Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 1994
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994jgr....9917069b&link_type=abstract
Journal of Geophysical Research (ISSN 0148-0227), vol. 99, no. E8, p. 17069-17074
Astronomy and Astrophysics
Astronomy
16
Absorptivity, Atmospheric Composition, Line Spectra, Low Temperature Environments, Nitrites, Satellite Atmospheres, Titan, Ultraviolet Spectra, Ultraviolet Spectroscopy, Albedo, Molecular Ions, Optical Thickness, Temperature Dependence, Ultraviolet Astronomy, Vapor Pressure, Voyager Project
Scientific paper
The interpretation of albedo spectra in the mid-UV range is critically dependent on the knowledge of the absolute absorption coefficient, at specific temperatures and with high resolution for molecular compounds likely to absorb the scattered solar radiation in this wavelentth range. Propynenitrile, a key molecule in prebiotic synthesis, already detected with IR and microwave sounding in Titan's atmosphere, exhibits intense absorption bands in the 185 to 230 nm interval. This paper deals with the absolute absorption coefficient k of propynenitrile at low temperature and high resolution and compares it to the room temperature values. The consequences of the observed k variations on the interpretation of Titan's atmosphere spectra, expected in the near future, are considered here. As an additional result, the pressure regulation system of the experiment allows us to assess the determination of the temperature dependence of the propynenitrile vapor pressure.
Benilan Yves
Bruston Paul
Cossart-Magos Claudina
Guillemin Jean Claude
Raulin François
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