C3H8 and C3H4 in Titan's atmosphere

Details C3H8 and C3H4 in Titan's atmosphere C3H8 and C3H4 in Titan's atmosphere

Aug 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981natur.292..683m&link_type=abstract

Nature, vol. 292, Aug. 20, 1981, p. 683-686. NASA-supported research.

Astronomy and Astrophysics

Astronomy

108

Acetylene, Astronomical Spectroscopy, Atmospheric Composition, Methyl Compounds, Propane, Satellite Atmospheres, Titan, Abundance, Atmospheric Temperature, Planetology, Temperature Distribution, Saturn, Satellites, Titan, Atmosphere, Propane, Methyl Acetylene, Iris, Voyager 1, Infrared, Stratosphere, Abundance, Optical Properties, Mixing, Infrared Interferometry Spectrometer, Comparisons, Frequencies, Absorption, Intensity, Data, Temperatures, Pressure, Opacity, Composition, Spectrum

Scientific paper

Four bands of propane C3H8 and two of methyl acetylene C3H4 have been identified in the Voyager IR spectrum of Titan. Stratospheric abundances of 2 x 10 to the -5 for C3H8 and 3 x 10 to the -8 for C3H4 have been determined for the mid-latitude region. A feature at 1,154/cm, previously assigned solely to CH3D, is now identified at least in part due to C3H8.

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