Mean molecular weight and hydrogen abundance of Titan's atmosphere

Details Mean molecular weight and hydrogen abundance of Titan's atmosphere Mean molecular weight and hydrogen abundance of Titan's atmosphere

Aug 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981natur.292..688s&link_type=abstract

Nature, vol. 292, Aug. 20, 1981, p. 688-693.

Computer Science

113

Abundance, Hydrogen, Molecular Gases, Molecular Weight, Satellite Atmospheres, Titan, Atmospheric Composition, Atmospheric Models, Stratosphere, Surface Temperature, Troposphere, Voyager 1 Spacecraft, Saturn, Satellites, Atmosphere, Titan, Hydrogen, Abundance, Surface, Optical Properties, Opacity, Troposphere, Stratosphere, Wavelengths, Emissions, Spectrum, Voyager 1, Iris, Data, Temperatures, Thickness, Models, Infrared Interferometry Spectrometer, Thermal Properties

Scientific paper

The 200-600/cm continuum opacity in the troposphere and lower stratosphere of Titan is inferred from thermal emission spectra from the Voyager 1 IR spectrometer (IRIS). The surface temperature and mean molecular weight are between 94 and 97 K and between 28.3 and 29.2 AMU, respectively. The mole fraction of molecular hydrogen is 0.002 + or - 0.001, which is equivalent to an abundance of approximately 0.2 + or - 0.1 km amagat.

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