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* Search for Extraterrestrial Intelligence Institute/National
Aeronautics and Space Administration Ames Research Center, MS 239-15, Moffett Field, CA 94035-1000; Edited by Robert O. Pohl, Cornell University, Ithaca, NY, and
approved December 29, 2000 (received for review October 27, 2000)
C---H stretching bands,
Special Feature
Chemistry
Organic protomolecule assembly in igneous minerals
,
, and
Stanford University,
Stanford, CA 94305; and § University of Kentucky,
Lexington, KY 40506
CH, in the infrared
spectrum of single crystals of nominally high purity, of
laboratory-grown MgO, and of natural upper mantle olivine, provide an
"organic" signature that closely resembles the symmetrical and
asymmetrical C---H stretching modes of aliphatic ---CH2
units. The
CH bands indicate that H2O and
CO2, dissolved in the matrix of these minerals, converted to form H2 and chemically reduced C, which in turn formed
C---H entities, probably through segregation into defects such as
dislocations. Heating causes the C---H bonds to pyrolyze and the
CH bands to disappear, but annealing at 70°C causes
them to reappear within a few days or weeks. Modeling dislocations in
MgO suggests that the segregation of C can lead to Cx chains,
x = 4, with the terminal C atoms anchored to the
MgO matrix by bonding to two O
. Allowing H2
to react with such Cx chains leads to
[O2C(CH2)2CO2] or
similar precipitates. It is suggested that such
Cx---Hy---Oz entities represent protomolecules
from which derive the short-chain carboxylic and dicarboxylic and the
medium-chain fatty acids that have been solvent-extracted from crushed
MgO and olivine single crystals, respectively. Thus, it appears that
the hard, dense matrix of igneous minerals represents a medium in which
protomolecular units can be assembled. During weathering of rocks, the
protomolecular units turn into complex organic molecules. These
processes may have provided stereochemically constrained organics to
the early Earth that were crucial to the emergence of life.
To whom reprint requests should be addressed. E-mail
ffreund{at}mail.arc.nasa.gov.
www.pnas.org/cgi/doi/10.1073/pnas.061513298
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