The increasing amount of debris in Earth orbit poses a danger to users of the orbital environment. During the design phase of a spacecraft, an important requirement may be specified for the survivability of the spacecraft against Meteoroid / Orbital Debris (M/OD) impacts throughout the mission; moreover, the spacecraft structure is designed to guarantee its integrity and reliability during the launch and, if it is reusable, during descent, re-entry and landing. In addition, the structure has to provide required rigidity for exact positioning of experiments and antennas, and it has to protect the payload against the space environment. In this frame, in order to decrease the probability of spacecraft failure caused by impacts, for M/OD with dimensions less than 1cm, shields are needed for every spacecraft. It is therefore necessary to determine the impact-related failure mechanisms and associated ballistic limit equations (BLEs) for typical spacecraft components and subsystems. In order to obtain the ballistic limit equations, numerical simulations and laboratory experiments are required. A high energy ballistic characterization of layered structures has been carried out by means of a new advanced electromagnetic accelerator, called railgun, that has been assembled and tuned. A railgun is an electrically powered linear electromagnetic projectile launcher. Such device consists of a couple of parallel conducting rails, that allow sliding metallic armature to be accelerated along, by the electromagnetic effect (Lorentz force) of a current flowing down one rail, into the armature and then back along the other rail, thanks to a high power pulse given by a capacitors bank. A tunable power supplier is used to set the capacitors charging voltage at the desired level: in this way the Railgun energy can be tuned as a function of the desired bullet velocity. In such a way this facility is able to analyse both low and high velocity impacts. A numerical simulation is also carried out, using the Ansys Autodyn code, in order to analyse the exposed structures and verify the correct behaviour of the facility. The experimental and numerical simulations results show that the railgun device can be used to perform impact testing of materials in the space debris energy range.

Hypervelocity debris impact damage of space composite structures / Delfini, A.; Vricella, A.; Pastore, R.; Micheli, D.; Albano, M.; Santoni, F.; Piergentili, F.; Marchetti, M.. - 12:(2017), pp. 8045-8051. (Intervento presentato al convegno 68th International Astronautical Congress: Unlocking Imagination, Fostering Innovation and Strengthening Security, IAC 2017 tenutosi a Adelaide (AUS)).

Hypervelocity debris impact damage of space composite structures

Delfini A.;Vricella A.;Pastore R.;Micheli D.;Albano M.;Santoni F.;Piergentili F.;Marchetti M.
2017

Abstract

The increasing amount of debris in Earth orbit poses a danger to users of the orbital environment. During the design phase of a spacecraft, an important requirement may be specified for the survivability of the spacecraft against Meteoroid / Orbital Debris (M/OD) impacts throughout the mission; moreover, the spacecraft structure is designed to guarantee its integrity and reliability during the launch and, if it is reusable, during descent, re-entry and landing. In addition, the structure has to provide required rigidity for exact positioning of experiments and antennas, and it has to protect the payload against the space environment. In this frame, in order to decrease the probability of spacecraft failure caused by impacts, for M/OD with dimensions less than 1cm, shields are needed for every spacecraft. It is therefore necessary to determine the impact-related failure mechanisms and associated ballistic limit equations (BLEs) for typical spacecraft components and subsystems. In order to obtain the ballistic limit equations, numerical simulations and laboratory experiments are required. A high energy ballistic characterization of layered structures has been carried out by means of a new advanced electromagnetic accelerator, called railgun, that has been assembled and tuned. A railgun is an electrically powered linear electromagnetic projectile launcher. Such device consists of a couple of parallel conducting rails, that allow sliding metallic armature to be accelerated along, by the electromagnetic effect (Lorentz force) of a current flowing down one rail, into the armature and then back along the other rail, thanks to a high power pulse given by a capacitors bank. A tunable power supplier is used to set the capacitors charging voltage at the desired level: in this way the Railgun energy can be tuned as a function of the desired bullet velocity. In such a way this facility is able to analyse both low and high velocity impacts. A numerical simulation is also carried out, using the Ansys Autodyn code, in order to analyse the exposed structures and verify the correct behaviour of the facility. The experimental and numerical simulations results show that the railgun device can be used to perform impact testing of materials in the space debris energy range.
2017
68th International Astronautical Congress: Unlocking Imagination, Fostering Innovation and Strengthening Security, IAC 2017
meteoroid/orbital debris (M/OD) impacts, railgun; hypervelocity impact
04 Pubblicazione in atti di convegno::04b Atto di convegno in volume
Hypervelocity debris impact damage of space composite structures / Delfini, A.; Vricella, A.; Pastore, R.; Micheli, D.; Albano, M.; Santoni, F.; Piergentili, F.; Marchetti, M.. - 12:(2017), pp. 8045-8051. (Intervento presentato al convegno 68th International Astronautical Congress: Unlocking Imagination, Fostering Innovation and Strengthening Security, IAC 2017 tenutosi a Adelaide (AUS)).
File allegati a questo prodotto
File Dimensione Formato  
Delfini_Hypervelocity_2017.pdf

solo gestori archivio

Note: https://iafastro.directory/iac/archive/browse/IAC-17/C2/6/38935/
Tipologia: Versione editoriale (versione pubblicata con il layout dell'editore)
Licenza: Tutti i diritti riservati (All rights reserved)
Dimensione 643.88 kB
Formato Adobe PDF
643.88 kB Adobe PDF   Contatta l'autore

I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.

Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11573/1346595
Citazioni
  • ???jsp.display-item.citation.pmc??? ND
  • Scopus 1
  • ???jsp.display-item.citation.isi??? ND
social impact