Bolometric albedos and diurnal temperatures of the brightest regions on Io

Physics

Scientific paper

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Bolometers, Brightness Temperature, Diurnal Variations, Io, Satellite Atmospheres, Surface Temperature, Iris Satellites, Voyager 1 Spacecraft, Jupiter, Satellites, Io, Brightness, Albedo, Diurnal Variations, Maps, Temperature, Surface, Features, Spacecraft Observations, Iris Instrument, Roughness, Sulfur Dioxide, Frost, Mapping, Voyager 1 Mission, Longitude, Position (Location), Calculations

Scientific paper

Cylindrical maps of the locations and estimated Bond albedos of the brightest regions on the Io surface have been constructed on the basis of Voyager data; the albedos are then rescaled to correct for radiometric calibration uncertainties. The highest surface albedos are found to be only moderately higher than the Bond albedo of Io as a whole. The brightest regions include two bright patches southeast of the Maui and Amirani active vents, as well as a large equatorial field of high-albedo material and a lone bright patch at high northern latitudes. These maps indicate that Io's albedos are strongly latitude-dependent.

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