Tuning of NASA Standard Breakup Model for Fragmentation Events Modelling
The continuous growth of space debris motivates the development and the improvement of tools that support the monitoring of a more and more congested space environment. Satellite breakup models play a key role to predict and analyze orbital debris evolution, and the NASA Standard Breakup Model repre...
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doaj-47caad6d9d6c4bb0a7208789c5a178322021-07-23T13:25:43ZengMDPI AGAerospace2226-43102021-07-01818518510.3390/aerospace8070185Tuning of NASA Standard Breakup Model for Fragmentation Events ModellingNicola Cimmino0Giorgio Isoletta1Roberto Opromolla2Giancarmine Fasano3Aniello Basile4Antonio Romano5Moreno Peroni6Alessandro Panico7Andrea Cecchini8Department of Industrial Engineering, University of Naples “Federico II”, P.le Tecchio 80, 80125 Naples, ItalyDepartment of Industrial Engineering, University of Naples “Federico II”, P.le Tecchio 80, 80125 Naples, ItalyDepartment of Industrial Engineering, University of Naples “Federico II”, P.le Tecchio 80, 80125 Naples, ItalyDepartment of Industrial Engineering, University of Naples “Federico II”, P.le Tecchio 80, 80125 Naples, ItalyVitrociset S.p.A., 00156 Rome, ItalyVitrociset S.p.A., 00156 Rome, ItalyFlight Test Wing of the Italian Air Force, 00040 Pomezia, ItalyFlight Test Wing of the Italian Air Force, 00040 Pomezia, ItalyFlight Test Wing of the Italian Air Force, 00040 Pomezia, ItalyThe continuous growth of space debris motivates the development and the improvement of tools that support the monitoring of a more and more congested space environment. Satellite breakup models play a key role to predict and analyze orbital debris evolution, and the NASA Standard Breakup Model represents a widely used reference, with current activities relevant to its evolution and improvements especially towards fragmentation of small mass spacecraft. From an operational perspective, an important point for fragmentation modelling concerns the tuning of the breakup model to achieve consistency with orbital data of observed fragments. In this framework, this paper proposes an iterative approach to estimate the model inputs, and in particular, the parents’ masses involved in a collision event. The iterative logic exploits the knowledge of Two Line Elements (TLE) of the fragments at some time after the event to adjust the input parameters of the breakup model with the objective of obtaining the same number of real fragments within a certain tolerance. Atmospheric re-entry is accounted for. As a result, the breakup model outputs a set of fragments whose statistical distribution, in terms of number and size, is consistent with the catalogued ones. The iterative approach is demonstrated for two different scenarios (i.e., catastrophic collision and non-catastrophic collision) using numerical simulations. Then, it is also applied to a real collision event.https://www.mdpi.com/2226-4310/8/7/185space debrisspace surveillance and trackingfragmentation events modellingNASA standard breakup modelcollision modelling |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Nicola Cimmino Giorgio Isoletta Roberto Opromolla Giancarmine Fasano Aniello Basile Antonio Romano Moreno Peroni Alessandro Panico Andrea Cecchini |
spellingShingle |
Nicola Cimmino Giorgio Isoletta Roberto Opromolla Giancarmine Fasano Aniello Basile Antonio Romano Moreno Peroni Alessandro Panico Andrea Cecchini Tuning of NASA Standard Breakup Model for Fragmentation Events Modelling Aerospace space debris space surveillance and tracking fragmentation events modelling NASA standard breakup model collision modelling |
author_facet |
Nicola Cimmino Giorgio Isoletta Roberto Opromolla Giancarmine Fasano Aniello Basile Antonio Romano Moreno Peroni Alessandro Panico Andrea Cecchini |
author_sort |
Nicola Cimmino |
title |
Tuning of NASA Standard Breakup Model for Fragmentation Events Modelling |
title_short |
Tuning of NASA Standard Breakup Model for Fragmentation Events Modelling |
title_full |
Tuning of NASA Standard Breakup Model for Fragmentation Events Modelling |
title_fullStr |
Tuning of NASA Standard Breakup Model for Fragmentation Events Modelling |
title_full_unstemmed |
Tuning of NASA Standard Breakup Model for Fragmentation Events Modelling |
title_sort |
tuning of nasa standard breakup model for fragmentation events modelling |
publisher |
MDPI AG |
series |
Aerospace |
issn |
2226-4310 |
publishDate |
2021-07-01 |
description |
The continuous growth of space debris motivates the development and the improvement of tools that support the monitoring of a more and more congested space environment. Satellite breakup models play a key role to predict and analyze orbital debris evolution, and the NASA Standard Breakup Model represents a widely used reference, with current activities relevant to its evolution and improvements especially towards fragmentation of small mass spacecraft. From an operational perspective, an important point for fragmentation modelling concerns the tuning of the breakup model to achieve consistency with orbital data of observed fragments. In this framework, this paper proposes an iterative approach to estimate the model inputs, and in particular, the parents’ masses involved in a collision event. The iterative logic exploits the knowledge of Two Line Elements (TLE) of the fragments at some time after the event to adjust the input parameters of the breakup model with the objective of obtaining the same number of real fragments within a certain tolerance. Atmospheric re-entry is accounted for. As a result, the breakup model outputs a set of fragments whose statistical distribution, in terms of number and size, is consistent with the catalogued ones. The iterative approach is demonstrated for two different scenarios (i.e., catastrophic collision and non-catastrophic collision) using numerical simulations. Then, it is also applied to a real collision event. |
topic |
space debris space surveillance and tracking fragmentation events modelling NASA standard breakup model collision modelling |
url |
https://www.mdpi.com/2226-4310/8/7/185 |
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