Published March 1989 | Version v1
Journal article

High-resolution infrared spectroscopy of Io and possible surface materials

  • 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