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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 2.

Thickness change at the equator after ejecta accumulation on Didymos (Modification I), i.e., Δte = (χ − 1)(a0 + b0)/2. The plot shows four different pre-impact shapes. The blue line shows the case when a0 = 413 m, b0 = 395.5 m, and c0 = 298 m. The yellow line illustrates the case when a0 = 393 m, b0 = 375.5 m, and c0 = 318 m. The green line shows the case when a0 = 433 m, b0 = 415.5 m, and c0 = 318 m. Finally, the red line shows the case when a0 = 413 m, b0 = 395.5 m, and c0 = 278 m.

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