Using Enceladus as an extremely simple example, the premise of this poster is to show how CSNB maps may function as Maxwellian graphical stress diagrams [see upper left]. The constant gravitational pull of Saturn on the ice-shell moon causes extremely active shear cracks at the south pole. The opposite pole holds the oldest (most cratered, most inactive) terrain. The four-map column on the right shows results when the map-interruption line is placed at various critical longitudinal planes. Note the colored lines in the 3-D sketch on the left: the red line is the plane of maximum outward gravitational pull, “high tide”; the blue line is “low tide”; the green and magenta lines are inflection planes. These four lines are the edges of the four maps in the righthand column. The abstract for this poster is here.









