Physical Characteristics and Possible Accretionary Origins for Saturn's Small Satellites

Details Physical Characteristics and Possible Accretionary Origins for Saturn's Small Satellites Physical Characteristics and Possible Accretionary Origins for Saturn's Small Satellites

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006lpi....37.2289p&link_type=abstract

37th Annual Lunar and Planetary Science Conference, March 13-17, 2006, League City, Texas, abstract no.2289

Physics

5

Scientific paper

From high quality Cassini images yielding the physical characteristics
of Saturn's small satellites, as well as numerical simulations of
accretion around a monolithic small "core" in a planetary ring, we have
found that the small saturnian satellites have likely formed by
accretion.

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