HR: 09:30h
AN: P21F-03 INVITED [Abstracts]
TI: Imaging Enceladus' Exotic South Polar Regions: Imaging Science Team Results
AU: * Johnson, T
EM: Torrence.V.Johnson@jpl.nasa.gov
AF: Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Dr., Altadena, CA 91001
United States
AB:
The Cassini spacecraft had a close (175 km altitute) encounter with Saturn's moon Enceladus on 14 July 2005, resulting in a
major discovery: evidence from multiple experiments show that there is a large `plume' of water vapor and particles emanating
from the satellite's south polar region. Infrared data from the CIRS instrument showed that this area is also anomalously
warm, providing evidence for internal heat. High resolution images taken by the Imaging Science System during the encounter
show that the warm region associated with water vapor venting is a unique area on this icy world. The region has very few if
any detectable impact craters, making it the youngest surface seen on Enceladus, or any of the other icy Saturnian
satellites; estimates from cratering models place its age at less than 10-100 million years. It is surrounded by tectonic
features suggesting a global stress pattern that may be associated with a change in spin rate. Long, parallel fractures,
informally dubbed `tiger stripes', cross the region and are correlated with at least some of the thermal anomalies, making
them good candidates for the source regions of the water venting. Spectral data and photometric studies also show that the
whole area and the tiger stripes in particular have fewer fine grained particles on the surface than most of the moon's
surface, in agreement with a young surface and crystalinity and grain size interpretations of data from the Visual and Near
Infrared Mapping Spectrometer experiment. Tidal forces and radioactive heating are probably responsible for the activity,
although generating such intense internal heating is challenging for current models. Portions of this work were done at the
Jet Propulsion Laboratory, California Institute of Technology, under a contract with NASA.
DE: 6280 Saturnian satellites
SC: Planetary Sciences [P]
MN: Fall Meeting 2005