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Didymos’s Reshaping Scale Revealed by Detection of Its Spin Slow-down

  • Authors: Masatoshi Hirabayashi, Harrison F. Agrusa, Petr Pravec

Masatoshi Hirabayashi et al 2026 The Planetary Science Journal 7 .

  • Provider: AAS Journals

Caption: Figure A1.

Thickness change at the equator after spin-driven reshaping (Modification II) for all the shape cases. Each panel shows a different shape. Panel (a) shows the case when a0 = 413 m, b0 = 395.5 m, and c0 = 298 m. Panel (b) illustrates the case when a0 = 393 m, b0 = 375.5 m, and c0 = 318 m. Panel (c) shows the case when a0 = 433 m, b0 = 415.5 m, and c0 = 318 m. Finally, Panel (d) illustrates the case when a0 = 413 m, b0 = 395.5 m, and c0 = 278 m. Panel (a) is identical to Figure 4.

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