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Amino Acid Contents of Meteorite Mineral SeparatesIndigenous amino acids have been found indigenous all 8 carbonaceous chondrite groups. However, the abundances, structural, enantiomeric and isotopic compositions of amino acids differ significantly among meteorites of different groups and petrologic types. This suggests that parent-body conditions (thermal or aqueous alteration), mineralogy, and the preservation of amino acids are linked. Previously, elucidating specific relationships between amino acids and mineralogy was not possible because the samples analyzed for amino acids were much larger than the scale at which petrologic heterogeneity is observed (sub mm-scale differences corresponding to sub-mg samples). Recent advances in amino acid measurements and application of techniques such as high resolution X-ray diffraction (HR-XRD) and scanning electron microscopy (SEM) with energy dispersive spectroscopy (EDS) for mineralogical characterizations allow us to perform coordinated analyses on the scale at which mineral heterogeneity is observed.
Document ID
20170005638
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
Authors
Berger, E. L.
(Jacobs Technologies Engineering Science Contract Group Houston, TX, United States)
Burton, A. S
(NASA Johnson Space Center Houston, TX, United States)
Locke, D.
(Jacobs Technologies Engineering Science Contract Group Houston, TX, United States)
Date Acquired
June 15, 2017
Publication Date
July 16, 2017
Subject Category
Space Sciences (General)
Report/Patent Number
JSC-CN-39279
Meeting Information
Meeting: International Conference on the Origin of Life
Location: San Diego, CA
Country: United States
Start Date: July 16, 2017
End Date: July 21, 2017
Sponsors: Lunar and Planetary Inst.
Distribution Limits
Public
Copyright
Public Use Permitted.
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