Collisional evolution of rotating, non-identical particles

DOI10.1007/BF00119681zbMath0679.70009OpenAlexW1990644397MaRDI QIDQ1823041

Heikki Salo

Publication date: 1987

Published in: Earth, Moon, and Planets (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/bf00119681

zbMATH Keywords

non-gravitating mass pointsSaturn's ringsself-gravitating collisional particle disksself-gravitational forces

Mathematics Subject Classification ID

Celestial mechanics (70F15) Collision of rigid or pseudo-rigid bodies (70F35)

Related Items

Systems of colliding bodies in a gravitational field: Evolution and role of the internal rotations ⋮ Generalized theory of impacts in particulate systems

Cites Work

• Collisional theory of non-identical particles in a gravitational field
• An improved and generalized theory for the collisional evolution of Keplerian systems
• Numerical simulations of colliding particles in a gravitational field
• Collisions in self-gravitating clouds of planetesimals
• Quasi-equilibrium in collisional systems
• Starn's rings and bimodality of Keplerian systems
• Self-gravitation in Saturn's rings