1977
DOI: 10.1029/js082i028p04635
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The composition of the atmosphere at the surface of Mars

Abstract: We have confirmed the discovery of N2 and 40Ar by the Entry Science Team, and we have also detected Ne, Kr, Xe, and the primordial isotopes of Ar. The noble gases exhibit an abundance pattern similar to that found in the terrestrial atmosphere and the primordial component of meteoritic gases. Xenon appears to be underabundant in comparison to the meteoritic ratio, as it is on earth. The isotopic ratios 15N/14N, 40Ar/36Ar, and 129Xe/132Xe are distinctly different from the terrestrial values, implying different … Show more

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Cited by 542 publications
(310 citation statements)
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“…b , Smith (2004), Smith et al (2009a). c Krasnopolsky et al (1997), Lodders and Fegley (1997), Owen et al (1977). d Krasnopolsky (2007), Smith et al (2009b).…”
Section: Water Cyclementioning
confidence: 99%
“…b , Smith (2004), Smith et al (2009a). c Krasnopolsky et al (1997), Lodders and Fegley (1997), Owen et al (1977). d Krasnopolsky (2007), Smith et al (2009b).…”
Section: Water Cyclementioning
confidence: 99%
“…Its molar fraction is about 0.953 (Owen et al 1977). CO 2 photolysis is the source of carbon monoxide.…”
Section: Introductionmentioning
confidence: 99%
“…The Rayleigh scattering optical depth is computed as in Hansen and Travis (1974), using parameters appropriate for Mars. Atmospheric composition is taken as 95% CO2 (Owen et al, 1977). The altitude dependence of 03 is based on model results (Lindner, 1988).…”
Section: Modeling Proceduresmentioning
confidence: 99%