Abstract
Carbonaceous residues from a variety of laboratory syntheses yield release patterns for C and H isotopes during stepwise combustion that fail to mimic the striking patterns characteristic of meteoritic kerogen-like residues that otherwise superficially resemble them. It seems likely that the meteoritic material comprises a complex mixture of substances having different origins and/or synthesis conditions.
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Schedule a callMore From: Origins of life and evolution of the biosphere : the journal of the International Society for the Study of the Origin of Life
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