The Europa Clipper mission, which is already in formulation, plans to do just that. Only, before an orbiter or lander can be sent to this moon which is only slightly smaller than ours, NASA needs to know where to land its spacecraft on surface covered by bounteous cracks, ridges, bands, etc. In other words, they need a map. And now, they have one, courtesy D. Alex Patthoff of Planetary Science Institute and his colleagues at UCLA, Wheaton College, and NASA’s Jet Propulsion Laboratory.
Creating the geological map was especially challenging because in addition to the complex surface of the moon, the variable lighting conditions and image resolutions from the Galileo solid state imager (SSI) data set made it difficult to differentiate between features like a ridge and a crack. But now, the finished product not only identifies individual units like chaos, bands, ridged plains, and craters, it also depicts structural features like ridges, cycloids, undifferentiated linea, crater rims, depression margins, dome margins, and troughs. The map has been created at the scale of 1:15 million.
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