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Micrometeoroid Impacts on the Hubble Space Telescope Wide Field and Planetary Camera 2: Smaller Particle Impacts

Authors :
Ross, D. K
Anz-Meador, P
Liou, J.C
Opiela, J
Kearsley, A. T
Grime, G
Webb, R
Jeynes, C
Palitsin, V
Colaux, J
Griffin, T
Gerlach, L
Wozniakiewicz, P. J
Price, M. C
Burchell, M. J
Cole, M. J
Publication Year :
2014
Publisher :
United States: NASA Center for Aerospace Information (CASI), 2014.

Abstract

The radiator shield on the Wide Field and Planetary Camera 2 (WFPC2) was subject to optical inspection following return from the Hubble Space Telescope (HST) in 2009. The survey revealed over 600 impact features of > 300 micrometers diameter, from exposure in space for 16 years. Subsequently, an international collaborative programme of analysis was organized to determine the origin of hypervelocity particles responsible for the damage. Here we describe examples of the numerous smaller micrometeoroid (MM) impact features (< 700 micrometers diameter) which excavated zinc orthotitanate (ZOT) paint from the radiator surface, but did not incorporate material from underlying Al alloy; larger impacts are described by [3]. We discuss recognition and interpretation of impactor remains, and MM compositions found on WFPC2.

Details

Language :
English
Database :
NASA Technical Reports
Notes :
ESA 4000105713_12_NL_GE
Publication Type :
Report
Accession number :
edsnas.20140005747
Document Type :
Report