Other
Scientific paper
Jul 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003hst..prop.9725k&link_type=abstract
HST Proposal ID #9725
Other
Hst Proposal Id #9725 Solar System
Scientific paper
Recording the seasonal change of Uranus is a key to understand seasonal changes in atmospheres due to Uranus' high obliquity. The best record to date comes from WFPC2 imaging of Uranus since 1994. We propose to image Uranus simultaneously with similar filters in WFPC2 and ACS so that this record can be extended with future ACS observations. Without such an observation, the long-term record of WFPC2 images cannot be linked with any future images because of Uranus' steep spectral features. Observations of the Uranian rings over a wide range of sub-solar latitudes allow powerful constraints on physical parameters, such as separation between ring particles. Our proposed observations will provide the necessary link between previous WFPC2 images and future ACS images near the ring-plane-crossing of 2007. The same reasoning applies to images of Uranian satellites, where a consistent record over a wide range of sub-solar latitudes yields information about satellite shape and albedo distribution. Since Cycle 12 is the last Cycle of WFPC2, there will be no other chance for the proposed observations. The investment of only two orbits will significantly enhance the scientific value of the previous 45 WFPC2 orbits on Uranus. Only HST has the spatial resolution and photometric stability for these studies.
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