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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 7.

Scattering timescale tS (in units of ﹩{P}_{p}/{M}_{p}^{2}﹩) as a function of ﹩{ \mathcal T }﹩ in different regimes. The red curves are computed using the full analytical expression (Equation (58)) in the closely coupled regime, with Mp = 1 × 10−2 (dotted), 1 × 10−5 (solid), and 1 × 10−8 (dashed), respectively. As ﹩{ \mathcal T }\to -\sqrt{8}﹩, tS shoots down to 0. The blue curve represents the best fit of the relaxation timescale in the diffusion regime, given by S. Hadden & S. Tremaine (2024), with a different approach. The narrow gap between the two regimes is the loosely coupled regime, where neither model is valid. The minimum (﹩{t}_{{S}_{0}}﹩), circular (tS,circ), and retrograde (tS,retro) scattering timescales defined in text (Equations (59) and (61)) are marked with black circles.

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