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High-Nickel Iron-Sulfides in Anhydrous, Gems-Rich CP IDPsChondritic porous interplanetary dust particles (CP IDPs) that were not severly heated during atmospheric deceleration are the best preserved samples of the solids that condensed from the Solar protoplanetary disk, as well as pre-Solar grains thatr survived incorporation into the disk, currently available for laboratory analysis [1]. These CP IDPs never experienced the aqueous and/or thermal processing, gravitational compaction, and shock effects that overprinted the record of Solar nebula processes in meteorites.
Document ID
20160007866
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
Authors
FLynn, G. J.
(State Univ. of New York Plattsburgh, NY, United States)
Keller, L. P.
(NASA Johnson Space Center Houston, TX, United States)
Wirick, S.
(Focused Beam Enterprises Westhampton, NY, United States)
Hu, W.
(Brookhaven National Lab. Upton, NY, United States)
Li, L.
(Brookhaven National Lab. Upton, NY, United States)
Yan, H.
(Brookhaven National Lab. Upton, NY, United States)
Huang, X.
(Brookhaven National Lab. Upton, NY, United States)
Nazaretski, E.
(Brookhaven National Lab. Upton, NY, United States)
Lauer, K.
(Brookhaven National Lab. Upton, NY, United States)
Chu, Y. S.
(Brookhaven National Lab. Upton, NY, United States)
Date Acquired
June 23, 2016
Publication Date
August 7, 2016
Subject Category
Lunar And Planetary Science And Exploration
Report/Patent Number
JSC-CN-36525
Meeting Information
Meeting: Meteoritical Society Annual Meeting (METSOC)
Location: Berlin
Country: Germany
Start Date: August 7, 2016
End Date: August 12, 2016
Sponsors: Meteoritical Society
Distribution Limits
Public
Copyright
Public Use Permitted.
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