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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 4.

Schematic illustrating basal melt rising from collection area at depth toward the surface of SP. Panel (A): map view showing detail in one representative, stylized polygonal cell, domed in the center (contours are dashed). Once on the surface, melt flows down gradient toward the cell margins, in a manner akin to flank eruptions on shield volcanoes. Whereas the channel guiding the flow is too narrow to be imaged in New Horizon imagery, the collection of such N2 lavas at the cell edges serve to darken the cell perimeters. Panel (B): schematic, cross-sectional view of a single convective cell. A conduit collects melt from the surrounding, and guides it toward the surface, here envisioned as flow in a dike. Once emerging on the surface, the melt cools as it flows down channel and ultimately pools and solidifies in the creased junctions between cells.

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