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Stereoisomers of isovaline in the Murchison meteoriteIsovaline is present in the Murchison meteorite as a racemic mixture (about equal concentrations of the R and S enantiomers). Since isovaline does not have a hydrogen atom on its asymmetric alpha-carbon atom, the racemic mixture could not have formed by commonly accepted mechanisms of racemization. Thus, isovaline in the meteorite most probably was synthesized as a racemic mixture and is not the result of the racemization of either the R or S enantiomer. Other chiral amino acids in the meteorite are present as racemic mixtures, and were probably synthesized in a similar manner by abiotic, extraterrestrial processes.
Document ID
19760028105
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Pollock, G. E.
(NASA Ames Research Center Moffett Field, CA, United States)
Cronin, S. E.
(NASA Ames Research Center Moffett Field, CA, United States)
Kvenvolden, K. A.
(NASA Ames Research Center Planetary Biology Div., Moffett Field, Calif., United States)
Cheng, C.-N.
(NASA Ames Research Center Moffett Field, CA, United States)
Date Acquired
August 8, 2013
Publication Date
November 1, 1975
Publication Information
Publication: Geochimica et Cosmochimica Acta
Volume: 39
Subject Category
Lunar And Planetary Exploration
Accession Number
76A11071
Distribution Limits
Public
Copyright
Other

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