Published March 1989
| Version v1
Journal article
High-resolution infrared spectroscopy of Io and possible surface materials
Creators
- 1. NASA, Ames Research Center, Moffett Field, CA (USA)
- 2. Infrared Telescope Unit, Hilo, HI (USA)
- 3. Edinburgh Royal Observatory, (England)
- 4. Groningen Rijksuniversiteit (Netherlands)
- 5. California Institute of Technology, Pasadena (USA)
- 6. Hawaii Univ., Honolulu (USA)
Description
A comparison of new spectra of Io with laboratory-simulated frosts confirms that the dominant materials on Io are SO2 frost in conjunction with a spectrally neutral material presumed to be sulfur. While the 4-micron region spectra are largely explainable in these terms, attention is drawn to a shoulder in the spectrum at 4.04 microns that is suggestive of adsorbed SO2 gas; two shallow, unidentified bands are also noted at 3.85 and 3.91 microns. The isotopic ratios of oxygen and sulfur appear to be normal. The absence of distinct bands in the new spectra in the 5-micron region limits the abundance of sulfate and sulfite compounds. 34 references
Additional details
Publishing Information
- Journal Title
- Icarus
- Journal Volume
- 78
- Series
- Icarus.
- Journal Page Range
- 27-37
- ISSN
- 0019-1035
- CODEN
- ICRSA
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 20078191
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- CHEMICAL COMPOSITION; JUPITER PLANET; REFLECTION; RESOLUTION; SATELLITE ATMOSPHERES; SATELLITES; SPECTROSCOPY; SULFUR OXIDES; SURFACES
- Descriptors DEC
- ATMOSPHERES; CHALCOGENIDES; OXIDES; OXYGEN COMPOUNDS; PLANETS; SULFUR COMPOUNDS