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Composition and structure of the Martian atmosphere - Preliminary results from Viking 1Results from the aeroshell-mounted neutral mass spectrometer on Viking 1 indicate that the upper atmosphere of Mars is composed mainly of CO2 with trace quantities of N2, Ar, O, O2, and CO. The mixing ratios by volume relative to CO2 for N2, Ar, and O2 are about 0.06, 0.015, and 0.003, respectively, at an altitude near 135 kilometers. Molecular oxygen is a major component of the ionosphere according to results from the retarding potential analyzer. The atmosphere between 140 and 200 kilometers has an average temperature of about 180 plus or minus 20 deg K. Atmospheric pressure at the landing site for Viking 1 was 7.3 millibars at an air temperature of 241 deg K. The descent data are consistent with the view that CO2 should be the major constituent of the lower Martian atmosphere.
Document ID
19760058640
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Nier, A. O.
(Minnesota, University Minneapolis, Minn., United States)
Hanson, W. B.
(Texas, University Dallas, Tex., United States)
Seiff, A.
(NASA Ames Research Center Moffett Field, Calif., United States)
Mcelroy, M. B.
(Harvard University Cambridge, Mass., United States)
Spencer, N. W.
(NASA Goddard Space Flight Center Greenbelt, Md., United States)
Duckett, R. J.
(NASA Langley Research Center Hampton, Va., United States)
Knight, T. C. D.
(Harvard Univ. Cambridge, MA, United States)
Cook, W. S.
(Martin Marietta Aerospace Denver, Colo., United States)
Date Acquired
August 8, 2013
Publication Date
August 27, 1976
Publication Information
Publication: Science
Volume: 193
Subject Category
Lunar And Planetary Exploration
Accession Number
76A41606
Funding Number(s)
CONTRACT_GRANT: NAS1-9699
CONTRACT_GRANT: NAS1-10492
CONTRACT_GRANT: NAS1-9697
Distribution Limits
Public
Copyright
Other

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