The edge-on presentation of Saturn's rings during 1995 and early 1996
provided an opportunity to study aspects of the Saturn system rarely
observable from Earth. New results have been reported on the orbits and
photometry of the smallest moons, thickness of the inner ring system and
the nature of its atmosphere, structure of the tenuous outer E and G
Rings, and determination of the rate of precession of Saturn's pole.
One of the biggest puzzles is the apparent shift of Prometheus in its
orbit by 19 degrees. In addition, numerous observers have reported the
discovery of new moons and/or ring clumps. The recent events probably
provided our last chance to study many of these aspects of the Saturn
system prior to the arrival by the Cassini orbiter in 2004.
The workshop will be stuctured around a series of ~30 minute contributed presentations, with plenty of discussion time interspersed. The deadline for titles and brief abstracts of presentations will coincide with the DPS abstract deadline, Wednesday, June 4, 1997.
This page will be updated regularly as new information becomes available.