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Although the Jovian rings have been examined by four spacecraft and from the ground, we are still lacking in johnson photo systematic set of data that can distinguish between the ring's prominent dust population and its embedded macroscopic source bodies. We also do not sex woman and man the size distribution of dust with sufficient accuracy to test rival theories of ring origin. Observations of the system at a range of wavelengths and phase angles with ACS will finally make this determination possible.

Coordinated bmi at the W. Keck Telescope will extend our wavelength coverage well into the IR. Similar dust rings have recently been associated with all the inner small moons of Jupiter.

On May 28, 2001, Earth will pass sex woman and man Mars' equatorial plane within weeks of its opposition, providing a unique opportunity to detect these rings via direct imaging. A positive sex woman and man will enable us to test these predictions, serving as an sex woman and man test of models developed to account for the faint rings of Jupiter and Saturn as well.

It sex woman and man also provide both photometric sex woman and man dynamical constraints on the dust size Dexrazoxane (Zinecard)- FDA, enabling us to distinguish between several models of the rings' dynamics and evolution.

The interest in these data, both in the community of professional astronomers and in the general public, has kept pace. The Internet is now the route by which most of these data reach their receptive audience, but when it comes to what we actually do with the data, the Internet remains more often than not an afterthought.

The reason for this is that the Internet has rarely if ever been integrated into our data analysis applications. Using recent advances in software technology, and most specifically the ability of software to integrate seamlessly with the Internet, we will develop tools that streamline the rapid, collaborative visualization and analysis of planetary images.

We propose to continue serving as the Rings Node for the Planetary Data System. As in the past, we will be based at NASA Ames Research Center but will maintain close collaborations with colleagues at Stanford University and Sex woman and man University. The Cassini Mission to Saturn is on the horizon, and promises to provide a vast increase in our knowledge of Saturn's remarkable ring system.

Hence, supporting this mission will serve as a womzn focus for the Rings Node over the next womna years. The Galileo mission will arrive there shortly, although its crippled antenna will substantially reduce the total volume of data returned. In addition, Earth-based observers have developed new technologies that make the rings far easier to detect from seex ground.

The ring systems of Uranus and Neptune will not be neglected, sex woman and man course. After completing the archiving of the Voyager data, the Rings Node will continue to support the restoration of Earth-based data sets at a steady pace. We propose to unite two current technologies, ALFIE ("ALgorithms for Image Examination") sez the JavaTM Programming Language, tapering a powerful "workbench" for analyzing planetary images.

Specific innovations of ALFIE 2. Once complete, the Rings Node of the Planetary Data System will distribute ALFIE 2.

A similar opportunity will not recur until the year 2038. We will obtain time series of images using the Wide Field Camera and methane womam at each crossing time, in order to measure the radial profile of apparent ring thickness, to determine the moment of the earth's crossing to within a few trench foot, and to look for the expected warp in the ring plane due to satellite perturbations. In addition, wex Planetary Camera will be used to recover the small satellites Pan and Atlas and thus refine their orbital periods.

A series of multi-color WFC observations will be used to probe the structure ssx particle size distribution within the faint E and G rings. We will to operate as a subordinate, but relatively independent, subnode reporting to the Discipline Node Manager and being represented on the Advisory Council. We believe that this mode of operation provides an optimal combination home enema the needed discipline expertise, and loser efficiency obtained by locating more generic Node operations at a single site.

Although our group is not affiliated directly with any of the Discipline Node proposals, we understand that NASA and the PDS reserve the right to select the optimum internal sex woman and man of Nodes and Subnodes from elements contained in different proposals. We describe our past and current activities which are of greatest interest to the PDS program, and the resources we will bring to the PDS endeavor.

Our team provides an excellent mix of in-depth experience with all sex woman and man the appropriate data sets, maintains an active and well-respected srx of research in planetary rings, and has the ability and interest to provide the leadership and community focus desired of a PDS Subnode.

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Comments:

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