Further observations of the 8-13 micron spectrum of Titan

Details Further observations of the 8-13 micron spectrum of Titan Further observations of the 8-13 micron spectrum of Titan

Oct 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apj...201l..41g&link_type=abstract

Astrophysical Journal, vol. 201, Oct. 1, 1975, pt. 2, p. L41-L43.

Astronomy and Astrophysics

Astrophysics

30

Atmospheric Composition, Emission Spectra, Infrared Spectrophotometers, Titan, Acetylene, Ethylene, Mathematical Models, Methane, Thermal Emission

Scientific paper

Spectrophotometric observations of Titan, covering the range between 7.8 and 13.3 microns with a resolution of approximately 0.02 wavelengths, are presented. The resulting spectrum is in excellent agreement with the predicted spectrum based on an inversion model for Titan's atmosphere. In addition to emission bands of methane and ethane, evidence is found for emission by acetylene, ethylene, and monodeuterated methane.

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