Search Results
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collection:
data collection for the "GASKELL DIONE SHAPE MODEL" bundle
This is the data collection for the gaskell.dione.shape-model bundle. 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. -
collection:
data collection for the "GASKELL MIMAS SHAPE MODEL" bundle
This is the data collection for the gaskell.mimas.shape-model bundle. 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. -
bundle:
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. -
collection:
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 -
collection:
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 -
collection:
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. -
collection:
data collection for the "GASKELL TETHYS SHAPE MODEL" bundle
This is the data collection for the gaskell.tethys.shape-model bundle. 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. -
bundle:
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. -
bundle:
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. -
bundle:
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. -
bundle:
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. -
bundle:
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. -
bundle:
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 -
bundle:
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. -
collection:
Raw Data Collection for the Cassini ISS Observations from the Cruise to Saturn
This is the collection of raw ISS images and associated metadata from the Cassini cruise to Saturn. -
collection:
data collection for the "GASKELL PHOEBE SHAPE MODEL" bundle
This is the data collection for the gaskell.phoebe.shape-model bundle. 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. -
collection:
Raw Data Collection for the Cassini ISS Observations from the Saturn Tour
This is the collection of raw ISS images and associated metadata from the Cassini tour of the Saturn system. -
collection:
Document collection for Arizona State University Ronald Greeley Center for Planetary Studies - The Ronald Greeley 35mm Slide Collection, The Jovian System, Io
This collection, included in document_io, consists of 292 digitized 35mm slides primarily of Io, Galilean Satellite of Jupiter, and other related bodies. Slides are divided into two databases, diagrams and photos, but are inventoried as a single collection. Information about each photograph, including location, description, and mission, are in the document_database in io_diagram_database.pdf and io_photo_database.pdf. The photographs and documentation are from the Dr. Ronald Greeley archive at the Arizona State University Ronald Greeley Center for Planetary Studies, Tempe, Arizona. -
collection:
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