Burst pressure failure of titanium tanks damaged by secondary plumes from hypervelocity impacts on aluminum shields
Author(s) -
Henry K. Nahra,
L. J. Ghosn,
E.L. Christiansen,
Bárbara Davis,
Christopher P. Keddy,
Kennedyn Edilberto Escobedo Rodríguez,
Jason Miller,
William Bohl
Publication year - 2012
Publication title -
aip conference proceedings
Language(s) - English
Resource type - Conference proceedings
SCImago Journal Rank - 0.177
H-Index - 75
eISSN - 1551-7616
pISSN - 0094-243X
DOI - 10.1063/1.3686231
Subject(s) - hypervelocity , impact crater , projectile , materials science , micrometeoroid , spall , fuel tank , shields , shield , aluminium , composite material , space debris , geotechnical engineering , spacecraft , geology , aerospace engineering , metallurgy , engineering , electromagnetic shielding , astrobiology , physics , thermodynamics , petrology
Metallic pressure tanks used in space missions are inherently vulnerable to hypervelocity impacts from micrometeoroids and orbital debris; thereby knowledge of impact damage and its effect on the tank integrity is crucial to a spacecraft risk assessment. This paper describes tests that have been performed to assess the effects of hypervelocity impact (HVI) damage on Titanium alloy (Ti-6Al-4V) pressure vessels burst pressure and characteristics. The tests consisted of a pair of HVI impact tests on water-filled Ti-6Al-4V tanks (water being used as a surrogate to the actual propellant) and subsequent burst tests as well as a burst test on an undamaged control tank. The tanks were placed behind Aluminum (Al) shields and then each was impacted with a 7 km/s projectile. The resulting impact debris plumes partially penetrated the Ti-6Al-4V tank surfaces resulting in a distribution of craters. During the burst tests, the tank that failed at a lower burst pressure did appear to have the failure initiating at a crater site with observed spall cracks. A fracture mechanics analysis showed that the tanks failure at the impact location may have been due to a spall crack that formed upon impact of a fragmentation on the Titanium surface. This result was corroborated with a finite element analysis from calculated Von-Mises and hoop stresses.
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