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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 12.

Similar to Figure 9 but for the Eunomia family. Gaussian distributions are fit to data in the range 1.53 au < a < 1.70 au. The semimajor axis distribution in the range ﹩0.23\,{\mathrm{km}}^{-1}\,\lesssim 1/D\lesssim 0.36\,{\mathrm{km}}^{-1}﹩ is clearly non-Gaussian, and thus no fit was attempted.

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