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Analytical Solutions for Planet-scattering Small Bodies

  • Authors: Yukun Huang, 宇坤 黄, Brett Gladman, Eiichiro Kokubo, 英一郎 小久保

Yukun Huang et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 13.

Histograms of ϕ for U = 1 (﹩{ \mathcal T }=2﹩) particles at t = 0.1tS and 1.0tS, respectively. The planet has mass mp = 1 × 10−4M and ap = 1 au, and the corresponding scattering timescale tS = 3.5 Myr is computed using Equation (58). The initial conditions for the particles are ﹩{{ \mathcal A }}_{0}=1.1﹩, e0 = 0.854, and i0 = 2﹩\mathop{.}\limits^{\unicode{x000b0}}﹩9, corresponding to ϕ0 = 88﹩\mathop{.}\limits^{\unicode{x000b0}}﹩2. The median ϕ during scattering is marked with a red vertical line.

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