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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 3.

Evolution of a particle with U = 1.0 (﹩{{ \mathcal A }}_{0}﹩=1.2, e0=0.61, i0=47﹩\mathop{.}\limits^{\unicode{x000b0}}﹩8, closely coupled case) in orbital elements (﹩{ \mathcal A }﹩, e, i, left panels) and relative-velocity vectors (θ, ϕ, U, right panels) scattered by a mp = 1 × 10−4m planet on a ap = 1 au circular orbit. The gray regions mark ﹩{\unicode{120006}}﹩ > 1 (red curves), corresponding to where the Öpik framework fails. The blue region in the top-right panel represents the loss cone θloss (Equation (13)).

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