Wes Patterson, a planetary scientist at the Johns Hopkins University Applied Physics Laboratory in Laurel, Maryland, led a seven-year effort to craft a detailed map of geological features on Ganymede, the largest moon of Jupiter. Patterson and a half-dozen scientists from several institutions compiled the global map - only the third ever completed of a moon, after Earth’s moon and Jupiter’s cratered satellite Callisto - using images from NASA’s historic Voyager and Galileo missions.

“The map really gives us a more complete understanding of the geological processes that have shaped the moon we see today,” says Patterson, whose team will present and discuss the map at the 2009 European Planetary Science Congress in Potsdam, Germany on Wednesday 16 September.

With a diameter of 5262 kilometers (3280 miles), Ganymede is the largest moon in the solar system. Larger than both planet Mercury and dwarf planet Pluto, it’s also the only satellite in the solar system known to have its own magnetosphere. The map details geologic features of the moon that formed and evolved over much of our Solar System’s history. These features record evidence of the internal evolution of this large icy satellite, of its dynamical interactions with the other Galilean satellites, and of the evolution of the population of small bodies impacting the surface of the satellite.

While scientists have crafted several regional geological maps of Ganymede’s surface using Voyager data, Patterson’s team was the first to combine the low-resolution Voyager photos with high-resolution Galileo images to create a global and consistent view of the moon’s geology

Enlarge

(Top) A global mosaic of Jupiter's moon Ganymede, constructed from the best images collected during flybys of the Voyager 1, Voyager 2, and Galileo spacecraft. (Bottom) A few layers of the geologic map of Ganymede, showing the boundaries between light terrain (white) and dark terrain (brown), and the massive number of tectonic features in the light terrain (black lines). The map is being used to analyze stress fields that could have been responsible for ripping apart the surface of Ganymede in the past (red arrows).

“By mapping the entirety of Ganymede’s surface, we can more accurately address scientific questions regarding the formation and evolution of this truly unique moon,” Patterson says. “Work done using the map by collaborator Geoff Collins at Wheaton College, for instance, has shown that vast swaths of grooved terrain covering the surface of the satellite formed in a specific sequence. The details of this sequence tell us something about the forces that must have been necessary to form those swaths.”

Patterson says scientists can look at Ganymede’s geological history as a “touchstone” for comparing and contrasting the characteristics and evolution of other large to mid-sized icy satellites. The map will also, he adds, be a reference for exploration of the Jovian system. NASA and the European Space Agency are currently developing that next voyage: the Europa Jupiter System Mission would include orbiters of Ganymede as well as the icy satellite Europa.

“A primary goal of the next flagship mission to the Jupiter system will be to characterize, in detail, the geophysical, compositional, geological, and external processes that affect icy satellites,” he says. “This map will be an invaluable tool in determining how best to address those goals for Ganymede.”

The team includes Patterson and Louise Prockter, also from APL; James Head, from Brown University; Geoffrey Collins of Wheaton College; Robert Pappalardo from NASA’s Jet Propulsion Laboratory; Baerbel Lucchitta of the U.S. Geological Survey; and Jonathan Kay of the University of Idaho.

Source: Europlanet