The deep atmosphere of Venus revealed by high-resolution nightside spectra

Computer Science

Scientific paper

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Atmospheric Chemistry, Infrared Spectra, Lower Atmosphere, Night Sky, Venus Atmosphere, Absorption Spectra, Carbon Dioxide, Carbon Monoxide, Emission Spectra, Remote Sensing, Water Vapor, Venus, Atmosphere, Nightside, Spectra, Emissions, Radiation, Pressure, Thermal Emissions, Spectroscopy, Absorption, Features, Depth, Water, Position (Location), Carbon Dioxide, Abundance, Troposphere, Chemistry, Comparisons, Hydrogen Chloride, Hydrogen Fluoride, Carbonyl Sulfide, Wavelengths, Spectra, Altitude, Distributio

Scientific paper

The first high-resolution spectroscopic observations of the night side of Venus obtained in two narrow spectral windows centered at 1.74 and 2.3 microns, where the nightside is anomalously bright, are reported. Absorption features from CO2, CO, H2O, HDO, HCl, HF, and COS are detected, and there are a number of unidentified features. A preliminary analysis indicates that the observed radiation is thermal emission from atmospheric layers in the eight-bar pressure region for the 2.3 micron window and even deeper at 1.7 micron. The derived CO and H2O abundances agree with in situ Pioneer measurements in the deep troposphere and are consistent with the high deuterium enrichment inferred from Pioneer data. The first measurements of HCl and HF below the clouds are reported along with the first firm detection of COS.

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