Scientists unveil solutions to enigmatic radar characteristics of Jupiter and Saturn's moons A collaborative investigation led by Dr. Jason Hofgartner, Senior Research Scientist at the Southwest Research Institute, sheds light on the puzzling radar signatures of icy satellites orbiting Jupiter and
A study co-authored by Southwest Research Institute Senior Research Scientist Dr. Jason Hofgartner explains the unusual radar signatures of icy satellites orbiting Jupiter and Saturn. Their radar signatures, which differ significantly from those of rocky worlds and most ice on Earth, have long been a vexing question for the scientific community. Credit: NASA/JPL-Caltech/SwRIA collaborative investigation led by Dr. Jason Hofgartner, Senior Research Scientist at the.
“When we look up at Earth’s moon it looks like a circular disk, even though we know it’s a sphere. Planets and other moons similarly look like disks through telescopes,” Hofgartner said. “While making radar observations, the center of the disk is very bright and the edges much darker. The change from center to edge is very different for these icy satellites than for rocky worlds.
An icy surface, Hofgartner explained, has an even stronger opposition effect than normal. For every scattering path of light bouncing through the ice, at opposition there is a path in the exact opposite direction. Because the two paths have precisely the same length, they combine coherently, resulting in further brightening.
“I think that tells us that the surfaces of these objects and their subsurfaces down to many meters are very tortured,” Hofgartner said. “They’re not very uniform. Icy rocks dominate the landscape, perhaps looking somewhat like the chaotic mess after a landslide. That would explain why the light is bouncing in so many different directions, giving us these unusual polarization signatures.”
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