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Where Do Hot Jupiters Come from? Revisiting Tidal Disruption and Ejection in High-eccentricity Migration

  • Authors: Qianli Fan, 千里 范, Shang-Fei Liu, 尚飞 刘

Qianli Fan et al 2026 The Astrophysical Journal Letters 1003 .

  • Provider: AAS Journals

Caption: Figure 1.

Bound mass versus initial rp/rt for planets with 10 M⊕ (blue) and 20 M⊕ (orange) cores. Progressively darker shades within each color group represent the initial state and the remnant mass after the first, second, and third encounters, respectively. All masses are in Earth masses.

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