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Cassini Science League

Cassini Science League


Predators and Prey, Fluffy and Slick
– The Ecology of Saturn’s Ring Particles

Jan. 12, 2012


Two sets of measurements made by NASA's Cassini spacecraft in the ultraviolet and infrared ranges of radiation have provided new insights into the behavior and make-up of Saturn’s ring particles. Researchers using Cassini’s ultraviolet imaging spectrograph have shown that the processes that form temporary clumps of particles and then destroy them are driven by the gravity of some of Saturn’s moons. The numbers of large and small clumps appear to follow what in biology is called a “predator-prey relationship” that governs, for example, the numbers of foxes and hares in an area. Researchers using Cassini’s composite infrared spectrometer and theoretical models have also characterized the sizes, speeds of rotation and the "surface densities" of particles in different zones of the rings.

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