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Viking gas exchange reaction - Simulation on UV-irradiated manganese dioxide substrateThe exchange of O2 for H2O, analogous to that recorded on Mars by the Viking GEX experiment, has been observed on humidifying powdered beta-MnO2 (pyrolusite) which had been irradiated by UV in a humidified analog of the Martian atmosphere. Pyrolusite irradiated in a dry atmosphere did not release O2 on humidification. The XPS spectra of Mn and O of the reactive pyrolusite were shifted toward higher binding energies during UV irradiation. These shifts are consistent with the creation of a surface layer of a Mn(V) or Mn(VI) compound. The destruction of such a layer on humidification could account for the observed O2 release. Although manganese has not been identified in the Martian regolith, the upper limit of the Mn concentration is sufficiently high that O2 release from pyrolusite could have been responsible for the results of the Viking GEX experiment.
Document ID
19800042221
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Blackburn, T. R.
(St. Andrews Presbyterian College Laurinburg N.C., United States)
Holland, H. D.
(Harvard University Cambridge, Mass., United States)
Ceasar, G. P.
(Xerox Corp. Webster, N.Y., United States)
Date Acquired
August 10, 2013
Publication Date
December 30, 1979
Publication Information
Publication: Journal of Geophysical Research
Volume: 84
Subject Category
Space Biology
Accession Number
80A26391
Funding Number(s)
CONTRACT_GRANT: NAS1-10492
Distribution Limits
Public
Copyright
Other

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