Observations of ejecta clouds produced by impacts onto Saturn's rings

Details Observations of ejecta clouds produced by impacts onto Saturn's rings Observations of ejecta clouds produced by impacts onto Saturn's rings

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf.1407t&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.1407

Physics

Scientific paper

We identify these observed dust clouds as ejecta produced by impacts
onto the rings, as this is by far the most likely mechanism for
producing such a cloud with the required rapidity. The implications for
projectile size, velocity, and frequency will be discussed.

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