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Adv Space Res. 1995 Mar;15(3):91-7.

Characteristics and formation of amino acids and hydroxy acids of the Murchison meteorite.

Author information

1
Department of Chemistry and Biochemistry, Arizona State University, Tempe 85287-1604, USA.
2
AZ St U, Tempe

Abstract

Eight characteristics of the unique suite of amino acids and hydroxy acids found in the Murchison meteorite can be recognized on the basis of detailed molecular and isotopic analyses. The marked structural correspondence between the alpha-amino acids and alpha-hydroxy acids and the high deuterium/hydrogen ratio argue persuasively for their formation by aqueous phase Strecker reactions in the meteorite parent body from presolar, i.e., interstellar, aldehydes, ketones, ammonia, and hydrogen cyanide. The characteristics of the meteoritic suite of amino acids and hydroxy acids are briefly enumerated and discussed with regard to their consonance with this interstellar-parent body formation hypothesis. The hypothesis has interesting implications for the organic composition of both the primitive parent body and the presolar nebula.

PMID:
11539265
[Indexed for MEDLINE]

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