New Map Helps Reveal Origins of Mysterious Features on Solar System's Biggest Moon The map supports the theory that Ganymede's grooves are the result of orbital resonances among Ganymede, Europa and Io as they circle Jupiter
Scientists complete first global geologic map of Jupiter's satellite Ganymede Scientists have assembled the first global geological map of the Solar System's largest moon - and in doing so have gathered new evidence into the formation of the large, icy satellite. 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" - Wes Patterson, whose team will present and discuss the map at the 2009 European Planetary Science Congress in Potsdam, Germany on Wednesday September 16.
With a diameter of 5262 kilometres, 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
"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. 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" - Wes Patterson.
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 characterise, in detail, the geophysical, compositional, geological, and external processes that affect icy satellites. This map will be an invaluable tool in determining how best to address those goals for Ganymede" - Wes Patterson.
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
Ganymede is Jupiter's largest moon, and the largest moon in the entire solar system; it is larger in diameter than Mercury but only about half its mass. Ganymede is one of four planetary satellites of Jupiter which can be seen with the naked eye with good eyesight, a clear night and without the pollution haze of cities. Other than these, the only planetary satellite visible with the naked eye is our own Moon.