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Laboratory Studies of Planetary Molecules and Ices: The Case of IO
Published online by Cambridge University Press: 07 August 2017
Abstract
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The techniques of low temperature spectroscopy are applied here to analyze infrared observational data of Io in the 2.0-5.0 μm range. The presence of solid H2S and traces of H2O in the SO2-dominant surface ices are derived from this analysis and it is suggested that CO2 clusters may as well be present near the surface of Io.
Information
- Type
- Solar System
- Information
- Symposium - International Astronomical Union , Volume 150: Astrochemistry of Cosmic Phenomena , 1992 , pp. 435 - 436
- Copyright
- Copyright © Kluwer 1992
References
References:
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