Pluto’s Northern Sputnik Planitia

  • Authors: S. A. Stern, Orkan Umurhan, Gary D. Clow, Robert S. Anderson, Alan Howard, Kelsi N. Singer

S. A. Stern et al 2026 The Planetary Science Journal 7 .

  • Provider: AAS Journals

Caption: Figure D3.

Sensitivity of mean vertical velocity w to mean dike width 2a under SP conditions for a range of dynamic viscosities (a). Turbulent and laminar flow are indicated by solid and dashed–dotted lines, respectively. Dike widths less than the critical value required for sustained flow are indicated by the “complete solidification” field. Times for N2 magma to ascend through 1 km of SP ice are shown in (b). Corresponding volumetric flow rates Q are shown in (c) assuming the dike breadth is 1000 times its width.

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