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Arizona State University Ronald Greeley Center for Planetary Studies - The Ronald Greeley 35mm Slide Collection, The Jovian System
This bundle contains the digitized products generated from Dr. Ronald Greeley's 35mm Slide Collection, the Jovian System, housed at the RGCPS, ASU, Tempe, AZ. Included is a User’s Guide for a further description of the products. -
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Small Body Optical Shape Models V1.0
The Small Body Shape Models data set contains the Peter Thomas shape models for small solar system bodies, as well as image mosaics constructed from these models. These shape models are based upon optical data from a variety of spacecraft instruments, including the Galileo SSI, NEAR MSI, Viking orbiter, Voyager 1 & 2, and the Hubble Space Telescope. The data has been published in a variety of publications between 1984 and 1999. -
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GASKELL DIONE SHAPE MODEL
The shape model of Dione derived by Robert Gaskell from Cassini images. The model is provided in the implicitly connected quadrilateral (ICQ) format. This version of the model was prepared on July 23, 2012. Vertex-facet versions of the models are also provided. -
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GASKELL MIMAS SHAPE MODEL
The shape model of Mimas derived by Robert Gaskell from Cassini ISSNA and ISSWA images and Voyager 1 ISSN images. The model is provided in the implicitly connected quadrilateral (ICQ) format. This version of the model was prepared on June 26, 2012. Vertex-facet versions of the models are also provided. -
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ISS Observations from the Cassini Cruise to Saturn
This bundle contains Cassini ISS images, metadata, and associated documentation from the cruise to Saturn--October 1997 through December 2003. -
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GASKELL PHOEBE SHAPE MODEL
The shape model of Phoebe derived by Robert Gaskell from Cassini images. The model is provided in the implicitly connected quadrilateral (ICQ) format. This version of the model was prepared on August 4, 2012. Vertex-facet versions of the models are also provided. -
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ISS Observations from the Cassini Tour of the Saturn System
This bundle contains Cassini ISS images, metadata, and associated documentation for the Saturn tour--January 2004 through end of mission in September 2017. -
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GASKELL TETHYS SHAPE MODEL
The shape model of Tethys derived by Robert Gaskell from Cassini Imaging Science Subsystem narrow and wide angle camera (ISSNA and ISSWA) images. The model is provided in the implicitly connected quadrilateral (ICQ) format. This version of the model was prepared on July 25, 2012. Vertex-facet versions of the models are also provided. -
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Saturn Small Moon Shape Models V1.0
Digital shape models have been constructed from Cassini Imaging Science Subsystem (ISS) data for eleven of the small satellites of Saturn and delivered to the Planetary Data System. These satellites are: Pan, Daphnis, Atlas, Prometheus, Pandora, Epimetheus, Janus, Telesto, Calypso, Helene, and Hyperion. These models typically have uncertainties well under 0.5 km. They are appropriate for global geometric, geologic, and geophysical studies, and regional slope and topography study. They are useful in studying morphologies of only the relatively largest-sized craters. Studies based on early versions of these shape models are in Thomas et al., 2013 -
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Restoring and Archiving Voyager 1 Cruise Images of Uranus and Neptune (RAV1CIUN) PDART Bundle
RAV1CIUN's charter is to reprocess all the V1 cruise images of Neptune and Uranus, using the best calibrations, analyze the results to derive planetary reflectance for each phase angle in each Voyager imaging spectral band, and archive all results in the PDS. -
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Phoebe SPC Shape Model and Assessment Products V1.0
This bundle contains a shape model for the Saturnian moon Phoebe, along with quality assessment data. The global model is similar to the previously archived "Gaskell Phoebe Shape Model", but is provided in multiple formats.
Data Sets and Information