Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF

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 C2.

Equilibrium grain size for model shown in Figure C1. For layer depths in which H < Ht, no equilibrium grain size is predicted, which is interpreted to mean that grain growth continues without bound. We note that the grain size grows by a factor of 2 as H → Ht.

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article

Show More

Copyright and Terms & Conditions

Additional terms of reuse