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(vesicle / amphiphile / origin of life / interstellar
ice / cometary delivery)
* Astrochemistry Laboratory, National Aeronautics and Space
Administration Ames Research Center, Mail Stop 245-6, Moffett Field, CA
94035-1000; Edited by Stanley L. Miller, University of California at San
Diego, La Jolla, CA, and approved December 13, 2000 (received for review October 25, 2000)
Interstellar gas and dust constitute the primary material from
which the solar system formed. Near the end of the hot early phase of
star and planet formation, volatile, less refractory materials were
transported into the inner solar system as comets and interplanetary
dust particles. Once the inner planets had sufficiently cooled, late
accretionary infall seeded them with complex organic compounds
[Oró, J. (1961) Nature (London) 190, 389-390; Delsemme, A. H. (1984) Origins Life 14, 51-60; Anders, E. (1989) Nature (London) 342, 255-257;
Chyba, C. F. & Sagan, C. (1992) Nature (London) 355, 125-131]. Delivery of such extraterrestrial compounds may have
contributed to the organic inventory necessary for the origin of life.
Interstellar ices, the building blocks of comets, tie up a large
fraction of the biogenic elements available in molecular clouds. In our
efforts to understand their synthesis, chemical composition, and
physical properties, we report here that a complex mixture of molecules
is produced by UV photolysis of realistic, interstellar ice analogs,
and that some of the components have properties relevant to the origin
of life, including the ability to self-assemble into vesicular structures.
Special Feature
Research Article
Chemistry
Self-assembling amphiphilic molecules: Synthesis in simulated
interstellar/precometary ices
,
,
Search for Extraterrestrial Intelligence
Institute, 2035 Landings Drive, Mountain View, CA 94043; and
Department of Chemistry and Biochemistry, University
of California, Santa Cruz, CA 95064
§
To whom reprint requests should be addressed. E-mail:
ssandford{at}mail.arc.nasa.gov.
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