V-shaped collision debris from proto-satellites evolves via inter-arm collisions to reaccrete at the original impact radius rather than forming rings.
Icarus168(2), 433–456 (2004)
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
citation-role summary
background 1
citation-polarity summary
fields
astro-ph.EP 2years
2026 2verdicts
UNVERDICTED 2roles
background 1polarities
background 1representative citing papers
A review of SPH modeling for global-scale impacts, emphasizing material properties across size regimes and links to Solar System observations.
citing papers explorer
-
Dynamical Evolution of V-Shaped Collision Debris
V-shaped collision debris from proto-satellites evolves via inter-arm collisions to reaccrete at the original impact radius rather than forming rings.
-
Recent advances in modelling of global-scale collisions using smoothed particle hydrodynamics
A review of SPH modeling for global-scale impacts, emphasizing material properties across size regimes and links to Solar System observations.