CS2 - Candidate for the 3150-A Venus band

Details CS2 - Candidate for the 3150-A Venus band CS2 - Candidate for the 3150-A Venus band

Jan 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979icar...37..297y&link_type=abstract

Icarus, vol. 37, Jan. 1979, p. 297-300.

Astronomy and Astrophysics

Astronomy

1

Carbon Disulfide, Planetary Composition, Ultraviolet Spectra, Venus Clouds, Absorption Spectra, Astronomical Spectroscopy, Chalcogenides, Thermodynamic Equilibrium, Sulfur, Clouds, Carbon, Absorption Spectra, Venus, Thermodynamics, Carbon Disulfide, Abundance, Equilibrium, Photochemistry, Carbon Monosulfide, Carbon Monoxide, Decomposition

Scientific paper

The 3150-A absorption on Venus, found by Barker et al. (1975), may be
due to carbon disulfide. The stability and thermodynamics of the carbon
chalcogenides are briefly discussed.

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