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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 10.

The red circle shows the extent of the one-hop exospheric water released from a topside water deposit located at 89°S, 90°W (as an example). Starship exospheric water from the topside deposit can access many cold polar locations including the floor of Shackleton, Shoemaker, and Haworth craters. The figure is adapted from https://www.lpi.usra.edu/lunar/lunar-south-pole-atlas/maps/SPole_85S_DLREallT_v20190829.pdf.

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