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Infrared Spectra of Venus

Published online by Cambridge University Press:  14 August 2015

Louise Gray Young
Louise Gray Young*
Affiliation:
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, Calif., U.S.A.

Abstract

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A historical account of observations of Venus and their interpretation is given. The major constituent of the atmosphere on Venus (CO2) was detected spectroscopically forty years ago, and minor constituents (CO, HF, HCl) have been found more recently. The infrared spectra also provide a means of studying the motions of her cloudy atmosphere. The composition of the clouds has been sought in the reflection spectrum of Venus, and some of the evidence for their nature is discussed.

Type
Part II Terrestrial Planets
Information
Symposium - International Astronomical Union , Volume 65: Exploration of the Planetary System , 1974 , pp. 77 - 160
Copyright
Copyright © Reidel 1974 

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