More than 400 years after Galileo's discovery of Io, the innermost（最里面的） of Jupiter's largest moons, a team of scientists led by Arizona State University (ASU) has produced the first complete global geologic¹ map of the Jovian satellite. The map, published by the U. S. Geological Survey, depicts² the characteristics and relative ages of some of the most geologically unique and active volcanoes and lava³ flows ever documented in the Solar System. Following its discovery by Galileo in January 1610, Io has been the focus of repeated telescopic and satellite scientific observation. These studies have shown that the orbital and gravitational relationships between Io, its sister moons Europa and Ganymede, and Jupiter cause massive, rapid flexing⁴ of its rocky crust. These tidal flexures generate tremendous heat within Io's interior, which is released through the many surface volcanoes observed.

"One of the reasons for making this map was to create a tool for continuing scientific studies of Io, and a tool for target planning of Io observations on future missions to the Jupiter system," says David Williams, a faculty⁵ research associate in the School of Earth and Space Exploration at ASU, who led the six-year research project to produce the geologic map.

The highly detailed⁶, colorful map reveals a number of volcanic⁷ features, including: paterae (caldera-like depressions), lava flow fields, tholi (volcanic domes), and plume⁸ deposits, in various shapes, sizes and colors, as well as high mountains and large expanses of sulfur⁹- and sulfur dioxide-rich plains. The mapping identified 425 paterae, or individual volcanic centers. One feature you will not see on the geologic map is impact craters¹⁰.

"Io has no impact craters; it is the only object in the Solar System where we have not seen any impact craters, testifying to Io's very active volcanic resurfacing," says Williams.

Io is extremely active, with literally¹¹ hundreds of volcanic sources on its surface. Interestingly, although Io is so volcanically¹² active, more than 25 times more volcanically active than Earth, most of the long-term surface changes resulting from volcanism are restricted to less than 15 percent of the surface, mostly in the form of changes in lava flow fields or within paterae.

"Our mapping has determined¹³ that most of the active hot spots occur in paterae, which cover less than 3 percent of Io's surface. Lava flow fields cover approximately 28 percent of the surface, but contain only 31 percent of hot spots," says Williams. "Understanding the geographical¹⁴ distribution of these features and hot spots, as identified through this map, are enabling better models of Io's interior processes to be developed."