![]() ![]() But where is the "missing" 40 percent? "We are investigating the possibility that there are many smaller volcanoes that are hard, but not impossible, to detect," said Veeder. This component mostly emanates from flat-floored volcanic craters called paterae, a common feature on Io. The team found that active volcanoes accounted for only about 60 percent of Io's heat. ![]() "What we see indicates a mixture of both deep and shallow heating." A mystery has also emerged. "Instead, the main thermal emission occurs about 40 degrees eastward of its expected positions." "The pattern that emerges points to a complex heating process within Io," said Matson. "The fascinating thing about the distribution of the heat flow is that it is not in keeping with the current preferred model of tidal heating of Io at relatively shallow depths," said Davies. The team examined data primarily from the NASA's Voyager and Galileo missions, but also incorporated infrared data obtained from telescopes on Earth. "This is the most comprehensive study of Io's volcanic thermal emission to date," said Glenn Veeder of the Bear Fight Institute, Winthrop, Wash., who led the work of a multi-faceted team that included Ashley Davies, Torrence Johnson and Dennis Matson of NASA's Jet Propulsion Laboratory, Pasadena, Calif., Jani Radebaugh of Brigham Young University, in Provo, Utah, and David Williams of Arizona State University, Tempe, Ariz. Most of Io's eruptions dwarf their contemporaries on Earth. A map of hot spots, classified by the amount of heat being emitted, shows the global distribution and wide range of volcanic activity on Io. These results come from data collected by NASA spacecraft and ground-based telescopes and appear in the June issue of the journal Icarus. The heat pouring out of Io's hundreds of erupting volcanoes indicates a complex, multi-layer source. A new study finds that the pattern of heat coming from volcanoes on Io's surface disposes of the generally-accepted model of internal heating. ![]()
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