In order to understand the origin of the artificial debris population in the 1 mm - 10 cm size range, we carried out a massive effort to estimate the contribution of past fragmentations events. Our research involved the development of a dedicated software code, CLDSIM, able to simulate the 117 catalogued fragmentation events in earth orbit occurred from 1961 to 1993, and to propagate the resulting debris clouds to a reference epoch (January 1, 1994). More than 10 millions of orbital debris with a mass larger than 1 mg were generated and about 6.8 millions resulted still in orbit at the reference epoch. The resulting data were used to investigate the properties of the uncatalogued population.

The contribution of the past fragmentation events to the uncatalogued orbital debris population

Pardini C;Rossi A;Anselmo L;
1996

Abstract

In order to understand the origin of the artificial debris population in the 1 mm - 10 cm size range, we carried out a massive effort to estimate the contribution of past fragmentations events. Our research involved the development of a dedicated software code, CLDSIM, able to simulate the 117 catalogued fragmentation events in earth orbit occurred from 1961 to 1993, and to propagate the resulting debris clouds to a reference epoch (January 1, 1994). More than 10 millions of orbital debris with a mass larger than 1 mg were generated and about 6.8 millions resulted still in orbit at the reference epoch. The resulting data were used to investigate the properties of the uncatalogued population.
1996
978-0-87703-407-0
Space debris
astrodynamics
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/20.500.14243/7682
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