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Organic and inorganic interpretations of the Martian UV-IR reflectance spectrumViking Lander biology experiment gas chromatography-mass spectrometer analysis has detected no organic molecules above a concentration of parts per billion. The questions considered here include the reason for the lack of organic molecules at the landing sites, whether the sterility of the two sites is representative of the whole of Mars, and whether there may be locations more conducive to organic compound formation and preservation. After simulating the destruction of organic compounds in Mars-like laboratory conditions and examining whether the destructive mechanism might obtain throughout the planet, UV and IR reflectance spectra are re-examined for any evidence of organic molecules and an upper limit is determined for organic carbon content of average Martian soil. It is found that the average Martian soil is poor in inorganics, presents a poor habitat for carbon chemistry-based life forms, and is not likely to preferentially preserve such organisms anywhere on the planet.
Document ID
19820037673
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Pang, K. D.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Ajello, J. M.
(California Institute of Technology, Jet Propulsion Laboratory, Pasadena CA, United States)
Chun, S. F. S.
(California, University San Francisco, CA, United States)
Nansheng, Z.
(Beijing Planetarium Beijing, People's Republic Of China)
Minji, L.
(Beijing Glass Institute Beijing, People's Republic Of China)
Date Acquired
August 10, 2013
Publication Date
January 7, 1982
Publication Information
Publication: Nature
Volume: 295
Subject Category
Space Biology
Accession Number
82A21208
Distribution Limits
Public
Copyright
Other

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