EnglishThe 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.
Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/11568/13023| Autori: | |
| 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 |
File in questo prodotto:
Non ci sono file associati a questo prodotto.
I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
Copyright © 2018