| Literature DB >> 11539748 |
J F Kerridge1, S Chang, R Shipp.
Abstract
Isotopic analyses of residues prepared by demineralisation of the Murchison meteorite using D-labelled reagents provide evidence for measurable exchange of H-isotopes between residue and reagents. Precise quantification of this effect is precluded by substantial inhomogeneity of the meteoritic organic matter. A conservative estimate of the degree of exchange is 3 to 5% of the H pyrolysable as H2O. This could affect the shape of the curve defining D-release as a function of temperature, but does not change conclusions previously drawn concerning the nature of the bulk D-enrichment of insoluble organic matter in meteorites.Entities:
Keywords: NASA Center ARC; NASA Discipline Exobiology; NASA Discipline Number 52-20; NASA Program Exobiology; Non-NASA Center
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Year: 1988 PMID: 11539748 DOI: 10.1016/0016-7037(88)90127-5
Source DB: PubMed Journal: Geochim Cosmochim Acta ISSN: 0016-7037 Impact factor: 5.010