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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 6.

Sensitivity of mean vertical fluid velocity w to dike width under SP conditions for a range of dynamic viscosities. Panel (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. Panel (b): corresponding volumetric flow rates Q assuming the dike breadth is 1000 times its width. Complete solidification of conduit fluid occurs when flow rates are less than 25 m3 s−1.

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