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Historical Trends in U.S. Antarctic Meteorite Allocations, With a Close Look at Cr ChondritesANSMET samples have been housed at and allocated from NASA-JSC since 1978. This nearly 40 year history of allocations from the collection has been contemporaneous with many major milestones such as the discovery that we have meteorites from Moon and Mars, missions to S-type asteroids (NEAR, Hayabusa, Dawn), and C-type asteroids (Dawn, Hayabusa 2, and OSIRIS-REx). We look for the possible influence of these major milestones on historical trends in the meteorite allocations, identify other factors that might contribute to allocation trends, and focus on the allocation history of a few select meteorites.
Document ID
20170005737
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
Authors
Righter, K.
(NASA Johnson Space Center Houston, TX, United States)
Satterwhite, C. E.
(Jacobs Technology, Inc. Houston, TX, United States)
Funk, R. C.
(Jacobs Technology, Inc. Houston, TX, United States)
Harrington, R.
(Jacobs Technology, Inc. Houston, TX, United States)
Date Acquired
June 23, 2017
Publication Date
July 23, 2017
Subject Category
Lunar And Planetary Science And Exploration
Report/Patent Number
JSC-CN-39726
Meeting Information
Meeting: The Meteorological Society Annual Meeting 2017
Location: Santa Fe, NM
Country: United States
Start Date: July 23, 2017
End Date: July 28, 2017
Sponsors: American Meteorological Society
Distribution Limits
Public
Copyright
Public Use Permitted.
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