The recent observational discovery of a nearly geosynchronous population of artificial debris in eccentric orbit, and with very high area-to-mass ratios (up to nearly 25 sqm/kg), stimulated the revisit of direct solar radiation pressure models, in order to assess their long-term performances in such extreme conditions. The dynamical behavior of objects with average area-to-mass ratios between 1 and 50 sqm/kg was investigated in the framework of a research program of detailed numerical simulations.
Long-term evolution of geosynchronous orbital debris with high area-to-mass ratios: effect of the sun-earth varying distance
Anselmo L;Pardini C
2007
Abstract
The recent observational discovery of a nearly geosynchronous population of artificial debris in eccentric orbit, and with very high area-to-mass ratios (up to nearly 25 sqm/kg), stimulated the revisit of direct solar radiation pressure models, in order to assess their long-term performances in such extreme conditions. The dynamical behavior of objects with average area-to-mass ratios between 1 and 50 sqm/kg was investigated in the framework of a research program of detailed numerical simulations.File in questo prodotto:
| File | Dimensione | Formato | |
|---|---|---|---|
|
prod_120584-doc_130380.pdf
solo utenti autorizzati
Descrizione: Long-term evolution of geosynchronous orbital debris with high area-to-mass ratios: effect of the sun-earth varying distance
Tipologia:
Versione Editoriale (PDF)
Dimensione
1.22 MB
Formato
Adobe PDF
|
1.22 MB | Adobe PDF | Visualizza/Apri Richiedi una copia |
I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.


