NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
Isotopic analyses of amino acids from the Murchison meteoriteAn account is given of the results of H-2, C-13 isotopic analyses of the Murchison meteorite incorporating an ultrafiltration step to exclude the possibility of fine particulate contaminants. The meteorite's amino acids were chromatographically separated in order to preclude isotopic enrichment by basic compounds other than the amino acids. The results indicate that the Murchison amino acids are isotopically highly unusual; delta-C-13 is elevated by about 40 percent, and delta-D by fully 2500 percent. This high D content of the meteorite's alpha-amino acids may be due to the synthesis of their molecular precursors by low-temperature ion-molecule reactions in an interstellar cloud.
Document ID
19910046583
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Pizzarello, S.
(Arizona State Univ. Tempe, AZ, United States)
Cronin, J. R.
(Arizona State University Tempe, United States)
Krishnamurthy, R. V.
(Arizona State Univ. Tempe, AZ, United States)
Epstein, S.
(California Institute of Technology Pasadena, United States)
Date Acquired
August 14, 2013
Publication Date
March 1, 1991
Publication Information
Publication: Geochimica et Cosmochimica Acta
Volume: 55
ISSN: 0016-7037
Subject Category
Space Biology
Accession Number
91A31206
Funding Number(s)
CONTRACT_GRANT: NAGW-1899
CONTRACT_GRANT: NSG-7255
Distribution Limits
Public
Copyright
Other

Available Downloads

There are no available downloads for this record.
No Preview Available