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Hypervelocity impacts on Skylab IV/Apollo windowsA description is presented of some new observations of crater morphology on the Skylab IV/Apollo windows. Aluminum is detected as the only foreign component in six of the seven lined glassy pit craters so far examined by EDS analysis. The most probable source is from aluminum oxide spherules, exhaust effluent of solid fuel rocket motors. The seventh crater contains titanium which may have been derived from an impact of a chip of thermal paint. The size distribution of the lined glassy pit craters appears to be compatible with an origin by hypervelocity impacts of aluminum spherules. If the aluminum oxide spherules are in earth orbit, impact velocities largely in the range of 7 to 10 km/s should be expected. Thus, the impact velocities are well below those expected for most impacts by micrometeorites and these lower velocities may be significant in the development of the lined glassy pit craters. The results indicate that there is a significant population of man-induced micro-debris in earth orbit.
Document ID
19820038849
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Clanton, U. S.
(Lunar and Planetary Inst. Houston, TX, United States)
Zook, H. A.
(NASA Johnson Space Center Geology Branch, Houston, TX, United States)
Schultz, R. A.
(Lunar and Planetary Institute Houston, TX, United States)
Date Acquired
August 10, 2013
Publication Date
January 1, 1980
Subject Category
Spacecraft Design, Testing And Performance
Meeting Information
Meeting: Lunar and Planetary Science Conference
Location: Houston, TX
Start Date: March 17, 1980
End Date: March 21, 1980
Accession Number
82A22384
Funding Number(s)
CONTRACT_GRANT: NAS9-3310
Distribution Limits
Public
Copyright
Other

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