Isotopic analyses of amino acids from the Murchison meteorite
- Arizona State Univ., Tempe (United States)
- California Inst. of Tech., Pasadena, CA (United States)
Previous isotopic analyses of the total amino acids of the Murchison meteorite showed these compounds to be substantially enriched in {sup 2}H, {sup 13}C, and {sup 15}N relative to terrestrial organic matter. These analyses have been repeated ({sup 2}H, {sup 13}C) with inclusion of an ultrafiltration step to exclude the possibility that a fine particulate contaminant carried the isotopic excesses observed in the previous work. In addition, the meteorite amino acids were chromatographically separated to rule out the possibility that the isotopic enrichment of the meteorite extract could reside in basic compounds other than amino acids. The results indicate that the Murchison amino acids are truly isotopically unusual, that the isotopic excesses reside in at least several different amino acids, and that the isotopic contents of some of these amino acids reach values of about +40{per thousand} ({delta}{sup 13}C) and +2,500{per thousand} ({delta}D). If it is assumed that the high deuterium content of the meteroite {alpha}-amino acids is a result of the synthesis of their molecular precursors by low temperature ion-molecule reactions in an interstellar cloud, their formation by aqueous phase Strecker reactions in the parent body is consistent with their general characteristics and with known parent body processes.
- OSTI ID:
- 6005065
- Journal Information:
- Geochimica et Cosmochimica Acta; (United States), Vol. 55:3; ISSN 0016-7037
- Country of Publication:
- United States
- Language:
- English
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AMINO ACIDS
ISOTOPE RATIO
METEORITES
CHEMICAL COMPOSITION
CARBON 13
COMPARATIVE EVALUATIONS
HYDROGEN IONS
NITROGEN 15
ORIGIN
PETROGENESIS
CARBON ISOTOPES
CARBOXYLIC ACIDS
CHARGED PARTICLES
EVALUATION
EVEN-ODD NUCLEI
IONS
ISOTOPES
LIGHT NUCLEI
NITROGEN ISOTOPES
NUCLEI
ODD-EVEN NUCLEI
ORGANIC ACIDS
ORGANIC COMPOUNDS
STABLE ISOTOPES
580000* - Geosciences