The role of families in determining collision probability in the asteroid main belt

Icarus

Volumn 153, Issue 1, 2001, Pages 52-60

  Dell'Oro, A ^a   Paolicchi, P ^a   Cellino, A ^b   Zappala V ^b   Tanga, P ^b   Michel, P ^c  

^a UNIVERSITY OF PISA   (Italy)

^b OSSERVATORIO ASTRONOMICO DI TORINO   (Italy)

^c UNIVERSITÉ CÔTE D'AZUR   (France)

Author keywords

Asteroids; Collisional physics

Indexed keywords

EID: 0035189933     PISSN: 00191035     EISSN: None     Source Type: Journal    
DOI: 10.1006/icar.2001.6621     Document Type: Article

References (24)

1. Asteroid collision probabilities
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3. The size distribution of main-belt asteroids from IRAS data
4. The velocity-size relationship for members of asteroid families and implications for the physics of catastrophic collisions
5. Structure and inventory of the asteroid Main Belt population
6. Collisional history of asteroids: Evidence from Vesta and from the Hirayama families
7. Asteroid collisional history: Effects on sizes and spin
8. Statistical properties of encounters among asteroids: A new, general purpose, formalism
9. The puzzling case of the Nysa-Polana family finally solved?
10. Asteroid collisional evolution: An integrated model for the collisional evolution of asteroid rotation rates
11. Dynamical life-times of objects injected into asteroid belt resonances
12. Orbital interactions: A new geometrical formalism
13. The orbital and absolute magnitude distributions of Main Belt asteroids
14. Collisional evolution of asteroid families
15. Interlopers within asteroid families
16. Origin of multikilometer Earth- and Mars-crossing asteroids: A quantitative simulation
17. Asteroid families close to mean motion resonances: Dynamical effects and physical implications
18. Collision probabilities with the planets and distribution of interplanetary matter
19. On the size distribution of asteroid families: The role of geometry
20. Collisions in the asteroid belt
21. Asteroid families: Search of a 12,487 asteroid sample using two different clustering techniques
22. Main Belt asteroids: Present and future inventory
23. Reconstructing the original ejection velocity fields of asteroid families
24. Asteroid showers on Earth after family break-up events