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Dynamical Evolution of V-shaped Collision Debris

  • Authors: Ryuki Hyodo, Naoya Torii

Ryuki Hyodo and Naoya Torii 2026 The Astrophysical Journal 1004 .

  • Provider: AAS Journals

Caption: Figure 2.

Post-collision orbital evolution of two particles in the ae diagram. Each panel shows the constraint curves for a collision at acol = 7 Rplanet: the apoapsis constraint (e = acol/a − 1; left branch) and the periapsis constraint (e = 1 − acol/a; right branch). The green- and blue-shaded regions indicate orbits with periapsis below the planetary surface and the Roche limit, respectively. Blue and red symbols trace the successive positions of particle 1 (initially at apoapsis) and particle 2 (initially at periapsis), respectively. The left column adopts e1 = e2 = 0.65, while the right column adopts e1 = 0.65 and e2 = 0.40. From top to bottom, the coefficient of restitution decreases: εn = 0.9, 0.5, and 0.1. For high εn, particle 1 crosses from the apoapsis curve to the periapsis curve, whereas for low εn, particles remain on their respective constraint curves and converge toward the circular orbit at (acol, 0).

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