The results of laboratory impact experiments and asteroid properties are presently interpreted in terms of a semiempirical theory that derives fragment properties observed on the basis of a suitable target material velocity field arising from the impact explosion and the target's original rotation. Numerical simulations based on a study of local target properties as a function of initial positions in the target have shown fragment rotation to arise from the superposition of velocity curve field and fragment shape asphericity effects; observed properties of main asteroid families are well reproduced by the model.
|Autori interni:||PAOLICCHI, PAOLO|
|Autori:||PAOLICCHI P; CELLINO A; FARINELLA P; ZAPPALA V|
|Titolo:||A SEMIEMPIRICAL MODEL OF CATASTROPHIC BREAKUP PROCESSES|
|Anno del prodotto:||1989|
|Digital Object Identifier (DOI):||10.1016/0019-1035(89)90016-X|
|Appare nelle tipologie:||1.1 Articolo in rivista|