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Young Surface of Pluto’s Sputnik Planitia Caused by Viscous Relaxation

  • Authors: Qiang Wei, Yongyun Hu, Yonggang Liu, Douglas N. C. Lin, Jun Yang, and Adam P. Showman

2018 The Astrophysical Journal Letters 856 L14.

  • Provider: AAS Journals

Caption: Figure 2.

Vertical cross-sections of a crater at different relaxation stages. The crater is initially 2 km in depth, 40 km in diameter, and the surface temperature is 38 K. Arrows represent N2 ice velocities. The length scale of the maximum N2 ice velocity is marked in the upper-right corner. (a) At the initial time; (b) within an Earth day; (c) after one month; and (d) after one year. In plots (c) and (d), the insets zoom in with greater vertical exaggeration.

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