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Interstellar organic chemistry.Most of the interstellar organic molecules have been found in the large radio source Sagittarius B2 toward the galactic center, and in such regions as W51 and the IR source in the Orion nebula. Questions of the reliability of molecular identifications are discussed together with aspects of organic synthesis in condensing clouds, degradational origin, synthesis on grains, UV natural selection, interstellar biology, and contributions to planetary biology.
Document ID
19720052954
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Sagan, C.
(Cornell University Ithaca, N.Y., United States)
Date Acquired
August 6, 2013
Publication Date
July 14, 1972
Publication Information
Publication: Nature
Volume: 238
Subject Category
Chemistry
Accession Number
72A36620
Funding Number(s)
CONTRACT_GRANT: NGR-33-010-082
Distribution Limits
Public
Copyright
Other

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