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Possible Magnetic Perturbations Associated with Starship Lunar Landings

  • Authors: William M. Farrell, Stefano Boccelli, Orenthal J. Tucker

William M. Farrell et al 2026 The Planetary Science Journal 7 .

  • Provider: AAS Journals

Caption: Figure 3.

The distribution of water desorption activation energy, F(U, t) for a surface consisting of ice (with a peak near 0.516 eV for water-ice desorption), with the last layer consisting of water–regolith desorption represented by the broader half-Gaussian between 0.5 and 1.5 eV. The dashed lines show the evolution of F(U, t) at three different times.

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