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Genesis Mission Bulk Metallic Glass Solar Wind Collector: Characterization of Return Samples Available for Re-AllocationThe Genesis mission collected solar wind atoms for 28 months with a variety of collectors mounted on a spacecraft. A total of fifteen pure materials were selected as collectors based on engineering and science requirements. One of the materials was the bulk metallic glass (BMG). It was intended for collecting noble gases and solar energetic particles (SEP). This material is an amorphous metal which was custom made by C.C. Hays at the California Institute of Technology. The final glass composition is Zr58.5Nb2.8Cu15.6Ni12.8Al10.3 (in atom percent). The BMG was located on top of the wafer array mechanism and was exposed for the entire time the science canister was open (~28 months). Fortunately, the BMG did not suffer any serious damage and was intact after the Genesis canister’s “hard-landing” into the Utah desert (Fig. 1).
Document ID
20200001836
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
Authors
Gonzalez, C. P.
(Jacobs Engineering Group Houston, TX, United States)
Allums, K. K.
(Jacobs Engineering Group Houston, TX, United States)
Allton, J. H.
(NASA Johnson Space Center Houston, TX, United States)
Harrington, R.
(Jacobs Engineering Group Houston, TX, United States)
Le, L.
(Jacobs Engineering Group Houston, TX, United States)
Thomas-Keprta, K.
(Jacobs Engineering Group Houston, TX, United States)
Date Acquired
March 19, 2020
Publication Date
March 16, 2020
Subject Category
Solar Physics
Report/Patent Number
JSC-E-DAA-TN77188
Report Number: JSC-E-DAA-TN77188
Meeting Information
Meeting: Lunar and Planetary Science Conference
Location: The Woodlands, TX
Country: United States
Start Date: March 16, 2020
End Date: March 20, 2020
Sponsors: NASA Headquarters, Lunar and Planetary Institute (LPI), Universities Space Research Association (USRA)
Funding Number(s)
CONTRACT_GRANT: NNJ13HA01C
Distribution Limits
Public
Copyright
Public Use Permitted.
Technical Review
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