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Evidence for Random Walk Transport of Small Asteroids from the Main Belt to the Inner Solar System

  • Authors: Stanley F. Dermott, Apostolos A. Christou, Dan Li

Stanley F. Dermott et al 2026 The Planetary Science Journal 7 .

  • Provider: AAS Journals

Caption: Figure A5.

(Top) Density maps of the Eunomia and Hungaria families in ﹩1/D﹩ space with pixel dimensions of 0.01 ﹩{\rm{au}}\times \,﹩ 0.025 ﹩{{\rm{km}}}^{-1}﹩. Straight lines represent family V shapes obtained in this work. (Bottom) Histograms of family asteroids as a function of ﹩\delta ﹩ with a 0.1﹩\delta ﹩ bin size. Dotted vertical lines correspond to the V-shaped line locations in the density maps (Table A2).

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