May 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984icar...58..197y&link_type=abstract
Icarus (ISSN 0019-1035), vol. 58, May 1984, p. 197-226.
Other
46
Io, Molecular Spectra, Satellite Surfaces, Sulfur, Astronomical Photography, Color, Cooling, Liquid Phases, Reflectance, Spectrum Analysis, Jupiter, Satellites, Io, Sulfur, Flows, Physical Properties, Chemistry, Volcanism, Composition, Colors, Quenching, Iron, Spectra, Reflectance, Data, Liquids, Thermal Effects
Scientific paper
Physical and chemical properties of elemental sulfur are incompatible with the suggestion that the colored flows associated with volcanoes on Io are quenched unstable allotropes of sulfur. Either the volcanic flows are not sulfur, or some mechanism other than quenching is required to produce colored forms of sulfur in them. The properties of sulfur are unsuited to the production and survival of colored unstable allotropes on Io. The color of this object is probably due to some other material, possibly iron compounds.
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