Physics
Scientific paper
Oct 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992natur.359..619s&link_type=abstract
Nature (ISSN 0028-0836), vol. 359, no. 6396, p. 619-621.
Physics
87
Gravitational Effects, Saturn Rings, Wakes, Dynamic Models, Particle Collisions
Scientific paper
Numerical simulations, including both gravitational interactions and dissipative impacts between particles, are used here to study realistic models for Saturn's rings. For the C-ring there is no instability, but for the B- and A-rings gravitational wakes form. In the A-ring these wakes are so strong that particles trapped in them from meter-sized aggregate particles, which themselves lead to further instability. These different behaviors are consistent with the observational evidence.
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