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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 1.

V-shaped distribution of collision debris in the ae diagram. Left: post-impact debris from L. F. A. Teodoro et al. (2023). Middle: Initial V-shaped configuration adopted in this study, defined by the apoapsis (acol = a(1 + e)) and periapsis (acol = a(1 − e)) constraint curves. The blue and red curves mark the conditions q = aRoche and aeq = aRoche, respectively, where q = a(1 − e) is the periapsis distance and aeq is the equivalent circular radius. Green curves indicate q = RSat. Right: corresponding orbital trajectories in Saturn’s equatorial plane, illustrating that particles on the two arms possess distinct angular momenta and orbital geometries, despite intersecting at the common radius acol.

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